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668</div><div id="imCell_196" class=""> <div id="imCellStyleGraphics_196" ></div><div id="imCellStyleBorders_196"></div><div id="imCellStyleTitle_196">Monte Baldo in diretta</div><div id="imHTMLObject_196" class="imHTMLObject" style="text-align: center; height: 220px; width: 100%; overflow: hidden;"><a target="_blank" href="http://www.astrofiliveronesi.it/uploads/images/webcam/montebaldo.jpg"> <img class="reload" width="333" height="187" alt="" src="http://www.astrofiliveronesi.it/uploads/images/webcam/montebaldo.jpg"></a></div></div><div id="imCell_199" class=""> <div id="imCellStyleGraphics_199" ></div><div id="imCellStyleBorders_199"></div><div id="imCellStyleTitle_199">TIME LAPSE NOTTE PRECEDENTE</div><div id="imHTMLObject_199" class="imHTMLObject" style="text-align: center; width: 100%; overflow: hidden;"><a target="_blank" href="https://www.osservatoriomontebaldo.it/allsky/videos/allsky.mp4"> 669 <video width="220" height="240" muted autoplay loop playsinline> 670 <source src="https://www.osservatoriomontebaldo.it/allsky/videos/allsky.mp4" type="video/mp4"> 671 </video> 672 </a></div></div><div id="imCell_197" class=""> <div id="imCellStyleGraphics_197" ></div><div id="imCellStyleBorders_197"></div><div id="imCellStyleTitle_197">Il cielo in diretta</div><div id="imHTMLObject_197" class="imHTMLObject" style="text-align: center; height: 220px; width: 100%; overflow: hidden;"><a target="_blank" href="https://www.osservatoriomontebaldo.it/allsky/image.jpg"> <img class="reload" width="220" height="240" alt="" src="https://www.osservatoriomontebaldo.it/allsky/image.jpg"></a></div></div><div id="imCell_149" class=""> <div id="imCellStyleGraphics_149" ></div><div id="imCellStyleBorders_149"></div><div id="imTextObject_149"> 673 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTextObject_149_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 674 <div class="text-inner"> 675 <div class="imTACenter"><a href="http://www.comune.ferraradimontebaldo.vr.it/" target="_blank" class="imCssLink inline-block"><img class="image-4" src="images/ComunediFerrara2.jpg" width="251" height="42" /></a> <a href="http://www.astrofiliveronesi.it" target="_blank" class="imCssLink inline-block"><img class="image-5" src="images/LogoCAV.jpg" width="42" height="42" /></a> <span class="fs10lh1-5"> </span><span class="fs10lh1-5 ff1"><a href="https://www.rifugionovezzina.com/" target="_blank" class="imCssLink inline-block"><img class="image-1" src="images/ParcoLogo.jpg" width="175" height="42" /></a></span><span class="fs10lh1-5 ff1"> </span><a href="index.html" class="imCssLink inline-block" onclick="return x5engine.utils.location('index.html', null, false)"><img class="image-3" src="images/LogoOMBfondo_w09yrfrt.png" width="41" height="42" /></a></div> 676 </div> 677 </div> 678 679 </div> 680 </div><div id="imCell_162" class=""> <div id="imCellStyleGraphics_162" ></div><div id="imCellStyleBorders_162"></div><div id="imTextObject_162"> 681 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTextObject_162_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 682 <div class="text-inner"> 683 <div class="imTALeft"><img class="image-1" src="images/RifugioNovezzina.jpg" width="185" height="139" /><br></div> 684 </div> 685 </div> 686 687 </div> 688 </div><div id="imCell_161" class=""> <div id="imCellStyleGraphics_161" ></div><div id="imCellStyleBorders_161"></div><div id="imTextObject_161"> 689 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTextObject_161_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 690 <div class="text-inner"> 691 <div class="imTALeft"><img class="image-0" src="images/OMB.jpg" width="185" height="139" /></div> 692 </div> 693 </div> 694 695 </div> 696 </div><div id="imCell_163" class=""> <div id="imCellStyleGraphics_163" ></div><div id="imCellStyleBorders_163"></div><div id="imTableObject_163"> 697 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_163_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 698 <div class="text-inner"> 699 <table data-minrequestedwidth="525" data-computedwidth="525" style="width: 525px;"><tbody><tr><td style="width: 517px; height: 139.891px; margin-top: 0px; margin-left: 0px; background-color: rgb(239, 239, 239);" class="imVt"><div class="imTAJustify"><span class="fs9lh1-5 ff1">LâOsservatorio Astronomico Monte Baldo "A.Gelodi", unico osservatorio pubblico della provincia di Verona, è di proprietà del Comune di Ferrara di Monte Baldo ed è gestito dal Circolo Astrofili Veronesi. <span><a href="https://www.rifugionovezzina.com/" target="_blank" class="imCssLink">L'</a></span><a href="https://www.rifugionovezzina.com/" target="_blank" class="imCssLink">orto botanico</a>, intende promuovere la conoscenza dellâambiente naturale baldense con visite, escursioni, attività didattiche, laboratori che trasmettano ai visitatori la grande ricchezza naturale, culturale, storica ed umana del territorio. Il <a href="https://www.rifugionovezzina.com/" target="_blank" class="imCssLink">Rifugio di Novezzina</a>, è gestito dalla cooperativa "<a href="https://www.ilpontecooperativasociale.it/" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.ilpontecooperativasociale.it/', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">Il Ponte</a>
699"</span></div></td></tr></tbody></table> 700 </div> 701 </div> 702 703 </div> 704 </div><div id="imCell_141" class=""> <div id="imCellStyleGraphics_141" ></div><div id="imCellStyleBorders_141"></div><div id="imCellStyleTitle_141">APERTURE PUBBLICHE</div><div id="imObjectImage_141"><div id="imObjectImage_141_container"><a href="https://www.astrofiliveronesi.it/uploads/pdf/DepliantAperture2026WEB.pdf" target="_blank"><img src="images/Banner-Programma-2026.jpg" width="461" height="242" /> 705 </a></div></div></div><div id="imCell_143" class=""> <div id="imCellStyleGraphics_143" ></div><div id="imCellStyleBorders_143"></div><div id="imCellStyleTitle_143">PROGRAMMA CIRCOLO ASTROFILI VERONESI</div><div id="imObjectImage_143"><div id="imObjectImage_143_container"><a href="https://www.astrofiliveronesi.it/uploads/pdf/2026CAV_WEB.pdf" target="_blank"><img src="images/Banner-CAV-I-SEM.jpg" width="461" height="327" /> 706 </a></div></div></div><div id="imCell_185" class=""> <div id="imCellStyleGraphics_185" ></div><div id="imCellStyleBorders_185"></div><div id="imCellStyleTitle_185">NOTIZIE OSSERVATORIO</div><div id="imTableObject_185"> 707 <div id="imTableObject_185_tab0" class="grid-prop current-tab" style="opacity: 1; text-align: start; overflow: hidden;"><div data-index="0" class="text-tab-content grid-prop current-tab text-inner" style="opacity: 1; " ><table data-minrequestedwidth="4272" data-computedwidth="4272" style="width: 4272px;"><tbody><tr><td rowspan="1" style="height: 399px; background-color: transparent; margin-top: 0px; margin-left: 0px; width: 300px;" class="imVc"><div data-text-align="center" class="imTACenter"><br></div><div data-text-align="center" class="imTACenter"><span class="fs12lh1-5"><a href="blog/?prima-nova-del-2026" class="imCssLink"><b>M81 REGALA LA PRIMA NOVA 2026</b></a></span></div><div data-text-align="center" class="imTACenter"><img class="image-4" src="images/M81_20260126_OMB31_SM.jpg" width="300" height="300" /></div><div data-text-align="center" class="imTACenter"><span class="fs10lh1-5"><a href="blog/?prima-nova-del-2026" class="imCssLink"><b class="fs12lh1-5">VAI ALLA NOTIZIA</b></a></span><br></div><br></td><td rowspan="1" style="height: 399px; background-color: transparent; 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background-color: transparent; margin-top: 0px; margin-left: 0px; width: 301px;" class="imVc"><div data-text-align="center" class="imTACenter"><span><a href="blog/?la-nuova-all-sky-camera-dell-osservatorio-monte-baldo" class="imCssLink" target ="_blank"><b class="fs12lh1-5">LA NUOVA ALL SKY CAMERA</b></a></span></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?la-nuova-all-sky-camera-dell-osservatorio-monte-baldo" class="imCssLink" target ="_blank"><b class="fs12lh1-5">DELL'OSSERVATORIO</b></a></span></div><div data-text-align="center" class="imTACenter"><b class="fs12lh1-5"><img class="image-0" src="images/ALL-SKY-sm300.jpg" width="301" height="301" /><br></b></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?la-nuova-all-sky-camera-dell-osservatorio-monte-baldo" class="imCssLink"><b class="fs12lh1-5">VAI ALLA NOTIZIA</b></a></span><br></div></td><td rowspan="1" style="height: 399px; background-color: transparent; margin-top: 0px; margin-left: 0px; width: 300px;" class="imVc"><div data-text-align="center" class="imTACenter"><span><a href="blog/?aurora-boreale-11-novembre-2025" class="imCssLink"><b class="fs12lh1-5">L'AURORA BOREALE DELL'11</b></a></span></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?aurora-boreale-11-novembre-2025" class="imCssLink"><b class="fs12lh1-5">NOVEMBRE 2025</b></a></span></div><div data-text-align="center" class="imTACenter"><img class="image-7" src="images/AURORA-11-NOVEMBRE300.jpg" width="300" height="300" /><br></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?aurora-boreale-11-novembre-2025" class="imCssLink"><b class="fs12lh1-5">VAI ALLA NOTIZIA</b></a></span></div></td><td rowspan="1" style="height: 399px; background-color: transparent; margin-top: 0px; margin-left: 0px; width: 301px;" class="imVc"><div data-text-align="center" class="imTACenter"><span><a href="blog/?pha-2025-fa22" class="imCssLink"><b class="fs12lh1-5">IL PASSAGGIO RAVVICINATO</b></a></span></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?pha-2025-fa22" class="imCssLink"><b class="fs12lh1-5">DELL'ASTEROIDE 2025 FA22</b></a></span></div><div data-text-align="center" class="imTACenter"><b class="fs12lh1-5"><img class="image-11" src="images/PHA300.jpg" width="301" height="300" /></b></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?pha-2025-fa22" class="imCssLink"><b class="fs12lh1-5">VAI ALLA NOTIZIA</b></a></span></div></td><td rowspan="1" style="height: 399px; background-color: transparent; margin-top: 0px; margin-left: 0px; width: 300px;" class="imVc"><div data-text-align="center" class="imTACenter"><span><a href="blog/?manifestazione-per-i-20-anni-dell-osservatorio-del-monte-baldo" class="imCssLink"><b class="fs12lh1-5">27 LUGLIO. MANIFESTAZIONE PER IL</b></a></span></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?manifestazione-per-i-20-anni-dell-osservatorio-del-monte-baldo" class="imCssLink"><b class="fs12lh1-5">VENTENNALE OSSERVATORIO</b></a></span></div><div data-text-align="center" class="imTACenter"><div><img class="image-8" src="images/VENTENNALE300.jpg" width="300" height="301" /><br></div></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?manifestazione-per-i-20-anni-dell-osservatorio-del-monte-baldo" class="imCssLink"><b class="fs12lh1-5">VAI ALLA NOTIZIA</b></a></span><br></div></td><td rowspan="1" style="height: 399px; background-color: transparent; margin-top: 0px; margin-left: 0px; width: 300px;" class="imVc"><div data-text-align="center" class="imTACenter"><span><a href="blog/?la-cometa-interstellare-3i-atlas-ripresa-dall-osservatorio-del-monte-baldo" class="imCssLink"><b class="fs12lh1-5">LA COMETA INTERSTELLARE</b></a></span></div><div data-text-align="center" class="imTACenter"><span><a href="blog/?la-cometa-interstellare-3i-atlas-ripresa-dall-osservatorio-del-monte-baldo" class="imCssLink"><b class="fs12lh1-5">3I/ATLAS</b></a></span></div><div data-text-align="center" class="imTACenter"><img class="image-9" src="images/3IATLAS-300.jpg" width="300" height="300" /><b class="fs12lh1-5"><br></b><div data-text-align="center" class="imTACenter"><b class="fs12lh1-5"><span><a href="blog/?la-cometa-interstellare-3i-atlas-ripresa-dall-osservatorio-del-monte-baldo" class="imCssLink">VAI ALLA NOTIZIA</a></span></b></div></div></td><td rowspan="1" style="height: 399px; background-color: transparent; margin-top: 0px; margin-left: 0px; width: 300px; display: table-cell;" class="imVc"><div><b class="fs12lh1-5"><span><a href="blog/?nuovi-occhi-sul-cielo-del-monte-baldo" class="imCssLink">NUOVI OCCHI SUL CIELO DEL MONTE</a></span></b></div><div><b class="fs12lh1-5"><span><a href="blog/?nuovi-occhi-sul-cielo-del-monte-baldo" class="imCssLink">BALDO<br></a></span></b><div data-text-align="start" style="text-align: start;"><b class="fs12lh1-5"><img class="image-14" src="images/SmartEye-300.jpg" width="300" height="300" /><br></b><div data-text-align="center" class="imTACenter"><b class="fs12lh1-5"><span><a href="blog/?nuovi-occhi-sul-cielo-del-monte-baldo" class="imCssLink">VAI ALLA NOTIZIA</a></span></b></div></div></div></td></tr></tbody></table></div></div> 708
708<script> 709 function loadimTableObject_185_tab0() { 710 var box = $("#imTableObject_185_tab0 .text-inner"); 711 var data = box.data('imRollover'); 712 if (data != null) { data.disable(); } 713 x5engine.imRollover({"id": "#imTableObject_185_tab0 .text-inner", "movement": "CONTINUE", "direction": "LEFT", "effect": "LINEAR", "height": 450, "time": 60, "autostart": true, "mouselock": true}); 714 } 715 x5engine.boot.push(loadimTableObject_185_tab0); 716 </script>
716 717 718 </div> 719 </div><div id="imCell_168" class=""> <div id="imCellStyleGraphics_168" ></div><div id="imCellStyleBorders_168"></div><div id="imTableObject_168"> 720 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_168_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 721 <div class="text-inner"> 722 <table data-minrequestedwidth="607" data-computedwidth="607" style="width: 607px;"><tbody><tr><td style="width: 599px; height: 24px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><span class="fs12lh1-5 cf1 ff1"><b>ATTIVITA'</b></span><b class="imTALeft"><span class="fs12lh1-5 cf2 ff1">________</span><span class="fs12lh1-5 cf2 ff1">____________________________________</span></b></div></td></tr></tbody></table> 723 </div> 724 </div> 725 726 </div> 727 </div><div id="imCell_165" class=""> <div id="imCellStyleGraphics_165" ><div style="position: relative; height: 100%;"><div id="imCellStyleGraphicsC_165"></div><div id="imCellStyleGraphicsT_165"></div><div id="imCellStyleGraphicsTL_165"></div><div id="imCellStyleGraphicsTR_165"></div><div id="imCellStyleGraphicsL_165"></div><div id="imCellStyleGraphicsR_165"></div><div id="imCellStyleGraphicsB_165"></div><div id="imCellStyleGraphicsBL_165"></div><div id="imCellStyleGraphicsBR_165"></div></div></div><div id="imCellStyleBorders_165"></div><div id="imCellStyleTitle_165">Visite Scuole</div><div id="imTableObject_165"> 728 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_165_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 729 <div class="text-inner"> 730 <table data-minrequestedwidth="150" data-computedwidth="150" style="width: 150px;"><tbody><tr><td style="width: 142px; height: 190px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><span class="cf1"><span class="fs10lh1-5 ff1">Visite per le scuole di ogni tipo e livello, con lezione e osservazione sia del Sole di giorno, sia degli oggetti celesti alla sera. </span></span><div><span class="cf1"><span class="fs10lh1-5 ff1"><a href="scuole.html" class="imCssLink" onclick="return x5engine.utils.location('scuole.html', null, false)">Per saperne di più...</a></span></span></div><div><span class="cf1"><span class="fs10lh1-5 ff1"><br></span></span></div></div></td></tr></tbody></table> 731 </div> 732 </div> 733 734 </div> 735 </div><div id="imCell_164" class=""> <div id="imCellStyleGraphics_164" ><div style="position: relative; height: 100%;"><div id="imCellStyleGraphicsC_164"></div><div id="imCellStyleGraphicsT_164"></div><div id="imCellStyleGraphicsTL_164"></div><div id="imCellStyleGraphicsTR_164"></div><div id="imCellStyleGraphicsL_164"></div><div id="imCellStyleGraphicsR_164"></div><div id="imCellStyleGraphicsB_164"></div><div id="imCellStyleGraphicsBL_164"></div><div id="imCellStyleGraphicsBR_164"></div></div></div><div id="imCellStyleBorders_164"></div><div id="imCellStyleTitle_164">Stage Astronomia</div><div id="imTableObject_164"> 736 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_164_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 737 <div class="text-inner"> 738 <table data-minrequestedwidth="150" data-computedwidth="150" style="width: 150px;"><tbody><tr><td style="width: 142px; height: 190px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div><span class="cf1"><span class="fs10lh1-5 ff1">Lo </span><span class="ff1"><b><span class="fs10lh1-5">stage di Astronomia </span></b><span class="fs10lh1-5">per i ragazzi del IV anno delle scuole superiori è stata una esperienza formativa dell'astronomia dal 2012 al 2016</span></span></span><br><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/stage-astronomia.html" target="_blank" class="imCssLink">Per saperne di più...</a></span></span></div></div></td></tr></tbody></table> 739 </div> 740 </div> 741 742 </div> 743 </div><div id="imCell_167" class=""> <div id="imCellStyleGraphics_167" ><div style="position: relative; height: 100%;"><div id="imCellStyleGraphicsC_167"></div><div id="imCellStyleGraphicsT_167"></div><div id="imCellStyleGraphicsTL_167"></div><div id="imCellStyleGraphicsTR_167"></div><div id="imCellStyleGraphicsL_167"></div><div id="imCellStyleGraphicsR_167"></div><div id="imCellStyleGraphicsB_167"></div><div id="imCellStyleGraphicsBL_167"></div><div id="imCellStyleGraphicsBR_167"></div></div></div><div id="imCellStyleBorders_167"></div><div id="imCellStyleTitle_167">Aperture Pubbliche</div><div id="imTableObject_167"> 744 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_167_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 745 <div class="text-inner"> 746 <table data-minrequestedwidth="150" data-computedwidth="150" style="width: 150px;"><tbody><tr><td style="width: 142px; height: 190px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><span class="cf1"><span class="fs10lh1-5 ff1">Durante il periodo primaverile ed estivo sono organizzate una serie di aperture pubbliche aperte a tutti. Non serve prenotazione </span></span><div><span class="cf1"><span class="fs10lh1-5 ff1"><a href="aperture-pubbliche.html" class="imCssLink" onclick="return x5engine.utils.location('aperture-pubbliche.html', null, false)">
