<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF
 xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" 
 xmlns="http://purl.org/rss/1.0/"
 xmlns:dc="http://purl.org/dc/elements/1.1/" >
 <channel rdf:about="https://www.astronomerstelegram.org/?rss+Variables" >
	<title>The Astronomer's Telegram:  Variables </title>
	<link> https://www.astronomerstelegram.org </link>
	<description> Variables, from The Astronomer's Telegram </description>

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

<items>
<rdf:Seq>

<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18025" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18009" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18008" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18005" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17989" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17981" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17972" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17962" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17951" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17947" />
</rdf:Seq></items></channel>

<item rdf:about="https://www.astronomerstelegram.org/?read=18025" >
	<title> ATel 18025: XMM-Newton detection of a high flux state in the HMXRB IGR J13020-6359 </title>
	<link> https://www.astronomerstelegram.org/?read=18025 </link>
	<creator> Robbie Webbe, Natalie A. Webb, Erwan Quintin, Laurent Michel  </creator>
	<author> Robbie Webbe, Natalie A. Webb, Erwan Quintin, Laurent Michel  </author>
	<creatoremail> robbie.webbe@cnrs.fr </creatoremail>
	<provenance> Credentialed by: Robbie Webbe (robbie.webbe@cnrs.fr) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18025</identifier>
	<description> We report the detection of X-ray brightening from the source IGR J13020-6359 with the XMM-Newton X-ray telescope in the energy range 0.2-12.0 keV.  On 7th August 2026 IGR J13020-6359 was observed in the field of view of an XMM-Newton observation, and the long-term variability was assessed using the multi-observatory STONKS pipeline. ... </description>
	<dc:date>2026-09-01T10:23:44-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18009" >
	<title> ATel 18009: Discovery and follow up observations of the likely Galactic Nova NMW-TTU-26bp (PNV J19450648+1822422) </title>
	<link> https://www.astronomerstelegram.org/?read=18009 </link>
	<creator> Katie Barnhart, Kirill Sokolovsky, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi, Bassam Debs, and Omar Kilo . </creator>
	<author> Katie Barnhart, Kirill Sokolovsky, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi, Bassam Debs, and Omar Kilo . </author>
	<creatoremail> eaydi@ttu.edu </creatoremail>
	<provenance> Credentialed by: Elias Aydi (eaydi@ttu.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18009</identifier>
	<description>  We report the discovery of the likely Galactic nova NMW-TTU-26bp (PNV J19450648+1822422). The transient was discovered by the NMW-TexasTech survey on 2026-08-25.12 UTC at an unfiltered magnitude of 9.0. ... </description>
	<dc:date>2026-08-25T18:04:56-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18008" >
	<title> ATel 18008: Spectroscopic Observation of PNV J19450648+1822422: Likely a Classical Nova? </title>
	<link> https://www.astronomerstelegram.org/?read=18008 </link>
	<creator> Kenta Taguchi, Akira Arai  </creator>
	<author> Kenta Taguchi, Akira Arai  </author>
	<creatoremail> kentagch@kusastro.kyoto-u.ac.jp </creatoremail>
	<provenance> Credentialed by: Keisuke Isogai (isogai@kusastro.kyoto-u.ac.jp) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18008</identifier>
	<description>     We report the spectroscopic observation of PNV J19450648+1822422.    We obtained its spectrum on 2026-08-25.431 UT with the fiber-fed integral field spectrograph (KOOLS-IFU; Matsubayashi et al. ... </description>
	<dc:date>2026-08-25T11:52:59-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18005" >
	<title> ATel 18005: Gaia16amd: a new SU UMa-type dwarf nova </title>
	<link> https://www.astronomerstelegram.org/?read=18005 </link>
	<creator> A. O. Simon, D. Yu. Rusanova, F.-J. Hambsch, W. Ogloza, N. Karaman, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz  </creator>
	<author> A. O. Simon, D. Yu. Rusanova, F.-J. Hambsch, W. Ogloza, N. Karaman, A. Yu. Korosko, 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>ATel18005</identifier>
	<description> Gaia16amd/MASTER OT J203529.80+063652.8/AT 2016dyj was identified by our Outbursts Alerting System as a promising candidate for an SU UMa-type dwarf nova. ... </description>
	<dc:date>2026-08-25T09:06:51-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17989" >
