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	<title>The Astronomer's Telegram:  Nova </title>
	<link> https://www.astronomerstelegram.org </link>
	<description> Nova, from The Astronomer's Telegram </description>

	<dc:language>en-us</dc:language>

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<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18096" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18091" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18090" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18088" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18087" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18086" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18084" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18083" />
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<item rdf:about="https://www.astronomerstelegram.org/?read=18103" >
	<title> ATel 18103: Sloan g&#39;r&#39;i&#39; Photometry of the Type Ic-BL SN 2026acxa </title>
	<link> https://www.astronomerstelegram.org/?read=18103 </link>
	<creator> J. Ricra, C. Avalos-Vega, N. Gomez-Pasten, C. Adam, C. Cardenas, J. P. Colque, and E. Unda-Sanzana  </creator>
	<author> J. Ricra, C. Avalos-Vega, N. Gomez-Pasten, C. Adam, C. Cardenas, J. P. Colque, and E. Unda-Sanzana  </author>
	<creatoremail> jose.ricra@uamail.cl </creatoremail>
	<provenance> Credentialed by: Eduardo Unda-Sanzana (eduardo.unda@uantof.cl) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18103</identifier>
	<description> We report optical photometric observations of SN 2026acxa, obtained on 2026 October 01 UT with the 0.6m telescope at Ckoirama Observatory, Universidad de Antofagasta, Chile. ... </description>
	<dc:date>2026-10-13T12:53:15-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18096" >
	<title> ATel 18096: Dust formation in the M31 nova AT2026aabo </title>
	<link> https://www.astronomerstelegram.org/?read=18096 </link>
	<creator> A. Evans, D. P. K. Banerjee, T. R. Geballe,  C. E. Woodward,  S. Starrfield  </creator>
	<author> A. Evans, D. P. K. Banerjee, T. R. Geballe,  C. E. Woodward,  S. Starrfield  </author>
	<creatoremail> dpkb12345@gmail.com </creatoremail>
	<provenance> Credentialed by: Dipankar P.K.  Banerjee (dpkb12345@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18096</identifier>
	<description>  The transient AT2026aabo in M31 was discovered on 2026 August 29 at 09:28:57 UT (ATel#18027), and was spectroscopically confirmed as a nova in the FeII phase (ATel#18029). ... </description>
	<dc:date>2026-10-08T13:34:15-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18091" >
	<title> ATel 18091: Independent Discovery and Time-Resolved Photometry of AT 2026adgl </title>
	<link> https://www.astronomerstelegram.org/?read=18091 </link>
	<creator> K. Hornoch, H. Kucakova, A. W. Shafter  </creator>
	<author> K. Hornoch, H. Kucakova, A. W. Shafter  </author>
	<creatoremail> k.hornoch@centrum.cz </creatoremail>
	<provenance> Credentialed by: Allen W. Shafter (ashafter@sdsu.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18091</identifier>
	<description> We report the independent discovery of a transient found during our survey of the central region of M31. The object was discovered on a co-added 1680-s R-band CMOS frame taken on 2026 Sep. ... </description>
	<dc:date>2026-10-05T20:43:09-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18090" >
	<title> ATel 18090: V488 Sge transitions to the nebular phase: the significant [O III] emission </title>
	<link> https://www.astronomerstelegram.org/?read=18090 </link>
	<creator>  Yi-Fei Qu, Rui-Xiang Hu, Bei You, Sai-En Xu, on behalf of the Match team. </creator>
	<author>  Yi-Fei Qu, Rui-Xiang Hu, Bei You, Sai-En Xu, on behalf of the Match team. </author>
	<creatoremail> youbei@whu.edu.cn </creatoremail>
	<provenance> Credentialed by: Bei You (youbei@whu.edu.cn) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18090</identifier>
	<description> V488 Sge (Nova Sge 2026; PNV J19450648+1822422) was discovered on 2026 Aug 25.1278 UTC (ATel #18009), and was classified as a very fast Fe II-type nova (ATel #18008, #18013). ... </description>
	<dc:date>2026-10-05T17:28:45-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18088" >
	<title> ATel 18088: VLA radio detection of Nova Sagittae 2026 (V488 Sge) </title>
	<link> https://www.astronomerstelegram.org/?read=18088 </link>
	<creator> Kirill Sokolovsky, Justin Linford, Laura Chomiuk, Peter Craig, Katie Barnhart, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi, Jennifer Sokoloski, Koji Mukai  </creator>
	<author> Kirill Sokolovsky, Justin Linford, Laura Chomiuk, Peter Craig, Katie Barnhart, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi, Jennifer Sokoloski, Koji Mukai  </author>
	<creatoremail> kirx@kirx.net </creatoremail>