746Per saperne di più...</a></span></span></div><div><span class="cf1"><span class="fs10lh1-5 ff1"><br></span></span></div></div></td></tr></tbody></table> 747 </div> 748 </div> 749 750 </div> 751 </div><div id="imCell_184" class=""> <div id="imCellStyleGraphics_184" ><div style="position: relative; height: 100%;"><div id="imCellStyleGraphicsC_184"></div><div id="imCellStyleGraphicsT_184"></div><div id="imCellStyleGraphicsTL_184"></div><div id="imCellStyleGraphicsTR_184"></div><div id="imCellStyleGraphicsL_184"></div><div id="imCellStyleGraphicsR_184"></div><div id="imCellStyleGraphicsB_184"></div><div id="imCellStyleGraphicsBL_184"></div><div id="imCellStyleGraphicsBR_184"></div></div></div><div id="imCellStyleBorders_184"></div><div id="imCellStyleTitle_184">Visite gruppi privati</div><div id="imTableObject_184"> 752 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_184_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 753 <div class="text-inner"> 754 <table data-minrequestedwidth="158" data-computedwidth="158" style="width: 158px;"><tbody><tr><td style="width: 150px; height: 139.891px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><span class="fs10lh1-5 cf1 ff1">L'Osservatorio apre anche su prenotazione di gruppi privati per una esperienza unica tutto il periodo dell'anno...</span></div><div><span class="cf2"><span class="fs10lh1-5 ff1"><a href="gruppi-privati.html" class="imCssLink" onclick="return x5engine.utils.location('gruppi-privati.html', null, false)">Per saperne di più...</a></span></span></div></div></td></tr></tbody></table> 755 </div> 756 </div> 757 758 </div> 759 </div><div id="imPageRow_2" class="imPageRow"> 760 <div style="position: absolute; top: 0; left: 0; right: 0; bottom: 0; overflow: hidden;"><div id="imPageRowGraphics_2" ></div></div> 761 </div> 762 <div id="imCell_169" class=""> <div id="imCellStyleGraphics_169" ></div><div id="imCellStyleBorders_169"></div><div id="imTableObject_169"> 763 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_169_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 764 <div class="text-inner"> 765 <table data-minrequestedwidth="607" data-computedwidth="607" style="width: 607px;"><tbody><tr><td style="width: 599px; height: 24px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><b class="imTALeft cf1"><span class="fs12lh1-5 ff1">RICERCA SCIENTIFICA</span><span class="fs12lh1-5 ff1">________</span><span class="fs12lh1-5 ff1">__________________</span></b></div></td></tr></tbody></table> 766 </div> 767 </div> 768 769 </div> 770 </div><div id="imCell_172" class=""> <div id="imCellStyleGraphics_172" ></div><div id="imCellStyleBorders_172"></div><div id="imCellStyleTitle_172">Astrometria</div><div id="imTableObject_172"> 771 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_172_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 772 <div class="text-inner"> 773 <table data-minrequestedwidth="175" data-computedwidth="175" style="width: 175px;"><tbody><tr><td style="width: 167px; height: 201px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><div><span class="fs10lh1-5 cf1 ff1">da gennaio 2006</span><span class="fs10lh1-5 ff2"><a href="astrometria.html" class="imCssLink inline-block" onclick="return x5engine.utils.location('astrometria.html', null, false)"><img class="image-0" src="images/Attivita2.jpg" width="158" height="119" /></a></span><span class="fs9lh1-5 ff1">Guido Rocca</span></div><div><span class="fs9lh1-5 ff1">Flavio Castellani</span></div></div><div><span class="cf2"><span class="fs10lh1-5 ff1"><br></span></span></div></div></td></tr></tbody></table> 774 </div> 775 </div> 776 777 </div> 778 </div><div id="imCell_170" class=""> <div id="imCellStyleGraphics_170" ></div><div id="imCellStyleBorders_170"></div><div id="imCellStyleTitle_170">Fotografia</div><div id="imTableObject_170"> 779 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_170_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 780 <div class="text-inner"> 781 <table data-minrequestedwidth="166" data-computedwidth="166" style="width: 166px;"><tbody><tr><td style="width: 158px; height: 205.922px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><span class="fs10lh1-5 cf1 ff1">da settembre 2005</span><span class="fs10lh1-5 ff2"><a href="galleria-fotografica.html" class="imCssLink inline-block" onclick="return x5engine.utils.location('galleria-fotografica.html', null, false)"><img class="image-0" src="images/Attivita6.jpg" width="158" height="123" /></a></span></div><div class="imTALeft"><span class="fs9lh1-5 ff1">Andrea Peretti</span></div><div class="imTALeft"><span class="fs9lh1-5 ff1">Gianfranco Martini</span></div><div><span class="cf2"><span class="fs10lh1-5 ff1"><br></span></span></div></div></td></tr></tbody></table> 782 </div> 783 </div> 784 785 </div> 786 </div><div id="imCell_171" class=""> <div id="imCellStyleGraphics_171" ></div><div id="imCellStyleBorders_171"></div><div id="imCellStyleTitle_171">Meteor Hunter</div><div id="imTableObject_171"> 787 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_171_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 788 <div class="text-inner"> 789 <table data-minrequestedwidth="175" data-computedwidth="175" style="width: 175px;"><tbody><tr><td style="width: 167px; height: 201px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><div><span class="fs10lh1-5 cf1 ff1">da novembre 2005</span><span class="fs10lh1-5 ff2"><span style="outline-color: black;" class="fs10lh1-5"><a href="meteore.html" class="imCssLink inline-block" onclick="return x5engine.utils.location('meteore.html', null, false)"><img class="image-1" src="images/Attivita1.jpg" width="158" height="116" /></a></span></span><span class="fs9lh1-5 ff1">Maurizio Carli</span></div></div><div><span class="cf2"><span class="fs10lh1-5 ff1"><br></span></span></div></div></td></tr></tbody></table> 790 </div> 791 </div> 792 793 </div> 794 </div><div id="imCell_175" class=""> <div id="imCellStyleGraphics_175" ></div><div id="imCellStyleBorders_175"></div><div id="imCellStyleTitle_175">Supernovae</div><div id="imTableObject_175"> 795 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_175_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 796 <div class="text-inner"> 797 <table data-minrequestedwidth="239" data-computedwidth="239" style="width: 239px;"><tbody><tr><td style="width: 231px; height: 272px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><div><span class="fs10lh1-5 cf1 ff1">da aprile 2011</span><span class="fs10lh1-5 ff2"><a href="https://www.osservatoriomontebaldo.it/supernovae.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.osservatoriomontebaldo.it/supernovae.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink inline-block"><img class="image-1" src="images/HST_NGC2748_SN2013ff_arena_r1kggr4i.jpg" width="158" height="108" /></a></span></div><div><span class="fs9lh1-5 ff1">Raffaele Belligoli</span></div><div><span class="fs9lh1-5 ff1">Flavio Castellani</span></div><div><span class="fs9lh1-5 ff1">Vittorio Andreoli</span></div><div><span class="fs9lh1-5 ff1">Claudio Marangoni</span></div></div></div></td></tr></tbody></table> 798 </div> 799 </div> 800 801 </div> 802 </div><div id="imCell_173" class=""> <div id="imCellStyleGraphics_173" ></div><div id="imCellStyleBorders_173"></div><div id="imCellStyleTitle_173">Spettroscopia</div><div id="imTableObject_173"> 803 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_173_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 804 <div class="text-inner"> 805 <table data-minrequestedwidth="239" data-computedwidth="239" style="width: 239px;"><tbody><tr><td style="width: 231px; height: 272px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><div><span class="fs10lh1-5 cf1 ff1">da marzo 2006</span><a href="https://www.osservatoriomontebaldo.it/spettroscopia.html" target="_blank" class="imCssLink inline-block"><img class="image-1" src="images/Spettrostamp.jpg" width="158" height="120" /></a></div><div><span class="fs9lh1-5 ff1">Flavio Castellani</span></div><div><span class="fs9lh1-5 ff1">Sergio Moltomoli</span></div><div><span class="fs9lh1-5 ff1">
805Vittorio Andreoli </span></div><div><span class="fs9lh1-5 ff1">Gabriele Zampieri</span></div></div></div></td></tr></tbody></table> 806 </div> 807 </div> 808 809 </div> 810 </div><div id="imCell_174" class=""> <div id="imCellStyleGraphics_174" ></div><div id="imCellStyleBorders_174"></div><div id="imCellStyleTitle_174">Fotometria</div><div id="imTableObject_174"> 811 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTableObject_174_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 812 <div class="text-inner"> 813 <table data-minrequestedwidth="239" data-computedwidth="239" style="width: 239px;"><tbody><tr><td style="width: 231px; height: 272px; margin-top: 0px; margin-left: 0px;" class="imVt"><div class="imTAJustify"><div class="imTALeft"><div><span class="fs10lh1-5 cf1 ff1">da gennaio 2007</span><span class="fs10lh1-5 ff2"><a href="https://www.osservatoriomontebaldo.it/fotometria.html" target="_blank" class="imCssLink inline-block"><img class="image-0" src="images/Attivita3.jpg" width="158" height="116" /></a></span></div><div><span class="fs9lh1-5 ff1">Flavio Castellani</span></div><div><span class="fs9lh1-5 ff1">Vittorio Andreoli</span></div><div><span class="fs9lh1-5 ff1">Raffaele Belligoli</span></div><div><span class="fs9lh1-5 ff1">Claudio Marangoni</span></div></div></div></td></tr></tbody></table> 814 </div> 815 </div> 816 817 </div> 818 </div><div id="imCell_176" class=""> <div id="imCellStyleGraphics_176" ></div><div id="imCellStyleBorders_176"></div><div id="imCellStyleTitle_176">Pubblicazioni e scoperte dei membri gruppo ricerca Osservatorio Monte Baldo</div><div id="imTableObject_176"> 819 <div id="imTableObject_176_tab0" class="grid-prop current-tab" style="opacity: 1; text-align: start; overflow: auto; height: 580px;"><div data-index="0" class="text-tab-content grid-prop current-tab text-inner" style="opacity: 1; " ><table data-minrequestedwidth="390.578" data-computedwidth="390.578" style="width: 390.578px;"><tbody><tr><td style="width: 382.578px; height: 31499.4px; margin-top: 0px; margin-left: 0px;" class="imVt"><div><div class="imTAJustify"><b><span class="fs14lh1-5 ff1">2026</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 289088</b></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2026-01-26 22:20:41</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: <b><b>AT 2026blf</b></b><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discoverer internal name: OMB32<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 09:54:46.470 (148.693625) DEC = +69:06:31.70 (69.108806)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2026-01-26 19:47:47.000 (JD=2461067.3248495)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M81<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by F.Castellani, R.Belligoli and V.Andreoli of a PNV (Mag. 19.3R +-0.20 â USNOB1 catalogue) in the host galaxy M81 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Italian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF unfiltered CCD camera)in a couple od 15*180 co-added images. No stellar source was visible at the position of the transient in our past images including reference image dated 2026-01-22 03:20:30 UT</span><br></div><div style="text-align: start;">(<span class="fs11lh1-5 ff1"><span><a href="https://www.wis-tns.org/object/2026blf" target="_blank" class="imCssLink"><b>AT 2026blf</b></a></span>)</span></div></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs14lh1-5 ff1">2025</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 283270 </b></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2025-12-28 20:49:00</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: <b><b>AT 2025ajgh</b></b><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 00:42:58.480 (10.743667) DEC = +41:08:11.40 (41.1365)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2025-12-28 18:22:08.000 (JD=2461038.2653704)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M31<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by F.Castellani, R.Belligoli and V.Andreoli of a PNV (Mag. 18.9R +-0.20 â GAIA DR3 catalogue) in the host galaxy M31 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Ital
819ian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF unfiltered CCD camera)20*180 co-added images. No stellar source was visible at the position of the transient in our past images including reference image dated 2025/12/22 20:58:02 and 2025/12/27 17:43:01. Position of the object is close to AT 2025aeum, identified as a possible eruption of the recurrent nova M31N 1963-09c. The difference of 0.74S East and 1.1" South as well as a careful verification of the position of the transient from the PanStarrs and the images of the reports leads to exclude that it is the same object.</span><br></div><div data-text-align="justify" class="imTAJustify"><div><b><b><span class="fs11lh1-5 ff1"><a href="https://www.wis-tns.org/object/2025ajgh" target="_blank" class="imCssLink">AT 2025ajgh</a></span></b></b></div></div><div data-text-align="justify" class="imTAJustify">(<span class="fs11lh1-5 ff1"><b><a href="https://www.astronomerstelegram.org/?read=17567" target="_blank" class="imCssLink">ATeL 17567</a></b>)</span></div><div data-text-align="justify" class="imTAJustify"><br></div></div></div><div data-text-align="justify" class="imTAJustify"><br></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 281988</b></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2025-12-22 22:55:52</span></div></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: <b><b>AT 2025ahzx</b></b><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discoverer internal name: OMB-PNV29<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 00:42:28.440 (10.6185) DEC = +41:18:24.50 (41.306806)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2025-12-22 20:58:02.000 (JD=2461032.3736343)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M31<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: At 0,76" from transient, a Red Supergiant Candidate with a R Magn of 20.662 is reristered on simbad database. (LGGS J004228.48+411825.6). Even if the 2 mag difference leads us to believe that the transient is not the cataloged object, an outburst cannot be excluded.<br></span></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">(<span><b><a href="https://www.wis-tns.org/object/2025ahzx" target="_blank" class="imCssLink">AT 2025ahzx</a></b></span>)</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">(</span><span class="fs11lh1-5 ff1"><b><a href="https://www.astronomerstelegram.org/?read=17558" target="_blank" class="imCssLink">ATEL 17558</a></b></span><span class="fs11lh1-5 ff1">)</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">(<span><b><a href="https://www.astronomerstelegram.org/?read=17568" target="_blank" class="imCssLink">ATEL 17568</a></b></span>)</span></div><div data-text-align="justify" class="imTAJustify"><br></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 280577 </b></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2025-12-14 19:31:19</span><br></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.</span><br></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation:</span><span class="fs11lh1-5 ff1"> </span><b><b class="fs11lh1-5 ff1">AT 2025agwf</b></b><br></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 00:43:17.640 (10.8235) DEC = +41:14:20.10 (41.238917)</span><br></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2025-12-14 17:53:49.000 (JD=2461024.245706)</span><br></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M31</span><br></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by F.Castellani, R.Belligoli and V.Andreoli of a PNV (Mag. 17.5R +-0.20 - USNOB1 catalogue) in the host galaxy M31 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Ital
819ian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF unfiltered CCD camera)15*180 co-added images. No stellar source was visible at the position of the transient in our past images including reference image dated 2025/12/13 17:29:26.</span><br></div></div><div><span class="fs11lh1-5 ff1">(<span><b><a href="https://www.wis-tns.org/object/2025agwf" target="_blank" class="imCssLink">AT 2025agwf</a></b></span>)</span></div><div><span class="fs11lh1-5 ff1">(<span><b><a href="https://www.astronomerstelegram.org/?read=17543" target="_blank" class="imCssLink">ATeL 17543</a></b></span>)</span></div><div><span class="fs11lh1-5 ff1">(<span><b><a href="https://www.astronomerstelegram.org/?read=17550" target="_blank" class="imCssLink">ATeL 17550</a></b></span>)</span></div><div><br></div></div></div><div class="imTAJustify"><div><span class="fs11lh1-5 ff1"><b>ATel #17351</b></span></div><div><div><span class="fs11lh1-5 ff1">22 Aug 2025; 16:24 UT</span></div></div><div><div><span class="fs11lh1-5 ff1">Comet C/2025 K1 (ATLAS) is deeply depleted of C2</span></div><div><div><span class="fs11lh1-5 ff1">Federico Manzini (Stazione Astronomica di Sozzago), Alessandra Mura (Padova University, INAF-OAPd), Andrea Reguitti (INAF-OAPd), Paolo Ochner (Padova University, INAF-OAPd), Virginio Oldani (Stazione Astronomica di Sozzago), Luigi R. Bedin (INAF-OAPd), Rachele Ottaviani (Padova University), <span class="cf1">Vittorio Andreoli (Osservatorio Astronomico Monte Baldo) </span></span></div></div></div><div><div><b><span class="fs11lh1-5 ff1">(<a href="https://www.astronomerstelegram.org/?read=17351" target="_blank" class="imCssLink">ATel17351</a>)</span></b></div></div><div><b><span class="fs11lh1-5 ff1"><br></span></b></div><div><div><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 257050</b></span></div><div><span class="fs11lh1-5 ff1">Date Received (UTC): 2025-05-28 09:15:28</span><br></div><div><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.</span></div><div><span class="fs11lh1-5 ff1">IAU Designation: AT 2025mho</span></div><div><span class="fs11lh1-5 ff1">Discoverer internal name: OMB-PNV27</span></div><div><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 00:43:55.890 (10.982875) DEC = +41:34:50.50 (41.580694)</span></div><div><span class="fs11lh1-5 ff1">Discovery date: 2025-05-28 02:06:35.000 (JD=2460823.5879051)</span></div><div><span class="fs11lh1-5 ff1">Potential host galaxy: M31</span><br></div><div><span class="fs11lh1-5 ff1"><br></span></div><div><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by F.Castellani, R.Belligoli and V.Andreoli of a PNV (Mag. 18.5R +-0.20 - USNOB1 catalogue) in the host galaxy M31 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Italian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF unfiltered CCD camera)9*180 co-added images. No stellar source was visible at the position of the transient in our past images including reference image dated 2025/03/08.7874</span><br></div></div><div><div><span class="fs11lh1-5 ff1"><b>(<a href="https://www.wis-tns.org/object/2025mho" target="_blank" class="imCssLink">AT 2025mho</a>)</b></span></div><div><br></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 cf2 ff1"><b>TCP J19065629+4019093</b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Ochner P.,<span class="cf1"> Andreoli V</span>., and Balcon C. report the spectroscopic classification of TCP J19065629+4019093. A low-resolution spectrum was obtained with the 1.22-m telescope and B&C spectrograph (dispersion 2.25 Ã
/pixel) located in Asiago (Italy) on 2025-05-1.048 UT. The spectrum shows a blue continuum with Balmer lines: Hα (6562.8 Ã
) is in emission, filled-up by the accretion disk;
819 Hβ (4860 Ã
) and Hγ (4340 Ã
) appear in absorption with weak central emission components, likely also originating from the disk. The other Balmer lines are present in absorption. The spectrum also shows weak helium features: He I 6678 Ã
in emission and He I 4472 Ã
in absorption. These characteristics are consistent with a cataclysmic variable (CV). We propose that TCP J19065629+4019093 is a CV.</span></div></div><div style="text-align: start;"><div><b><span class="fs11lh1-5 cf2 ff1"><span><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J19065629+4019093.html" target="_blank" class="imCssLink">TCP J19065629+4019093</a></span></span></b></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 cf2 ff1"><b>TCP J13560585+3727068</b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Farina.A, <span class="cf1">Andreoli.V,</span> Ochner.P , Reguitti.A, Balcon.C report the classification of TCP J13560585+3727068. A low resolution spectrum was obtained with the 1.22-m telescope and B&C spectrograph (dispersion: 2.25 Ã
