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	<title>The Astronomer's Telegram:  Cataclysmic Variable </title>
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	<description> Cataclysmic Variable, from The Astronomer's Telegram </description>

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<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=18083" />
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<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18045" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18033" />
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<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=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=18068" >
	<title> ATel 18068: A new superoutburst of the period-gap SU UMa-type dwarf nova Gaia22cax </title>
	<link> https://www.astronomerstelegram.org/?read=18068 </link>
	<creator> D. Yu. Rusanova, S. Dufoer, A. O. Simon, A. Yu. Korosko, J. K.T. Qvam, S. Kurowski, F.-J. Hambsch, W. Ogloza, N. Karaman, M. Dominik, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz  </creator>
	<author> D. Yu. Rusanova, S. Dufoer, A. O. Simon, A. Yu. Korosko, J. K.T. Qvam, S. Kurowski, F.-J. Hambsch, W. Ogloza, N. Karaman, M. Dominik, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz  </author>
	<creatoremail> andrii.o.simon@gmail.com </creatoremail>
	<provenance> Credentialed by: Andrew Simon (skazhenijandrew@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18068</identifier>
	<description> Gaia22cax/CSS101127:000130+050624/AT 2020qvd is an SU UMa-type dwarf nova located in the period gap. Kato et al. (2017; doi: 10.1093/pasj/psx058) reported a superhump period of 0.09477(1)d during its 2016 superoutburst. ... </description>
	<dc:date>2026-09-21T23:02:55-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18059" >
	<title> ATel 18059: Gaia20cnt: photometric observations of a new outburst </title>
	<link> https://www.astronomerstelegram.org/?read=18059 </link>
	<creator> D. Yu. Rusanova, A. O. Simon, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz, V. V. Vasylenko  </creator>
	<author> D. Yu. Rusanova, A. O. Simon, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz, V. V. Vasylenko  </author>
	<creatoremail> andrii.o.simon@gmail.com </creatoremail>
	<provenance> Credentialed by: Andrew Simon (skazhenijandrew@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18059</identifier>
	<description> The beginning of a new outburst of Gaia20cnt/ASASSN-14fc/AT 2020loj was detected during our monitoring of the object with a Unistellar eVscope (provided by Mike Simmons through the Astronomy for Equity program). ... </description>
	<dc:date>2026-09-19T07:45:08-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18056" >
	<title> ATel 18056: MGAB-V233: superhumps detected during the current superoutburst </title>
	<link> https://www.astronomerstelegram.org/?read=18056 </link>
	<creator> D. Yu. Rusanova, A. O. Simon, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz, J. K.T. Qvam, V. Bozza, S. Dufoer, S. Kurowski, V. V. Vasylenko  </creator>
	<author> D. Yu. Rusanova, A. O. Simon, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz, J. K.T. Qvam, V. Bozza, S. Dufoer, S. Kurowski, V. V. Vasylenko  </author>
	<creatoremail> andrii.o.simon@gmail.com </creatoremail>
	<provenance> Credentialed by: Andrew Simon (skazhenijandrew@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18056</identifier>
	<description> MGAB-V233 is a well-known ER UMa-type dwarf nova characterized by frequent superoutbursts and a short supercycle of approximately 70-90 days. Its superoutbursts typically last about 20-30 days. ... </description>
	<dc:date>2026-09-18T21:05:56-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18045" >
	<title> ATel 18045: Detection of superhumps in Gaia16ahk during its ongoing superoutburst  </title>
	<link> https://www.astronomerstelegram.org/?read=18045 </link>
	<creator> A. O. Simon, D. Yu. Rusanova, W. Ogloza, A. Yu. Korosko, P. J. Mikolajczyk, L.  Wyrzykowski, K. Kotysz, O. Witkowska ), K. Siennicki  </creator>
	<author> A. O. Simon, D. Yu. Rusanova, W. Ogloza, A. Yu. Korosko, P. J. Mikolajczyk, L.  Wyrzykowski, K. Kotysz, O. Witkowska ), K. Siennicki  </author>
	<creatoremail> andrii.o.simon@gmail.com </creatoremail>
	<provenance> Credentialed by: Andrew Simon (skazhenijandrew@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18045</identifier>
	<description> We identified Gaia16ahk/AT 2016dun as a promising candidate for an SU UMa-type dwarf nova. Consequently, the occurrence of its next superoutburst was predicted by our Outbursts Alerting System. ... </description>
	<dc:date>2026-09-15T18:56:08-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18033" >
	<title> ATel 18033: Follow-up Imaging &amp; Spectroscopy of Nova Sagittae 2026 (V488 Sge) </title>
	<link> https://www.astronomerstelegram.org/?read=18033 </link>
	<creator> M. Mugrauer, L. Maul, and P. Rajkumari  </creator>
	<author> M. Mugrauer, L. Maul, and P. Rajkumari  </author>
	<creatoremail> markus@astro.uni-jena.de </creatoremail>
	<provenance> Credentialed by: Markus Mugrauer (markus@astro.uni-jena.de) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18033</identifier>
	<description> We carried out follow-up imaging and spectroscopic observations of Nova Sagittae 2026 (ATel #18009) on 1 and 2 September 2026 at the University Observatory Jena. ... </description>
	<dc:date>2026-09-07T12:42:45-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18014" >
	<title> ATel 18014: Spectroscopic observations of Nova Sge 2026 (PNV J19450648+1822422) </title>
	<link> https://www.astronomerstelegram.org/?read=18014 </link>
	<creator> Gesesew Reta Habtie  </creator>
	<author> Gesesew Reta Habtie  </author>
	<creatoremail> gesesew@bose.res.in </creatoremail>
	<provenance> Credentialed by: Gesesew Reta Habtie (gesesew@bose.res.in) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18014</identifier>
	<description>  I report optical spectroscopic observations of the newly discovered nova Nova Sge 2026 (ATel #18009), located at RA (J2000) = 19h 45m 06.48s, Dec (J2000) = +18 &amp; deg; 22 &amp; prime; 42.2 &amp; Prime;. ... </description>
	<dc:date>2026-08-27T16:02:53-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18012" >
	<title> ATel 18012: Spectroscopic Classification of PNV J19450648+1822422 as an Fe II-type Nova with Concurrent Photometry </title>
	<link> https://www.astronomerstelegram.org/?read=18012 </link>
	<creator> Jingyuan Zhao, Jiashuo Zhang, Wang Li, Yaozhang Ou, Ezhar Elijan, Xinyan Chen  </creator>
	<author> Jingyuan Zhao, Jiashuo Zhang, Wang Li, Yaozhang Ou, Ezhar Elijan, Xinyan Chen  </author>
	<creatoremail> runwuyu20090722@foxmail.com </creatoremail>
	<provenance> Credentialed by: Kirill Sokolovsky (kirx@scan.sai.msu.ru) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18012</identifier>
	<description>  The NMW-TexasTech survey (Rokinon 135-mm f/2.2 telephoto lens + QHY600PH-M CMOS camera) discovered an optical transient of 9.0 mag in Sagitta on 2026 Aug 25.1278 UTC, and reported it to the CBAT Transient Objects Confirmation Page, where it was designated PNV J19450648+1822422 http://www.cbat.eps.harvard.edu/unconf/followups/J19450648+1822422.html Its possible progenitor star is Gaia DR3 1824166210904571136. ... </description>
	<dc:date>2026-08-26T14:28:29-00:00</dc:date></item>

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