	<provenance> Credentialed by: Kirill Sokolovsky (kirx@scan.sai.msu.ru) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18088</identifier>
	<description>  Peaking at visual magnitude 7 around 2026-08-25.9 UT and being  (so far) the brightest classical nova of the year,  Nova Sagittae 2026 (V488 Sge, PNV J19450648+1822422) has been  the target of optical photometric and spectroscopic (CBET #5729,  ATel #18008, #18009, #18012, #18014, #18021, #18022, #18033,  #18053) as well as X-ray observations (ATel #18028, #18084). ... </description>
	<dc:date>2026-10-03T19:36:11-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18087" >
	<title> ATel 18087: S-CUBED Detects Supersoft X-ray Counterpart to the SMC Nova ASASSN-26dt </title>
	<link> https://www.astronomerstelegram.org/?read=18087 </link>
	<creator> Thomas M. Gaudin, Jamie A. Kennea, Malcolm J. Coe, Kim L. Page, Itumaleng Monageng, David A. H. Buckley, Phil A. Evans  </creator>
	<author> Thomas M. Gaudin, Jamie A. Kennea, Malcolm J. Coe, Kim L. Page, Itumaleng Monageng, David A. H. Buckley, Phil A. Evans  </author>
	<creatoremail> tmg6006@psu.edu </creatoremail>
	<provenance> Credentialed by: Thomas Gaudin (tmg6006@psu.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18087</identifier>
	<description> An X-ray counterpart to the Small Magellanic Cloud (SMC) nova ASASSN-26dt, also known as AT 2026oyp, has been detected for the first time by an observation of the Swift SMC Survey (S-CUBED). ... </description>
	<dc:date>2026-10-03T12:18:25-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18086" >
	<title> ATel 18086: Swift X-ray and ultraviolet followup observations of the new enhanced activity phase of SU Lyn </title>
	<link> https://www.astronomerstelegram.org/?read=18086 </link>
	<creator> N. Masetti, U. Munari  </creator>
	<author> N. Masetti, U. Munari  </author>
	<creatoremail> nicola.masetti@inaf.it </creatoremail>
	<provenance> Credentialed by: Nicola Masetti (nicola.masetti@inaf.it) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18086</identifier>
	<description> Following the announcement in ATel #18083 that the symbiotic star  SU Lyn has entered a new phase of high optical activity likely due to enhanced accretion onto the white dwarf hosted in the system, we observed the source in X-rays and ultraviolet (UV) with the Neil  Gehrels Swift satellite, starting at 02:17 UT of 2026 October 02. ... </description>
	<dc:date>2026-10-02T16:12:23-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18084" >
	<title> ATel 18084: V488 Sge has become a super-soft X-ray source </title>
	<link> https://www.astronomerstelegram.org/?read=18084 </link>
	<creator> K. L. Page  and  G. J. M. Luna  </creator>
	<author> K. L. Page  and  G. J. M. Luna  </author>
	<creatoremail> kpa@star.le.ac.uk </creatoremail>
	<provenance> Credentialed by: Kim Page (kpa@star.le.ac.uk) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18084</identifier>
	<description>  V488 Sge (Nova Sagittae 2026) was discovered on 2026 Aug. 25.1278 UTC, and classified as a classical Fe II-type nova (CBET #5729, ATel #18009, #18008, ,#18012, #18014, #18021, #18022, #18033, #18053). ... </description>
	<dc:date>2026-10-01T19:09:38-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18083" >
	<title> ATel 18083: SU Lyn, the prototype of LowAcc symbiotic stars, is undergoing a major surge in accretion </title>
	<link> https://www.astronomerstelegram.org/?read=18083 </link>
	<creator> U. Munari, P. Valisa, G. L. Righetti, and S. Dallaporta  </creator>
	<author> U. Munari, P. Valisa, G. L. Righetti, and S. Dallaporta  </author>
	<creatoremail> ulisse.munari@inaf.it </creatoremail>
	<provenance> Credentialed by: U. Munari (ulisse.munari@oapd.inaf.it) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18083</identifier>
	<description> The S6,1 red giant SU Lyn was discovered by Mukai et al. (2016, MNRAS 461, L1) to be the counterpart of the unidentified hard X-ray source 4PBC J0642.9+5528 detected during the Swift Burst Alert Telescope (BAT) survey. ... </description>
	<dc:date>2026-10-01T10:25:49-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18074" >
	<title> ATel 18074: Spectroscopic Classification of Astrophysical Transients with the Lick Shane Telescope </title>
	<link> https://www.astronomerstelegram.org/?read=18074 </link>
	<creator> R. Kaur, R. J. Foley, K. C. Patra  </creator>
	<author> R. Kaur, R. J. Foley, K. C. Patra  </author>
	<creatoremail> ravkaur@ucsc.edu </creatoremail>
	<provenance> Credentialed by: Ravjit Kaur (ravkaur@ucsc.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18074</identifier>
	<description>  We report the classifications of astrophysical transients from spectroscopic observations with the Kast spectrograph on the Shane telescope obtained on 2026 September 21 UT. ... </description>
	<dc:date>2026-09-23T00:08:26-00:00</dc:date></item>

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