/pixel) located at the Asiago Observatory (Italy) on 2025-04-27.816 UT. The spectrum shows a blue continuum with Balmer absorption lines, except for Hα (6562.8 Ã
), which appears filled-up due to emission from the accretion disk. The Hβ (4861 Ã
) line exhibits a FWHM of â1700 km/s. A likely progenitor is identified as DR31495451060634509696 in the GAIA DR3 database (Gaia collaboration et al. 2023) with a g-mag of 17.825 implying a brightness increase of approximately 3 magnitudes (Îmag â 3.5). These features are characteristic of a cataclysmic variable (CV). We propose to classify TCP J13560585+3727068 as a CV.</span></div></div><div style="text-align: start;"><div><b><span class="fs11lh1-5 cf2 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J13560585+3727068.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'http://www.cbat.eps.harvard.edu/unconf/followups/J13560585+3727068.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">TCP J13560585+3727068</a></span></b></div></div><div style="text-align: start;"><span class="fs11lh1-5 ff1"><br></span></div></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 ff1"><b><span class="cf2"> </span><span class="cf2">AT2025img</span></b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><span class="cf1">Andreoli.V</span>, Balcon.C, Farina.A , Ochner.P , Reguitti.A</span></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">A low resolution spectrum was obtained with the 1.22-m telescope and B&C spectrograph (dispersion: 2.25 Ã
/pixel) located at the Asiago Observatory (Italy) on 2025-04-27.831 UT. The spectrum shows a blue continuum with Balmer absorption lines, except for Hα (6562.8 Ã
) which has a weak emission caused by the accretion disk. The Hβ (4861 Ã
) line exhibits a FWHM of â2000 km/s. A likely progenitor is identified as DR3 3816231274612268544 in the GAIA DR3 database (Gaia collaboration et al. 2023) with a g-mag of 20.428 implying a brightness increase of approximately 5 magnitudes (Îmag â 5.2). These features are characteristic of a cataclysmic variable (CV). We propose to classify 2025img as a CV.</span></div></div></div><div style="text-align: start;"><div><span class="fs11lh1-5 ff1"><b><span class="cf2"> </span><span class="cf2"><a href="https://www.wis-tns.org/object/2025img" target="_blank" class="imCssLink">AT2025img</a></span></b></span></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 ff1"><b><span class="cf2">AT2025hwl</span><span class="cf2"> </span></b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Ochner P., Ferrigno F., and<span class="cf1"> Andreoli V.</span></span></div><div data-text-align="justify" class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">reports the spectroscopic classification of AT2025hwl (TCP J18225593+1020013). A low resolution spectrum was obtained with the 1.22-m telescope and B&C spectrograph (dispersion: 2.25 Ã
/pixel) at Asiago Observatory (Italy) on 2025-04-22.027. The spectrum shows a blue continuum with Balmer absorption lines, except for Hα (6562.8 Ã
), which appears filled-up due to emission from the accretion disk. The Hβ (4861 Ã
) line exhibits a full width at half maximum (FWHM) of 1230 km/s. A likely progenitor is identified in ZTF data (Bellm et al. 2019) with a mean r-band magnitude of 18, implying a brightness increase of approximately 3 magnitudes (Îmag â 3). These features are characteristic of a cataclysmic variable (CV). We propose that AT2025hwl be classified as a CV.</span></div></div></div><div style="text-align: start;"><div><span style="font-weight: 700;" class="fs11lh1-5 cf2 ff1">
819<a href="https://www.wis-tns.org/object/2025hwl" target="_blank" class="imCssLink">AT2025hwl</a></span></div><div><div><span><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J18225593+1020013.html" target="_blank" class="imCssLink"><b class="fs11lh1-5 ff1">TCP J18225593+1020013</b></a></span></div></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 246809</b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2025-03-05 22:24:06</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: <b><b>AT 2025dkp</b></b><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discoverer internal name: OMB-PNV24<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 09:55:12.610 (148.802542) DEC = +69:02:46.20 (69.046167)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2025-03-05 21:04:59.000 (JD=2460740.3784606)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M81<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by <span class="cf1">F.Castellani, V.Andreoli, R.Belligoli</span> of a PNV on a co-added 24*180 images (Mag.18.8R +-0.2 - USNOB1 catalogue) in the host galaxy M81 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Italian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF CCD unfiltered CCD camera). No stellar source is visible at the position of the transient in our past images including reference image dated 2025/03/04.84208</span></div><div><span class="fs11lh1-5 ff1">(<a href="https://www.wis-tns.org/object/2025dkp" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2025dkp', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink"> </a><b><b><a href="https://www.wis-tns.org/object/2025dkp" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2025dkp', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">AT 2025dkp</a>)</b></b></span></div><div><b><b><span class="fs11lh1-5 ff1"><a href="https://www.astronomerstelegram.org/?read=17066" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.astronomerstelegram.org/?read=17066', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">(ATEL 17066</a>)</span></b></b></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 246714</b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2025-03-04 22:54:16</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: AT 2025dih<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 09:55:43.430 (148.930958) DEC = +69:05:15.40 (69.087611)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2025-03-04 20:50:43.000 (JD=2460739.3685532)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M81<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by <span class="cf1">
819F.Castellani, V.Andreoli, R.Belligoli </span>of a PNV on a co-added 24*180 images (Mag.19.2R +-0.2 - USNOB1 catalogue) in the host galaxy M81 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Italian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF CCD unfiltered CCD camera). No stellar source is visible at the position of the transient in our past images including reference image dated 2025/02/20.89375</span></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1">(<a href="https://www.wis-tns.org/object/2025dih" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2025dih', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">AT2025dih</a>)</span></b></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1">(<a href="https://www.astronomerstelegram.org/?read=17064" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.astronomerstelegram.org/?read=17064', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">ATEL 17064</a>)</span></b></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs14lh1-5 ff1">2024</span></b></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 cf2 ff1"><b>TCP J17374270+4915116</b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Trabacchin.N,<span class="cf1"> Andreoli.V</span> and Ochner.P report the classification of TCP J17374270+4915116. Low resolution spectrum was obtained with 1.22-m telescope + B&C spectrograph (with dispersion 2.25 Ang/pix) located in Asiago (Italy) on 2024-12-23.722. Spectrum shows a blue continuum consistent with the photometry obtained (see below) and broad absorption of Balmer lines (mean FWHM 3300 km/s) except for Hα (6562.8 Ang) probably filled up by the disk, He I 4471; 4026 Ang is also weakly present. We also obtained BV photometry with 0.4m DK telescope + Moravian G4 CCD full frame located in Novezzina (Italy) on 2024-12-23.77 with results: B:13.3 ± 0.1 V:13.5 ± 0.1. These characteristics are typical of dwarf novae. We propose to classify this object as a CV. (you can find the spectrum at the link: <a href="https://photos.app.goo.gl/HWaQoUebQUo3NfLB6" target="_blank" class="imCssLink">https://photos.app.goo.gl/HWaQoUebQUo3NfLB6</a>)</span></div></div><div style="text-align: start;"><div class="imTAJustify"><b><span class="fs11lh1-5 cf2 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J17374270+4915116.html" target="_blank" class="imCssLink">TCP J17374270+4915116</a></span></b></div><div class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div></div><div style="text-align: start;"><span class="fs11lh1-5 ff1"><br></span></div></div><div class="imTAJustify"><div><b><span class="fs11lh1-5 ff1">TCP J18174546+4324564</span></b></div><div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Fiscale.S ; Ochner.P and<span class="cf1"> Andreoli.V</span> report the spectroscopic classification of TCP J18174546+4324564. We obtained a low resolution spectrum (3600-8000 Ang, dispersion 2.31 Ang/pix) of 2024rkw on 2024-08-06.969 with the Asiago 1.22m + B&C spectrograph . The spectrum shows a blue continuum and absorption of Balmer lines except for H alpha (6562.8 Ang) which is not present in our spectrum, probably filled-up by the disk emissions, also D1 and D2 interstellar sodium are presents.We propose to classify TCP J18174546+4324564 as CV. (the spectrum is available at the following link: <a href="https://photos.app.goo.gl/tsDzSiuwRQGbY5pQ9" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://photos.app.goo.gl/tsDzSiuwRQGbY5pQ9', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">https://photos.app.goo.gl/tsDzSiuwRQGbY5pQ9</a>)</span></div></div><div><div><b><span class="fs11lh1-5 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J18174546+4324564.html" target="_blank" class="imCssLink">TCP J18174546+4324564</a></span></b></div></div></div><div class="imTAJustify"><br></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div><b class="fs11lh1-5 ff1">TCP J19470832-0924198</b></div><div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Fiscale.S ; Ochner.P and <span class="cf1">Andreoli.V</span> report the spectroscopic classification of TCP J19470832-0924198 (2024rkw). We obtained a low resolution spectrum (3600-8000 Ang, dispersion 2.31 Ang/pix) of 2024rkw on 2024-08-06.908 with the Asiago 1.22m + B&C spectrograph . The spectrum shows a blue continuum and absorption of Balmer lines except for H alpha (6562.8 Ang) which is not present in our spectrum, probably f
819illed-up by the disk emissions, also D1 and D2 interstellar sodium are presents. All the characteristics are typical of CV stars. We propose to classify 2024rkw as CV.</span></div></div><div class="imTALeft"><div class="imTAJustify"><span><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J19470832-0924198.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'http://www.cbat.eps.harvard.edu/unconf/followups/J19470832-0924198.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink"><b class="fs11lh1-5 ff1">TCP J19470832-0924198</b></a></span></div></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs11lh1-5 ff1"><span style="text-align: start;"><b>TNS Astronomical Transient Report No. 238313</b></span><br></span></div><div class="imTAJustify"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">date Received (UTC): 2024-12-30 23:00:15</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: <b><b>AT 2024agal</b></b><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discoverer internal name: OMB-PNV22<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 00:41:33.690 (10.390375) DEC = +40:57:13.30 (40.953694)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2024-12-30 19:13:43.000 (JD=2460675.3011921)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M31<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: Flavio Castellani report the discovery by <span class="cf1">F.Castellani, R.Belligoli and V.Andreoli</span> of a PNV (Mag. 19.3R +-0.20 - USNOB1 catalogue) in the host galaxy M31 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Italian Supernovae Search Project using a 0.40m f/7 Dall-Kirkham telescope (+ Moravian G4-9000 KAF unfiltered CCD camera)20*180 co-added images. No stellar source was visible at the position of the transient in our past images including reference image dated 2024/12/29.7370.<br></span></div><div style="text-align: start;"><span class="fs11lh1-5 ff1"><br></span></div></div><div class="imTAJustify"><b><span class="fs11lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 ff1"><b>TNS Astronomical Transient Report No. 222635</b></span></div><div style="text-align: start;"><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Date Received (UTC): 2024-08-25 10:57:09</span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Flavio Castellani report/s the discovery of a new astronomical transient.<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">IAU Designation: <b><b>AT 2024ssq</b></b><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Coordinates (J2000): RA = 00:43:00.010 (10.750042) DEC = +41:00:24.30 (41.00675)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Discovery date: 2024-08-24 23:54:42.000 (JD=2460547.4963194)<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Potential host galaxy: M31<br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1"><br></span></div><div data-text-align="justify" class="imTAJustify"><span class="fs11lh1-5 ff1">Remarks: F. Castellani, Verona, Italy reports the discovery by <span class="cf1">Flavio Castellani, Vittorio Andreoli and Raffaele Belligoli</span>
819, in the course of the ISSP Italian Supernovae Search Project, of an apparent nova on a co-added 6000sec unfiltered images taken with a Moravian G4-9000 KAF CCD unfiltered, from Monte Baldo Observatory (Ferrara di Monte Baldo, Verona, Italy), with the 0.4m f.8 Ritchey-Chrétien telescope, obtained on 2024/08/24.927 UT. The new object is located at RA 00 43 00.01 DEC +41 00 24.3 (equinox 2000.0) Apparent magnitude about 17.1 in host Galaxy M31 Nothing is visible at this position on 2024/08/17.9291 as reference.<br></span></div><div><span class="fs11lh1-5 ff1">(<a href="https://www.wis-tns.org/object/2024ssq" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2024ssq', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">AT2024ssq</a>)</span></div><div><span class="fs11lh1-5 cf3"><br></span></div></div></div><div class="imTAJustify"><br></div><div class="imTAJustify"><div><span class="fs10lh1-5 ff1"><b>TCP J17490276-2324066 (=ASASSN 24fb) is a highly reddened nova, of the FeII class, caught close to maximum brightness</b></span></div><div class="imTAJustify"><span style="text-align: -webkit-center;" class="fs10lh1-5 ff1">ATel #16727;</span><span style="text-align: -webkit-center;" class="fs10lh1-5 ff1"> </span><span style="text-align: -webkit-center;" class="fs10lh1-5 ff1">U. Munari (INAF Padova), A. Farina (UniPD), A. Maitan, S. Dallaporta, <span class="cf1">V. Andreoli</span> (ANS Collaboration).</span></div><div><div class="imTAJustify">TCP J17490276-2324066 has been discovered by K. Itagaki on 2024 Juy 20.476 UT. It coincides with ASASSN 24fb discovered by the ASAS-SN survey on 2024 July 17.05 UT at a reported V=12.43 mag. Refined coordinates listed in CBAT-TOCP (averaging on end figures 02s.735, 05".5) coincides within 0.384 arcsec with a Gaia DR3 star of G=20.8 mag (no BP, RP listed).</div><div class="imTAJustify">We have obtained BVRI transformed photometry of the transient with ANS Collaboration telescopes ID 0310 and 2202, with the results listed in the table below. The local photometric sequence has been extracted from the APASS DR8 survey, and the quote errors include quadratically the transformation uncertainty from color equations.</div><div class="imTAJustify"><br></div><center class="imTALeft"><span class="fs9lh1-5 ff1">UT ID B V R I </span></center><center class="imTALeft"><span class="fs9lh1-5 ff1">July </span><span class="fs9lh1-5 ff1">2202</span><span class="fs9lh1-5 ff1"> </span><span class="fs9lh1-5 ff1">13.000 </span><span class="fs9lh1-5 ff1">11.315 </span><span class="fs9lh1-5 ff1">10.176 </span><span class="fs9lh1-5 ff1">9.059</span><span class="fs9lh1-5 ff1"> </span></center><center class="imTALeft"><span class="fs9lh1-5 ff1">20.855 </span><span class="fs9lh1-5 ff1"> </span><span class="fs9lh1-5 ff1">+/-0.013 </span><span class="fs9lh1-5 ff1">+/-0.011 </span><span class="fs9lh1-5 ff1">+/-0.019 </span><span class="fs9lh1-5 ff1">+/-0.011</span><span class="fs9lh1-5 ff1"> </span></center><center class="imTALeft"><span class="fs9lh1-5 ff1">July </span><span class="fs9lh1-5 ff1">0310 </span><span class="fs9lh1-5 ff1">12.958 </span><span class="fs9lh1-5 ff1">11.316 </span><span class="fs9lh1-5 ff1"> </span><span class="fs9lh1-5 ff1">10.197 </span><span class="fs9lh1-5 ff1"> </span><span class="fs9lh1-5 ff1">9.124</span><span class="fs9lh1-5 ff1"> </span></center><center class="imTALeft"><span class="fs9lh1-5 ff1">20.862 </span><span class="fs9lh1-5 ff1"> </span><span class="fs9lh1-5 ff1"> +/-0.013 </span><span class="fs9lh1-5 ff1">+/-0.010 </span><span class="fs9lh1-5 ff1"> +/-0.010</span><span class="fs9lh1-5 ff1"> +/-0.010</span><br></center><center class="imTALeft"><span class="fs9lh1-5 ff1"><br></span></center><div class="imTAJustify">Low resolution spectra (3600-8000 Ang, dispersion 2.31 Ang/pix) of TCP J17490276-2324066 have been recorded between July 20.851 and 20.909 UT with the Asiago 1.22m + B&C spectrograph. They are dominated by a very red continuum, in fine agreement with the V-J=+2.2 photometric color index in the table above, with superimposed broad emission lines of the Balmer series and FeII multiplets. The strongest FeII multiplets in emission are 55, 74, and 49 (all with P-Cyg absorption components), with multiplets 42 and 48 present at a significant lower intensity. No HeI lines are present and OI 7772 is present in
819weak emission and displays the strongest P-Cyg aborption of all, with a structurated profile, at an overall velocity -790 km/s and FWHM=560 km/s.</div><div class="imTAJustify">The Halpha has a FWHM=1560 km/s with a sharp P-Cyg absorption of FWHM=530 km/s placed on its blue wing at velocity of -625 km/s with respect to the emission component, which is rather Guassian in shape. The integrated absolute flux of the Halpha emission component is 9.12E-12 erg/cm2/s. The Halpha/Hbeta flux ratio is 8.8.</div><div class="imTAJustify">Overall, TCP J17490276-2324066 appears to be a classical nova, of the FeII type, caught close to maximum brightness, and suffering from a large reddening, possibly amounting to E(B-V)=1.5 mag as supported by the very strong interstellar atomic lines and diffuse interstellar bands, and the large Halpha/Hbeta ratio.</div></div><div class="imTAJustify"><div class="imTALeft"><span class="fs10lh1-5 ff1"><b><a href="https://www.astronomerstelegram.org/?read=16727" target="_blank" class="imCssLink">ATel #16727</a></b></span></div></div></div><div class="imTAJustify"><br></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>TCP J00003597+1757408 (2024/07/11)</b></span><br></div><div class="imTAJustify"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V and Castellani.</span>F report the classification of TCP J00003597+1757408. We obtained, From Monte Baldo Observatory (OMB) located in Novezzina (Italy), a low resolution spectra (7x600s), by 0.25-m telescope + Alpy600 spectrograph (dispersion 4.9 Ang/pix), on 2024-07-11.007 . The spectrum shows a blue continuum and absorption in H delta (4100 Ang) and H gamma (4340 Ang) while H beta (4861 Ang) and H alpha (6562.8 Ang) are not present in our spectrum, probably filled-up by a disk. All the characteristics are typical of CV stars. We propose the classification of TCP J00003597+1757408 as a CV star.</span></div><div class="imTAJustify"><div><span class="fs10lh1-5 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J00003597+1757408.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'http://www.cbat.eps.harvard.edu/unconf/followups/J00003597+1757408.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">TCP J00003597+1757408</a></span></div></div></div><div class="imTAJustify"><br></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>TCP J02055218+1440593 (2024/01/26)</b></span><br></div><div class="imTAJustify"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V and Castellani.F</span> reports a follow up of TCP J02055218+1440593. 6x300s (clear filter) images were obtained with the 0.4m telescope + Moravian G4 CCD full frame located at Osservatorio Monte Baldo in Novezzina (Italy), date 2024-01-26.875 (limit mag 19.3). A very weak object is present at coordinate 02:05:52.15 +14:40:59.5 in our image with an estimate magn. of 19.1. The luminosity is clearly decreased compared to that taken by XOSS our image can be found on</span><span class="fs10lh1-5 ff1"> <a href="https://photos.app.goo.gl/b1ZBhZffukQKMLiV8" target="_blank" class="imCssLink">https://photos.app.goo.gl/b1ZBhZffukQKMLiV8</a></span></div><div><span class="fs10lh1-5 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J02055218+1440593.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'http://www.cbat.eps.harvard.edu/unconf/followups/J02055218+1440593.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">TCP J02055218+1440593</a></span></div></div><div class="imTAJustify"><br></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>2024aru (2024/01/24)</b></span><br></div><div class="imTAJustify"><div style="text-align: start;"><span class="fs11lh1-5 ff2">TNS Classification Report No.</span><span class="fs11lh1-5 ff2"> </span><em class="fs10lh1-5"><span class="fs11lh1-5 ff2">16468</span></em></div></div><div class="imTAJustify"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><em><span class="cf1">Andreoli.V</span> , <span class="cf1">Castellani.F</span> and <span class="cf1">Vesentini.F</span></em> report/s a classification of object: <b><em>AT 2024aru</em></b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Type: <em>CV</em></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: <br></span></div><div class="imTAJustify"><em><span class="fs10lh1-5 ff1">Low resolution spectrum was obtained 0.25-m telescope + Alpy600 spectrograph (with dispersion 4.9 Ang/pix) located in Novezzina (Italy) on 2024-01-23.9375. The spectrum shows a blue continuum and a weak absorption of balmer lines expept Halpha (6562.8 Ang) that is no visible in our spectrum. B,V,R photometry was also collected with 0.4m telescope + Moravian G4 CCD full frame located in Novezzina (Italy) at 2024/01/23.9375 with results B=14.441, V=13.8
81966, R=14.278; (B-V) =0.575; (V-R)=-0.414. A probable progenitor was found on ZTF with mag r of 19.6 (mean mag) this means that Îmag â 5. All this feature are typically of a CV stars so we propose to classified TCPJ07593036+0459025 as a CV. The astrometric measurement was also made and giving the coordinates 07:59:30.33 +04:59:03.1 (the png of the spectrum is available on</span></em></div><div class="imTAJustify"><em><span class="fs10lh1-5 ff1"><a href="https://photos.app.goo.gl/erc165PHN48tW9pA6)" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://photos.app.goo.gl/erc165PHN48tW9pA6)', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">https://photos.app.goo.gl/erc165PHN48tW9pA6)</a></span></em></div><div class="imTAJustify"><i><span class="fs10lh1-5 ff1"><a href="https://www.wis-tns.org/object/2024aru" target="_blank" class="imCssLink">AT 2024aru</a></span></i></div></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2023</span></b><br></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div><span class="fs10lh1-5 ff1">TNS Astronomical Transient Report No. 194448</span></div></div><div class="imTAJustify"><div><span class="fs10lh1-5 ff1"><b>Discovery certificate for object 2023yij</b></span></div><div><span class="fs10lh1-5 ff1">IAU Designation: AT 2023yij</span><br></div><div><span class="fs10lh1-5 ff1">Discoverer internal name: OMB-PNV21</span></div><div><span class="fs10lh1-5 ff1">Coordinates (J2000): RA = 00:42:45.870 (10.691125) DEC = +41:21:37.90 (41.360528)</span></div><div><span class="fs10lh1-5 ff1">Discovery date: 2023-11-23 19:11:12.000 </span></div><div><span class="fs10lh1-5 ff1">Potential host galaxy: M31. </span><span class="fs10lh1-5 ff1">Host redshift: -0.001</span></div><div><span class="fs10lh1-5 ff1">Flavio Castellani report the discovery by <span class="cf1">F.Castellani, R.Belligoli,and V.Andreoli</span> of a PNV (Mag. 19.1R +-0.2 â USNOA2 catalogue) in the host galaxy M31 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Italian Supernovae Search Project using a 0.40m f/8 Ritchey-Chretien telescope (+ Moravian G4-9000 KAF CCD unfiltered CCD camera). No stellar source is visible at the position of the transient in our past images including reference image dated 2023-11-22 19:05:27 </span><span class="fs10lh1-5">(</span><span class="fs10lh1-5"><a href=" https://www.wis-tns.org/object/2023yij" target="_blank" class="imCssLink">AT2023yij</a></span><span class="fs10lh1-5">)</span></div><div><span class="fs10lh1-5"><br></span></div><div><div><span class="fs10lh1-5 ff1"><b>AT2023ylu TCP J20315286+2740166 </b></span></div></div><div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V</span> ; Ochner.P :<span class="cf1"> Castellani.F</span>, Cazzola.R reports a spectroscopic classification of TCP J20315286+2740166. Low resolution spectra was obteined by 1.22-m tlescope + B&C spectrograph (with dispersion 2.25 Ang/pix) located in Asiago (Italy) on 2023-11-12.788 and with 0.25-m tlescope + Alpy600 spectrograph (with dispersion 4.9 Ang/pix) located in Novezzina (Italy) on 2023-11-12.823, the spectra show emission of Halpha (6562.8 Ang) and [O I] (5577 Ang), absorption of Hbeta, Hdelta, Hgamma, Hepsilon and He I (4471 Ang) and has a blue continuum. Considered d=0.406 kpc from the 3D dust mapping (Green et al 2019) get E(B-V)â0.00 B,V,R photometry was also collected with 0.4m telescope + Moravian G4 CCD full frame located in Novezzina (Italy) at 2023/11/12.788 with results B=13.961, V=13.466, R= 13.036 , (B-V)0 =0.495 . Gaia DR2 1857057959447151616 is also present in ZTF database at magnitude 17.9 (filter zg) thatâs means Îmag â 5 mag (referring to the magnitude of discovery) All this feature are typically of a dwarf nova outburst, so a classification as dwarf nova was proposed. </span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">(<a href="http://www.cbat.eps.harvard.edu/unconf/followups/J20315286+2740166.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'http://www.cbat.eps.harvard.edu/unconf/followups/J20315286+2740166.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">TCP J20315286+2740166</a>) </span><span class="fs10lh1-5">(</span><span class="fs10lh1-5"><a href="https://www.wis-tns.org/object/2023ylu" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2023ylu', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">AT2023ylu</a></span><span class="fs10lh1-5">)</span></div><div class="imTAJustify"><br></div><div class="imTAJustify"><b class="ff1">TCP J06333486-2305449</b></div></div><div><div><span class="fs10lh1-5 ff1">Transient Object Followup Reports</span></div></div><div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V</span>, Vagnozzi.A, <span class="cf1">Castellani.F</span> and Ochner.P obtained low resolution spectrum at 2023/11/02.022 with 0.5m telescope + MARK III spectrograph (resolution 2.74 Ang/pix ,self-build) located in Stroncone (Italy), Hight resolution spectrum with 1.22m telescope + B&C spectrograph (resolution 0.6 Ang/pix) at 2023/11/01.118 and 2023/11/4.132. Spectra shows a blue continuum, no evidence of Hα (6562.8 Ang) probably f
819illed by accretion disk the other Balmer absorptions are presents. Hβ shows an FWHM of 2639 km/s . Also emission of O I (5577 Ang) and He I (4922 Ang) are clearly present in the low resolution spectrum. Considered d=0.2876 kpc from the 3D dust mapping (Green et al 2019) get E(B-V)â0.005 B,V,I photometry was also collected with 0.25-m f/3.4 reflector + SBIG ST-10XME (T05 - iTelescope.NET) at 2023/11/02.358 with results B=12.879 ±0.047 , V=12.903 ± 0.033 and I= 12.953 ± 0.058 , (B-V)0 = -0.02 . Also considering the light curve reported by AAVSO which shows a "rapid" variation where 90 minutes pass between one maximum and the next within a slower decline. Gaia DR3 2924954955730613376 is also present in ZTF database at magnitude 19 (filter zr) thatâs means Îmag â 6.5 All this feature are compatible of WZ Sge stars so a classification as a dwarf nova WZ Sge type was proposed. (</span><span class="fs10lh1-5"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J06333486-2305449.html" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'http://www.cbat.eps.harvard.edu/unconf/followups/J06333486-2305449.html', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">TCP J06333486-2305449</a>)</span></div></div><div><br></div></div><div class="imTAJustify"><div style="text-align: start;"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>TNS Astronomical Transient Report No. 192558 </b></span></div><div class="imTAJustify"><div style="text-align: start;"><b><span class="fs10lh1-5 ff1">Discovery certificate for object 2023wnh</span></b></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">IAU Designation: AT 2023wnh</span><br></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Discoverer internal name: OMB-TNS01</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Coordinates (J2000): RA = 00:43:48.700 (10.952917) DEC = +41:32:43.90 (41.545528)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Discovery date: 2023-11-03 19:04:14.000 </span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Potential host galaxy: m31</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Transient observed By <span class="cf1">F.Castellani, R.Belligoli and V.Andreoli</span>, in the course of Italian Supernovae Search Project using a 0.40m f/8 Ritchey-Chretien telescope (+ Moravian G4-9000 KAF CCD unfiltered CCD camera). No stellar source is visible at the position of the transient in our past images including reference image dated 15Th sept 2023. The transient has been already detected by Zwicky Transient Facility as ZTF23abighaj. (<a href=" https://www.wis-tns.org/object/2023wnh" target="_blank" class="imCssLink">AT2023whn</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div></div></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Spectroscopic analysis of the binaries systems Epsilon Herculis and HIP107162</span></b><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V;Nogara.M3;Grazioli.M.G;Castellani.F;</span> Vagnozzi.A;</span><span class="fs10lh1-5 ff1"><span class="cf1">Penayo.M1;Moltomoli.S;Zampieri.G;Pomari.C</span></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: </span><span class="fs10lh1-5 ff1">During the 2022 internship involving a group of high school students at the Monte Baldo Astronomical Observatory </span><span class="fs10lh1-5 ff1">(hereafter referred to as OMB) in Ferrara di Monte Baldo, Verona, Italy, the two stellar systems</span><div><span class="fs10lh1-5 ff1">of HIP107162 and Eps Her were observed, and high and low-resolution spectroscopic analysis was conducted.</span></div><div><span class="fs10lh1-5 ff1">The construction of the radial velocity curve allowed for the determination of the binary systemsâ structure,</span></div><div><span class="fs10lh1-5 ff1">while the low-resolution spectra enabled the identification of present elements and consequently their spectral </span><span class="fs10lh1-5 ff1">classification. See more </span><span class="fs10lh1-5 ff1">(<a href="http://osservatoriomontebaldo.it/uploads/CBETOMB/20230608-ArticoloStage2022.pdf" target="_blank" class="imCssLink">20230608-ArticoloStage2022</a>)</span></div></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><div style="text-align: start;"><b><span class="fs10lh1-5 ff1">TNS Classification Report No.</span><span class="fs10lh1-5 ff1"> 14816</span></b></div><div style="text-align: start;"><span class="fs10lh1-5 ff1"><b>classification of object: </b></span><b class="fs10lh1-5 ff1">AT 2023gfj</b><br></div><div style="text-align: start;"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V</span> ; <span class="cf1">Castellani.F</span> reports the classification of object AT 2023gfj. We obtained, From Monte Baldo Observatory (OMB) located in Novezzina (Italy), low resolution spectra by 0.25-m telescope + Alpy600 spectrograph (dispersion 4.9 Ang/pix) on 2023-04-26.851 (4x300s), on 2023-04-27.828 (3x300s) and V (Jhonson) photometry with 0.4m telescope + Moravian G4 CCD full frame on 2023-04-27.828 . Photometry reduction give V mag 12.8. The spectra show red continuum and TiO molecular bands ( 4760, 4954 ,4956 ,5448 ,5450 ,5847 ,6149 ,6357 ,6714 ,7087 Ang) typically feature of M-type stars. V mag and spectral features are correspondent with the near star ROSS 619 that have a very high proper motion (1069 , -5094) mas/yr in module 5204 mas/yr. If we assume that ROSS 619 is 2023gfj then the distance from the coordinates reported on SIMBAD (Wenger.M et al, 2000) by the coordinates presented on the TNS N°175337 is 2.4â (144 arcsec) , this distance has been travelled in 27.67 years. This time scale is consistent with our hypothesis. We propose that the transient 2023gfj is ROSS 619 in the new position.</span></div></div><div style="text-align: start;"><div class="imTAJustify"><span class="fs10lh1-5 ff1">Details of the object and its spectra can be viewed here:</span><span class="fs11lh1-5 cf3 ff2"> </span><span class="imUl fs10lh1-5 cf4 ff1"><span><a href="https://www.wis-tns.org/object/2023gfj" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2023gfj', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">https://www.wis-tns.org/object/2023gfj</a></span></span></div><span class="fs10lh1-5 ff1">(<a href="https://www.wis-tns.org/object/2023gfj/classification-cert" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2023gfj/classification-cert', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">Classification-cert</a>) (<a href="https://www.wis-tns.org/object/2023gfj" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'https://www.wis-tns.org/object/2023gfj', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">AT2023gfj</a>)</span></div></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">TNS Classification Report No.</span></b><b><span class="fs10lh1-5 ff1">14539</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Classification of object: AT2023dez</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: </span><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V ; Castellani.F</span> report/s a classification of object: AT 2023dez. </span><span class="fs10lh1-5 ff1">Low resolution spectrum (6 X 600s) was obtained on 2023-03-17.802 from Osservatorio Monte Baldo located in Novezzina (Italy) by 0.25-m telescope + Alpy600 spectrograph (with dispersion 4.9 Ang/pix). The spectrum shows H-alpha emission (6562.8 Ang), a weak absorpion of H-beta (4861.03) problably f
819illed up by the accretion disk and strong absorpions of the other Balmer lines and He I (4471;4922;5876 Ang). It also shows interstellar NaI D1,D2 (5885,5890 Ang). These features belong to a type Be Herbig star. Furthermore the coordinates are coincident to LS I+56 76, object prensent in the Catalog of galactig OB stars (Reed 2003). We propose the identification for this transient as a Be star.</span></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">(<a href="https://www.wis-tns.org/object/2023dez/classification-cert" target="_blank" class="imCssLink">Classification-cert</a>) (<a href="https://www.wis-tns.org/object/2023dez" target="_blank" class="imCssLink">AT2023dez</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div><div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">T</span><span class="fs10lh1-5 ff1">NS Classification Report No.</span></b><b><span class="fs10lh1-5 ff1">14508</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Classification of object: AT2023cub</span></b></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: </span><span class="fs10lh1-5 ff1"><span class="cf1">Andreoli.V ; Castellani.F ; Vesentini.F</span> report/s a classification of object: AT 2023cub. </span><span class="fs10lh1-5 ff1">Low resolution spectrum (5 X 600s) was obtained by 0.25-m telescope + Alpy600 spectrograph (with dispersion 4.9 Ang/pix) located in Novezzina (Italy) on 2023-03-09.792. The spectrum shows red continuum and absorption of H-alpha (6562.825 Ang), H-Beta (4861.03 Ang), D1,D2 Na doublet (5885;5890 Ang) and Ca I (4302 Ang) ; also the coordinates are coincident to V*520Mon (MAXI J0655-013) and at these coordinates an hard X-ray was detected (Serino et al. ATel #15442). We propose the identification of the transient as a brightness of the X-ray variable. (<a href="https://www.wis-tns.org/object/2023cub/classification-cert" target="_blank" class="imCssLink">Classification-cert</a>) (<a href="https://www.wis-tns.org/object/2023cub" target="_blank" class="imCssLink">AT2023cub</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">T</span><span class="fs10lh1-5 ff1">NS Classification Report No.</span></b><b><span class="fs10lh1-5 ff1">14413</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Classification of object: AT2023bne</span></b><br></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: </span><span class="fs10lh1-5 ff1"><span class="cf1">Flavio Castellani, </span>Claudio Balcon <span class="cf1">and Vittorio Andreoli </span>reports: We obtained BVRI photometry of PNV J01345297+3047145 (AT 2023bne) with 0.4m telescope + Moravian G4 CCD full frame located in Novezzina (Italy), date 2023/02/11.7868 B=17.11 ; V=17.04 ; R=17.01 ; I=16.84 (Vphot AAVSO photometry tool). Color index B-V=0.07 is similar to cataclysmic variable (CV) Z Cam B-V=0.05 (Bruch 1984) at maximum. We also obtained two low resolution spectra (2x2400s , R=100) by 0.2m telescope on 2023-02-11.772 UT, the spectrum shows a blue continuum with no features above noise level. These characteristics are compatible with those of a CV in outburst. (<a href="https://www.wis-tns.org/object/2023bne/classification-cert" target="_blank" class="imCssLink">Classification-cert</a>) (<a href="https://www.wis-tns.org/object/2023bne" target="_blank" class="imCssLink">AT2023bne</a>)</span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">TNS Astronomical Transient Report No.</span></b><b><span class="fs10lh1-5 ff1">168720</span></b><b><span class="fs10lh1-5 ff1"> </span></b><b><span class="fs10lh1-5 ff1">Discovery certificate for object 2023ps</span></b><b><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks:</span><span class="fs10lh1-5 ff1"> </span><span class="fs10lh1-5 cf1 ff1">F.Castellani, </span><span class="fs10lh1-5 cf1 ff1">R.Belligoli</span><span class="fs10lh1-5 cf1 ff1">,</span><span class="fs10lh1-5 cf1 ff1"> </span><span class="fs10lh1-5 cf1 ff1">V.Andreoli, C.Marangoni</span><span class="fs10lh1-5 ff1">,</span></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">OMB extragalactic nova monitoring by ISSP collaboration reports the discovery of a probable nova in M31. The transient designated also <a href="http://www.cbat.eps.harvard.edu/unconf/followups/J00424623+4117357.html" target="_blank" class="imCssLink">PNV J00424623+4117357</a>. </span><span class="fs10lh1-5 ff1">New transient was clearly detected on '2023 1 14,7674' UT using 16 x 300s frames (4800s total) obtained by a Morav
819ian G4-9000 KAF unfiltered CCD with the 0.4m f.8 Ritchey-Chrétien telescope from Monte Baldo "A.Gelodi" Astronomic Observatory, località Novezzina, Ferrara di Monte Baldo, Verona, Italy. The discovery magnitude is 19.3±0.5 mag in the CV band (clear visual). Offset 25" Est e 90" Nord from M31 galactic centre. The new transient is close to Globular Cluster M31GC J004246+411737 (1.78"). (<a href="https://www.wis-tns.org/object/2023ps/discovery-cert" target="_blank" class="imCssLink">AT2023ps</a>)</span><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Spectroscopic Observation of the Dwarf Nova PNV J00215475+5231007</span></b><b><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks:</span><span class="fs10lh1-5 cf1 ff1">V.Andreoli, A.Vagnozzi</span><span class="fs10lh1-5 ff1">. </span><span class="fs10lh1-5 ff1">Also, weak absorption lines of Hα, Na I, and Mg II are seen. Therefore, my spectrum is consistent with the report on CBAT by <span class="cf1">V. Andreoli & A. Vagnozzi</span>, confirming their classification as a cataclysmic variable. According to the photometric observations by S. Kiyota, H. Itoh, and the Kyoto U team, this object is likely a WZ Sge-type dwarf nova (vsnet-alert 27305 & 27306).</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">(</span><span class="fs10lh1-5 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J00215475%2B5231007.html" target="_blank" class="imCssLink">PNV J00215475+5231007</a></span><span class="fs10lh1-5 ff1">; </span><span class="fs10lh1-5 ff1"><a href="https://www.astronomerstelegram.org/?read=15857" target="_blank" class="imCssLink">ATel #15857</a>)</span></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2</span><span class="fs10lh1-5 ff1">022</span></b><br></div><div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">TNS Astronomical Transient Report No.</span></b><b><span class="fs10lh1-5 ff1">154172</span></b><b><span class="fs10lh1-5 ff1"> </span></b><b><span class="fs10lh1-5 ff1">Discovery certificate for object 2022qpg</span></b><b><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks:</span><span class="fs10lh1-5 ff1"> </span><span class="fs10lh1-5 cf1 ff1">R.Belligoli, </span><span class="fs10lh1-5 cf1 ff1">F.Castellani,</span><span class="fs10lh1-5 cf1 ff1"> </span><span class="fs10lh1-5 cf1 ff1">V.Andreoli, C.Marangoni</span><span class="fs10lh1-5 ff1">, OMB extragalactic nova monitoring with ISSP collaboration, reports the discovery of a probable nova in M31. </span><span class="fs10lh1-5 ff1">Offset 1091E 425N. </span><span class="fs10lh1-5 ff1">It should be noted that in the same position a optical transient TSS J004420.7 + 412311 was reported ATel #627; R. Quimby, M. Sellers, P. Hoeflich, J. C. Wheeler (University of Texas), and C. Gerardy (Imperial College) on 12 Oct 2005; 19:30 UT. </span><span class="fs10lh1-5 ff1">The transient designated also </span><span class="fs10lh1-5 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J00442079+4123111.html" target="_blank" class="imCssLink">PNV J00442079+4123111</a></span><span class="fs10lh1-5 ff1">;</span><span class="fs10lh1-5 ff1"> <a href="https://www.wis-tns.org/object/2022qpg" target="_blank" class="imCssLink">AT2022qpg</a></span></div></div><div class="imTAJustify"><b class="fs10lh1-5"><span class="fs10lh1-5 ff1"><br></span></b></div><div><div class="imTAJustify"><b class="fs10lh1-5"><span class="fs10lh1-5"><span class="fs10lh1-5 ff1">A new outburst of the symbiotic star V919 Sgr, again 15 yrs past the previous one</span></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #15528; U. Munari (INAF Padova), A. Vagnozzi, A. Maitan, <span class="cf1">F. Castellani</span>, M. Graziani (ANS Collaboration), P. Ochner, A. Reguitti (Padova Univ.) </span><span class="fs10lh1-5 ff1">on 25 Jul 2022; 15:44</span></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">V919 Sgr is a bright symbiotic star, of the burning type, which is largely ignored by observers. Its first known outburst in 1991-92 was described by Ivison et al. (1993, A&A 277, 510), with a second one in 2007 reported by Munari et al. (2007, CBET 999). V919 Sgr is currently again in outburst, as also noted by B. Monard in vsnet-alert N. 26878. The three recorded outburst are separated by similar ~15 yrs intervals. (<a href="https://www.astronomerstelegram.org/?read=15528" target="_blank" class="imCssLink">ATel15528</a>)(<a href="files/77.ATel15528_V919_Sgr.pdf" target="_blank" class="imCssLink">PDF</a>)</span><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b class="fs10lh1-5"><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">TNS Astronomical Transient Report No. 140016 </span></b><b class="fs10lh1-5"><span class="fs10lh1-5 ff1">Discovery certificate for object 2022eqj</span></b><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: <span class="cf1">F.Castellani, R.Belligoli, V.Andreoli, C.Marangoni</span>, OMB extragalactic nova monitoring with ISSP collaboration, reports the discovery of a probable nova in M31. The coordinates of the new transient are only 0.5 arc/sec from Nova Bryan 1990A/M31N2007-07a The transient designated also <a href="http://www.cbat.eps.harvard.edu/unconf/followups/J00430406+4117080.html" target="_blank" class="imCssLink">PNV J00430406+4117080</a> ; <a href="https://www.wis-tns.org/object/2022eqj/discovery-cert" target="_blank" class="imCssLink">AT2022eqj</a></span><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">TNS Astronomical Transient Report No. 139430</span></b><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Discovery certificate for object 2022elz</span></b><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Remarks: Flavio Castellani report the discovery by <span class="cf1">F.Castellani, R.Belligoli, V.Andreoli</span> of a PNV (Mag.19.5R +-0.2 - USNOB1 catalogue) in the host galaxy M81 at Monte Baldo Observatory, Ferrara di Monte Baldo, Verona, Italy (A99), in the course of Ital
819ian Supernovae Search Project using a 0.40m f/8 Ritchey-Chretien telescope (+ Moravian G4-9000 KAF CCD unfiltered CCD camera). No stellar source is visible at the position of the transient in our past images including reference image dated 02 March 2022. </span><span class="fs10lh1-5 ff1"><a href="http://www.cbat.eps.harvard.edu/unconf/followups/J09552559+6907558.html" target="_blank" class="imCssLink">PNV J09552559+6907558</a></span><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><a href="https://www.wis-tns.org/object/2022elz/discovery-cert" target="_blank" class="imCssLink">AT2022elz</a></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"> </span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2021</span></b></div><div><div class="imTAJustify"><b class="fs10lh1-5"><span class="fs10lh1-5 ff1">Nova TCP J20210770+2914093 turns into an FeII-type as it keeps rising in brightness</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #14816; U. Munari (INAF Padova), S. Moretti, A. Maitan, <span class="cf1">V. Andreoli </span>(ANS Collaboration)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The transient TCP J20210770+2914093 was discovered by K. Itagaki on 2021 Jul 16.492 UT at unfiltered magnitude 12.0, and classified as a nova by Munari et al. (ATel #14793) based on a spectrum taken on July 17.102 UT.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">This initial spectrum resembled novae of the He/N type, with Balmer, HeI, and NII lines present in emission. However, Munari et al. (ATel #14793) warned that with the nova possibly still progressing toward maximum light, the spectral type could evolve toward the FeII type. This has been indeed what happened and here we report about the evolution of the nova during the last two weeks.</span></div></div><div><div class="imTAJustify"><span class="fs10lh1-5 ff1">(</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="https://www.astronomerstelegram.org/?read=14816" target="_blank" class="imCssLink">ATel14816</a></span></span><span class="fs10lh1-5 ff1">) (</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="files/76.ATel14816_-Nova-TCP-J20210770-2914093.pdf" target="_blank" class="imCssLink">PDF</a></span></span><span class="fs10lh1-5 ff1">)</span></div></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Spectroscopic follow-up observations of Nova Herculis 2021</span></b><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #14718; I. Albanese, A. Farina, <span class="cf1">V. Andreoli</span>, P. Ochner (UniPd), A. Reguitti (UNAB)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">We report spectroscopic follow-up observations of Nova Herculis 2021 (TCP J18573095+1653396). It was discovered by Seiji Ueda on 2021-06-12.548 UT and spectroscopically classified as a classical nova by Munari et al. 2021 (ATel #14704). We obtained a low-resolution spectrum with Monte Baldo Observatory 0.25-m Telescope + Alpy 600 spectrograph (380-800 nm, 0.497 nm/px) on 12/06/2021 and 13/06/2021, and a medium resolution spectrum with Asiago 1.22-m 'Galileo' telescope + B&C spectrograph (460-700 nm, resolution 0.25 nm) on 13/06/2021. </span><span class="fs10lh1-5 ff1">(</span><span class="fs10lh1-5 ff1"><a href="https://www.astronomerstelegram.org/?read=14718" target="_blank" class="imCssLink">ATel14718</a></span><span class="fs10lh1-5 ff1">) (</span><span class="fs10lh1-5 ff1"><a href="files/75.ATel14718_-SpectroscopicNova-Herculis2021.pdf" target="_blank" class="imCssLink">PDF</a></span><span class="fs10lh1-5 ff1">)</span><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div><div class="imTAJustify"><b class="fs10lh1-5"><span class="fs10lh1-5 ff1">Photometry and spectroscopy of the 2021 outburst of the symbiotic star YY Her</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #14464; U. Munari (INAF Padova), P. Ochner (Univ. Padova), S. Dallaporta, G. L. Righetti, M. Graziani, <span class="cf1">F. Castellani</span>, A. Maitan, S. Moretti, (ANS Collaboration), and N. Masetti (INAF Bologna)</span></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The symbiotic star YY Her has just been announced in outburst (ATel #14458), based on unfiltered telephoto lens images taken on March 15.006 UT during the New Milky Way survey for transients. (<a href="http://www.astronomerstelegram.org/?read=14464" target="_blank" class="imCssLink">ATel14464</a>) (<a href="files/74.ATel14464_-2021_YY-Her.pdf" target="_blank" class="imCssLink">PDF</a>)</span><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2020</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Nova Cas 2020 (=V1391 Cas) is likely forming dust</span></b><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF Padova), D. P.K. Banerjee (PRL, India), <span class="cf1">F. Castellani</span>, S. Dallaporta, A. Maitan, and A. Vagnozzi (ANS Collaboration)</span><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The brightness of the nova has dramatically dropped over the last couple of days with a marked reddening of colors. The presence of a faint and nearby field star, just a few arcsec away from the nova, now requires that the photometry be performed via PSF- fitting. The night values, averaged over PSF-fitting measurements from data that we collected with ANS Collaboration telescopes...(<a href="http://www.astronomerstelegram.org/?read=14267" target="_blank" class="imCssLink">Atel14267</a>) (<a href="files/72.ATel14267_-NovaCas2020-V1391Cas.pdf" target="_blank" class="imCssLink">PDF</a>)</span><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Classification of TCP J04291884+4354232 as a classical nova </b></span><span class="fs10lh1-5 ff1">U. Munari (INAF Padova), <span class="cf1">F. Castellani</span>, S. Dallaporta, <span class="cf1">V. Andreoli</span> (ANS Collaboration)</span><span class="fs10lh1-5 ff1"><b><br></b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">We have obtained low-resolution spectroscopy of the transient TCP J04291884+4354232 with a 25cm telescope + Alpy600 on Nov 26.05 UT. The spectrum shows broad Balmer emission lines with deep P-Cyg as typical of a nova close to maximum brightness. (<a href="http://www.astronomerstelegram.org/?read=14224" target="_blank" class="imCssLink">Atel14224</a>) (<a href="files/70.ATel14224_-Classification_TC-J04291884_4354232.pdf" onclick="return x5engine.imShowBox({ media:[{type: 'iframe', url: 'files/70.ATel14224_-Classification_TC-J04291884_4354232.pdf', width: 1920, height: 1080, description: ''}]}, 0, this);" class="imCssLink">PDF</a>)</span><span class="fs10lh1-5 ff1"><b><br></b></span></div><div class="imTAJustify"><br></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Spectroscopic confirmation and photometry of the recent nova M31 2020-11c (<span class="cf1">AT 2020yye</span>) (= <span class="cf1">OMB-PNV12</span>) (= PNV J00431316+4124562)</b></span><span class="fs10lh1-5 ff1"> </span><span class="fs10lh1-5 ff1">S. Fabrika, O. Sholukhova, A. Sarkisyan, A, Vinokurov, Yu. Solovyeva (SAO RAS), A. W. Shafter (SDSU), A. Valeev (SAO RAS)<br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">We report optical spectroscopic confirmation of the nova <span class="cf1">M31 2020-11c (PNV J00431313+4124567) announced in <a href="http://www.astronomerstelegram.org/?read=14155" target="_blank" class="imCssLink">ATel #14155</a>. </span>(<a href="http://www.astronomerstelegram.org/?read=14217" target="_blank" class="imCssLink">Atel14217</a>) (<a href="files/71.ATel14217_-SpectroscopicconfirmationAT-2020yye.pdf" target="_blank" class="imCssLink">PDF</a>)</span><span class="fs10lh1-5"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>The optical counterpart of the X-ray source 2SXPS J173508.4-292958 is a new, yellow-type symbiotic star. </b>U. Munari (INAF Padova), P. Valisa, S. Dallaporta, A. Vagnozzi,<span class="cf1"> V. Andreoli, F. Castellani </span>(ANS Collaboration)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">With an assortment of telescopes operated by ANS Collaboration, we have obtained optical spectroscopy (low and high resolution) and BVRI photometry of the optical counterpart of 2SXPS J173508.4-292958, the source recently reported by Heinke et al. (ATel #13648) to have brightened in the X-rays. (<a href="http://www.astronomerstelegram.org/?read=13660" target="_blank" class="imCssLink">Atel</a><span style="text-align: -webkit-center;"><a href="http://www.astronomerstelegram.org/?read=13660" target="_blank" class="imCssLink">13660</a>) (<a href="files/69.ATel13660_-The-optical-counterpart-of-the-X-ray.pdf" target="_blank" class="imCssLink">PDF</a>)</span></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>LAMOST J202629.80+423652.0 is not a symbiotic star - </b><span class="cf1">V. Andreoli</span> and U. Munari <b>Abstract.</b> LAMOST J202629.80+423652.0 has been recently classi�ed as a new symbiotic star containing a long-period Mira, surrounded by dust (D- type) and displaying in the optical spectra high ionization emission lines, in- cluding the Raman-scattered OVI at 6825 �A. We have observed LAMOST J202629.80+423652.0 photometrically in the BVRI bands and spectroscopically over the 3500-8000 A range. (<a href="CAOSP Vol.50" target="_blank" class="imCssLink">CAOSP Vol.50</a>) (<a href="files/68.Andreoli_pp672-680.pdf" target="_blank" class="imCssLink">PDF</a>)</span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">
819The OMB-supernova monitoring (ISSP collaboration), <span class="cf1">R.Belligoli, F.Castellani, C.Marangoni, F.Marziali </span><b>reports the discovery of a PSN J16393220+6602141 SN2020gpe in NGC6214 </b>by a Moravian G4-9000 KAF unfiltered CCD frames taken on '2020-04-12T03:21:49' UT on the 0.4m f.8 Ritchey-Chrétien telescope. The object observed is located at RA= '16 39 32.19' DEC= '+66 02 14.01' (equinox 2000.0) Offset 2"W 9"S from the center of NGC6214 galaxy (see link to discovery image below). Apparent magnitude 17.0 Clear (err +/- 0,5). (<a href="http://www.astronomerstelegram.org/?read=13640" target="_blank" class="imCssLink">Atel13640</a>) (<a href="files/67.ATel13640_SN-2020gpe.pdf" target="_blank" class="imCssLink">PDF</a>)<b><br></b></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1"><br></span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>We report the independent discovery of a probable nova in M31 on a co-added 810-s R-band CCD </b><b>frame taken on 2020 Mar. 15.768 UT with the 0.65-m telescope at Ondrejov.</b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The object was independently discovered and first announced <span class="cf1">by F. Castellani and R. Belligoli</span> <span class="cf1">and designated as PNV J00424612+4111362 = AT 2020emi</span>. The object was designated by us as M31N 2020-03c and is located at R.A. = 0h42m52s.16, Decl. = +41o13'37".2 (equinox 2000.0), which is 88.4" east and 151.3" south of the center of M31 ... (<a href="http://www.astronomerstelegram.org/?read=13561" target="_blank" class="imCssLink">ATel_13561</a>) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/66.ATel13561_AT2020emi_novaM31.pdf" target="_blank" class="imCssLink">PDF</a>)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Remarks: F. Castellani, Verona, Italy reports the discovery <span class="cf1">by Flavio Castellani, Raffaele Belligoli and Claudio Marangoni</span>, in the course of the ISSP Italian Supernovae Search Project,</b> of an apparent nova in two images taken with a Moravian G4-9000 KAF CCD unfiltered, from Monte Baldo Observatory (Ferrara di Monte Baldo, Verona, Italy), with the 0.4m f.8 Ritchey-Chrétien telescope, obtained on 2020 March 04.7596. The new object is located at RA 00 42 08.56 DEC +41 26 00.8 (equinox 2000.0) Apparent magnitude about 18.0 in host Galaxy M31 Nothing is visible at this position on the reference image taken on 2020-02-28.769... (<a href="https://wis-tns.weizmann.ac.il/object/2020dzr/discovery-cert" target="_blank" class="imCssLink">TNS Astronomical Transient Report No. 63512</a>)<b><br></b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2019</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>The 2018 eruption and long-term evolution of the new high-mass Herbig </b><b>Ae/Be object Gaia-18azl = VES 263</b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">MNRAS U. Munari, V. Joshi, D. P. K. Banerjee, K. Cotar, S. Y. Shugarov, R. Jurdana-Sepi, <span class="cf1">R. Belligoli</span>, A. Bergamini, M. Graziani, G. L. Righetti, A. Vagnozzi and P. Valisa</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">We have been monitoring, at high cadence, the photometric and spectroscopic evolution of VES 263 following the discovery in 2018 of a brightening labelled as event Gaia-18azl.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">VES 263 is so far a neglected emission-line object discovered in the 1960s on objective prism plates, tentatively classified as a semiregular AGB cool giant by automated analysis of ASASSN light curves. We have discovered that VES 263 is a bona fide massive pre-mainsequence object (â¼12 M), of the Herbig AeBe type. (<a href="https://academic.oup.com/mnras/article-abstract/488/4/5536/5541072?redirectedFrom=fulltext" target="_blank" class="imCssLink">MNRAS 488, 5536â5550</a> (2019) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/65.MNRAS-20190821-VES263.pdf" target="_blank" class="imCssLink">PDF</a>)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2018</span></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Liverpool Telescope classification of optical transients AT2018hho and AT2018hhy</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #12138; S. C. Williams (Lancaster), M. J. Darnley (LJMU), M. W. Healy (LJMU) on 22 Oct 2018; 22:36 UT Credential Certification: Steven Williams ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">
819A faint continuum is detected in each case, but the S/N is too low for a classification. <span class="cf1">AT2018hho</span> was observed at 2018-10-16.94 UT. We detect a Hα emission line with FWHM ~ 3100 km/s. We obtained a spectrum of AT2018hhy at 2018-10-17.99 UT, which shows TiO absorption bands on a red continuum, indicating that this object is a red LPV. We also note that there is a variable coincident with the position of AT2018hhy in Macri et al. (2001) and Hartman et al. (2006). (<a href="http://www.astronomerstelegram.org/?read=12138" target="_blank" class="imCssLink">Atel_12138</a>) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/64.ATel12138_%20Liverpool_AT2018hho_At2018hhy.pdf" target="_blank" class="imCssLink">PDF</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Independent INT/WFC discovery, improved position and IAC80/CAMELOT photometry of AT2018hho (= PNV J00424012+4117273) in M31</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #12127; Credential Certification: Ismael Perez-Fournon ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">We report the independent discovery of a nova candidate in M31 on CCD images taken from 2018 Oct 13.937 to 2018 Oct 14.176 with the Wide Field Camera of the Isaac Newton Telescope. The discovery of this nova candidate was reported to TNS by<span class="cf1"> </span><span class="cf1">Raffaele Belligoli, Flavio Castellani and Claudio Marangoni.</span> We also observed AT2018hho with the CAMELOT CCD camera of the IAC80 telescope at Teide Observatory in Tenerife on the same night. (<a href="http://www.astronomerstelegram.org/?read=12127" target="_blank" class="imCssLink">Atel_12127</a>) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/63.ATel12127_%20Fotometria%20AT2018hho%20in%20M31.pdf" target="_blank" class="imCssLink">PDF</a>)<br></span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Independent Discovery of PNV J00424012+4117273 and Confirmation of PNV J01334673+3032181</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #12113; K. Hornoch (Astronomical Institute, Ondrejov, Czech Republic) on 15 Oct 2018; 07:55 UT Credential Certification: Matt Darnley ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">I report the independent discovery of a probable nova in M31 on a co-added 770-s R-band CCD frame taken on 2018 Oct. 14.740 UT with the 0.65-m telescope at Ondrejov.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The object was independently discovered by <span class="cf1">R. Belligoli et al.</span> (designated as PNV J00424012+4117273 = AT2018hfs) and is located at R.A. = 0h42m40s.11, Decl. = +41o17'26".9 (equinox 2000.0), which is 47.5" west and 78.4" north of the center of M31. (<a href="http://www.astronomerstelegram.org/?read=12113" target="_blank" class="imCssLink">Atel_12113</a>) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/62.ATel12113_%20AT2018hho_At2018hhy.pdf" target="_blank" class="imCssLink">PDF</a>)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">The Mass Accretion Rate of the Young Variable Star GM Cep</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Authors: </b>Giannini, T.; Munari, U.; Lorenzetti, D.; Antoniucci, S.; <span class="cf1">Castellani, F.</span>; Dallaporta, D.; Jurdana-Å epiÄ, R.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Affiliation: </b>AA(INAFâOsservatorio Astronomico di RomaâVia Frascati, 33âMonte Porzio Catone I-00078, Italy <id system="ORCID">0000-0002-0224-096X</id>), AB(INAFâOsservatorio Astronomico di Padovaâvia dellOsservatorio 8, Asiago (VI) I-36012, Italy <id system="ORCID">0000-0001-6805-9664</id>), AC(INAFâOsservatorio Astronomico di RomaâVia Frascati, 33âMonte Porzio Catone I-00078, Italy <id system="ORCID">0000-0001-6415-4162</id>), AD(INAFâOsservatorio Astronomico di RomaâVia Frascati, 33âMonte Porzio Catone I-00078, Italy <id system="ORCID">0000-0002-0666-3847</id>), AE(ANS Collaboration, Astronomical Observatory, I-36012, Asiago (VI), Italy), AF(ANS Collaboration, Astronomical Observatory, I-36012, Asiago (VI), Italy), AG(Physics Department, University of Rijeka, Radmile MatÄicË, 51000 Rijeka, Croatia) <b>Publication: </b>Research Notes of the American Astronomical Society, Volume 2, Issue 3, article id. 124, <numpages>0</numpages> pp. (2018). <b>Publication Date: </b>07/2018</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><a href="https://iopscience.iop.org/article/10.3847/2515-5172/aad244/meta" target="_blank" class="imCssLink">Electronic On-line Article</a> (HTML) - (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/61.The%20Mass%20Accretion%20Rate%20of%20the%20Young%20Variable%20Star%20GM%20Cep%20-%20IOPscience.pdf" target="_blank" class="imCssLink">PDF</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>
819The super-soft X-ray and CH/Ba-enhanced symbiotic star StHa 32 is in outburst</b><b><br></b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ATel #11304; U. Munari (INAF Padova), S. Dallaporta, M. Graziani, G. L. Righetti, S. Tomaselli, S. Moretti, A. Maitan,<span class="cf1"> </span><span class="cf1">F. Castellani,</span> P. Valisa, L. Baldinelli (ANS Collaboration) on 15 Feb 2018; 11:12 UT Credential Certification: U. Munari ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The supersoft X-ray source, Barium-enhanced, metal-deficient and Halo symbiotic star StHa 32 in going into outburst, the first ever recorded to the best of our knowledge.(<a href="http://www.astronomerstelegram.org/?read=11304" target="_blank" class="imCssLink">ATel_11304</a>)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Asiago spectroscopic classification of 3 transients</b><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The Asiago Transient Classification Program (Tomasella et al. 2014, AN, 335, 841) reports the <span class="cf1">spectroscopic classification of AT 2018eq discovered by R. Belligoli (ISSP)</span> <span class="cf1">in the direction of M31</span>; PS18bq (AT2018bi) discovered by J. Grzegorzek and Pan-STARRS1 in UGC1791; and AT2018C (= Gaia18aak), a blue hostless transient discovered by Gaia.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The observations were performed with the Asiago 1.82 m Copernico Telescope equipped with AFOSC (range 340-820 nm; resolution 1.4 nm).(ATel_11168)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2017</span></b></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>Spectroscopic classification AT 2017jdm as a nova, and likely recurrent eruption of M31N 2007-10b</b><b><br></b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">We obtained a spectrum of the transient <span class="cf1">AT 2017jdm (discovered by F. Castellani, R. Belligoli, C. Marangoni and F. Marziali;</span><span class="cf1"> <a href="https://wis-tns.weizmann.ac.il/object/2017jdm" target="_blank" class="imCssLink">see TNS</a></span><span class="cf1">)</span> with the SPRAT spectrograph (resolution R ~ 350; Piascik et al. 2014) on the 2-m Liverpool Telescope (Steele et al. 2004) on 2017 Dec 24.86 UT. (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/55.ATel 11088_ Spectroscopic_classification_AT2017jdm.pdf" target="_blank" class="imCssLink">Atel_11088</a>)<b><br></b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">A sudden brightness decrease of the young pre-MS object GM Cep</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF - Osservatorio Astronomico di Padova, Italy), <span class="cf1">F. Castellani</span> (ANS Collaboration, Italy), T. Giannini, S. Antoniucci, D. Lorenzetti (INAF - Osservatorio Astronomico di Roma, Monte Porzio, Italy) on 24 Nov 2017; 14:38 UT Credential Certification: Simone Antoniucci ([email protected]) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/54.2017ATel-11004-A%20sudden%20brightness%20decrease%20of%20the%20young%20pre-MS%20object%20GM%20Cep.pdf" target="_blank" class="imCssLink">Atel_11004</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">Nova ASASSN-17hx fast returning to maximum brightness, now at much larger velocities</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF Padova), P. Ochner (Univ. Padova), F.-J. Hambsch, A. Frigo, <span class="cf1">F. Castellani</span>, A. Milani, P. Valisa, A. Vagnozzi (ANS Collaboration)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">on 11 Sep 2017; 21:54 UT Credential Certification: U. Munari ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Nova ASASSN-17hx continues its unexpected and rapid re-brightening (ATel #10725), approaching the brightness attained at primary maximum when it peaked at B=9.65, V=8.44, R=7.79, I=7.05 around July 3
8190.1 UT (ATel #10641)... (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/58.ATel10736_%20Nova%20ASASSN-17hx%20fast%20returning.pdf" target="_blank" class="imCssLink">ATel_10736</a>)<br></span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>"Photometry and spectroscopy of declining Nova ASASSN-17hx, now passing </b><b>at t_2"</b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF Padova), G. Traven (Univ. Ljubljana), F.-J. Hambsch, <span class="cf1">F. Castellani</span>, A. Frigo, A. Milani, P. Valisa (ANS Collaboration), P. Ochner (Univ. Padova)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">ASASSN-17hx was discovered (Atel #10524) when still >4 mag below and ~41 days before maximum. Spectral classification and pre-maximum evolution have been reported (Atel #10527, #10558, #10572, #10613), as well as the identification in the VVVX survey of a Ks=16.7 mag star as the likely progenitor of the nova, and recently UV observations and an upper limit to X-ray flux obtained with Swift (Atel 10636) (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/53.2017ATel10641_%20ASASSN-17hx.pdf" target="_blank" class="imCssLink">ATel_10641</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>"Photometry and spectroscopy of FeII nova ASASSN-17hx, </b><b>finally passing through maximum"</b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF Padova), F.-J. Hambsch, A. Frigo, <span class="cf1">F. Castellani</span><span class="cf1"> </span>(ANS Collaboration),G. La Mura (Univ. Padova), G. Traven (Univ. Ljubljana), M. Ozbey Arabaci, T. Saguner (Ataturk Univ.) on 13 Jul 2017; 10:08 UT Credential Certification: U. Munari ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">More than two weeks past its discovery, nova ASASSN-17hx has finally reached what appears to be its peak optical brightness. Announced as a candidate nova on June 23.7 UT (ATel #10523), we begun daily photometric monitoring of ASASSN-17hx on June 24.07 UT when we measured V=12.39, B-V=+0.72, V-I=+1.19. After a monotonic - although structured - rise toward maximum, peak brightness has been reached at V=10.90, B-V=+0.85 on June 10, followed by a slow decline. (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/52.ATel10572_%20PhotometrySpectroscopyASASSN-17hx.pdf" target="_blank" class="imCssLink">ATel_10572</a>)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b class="fs10lh1-5 ff1">After 23 years the yellow symbiotic star LT Del is again in outburst</b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF Padova), P. Ochner (Univ. Padova), S. Dallaporta and <span class="cf1">R.</span><span class="cf1">Belligoli</span> (ANS Collaboration)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The ANS Collaboration photometric and spectroscopic monitoring of symbiotic stars has detected LT Del (= Hen 2467 = PK 06312.1 = StHa 179) in outburst. This is the first recorded outburst since the last one of 19941995, which was discovered by Passuello et al. (1994, IAUC 6065 ) and described by Arkhipova et al. (1995a, ALett 21, 339; 1995b, ALett 21, 391). LT Del is steeply rising in brightness. Last ANS photometric observation on UT (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/51.ATel10361_%20LTDeloutburst.pdf" target="_blank" class="imCssLink">ATel 10361</a>)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>NOVA </b><b>2017-04b (= PNV J09551279+6900093) </b><b>IN M81</b></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The extended M81 nova monitoring collaboration reports the discovery of a probable nova in M81 on pair of co-added 3900-s and 4200-s unfiltered CCD frames taken on 2017 Apr. 18.799 UT and 18.848 UT, respectively with the 0.4-m telescope at the <span class="cf1">Monte Baldo Observatory, Verona, Italy</span> (MBO). The object designated PNV J09551279+6900093 is located at R.A. = 9h55m12s.79, Decl. = +69o00'09".3 (equinox 2000.0), which is 109.4" west and 225.8" south of the center of M81 (see link to discovery image below). (<a href="http://www.osservatoriomontebaldo.it/blog/?id=86h62tjn" target="_blank" class="imCssLink">see link to discovery image</a>). <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/50.2017ATel_NovaM81.pdf" target="_blank" class="imCssLink">Atel#10290</a></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">NOVA AT2017blf in M81</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The M81 nova monitoring collaboration reports the independent discovery of an apparent nova in M81 on a coadded 3510s unfiltered CCD frame taken on 2017 Feb. 24.119 UT with the 0.65m telescope at Ondrejov.The object designated PNV J09563149+6907301 was first announced and designated AT2017blf <span class="cf1">by</span><span class="cf1"> </span><span class="cf1">F. Castellani et al.</span><span class="cf1"> </span>(<a href="https://wis-tns.weizmann.ac.il/object/2017blf" target="_blank" class="imCssLink">see here</a>) and is located at R.A. = 9h56m31s.49, Decl. = +69o07'30".1 (equinox 2000.0), which is 312.1" east and 215.0" north of the center of M81 (<a href="http://www.osservatoriomontebaldo.it/blog/?id=wxcdrq6y" target="_blank" class="imCssLink">see link to discovery image below</a>). <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/49.2017ATel10133_%20AT2017blf.pdf" target="_blank" class="imCssLink">Atel#10133</a></span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">NOVA AT2017axz in M81</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The M81 nova monitoring collaboration reports the independent discovery of an apparent nova in M81 on a co-added 5400-s unfiltered CCD frame taken on 2017 Feb. 19.962 UT with the 0.65-m telescope at Ondrejov (OND). The object designated PNV J09553619+6906210 was first announced and designated AT2017axz by<span class="cf1"> </span><span class="cf1">F. Castellani et al.</span> <align=center><em><span class="cf5">(<a href="https://wis-tns.weizmann.ac.il/object/2017axz" target="_blank" class="imCssLink">see here</a>)</span></em> and is located at R.A. = 9h55m36s.19, Decl. = +69o06'21".0 (equinox 2000.0), which is 16.2" east and 145.9" north of the center of M81 (<a href="http://www.osservatoriomontebaldo.it/blog/?id=tejpvxnm" target="_blank" class="imCssLink">see link to discovery image below</a>). <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/48.2017ATel10102_AT2017axz.pdf" target="_blank" class="imCssLink">ATel#10102</a></align=center></span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">NOVA AT2017axi in M31</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Nova M31 2017-02a? (= AT2017axi), TNS discovered 2017/02/18.746<b><span class="cf1"> </span></b><span class="cf1">by Raffaele Belligoli</span><span class="cf1"> </span><span class="cf1">et al</span><span class="cf1">.</span>
819(<a href="http://italiansupernovae.org/" target="_blank" class="imCssLink">ISSP</a>) Found in M31 at R.A. = 00h42m38s.120, Decl. = +41°14'10".70 Located 3".0 east and 115".0 south of the center of M31 (<a href="http://www.osservatoriomontebaldo.it/blog/?id=x3290l6u" target="_blank" class="imCssLink">Discovery image</a>) (ISSP image) Mag 18.3:2/18, Type unknown (References: <a href="http://www.cbat.eps.harvard.edu/unconf/followups/J00423810+4114105.html" target="_blank" class="imCssLink">CBAT TOCP</a>)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">2016</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div><div class="imTAJustify"><b class="fs10lh1-5 ff1">The 2016 outburst of the unique symbiotic star MWC 560 ( = V694 Mon), its long-term BVRI evolution and a marked 331 days periodicity</b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari, S. Dallaporta, <span class="cf1">F. Castellani</span>, L. Baldinelli, G.L. Righetti, M. Graziani, G. Cherini, A. Maitan, S. Moretti, S. Tomaselli, A. Frigo</span></div><div><div class="imTAJustify"><span class="fs10lh1-5 ff1">BVRI photometry obtained in 357 nights distributed between 2005 and 2016.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Analysis of the long term photometric evolution and of the record breaking 2016 outburst.</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Detection of strong periodicities at 331 and 1860 days, and their relation to orbital period. <a href="https://arxiv.org/abs/1607.06309" target="_blank" class="imCssLink">New Astronomy 49</a>, <a href="files/73.2016-V694MON-NewAstronomy49.pdf" target="_blank" class="imCssLink">PDF.</a></span></div></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>MASTER Independent Detection: Possible Nova in M31</b><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">After our detection we found discovery information at Bishop pages by Emmanuel Conseil (see at TNS <a href="https://wis-tns.weizmann.ac.il/object/2016jbx" target="_blank" class="imCssLink">https://wis-tns.weizmann.ac.il/object/2016jbx</a> ) <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/47.ATel9912_%20MASTERIndependentDetection_%20NovaM31.pdf" target="_blank" class="imCssLink">Atel#9912</a></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Indipendent and prediscovery nova AT2016jbx<b><span class="cf1"> </span></b><span class="cf1">by R.Belligoli, F.Castellani, C.Marangoni and F.Marziali</span> <span class="cf1">on <a href="https://wis-tns.weizmann.ac.il/object/2016jbx" target="_blank" class="imCssLink">TNS UAI AT2016jbx</a></span><span class="cf1">.</span></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Confirmation and Photometry of M31 Transients AT2016jbg and <span class="cf1">AT2016ize</span><span class="cf1"> </span>Roughly 2.9' almost directly west of AT2016jbg lies the transient AT2016ize, reported to the IAU-TNS<span class="cf1"> </span><span class="cf1">by Belligoli</span><span class="cf1"> </span><span class="cf1">et al</span><span class="cf1">.</span><span class="cf1"> </span>on 2016 December 21.7139 UT with an unfiltered magnitude of 18.5 from observations conducted with <span class="cf1">ISSP</span>. <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/46.2016ATel_9915_%20Confirmation_AT2016ize.pdf" target="_blank" class="imCssLink">ATel#9915</a></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><b><span class="fs10lh1-5 ff1">NOVA AT2016ize in M31</span></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The object designated PNV J00424659+4116578 was first announced and designated AT2016ize by <span class="cf1">R. Belligoli et al.</span> (<a href="https://wis-tns.weizmann.ac.il/object/2016ize" target="_blank" class="imCssLink">see here</a>) and is located at R.A. = 0h42m46s.59, Decl. = +41o16'57".8 (equinox 2000.0), which is 25.5" east and 49.3" north of the center of M31 (see link to discovery image below). <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/45.2016ATel_9896_NovaM31.pdf" target="_blank" class="imCssLink">Atel#9896</a></span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><b class="fs10lh1-5 ff1">Congratulations! Your paper is one of the 5 most highly cited papers published in New Astronomy.</b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Dear Dr. Munari, The editors of New Astronomy are delighted to inform you that your paper, <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/28.2013Paper_LightCurveSNIa.pdf" target="_blank" class="imCssLink">BVRI lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95, and SN 2012cg in NGC 4424</a>, published in 2013 is one of the most highly cited papers during 2014, 2015 and up until June 2016. We would like to take this opportunity to thank you for publishing with us and to congratulate you. <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/45.2016_SN2011feM101.pdf" target="_blank" class="imCssLink">See more...</a></span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The 2016 outburst of the unique symbiotic star MWC 560 ( = V694 Mon), its long-term BVRI evolution and a marked 331 days periodicity</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari, S. Dallaporta, <span class="cf1">F. Castellani</span>, L. Baldinelli, G.L. Righetti, M. Graziani, G. Cherini, A. Maitan, S. Moretti, S. Tomaselli, A. Frigo <a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/44.2016_Munari_NewA_49_43.pdf" target="_blank" class="imCssLink">NewAstronomy_49_43.pdf</a></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><b>SUPERNOVA AT2016bry IN UGC 11635</b><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">The Asiago Transient Classification Program (Tomasella et al. 2014, AN, 335, 841) reports the spectroscopic classification of AT2016bry, discovered by V. Tinella in UGC 11635, and preliminary photometric follow-up. Additional CCD magnitudes for AT2016bry: 2016-04-27.35 | Bj 15.87 +- 0.02 | Vj 15.57 +- 0.01 | Rc15.17 +- 0.01 (<span class="cf1">R. Belligoli, F. Castellani</span>, Verona, Italy)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/43.2016_Atel9018.pdf" target="_blank" class="imCssLink">ATel#9018</a>; (2016)</span></div><div class="imTAJustify"><b class="fs10lh1-5 ff1"><br></b></div><div><div class="imTAJustify"><b class="fs10lh1-5 ff1">2015</b></div><div class="imTAJustify"><span class="ff1"><span class="fs10lh1-5"><b><br></b></span></span></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">SUPERNOVA 2015Q IN NGC 3888 = PSN J11473508+5558147</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Additional CCD magnitudes for 2015Q: 19.905, 16.3 (</span></span><span class="fs10lh1-5 cf1">R. Belligoli, F. Castellani, and C. Marangoni</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Verona, Italy)</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/42.2015_CBET4128.pdf" target="_blank" class="imCssLink">CBET4128</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">;
819 (2015)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/42.2015_CBET4128.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><span class="ff1"><span class="fs10lh1-5"><b><br></b></span></span></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">"The symbiotic binary and super-soft X-ray source AG Dra is going into outburst"</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari (INAF Padova-Asiago), G. L. Righetti, U. Sollecchia, </span></span><span class="fs10lh1-5 cf1">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (ANS Collaboration)</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/41.2015_ATel7582.pdf" target="_blank" class="imCssLink">ATel #7582</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">; (2015)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/41.2015_ATel7582.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><span class="ff1"><span class="fs10lh1-5"><b><br></b></span></span></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2014</b></div></b><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">âThe symbiotic star Hen 2-468 is undergoing a rare and bright outburstâ</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari (INAF-Padova), S. Dallaporta and </span></span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (ANS Collaboration)</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/40.2014_The%20symbiotic%20star%20Hen%202-468.pdf" target="_blank" class="imCssLink">ATel 6841</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">; (2014)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/40.2014_The%20symbiotic%20star%20Hen%202-468.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">"The prototype symbiotic star AX Per is in outburst"</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari (INAF Padova-Asiago), S. Dallaporta, G. L. Righetti, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, G. Cherini (ANS Collaboration)</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/39.2014_ATel6382.pdf" target="_blank" class="imCssLink">ATel 6382</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2014)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/39.2014_ATel6382.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><br></span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Study of three 2013 novae: V1830 Aql, V556 Ser and V809 Cep</span><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, P. Ochner, S. Dallaporta, P. Valisa, M. Graziani, G.L. Righetti, G. Cherini, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, G. Cetrulo and A., Englaro</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/38.2014_MNRAS440.pdf" target="_blank" class="imCssLink">MNRAS 440, 3402â3415</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2014)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/38.2014_MNRAS440.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">NOVA SCORPII 2014 = TCP J17154683-3128303</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, S. Dallaporta, </span></span><span class="fs10lh1-5 cf6">F. Castellani, R. Belligoli</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Electronic Telegram No. 3841*</span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">NOVA CYGNI 2014 = PNV J20214234+3103296</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, G. Cetrulo, D. Degano, and </span></span><span class="fs10lh1-5 cf6">F. Castellani</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Electronic Telegram No. 3842*</span></div></div><div class="imTAJustify"><br></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Optical photometry of the rapidly declining Nova Scorpii 2014</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">U. Munari (INAF Padova-Asiago), S. Dallaporta, <span class="cf1">F. Castellani</span>, C. Marangoni (ANS Collaboration)</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">on 1 Apr 2014; 09:05 UT Credential Certification: U. Munari ([email protected])</span></div><div class="imTAJustify"><span class="fs10lh1-5 ff1">Nova Scorpii 2014 was discovered as optical transient TCP J17154683-3128303 by Nishiyama and Kabashima, and classified from optical spectra as a nova by Jelinek et al (ATEL #6025). X-ray emission was detected on Swift observations by Kuulkers et al. (ATEL #6015),... (<a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/59.ATel6034_%20Optical%20photometry%20Nova%20Scorpii%202014.pdf" target="_blank" class="imCssLink">ATel_6034</a>) <br></span></div><div><div class="imTAJustify"><br></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5">NOVA CEPHEI 2014 = TCP J20542386+6017077</span></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, A. Milani, P. Valisa, </span><span class="fs10lh1-5 cf6">
819F. Castellani, and R. Belligoli </span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/35.2014_CBET03825.pdf" target="_blank" class="imCssLink">Electronic Telegram No. 3825</a></span></div><div class="imTAJustify"><span class="ff1"><span class="fs10lh1-5"><br></span></span></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">SUPERNOVA 2014J IN M82 = PSN J09554214+6940260</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, </span></span><span class="fs10lh1-5 cf6">F. Castellani, R. Belligoli</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, G. L. Righetti</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/34.2014_CBET003792.pdf" target="_blank" class="imCssLink">Electronic Telegram No. 3792</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/34.2014_CBET003792.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The symbiotic star TX CVn has entered an active state.</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, P. Valisa, S. Dallaporta, G. Cherini, A. Vagnozzi, G. L. Righetti, </span></span><span class="fs10lh1-5 cf6">R. Belligoli</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">14 Jan 2014; 15:56 UT </span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/33.2014_ATel5761.pdf" target="_blank" class="imCssLink">ATel 5761 </a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">(2014)</span></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The Metrology of Supernova Lightcurves 223rd American Astronomical Society Meeting</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Authors: Rust, Bert W.1; Mullen, Katharine M.2 Institutions: 1. NIST, Gaithersburg, MD, United States. 2. UCLA, Los Angeles, CA, United States. 3. ANS Collaboration: U.Munari, Italia</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/32.2014_AAS%20223_%20354.pdf" target="_blank" class="imCssLink">AAS 223_ 354abstract</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> </span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/32b.2014_posterAAS.jpg" target="_blank" class="imCssLink">ASS223_354poster</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/32.2014_AAS%20223_%20354.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2013</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">SUPERNOVA 2013ff IN NGC 2748 = PSN J09133888+7628108</span></div></div><div class="fs10lh1-5 cf6 ff1"><div class="imTAJustify"><span class="fs10lh1-5">Belligoli R, Castellani F.</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/31.2013_CBET003647.pdf" target="_blank" class="imCssLink">Cbet 3647</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> </span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/31b.2013_CBET003656.pdf" target="_blank" class="imCssLink">Cbet3656</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/31.2013_CBET003647.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Photometric evolution, orbital modulation and progenitor of Nova Mon 2012.</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Dallaporta, S., </span></span><span class="fs10lh1-5 cf6">Castellani, F</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">., Valisa, P., Frigo, A., Chomiuk, L., Ribeiro, V.A.R.M.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/30.2013_MNRAS_1306.1501.pdf" target="_blank" class="imCssLink">MNRAS 435, 771</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2013)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/30.2013_MNRAS_1306.1501.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">An ongoing active phase for the old symbiotic nova AG Peg Munari, U., Valisa, P., Dallaporta, S., Cherini, G.L. Righetti, G., </span></span><span class="fs10lh1-5 cf6">Castellani, F. </span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/29.2013_ATel5258.pdf" target="_blank" class="imCssLink">ATel 5258</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2013)</span></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">BVRI lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95, and SN 2012cg in NGC 4424.</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Henden, A., </span></span><span class="fs10lh1-5 cf6">Belligoli, R., Castellani, F</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">., Cherini, G., Righetti, G.L., Vagnozzi, A.</span></span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">NewAstronomy 20, 30 (</span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/28.2013Paper_LightCurveSNIa.pdf" target="_blank" class="imCssLink">
8192013NewA...20...30M</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">)</span></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Nova Cephei 2013 has emerged from dust obscuration</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, P. Ochner, A. Siviero, M. Graziani, S. Dallaporta, G. L. Righetti, G. Cherini, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/27.2013_ATel5389.pdf" target="_blank" class="imCssLink">ATel 5389</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2013)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/27.2013_ATel5389.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">An ongoing active phase for the old symbiotic nova AG Peg Munari, U., Valisa, P., Dallaporta, S., Cherini, G.L. Righetti, G., </span></span><span class="fs10lh1-5 cf6">Castellani, F. </span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/26.2013_ATel5258.pdf" target="_blank" class="imCssLink">ATel 5258 </a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">(2013)</span></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The symbiotic star YY Her is in outburst</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Dallaporta S., </span></span><span class="fs10lh1-5 cf6">Castellani F., Belligoli R.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Cherini G., Righetti G.L., Graziani M., Valisa P., Milani A.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/25.2013_ATel4996.pdf" target="_blank" class="imCssLink">ATel 4996 </a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">(2013)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/25.2013_ATel4996.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Is Nova Cep 2013 currently forming dust ?</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Dallaporta, S., Cherini, G., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Cetrulo, G., Valisa, P., Graziani, M.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/24.2013_ATel4893.pdf" target="_blank" class="imCssLink">ATel 4893</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2013)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/24.2013_ATel4893.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The decline of the super-soft X-ray source in Nova Mon 2012.</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Page, K.L., Osborne, J.P., Munari, U., Wagner, R.M., Beardmore, A.P., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Dallaporta, S., Shore, S.N., Starrfield, S., Woodward, C.E. </span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/23.2013_ATel4845.pdf" target="_blank" class="imCssLink">ATel 4845</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2013)</span></span></div></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2012</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">SUPERNOVA 2012fm IN UGC 3528 = PSN J06561339+8404502 </span></span><span class="fs10lh1-5 cf6">Belligoli R, Castellani F.</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/22.2012_CBET003272.pdf" target="_blank" class="imCssLink">
8192012CBET 3272</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/22.2012_CBET003272.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">ABELL-35 PHENOMENA IN SYMBIOTIC STARS: DISCOVERY OF 1.2 AND 6.4 DAY PERIODS IN VV8 (V471 PER)</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, A. Siviero, E. Tamajo, M. Fiaschi, S. Dallaporta, G. Cherini, A. Frigo,</span></span><span class="fs10lh1-5 cf6"> </span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, M. Graziani, S. Moretti and S. Tomaselli</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/21.2012_BaltA__21__180M.pdf" target="_blank" class="imCssLink">Baltic Astronomy, vol. 21, 189â192, </a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">2012</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/21.2012_BaltA__21__180M.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The ANS Collaboration Monitoring Program</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Bacci, S., Baldinelli, L., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Cetrulo, G., Cherini, G., Dallaporta, S., Dallavia, G., Englaro, A., Frigo, A., Graziani, M., Luppi, V., Maitan, A., </span></span><span class="fs10lh1-5 cf6">Marangoni, C.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Milani, A., Moretti, S., Moschini, F., Ochner, P., Siviero, A., Righetti, G. L., Tomaselli, S., Tomasoni, S., Vagnozzi, A., Valisa, P.</span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/20.2012_BaltA__21___13M.pdf" target="_blank" class="imCssLink"> Informational Bulletin on Variable Stars</a></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/20.2012_BaltA__21___13M.pdf" target="_blank" class="imCssLink">Baltic Astronomy, vol.21, 2012</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/20.2012_BaltA__21___13M.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">SUPERNOVA 2012aw IN M95 = PSN J10435372+1140177</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">A. Vagnozzi, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/19.2011_CBET%203054.pdf" target="_blank" class="imCssLink">2012 CBET 3054</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/19.2011_CBET%203054.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2011</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The 2010 nova outburst of the symbiotic Mira V407 Cyg</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, V.H. Joshi, N.M. Ashok, D.P.K. Banerjee, P. Valisa, A. Milani, A. Siviero, S. Dallaporta, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/18.2011_v407_mnras_2010.pdf" target="_blank" class="imCssLink">2011 January, MNRAS Letters, vol 410, L52-L56</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/18.2011_v407_mnras_2010.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Formation of a disk structure in the symbiotic binary AX Per during its 2007-10 precursor-type activity</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">A. Skopal, T. N. Tarasova, Z. Cariková,</span></span><span class="fs10lh1-5 cf6"> </span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, G. Cherini, S. Dallaporta, A. Frigo, </span></span><span class="fs10lh1-5 cf6">C. Marangoni</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, S. Moretti, U. Munari, G. L. Righetti, A. Siviero, S. Tomaselli, A. Vagnozzi, P. Valisa</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/17.2011_1110.2801.pdf" target="_blank" class="imCssLink">2011 Astronomy & Astrophysics arXiv:1110.2801v1 [astro-ph.SR]</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/17.2011_1110.2801.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">YY HERCULIS</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, Istituto Nazionale di Astrofisica, Padova Astronomical Observatory; A. Siviero Department of Astronomy, University of Padova; G. L. Righetti,</span></span><span class="fs10lh1-5 cf6"> </span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, S. Dallaporta, M. Graziani, G. Cherini, S. Moretti, S. Tomaselli, and A. Frigo</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/16.2011_CBET2861.pdf" target="_blank" class="imCssLink">2011, CBET, 2861</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/16.2011_CBET2861.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">SUPERNOVA 2011fe IN M101</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Magnitude estimates: B. Mikuz and J. Vales, Crni Vrh Observatory, W. Souza,</span></div></div><div class="fs10lh1-5 cf6 ff1"><div class="imTAJustify"><span class="fs10lh1-5">F. Castellani and R. Belligoli, Monte Baldo</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, G. Masi, J. Carvajal,P. Schmeer, Bischmisheim.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/15.2011_CBET002804.pdf" target="_blank" class="imCssLink">2011 CBET 2804</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/15.2011_CBET002804.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2010</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">BVRcIc Photometric Evolution and Flickering during the 2010 Outburst of the Recurrent Nova U Scorpii</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Dallaporta, S., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/14.2010_IBVS5930.pdf" target="_blank" class="imCssLink">2010, IBVS, 5930, 1M</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/14.2010_IBVS5930.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">AX Persei </span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari U., Siviero, A., R.L.M. Corradi R.L.M., Valisa P., Cherini G.,</span></span><span class="fs10lh1-5 cf6"> </span><span class="fs10lh1-5 cf6">Castellani F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Dallaporta S.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/13.2010_CBET_2555.pdf" target="_blank" class="imCssLink">2010, CBET, 2555.</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/13.2010_CBET_2555.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">COMET C/2010 G1 (BOATTINI)</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">A. Boattini, R. Ligustri , E. Pettarin, </span></span><span class="fs10lh1-5 cf6">F. Castellani and C. Marangoni</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, P. Birtwhistle, L. Buzzi, J. E. McGaha</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/12.2010_IAUC%209133.pdf" target="_blank" class="imCssLink">2010, IAUC 9133</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/12.2010_IAUC%209133.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">CI Cygni</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, (INAF Padova-Asiago, Italy), P. Valisa, A. Milani, G. Cherini, </span></span><span class="fs10lh1-5 cf6">F. Castellani</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, S. Dallaporta, A. Siviero, A. Frigo (ANS Collaboration)</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/11.2010_ATEL_2913.pdf" target="_blank" class="imCssLink">2010 (09 October), ATEL, 2913</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/11.2010_ATEL_2913.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2009</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The 2006-2008 Outburst of AG Draconis</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Siviero, A., Ochner, P., Wallerstein, G., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">
819, Righetti, G., Cherini, G., Valisa, P., Cetrulo, G.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/10.2009_AGDra.pdf" target="_blank" class="imCssLink">2009, PASP, 121, 1070</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/10.2009_AGDra.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">AX PERSEI</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Siviero, A., Dallaporta, S., Cherini, G., Valisa, P., </span></span><span class="fs10lh1-5 cf6">Castellani, F</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">., Frigo, A., Vagnozzi, A., Bacci, S., Righetti, G., Moretti, S., Tomaselli, S.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/9.2009_CBET1757.pdf" target="_blank" class="imCssLink">2009, CBET, 1757</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/9.2009_CBET1757.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Ongoing meteor work - A Comprehensive List of Meteor Showers Obtained from 10 Years of Observations with the IMO Video Meteor</span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/8.2009_IMOVideo.pdf" target="_blank" class="imCssLink">Network WGN, the Journal of the IMO 37:4</a></span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5"> (2009)</span></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/8.2009_IMOVideo.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2008</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">NOVA SAGITTARII 2008</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Siviero, A., Moretti, S., Tomaselli, S., Maitan, A., Baldinelli, L.,</span></span><span class="fs10lh1-5 cf6"> </span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Dallaporta, S., Ochner, P.</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/7.2008_CBET1352.pdf" target="_blank" class="imCssLink">2008, CBET, 1352</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/7.2008_CBET1352.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">V2468 CYGNI</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Siviero, A., Valisa, P., Dallaporta, S., Cherini, G., Ochner, P., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Buzzi, L., Brienza, M., Luppi, V. </span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/6.2008_CBET1431.pdf" target="_blank" class="imCssLink">2008, CBET, 1431</a></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">Characterization of the HD 17156 planetary system</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">M. Barbieri, R. Alonso, S. Desidera, A. Sozzetti, A.F. Martinez Fiorenzano, J. M. Almenara, M. Cecconi, R.U.Claudi, D. Charbonneau, M. Endl, V. Granata, R. Gratton, G. Laughlin, B. Loeillet, Amateur Consortium ââ</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">E.A.C. observations obtained by: </span></span><span class="fs10lh1-5 cf6">F. Castellani (Mt. BaldoObservatory)</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, B. Gary, J. Gregorio, C. Lopresti, A. Marchini (SienaUniversity Observatory),M. Nicolini (Cavezzo Observatory), R. Papini, C. Vallerani</span></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/5.2008_arXiv.pdf" target="_blank" class="imCssLink">2008 Astronomy & Astrophysics manuscript no. barbieriËhd17156 c arXiv:0812.0785v1</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/5.2008_arXiv.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><b class="fs10lh1-5 ff1"><div class="imTAJustify"><b class="fs10lh1-5">2007</b></div></b><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">V2467 Cygni (Nova Cyg 2007)</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Dalla Via, G., Valisa, P., Dallaporta, S., </span></span><span class="fs10lh1-5 cf6">Castellani, F. </span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/4.2007_CBET897.pdf" target="_blank" class="imCssLink">2007, CBET, 897</a></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">V919 Sgr</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Siviero, A., Navasardyan H., Castellani, F., Bortolotti M., Valisa, P., Luppi V. </span></span><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/3.2007_CBET999.pdf" target="_blank" class="imCssLink">2007, CBET, 999</a></span></div></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">AG DRACONIS</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">Munari, U., Siviero, A., </span></span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Valisa, P., Cherini, G., Bano, I., Englaro, A., Cetrulo, G.</sp
819an></span></div></div><div class="imTAJustify fs10lh1-5 ff1"><span class="fs10lh1-5"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/2.2007_CBET1091.pdf" target="_blank" class="imCssLink">2007, CBET, 1091</a></span><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/2.2007_CBET1091.pdf" target="_blank" class="imCssLink"><br></a></span></div><div class="imTAJustify"><br></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">The 2006 outburst of the recurrent nova RS Oph</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">U. Munari, A. Siviero, Sostero, G., Guido, E., Dallaporta, S., Moretti, S., Graziani, M., Tomaselli, S.,</span></span><span class="fs10lh1-5 cf6"> </span><span class="fs10lh1-5 cf6">Castellani, F.</span><span class="fs10lh1-5 ff1"><span class="fs10lh1-5">, Ochner, P.</span></span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">in "Evolution and Chemistry of Symbiotic Stars, Binary post-AGB and related Objects",</span></div></div><div class="ff1"><div class="imTAJustify"><span class="fs10lh1-5">held 29-31 August, 2006 in Wierzba, Mazury Lakes (Poland)</span></div></div><div class="imTAJustify"><span class="fs10lh1-5 ff1"><a href="http://www.osservatoriomontebaldo.it/uploads/CBETOMB/1.2006RS_OPH_BalticAstronomy.pdf" target="_blank" class="imCssLink">Baltic Astronomy Special Issue 16, 2007, pag. 46</a></span></div></div></td></tr></tbody></table></div></div> 820 821 </div> 822 </div><div id="imPageRow_3" class="imPageRow"> 823 <div style="position: absolute; top: 0; left: 0; right: 0; bottom: 0; overflow: hidden;"><div id="imPageRowGraphics_3" ></div></div> 824 </div> 825 <div id="imCell_157" class=""> <div id="imCellStyleGraphics_157" ></div><div id="imCellStyleBorders_157"></div>
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LP ripresa di 16-36 (High proper-motion Star)", thumbUrl: "gallery/20181228-LP16-36OMB_sb_thumb.png" }, 853 {type: "image", url: "gallery/20181013-AT2018hhy_uzvhaipl.jpg", width: 426, height: 411, description: "2018/10/13-Scoperta PNV in M33- AT2018hhy", thumbUrl: "gallery/20181013-AT2018hhy_sb_thumb.png" }, 854 {type: "image", url: "gallery/20181013-AT2018hho_gnflpyqa.jpg", width: 426, height: 411, description: "2018/10/13-Scoperta Nova in M31- AT2018hho", thumbUrl: "gallery/20181013-AT2018hho_sb_thumb.png" }, 855 {type: "image", url: "gallery/20180731-AT2018ely.jpg", width: 426, height: 411, description: "2018/07/31-Scoperta Nova in M31- AT2018ely", thumbUrl: "gallery/20180731-AT2018ely_sb_thumb.png" }, 856 {type: "image", url: "gallery/20180112_M31_AT2018eq.jpg", width: 426, height: 411, description: "2018/01/12-Scoperta Nova galattica - AT2018eq<br />Prima nova scoperta all\'interno della Via Lattea dall\'Osservatorio astronomico Monte Baldo", thumbUrl: "gallery/20180112_M31_AT2018eq_sb_thumb.png" }, 857 {type: "image", url: "gallery/20171224-M31_AT2017jdm.jpg", width: 426, height: 411, description: "2017/12/24-Scoperta Nova ricorrente in M31- AT2017jdm", thumbUrl: "gallery/20171224-M31_AT2017jdm_sb_thumb.png" }, 858 {type: "image", url: "gallery/20170605-drum_MB_EHN.gif", width: 784, height: 518, description: "Registrato il sisma ML 3.6 avvenuto nella zona a 3 km SE Gargnano (BS) prima registrazione del sismografo", thumbUrl: "gallery/20170605-drum_MB_EHN_sb_thumb.png" }, 859 {type: "image", url: "gallery/20170418-M81_PNV-J09551279-6900093.jpg", width: 426, height: 411, description: "2017/04/18-Scoperta Nova in M81- PNV J09551279+6900093", thumbUrl: "gallery/20170418-M81_PNV-J09551279-6900093_sb_thumb.png" }, 860 {type: "image", url: "gallery/20170225-AT2017blf.jpg", width: 426, height: 411, description: "2017/02/25-Scoperta Nova in M81- AT2017blf", thumbUrl: "gallery/20170225-AT2017blf_sb_thumb.png" }, 861 {type: "image", url: "gallery/20170219-AT2017axz.jpg", width: 426, height: 411, description: "2017/02/19-Scoperta Nova in M81- AT2017axz", thumbUrl: "gallery/20170219-AT2017axz_sb_thumb.png" }, 862 {type: "image", url: "gallery/20170218_M31_AT2017axi_.jpg", width: 426, height: 411, description: "2017/02/18-Scoperta Nova in M31- AT2017axi", thumbUrl: "gallery/20170218_M31_AT2017axi__sb_thumb.png" }, 863 {type: "image", url: "gallery/20161227-M31-AT2016jbx.jpg", width: 426, height: 411, description: "2016/12/27-Scoperta Nova ricorrente in M31- AT2016jbx", thumbUrl: "gallery/20161227-M31-AT2016jbx_sb_thumb.png" }, 864 {type: "image", url: "gallery/PNV_AT2016ize.jpg", width: 426, height: 411, description: "2016/12/21-Scoperta Nova in M31- AT2016ize", thumbUrl: "gallery/PNV_AT2016ize_sb_thumb.png" },
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918<a role="button" href="#" onclick="return x5engine.imShowBox(showboxlink28b1f31e498816dc280b34d856ba2003, 0, this)"><img src="gallery/M81_20250304_AT2025dih_annotata_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Scoperta la Nova AT 2025dih in M81' });" style="" alt="" width="234" height="234" /></a> 919 <a href="at2025dkp.html" onclick="return x5engine.utils.location('at2025dkp.html', null, false)"><img src="gallery/M31_AT2024agal_annotata_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Scoperta la Nova AT2024AGAL in M31' });" style="" alt="" width="234" height="234" /></a> 920 <a href="at2024ssq.html" onclick="return x5engine.utils.location('at2024ssq.html', null, false)"><img src="gallery/M31_AT2024ssq_annotata_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Scoperta la Nova AT2024ssq in M31' });" style="" alt="" width="234" height="234" /></a> 921 <a href="at2023wnh.html" onclick="return x5engine.utils.location('at2023wnh.html', null, false)"><img src="gallery/AT2023wnh_20231207_Cl_Annotata_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Scoperta Nova AT2023whn nella galassia di Andromeda M31 2023/11/03.795' });" style="" alt="" width="234" height="234" /></a> 922 <a href="at2023yij.html" onclick="return x5engine.utils.location('at2023yij.html', null, false)"><img src="gallery/M31_20231125_AT2023yij_Scritte_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Scoperta Nova AT2023yij nella galassia di Andromeda M31 2023/11/23.7171' });" style="" alt="" width="234" height="234" /></a> 923 <a href="at2023ps.html" onclick="return x5engine.utils.location('at2023ps.html', null, false)"><img src="gallery/AT2023ps-J00424623_4117357_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Scoperta Nova AT2023ps
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948<img src="gallery/2015MoravianG4_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Donato da BIM Adige nuovo CCD per Osservatorio' });" style="" alt="" width="234" height="234" /></a> 949 <a href="http://www.osservatoriomontebaldo.it/news2013.html#20130909" target="_blank"><img src="gallery/SN_2013ff_NGC2748_negativo_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: '2018/08/31-Scoperta SuperNova in NGC2748 - SN2013ff' });" style="" alt="" width="234" height="234" /></a> 950 <a href="http://www.osservatoriomontebaldo.it/news2013.html#20130817" target="_blank"><img src="gallery/20130817-NovaDel_thumb_99u3b4vo.png" onmouseover="x5engine.imTip.Show(this, { text: 'Ripresa NOVA Del2013 dall\'Osservatorio' });" style="" alt="" width="234" height="234" /></a> 951 <a href="http://www.osservatoriomontebaldo.it/news2013.html#20130729" target="_blank"><img src="gallery/20130729-AsteroideDZ15_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Ripreso asteroide 2003 DZ15 dall\'Osservatorio' });" style="" alt="" width="234" height="234" /></a> 952 <a href="http://www.osservatoriomontebaldo.it/news2013.html#20130217" target="_blank"><img src="gallery/20130217-AasteroideDA14_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: 'Ripreso asteroide 2012 DA14 dall\'Osservatorio' });" style="" alt="" width="234" height="234" /></a> 953 <a href="http://www.osservatoriomontebaldo.it/news2012.html#20121024" target="_blank"><img src="gallery/2012fm-21102012_thumb.png" onmouseover="x5engine.imTip.Show(this, { text: '2012/10/21-Scoperta SuperNova in UGC3528 - SN2012fm' });" style="" alt="" width="234" height="234" /></a> 954 </div></div><button type="button" class="clear-button-style imRightArrow" aria-label="Successivo"></button></div> 955 </div><div id="imCell_158" class=""> <div id="imCellStyleGraphics_158" ></div><div id="imCellStyleBorders_158"></div><div id="imCellStyleTitle_158">La Luna oggi</div><div id="imTextObject_158"> 956 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTextObject_158_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 957 <div class="text-inner"> 958 <p class="imTACenter"><span class="fs10lh1-5 cf1 ff1"><a href="http://www.astrofiliveronesi.it/moon.html" target="_blank" class="imCssLink inline-block"><img class="image-2" src="images/Moon_thumb_kzqtp8tu.gif" width="203" height="77" /></a></span><br></p> 959 </div> 960 </div> 961 962 </div> 963 </div><div id="imCell_159" class=""> <div id="imCellStyleGraphics_159" ></div><div id="imCellStyleBorders_159"></div><div id="imCellStyleTitle_159">Il Sole oggi</div><div id="imTextObject_159"> 964 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTextObject_159_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 965 <div class="text-inner"> 966 <p class="imTACenter"><span class="fs10lh1-5 ff1"><a href="http://www.astrofiliveronesi.it/sun.html" target="_blank" class="imCssLink inline-block"><img class="image-3" src="images/Sun_thumb_l6npujkp.gif" width="203" height="77" /></a></span><br></p> 967 </div> 968 </div> 969 970 </div> 971 </div><div id="imCell_53" class=""> <div id="imCellStyleGraphics_53" ></div><div id="imCellStyleBorders_53"></div><div id="imCellStyleTitle_53">Il cielo del mese</div><div id="imTextObject_53"> 972 <div data-index="0" class="text-tab-content grid-prop current-tab " id="imTextObject_53_tab0" style="opacity: 1; " role="tabpanel" tabindex="0"> 973 <div class="text-inner"> 974 <p class="imTACenter"><span class="fs10lh1-5 cf1 ff1"><a href="https://divulgazione.uai.it/index.php/Cielo_di_Giugno_2024" target="_blank" class="imCssLink inline-block"><img class="image-1" src="images/Cielo_thumb_8bxd1iln.gif" width="203" height="77" /></a></span><br></p> 975 </div> 976 </div> 977 978 </div> 979 </div><div id="imCell_78" class=""> <div id="imCellStyleGraphics_78" ></div><div id="imCellStyleBorders_78"></div><div id="imCellStyleTitle_78">SQM: ultima lettura</div><div id="imHTMLObject_78" class="imHTMLObject" style="text-align: center; height: 140px; width: 100%; overflow: hidden;">
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