	<title> ATel 17989: Spectroscopic Classification of TCP J18251276-2225293 as a Classical Nova </title>
	<link> https://www.astronomerstelegram.org/?read=17989 </link>
	<creator> Kenta Taguchi  </creator>
	<author> Kenta Taguchi  </author>
	<creatoremail> kentagch@kusastro.kyoto-u.ac.jp </creatoremail>
	<provenance> Credentialed by: Keisuke Isogai (isogai@kusastro.kyoto-u.ac.jp) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel17989</identifier>
	<description>       I report the spectroscopic classification of TCP J18251276-2225293 (ATel #17987) as a classical nova.    I obtained its spectrum on 2026-08-19.482 UT with the fiber-fed integral field spectrograph (KOOLS-IFU; Matsubayashi et al. ... </description>
	<dc:date>2026-08-19T14:56:50-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17981" >
	<title> ATel 17981: Gaia22dbc: a new SU UMa-type dwarf nova during its ongoing superoutburst </title>
	<link> https://www.astronomerstelegram.org/?read=17981 </link>
	<creator> A. O. Simon, S. A. Simon-Reshetnik, D. Yu. Rusanova, A. V. Grytsai, M. V. Matiushenko, A. Yu. Korosko, P. J. Mikolajczyk, {\L}. Wyrzykowski, K. Kotysz, Y. V. Rudnieva  </creator>
	<author> A. O. Simon, S. A. Simon-Reshetnik, D. Yu. Rusanova, A. V. Grytsai, M. V. Matiushenko, A. Yu. Korosko, P. J. Mikolajczyk, {\L}. Wyrzykowski, K. Kotysz, Y. V. Rudnieva  </author>
	<creatoremail> andrii.o.simon@gmail.com </creatoremail>
	<provenance> Credentialed by: Andrew Simon (skazhenijandrew@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel17981</identifier>
	<description> Gaia22dbc/ASASSN-15qa/AT 2022qcr was identified by our Outbursts Alerting System as a promising candidate for an SU UMa-type dwarf nova.   Analysis of its long-term light curve revealed, in addition to relatively short outbursts lasting about 4 days, two substantially longer outbursts that are likely superoutbursts. ... </description>
	<dc:date>2026-08-17T20:25:07-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17972" >
	<title> ATel 17972: Optical spectro-photometric follow up of nova Tauri 2026 (TCP J05210763+2338194) </title>
	<link> https://www.astronomerstelegram.org/?read=17972 </link>
	<creator> Pragati Acharya, Willem Hoogendam, Kirill V. Sokolovsky, Darien Perla, Katie Barnhart, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi  </creator>
	<author> Pragati Acharya, Willem Hoogendam, Kirill V. Sokolovsky, Darien Perla, Katie Barnhart, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi  </author>
	<creatoremail> eaydi@ttu.edu </creatoremail>
	<provenance> Credentialed by: Elias Aydi (eaydi@ttu.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel17972</identifier>
	<description>  We report optical spectroscopy and photometry of Nova Tauri 2026 (TCP J05210763+2338194), which was discovered on 2026 Aug 06.41 UTC at unfiltered magnitude of 11.2 by the NMW-TexasTech survey (ATel #17947) and spectroscopically confirmed as a classical nova on 2026 Aug 8.125 (ATel #17950). ... </description>
	<dc:date>2026-08-15T23:40:36-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17962" >
	<title> ATel 17962: Detection of superhumps in the ER UMa-type dwarf nova Gaia24aeg  </title>
	<link> https://www.astronomerstelegram.org/?read=17962 </link>
	<creator> D. Yu. Rusanova, A. O. Simon, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz, M. V. Matiushenko, V. V. Vasylenko  </creator>
	<author> D. Yu. Rusanova, A. O. Simon, A. Yu. Korosko, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz, M. V. Matiushenko, 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>ATel17962</identifier>
	<description> Gaia24aeg/AT 2024re/ASASSN-18hr is an ER UMa-type dwarf nova characterized by frequent superoutbursts, with a typical superoutburst recurrence time of 55-65 days. ... </description>
	<dc:date>2026-08-12T20:16:31-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17951" >
	<title> ATel 17951: Detection of Superhumps during a Superoutburst in Gaia20ffw </title>
	<link> https://www.astronomerstelegram.org/?read=17951 </link>
	<creator> D. Yu. Rusanova, F.-J. Hambsch, A. O. Simon, P. J. Mikolajczyk, L. Wyrzykowski, K. Kotysz  </creator>
	<author> D. Yu. Rusanova, F.-J. Hambsch, A. O. Simon, 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>ATel17951</identifier>
	<description> We report the detection of superhumps during a superoutburst in the cataclysmic variable Gaia20ffw/AT2020znz/ASASSN-18jq, which was detected by our Outbursts Alerting System. ... </description>
	<dc:date>2026-08-09T08:57:22-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17947" >
	<title> ATel 17947: Photometric follow up observations of the possible Galactic Nova in Taurus TCP J05210763+2338194 </title>
	<link> https://www.astronomerstelegram.org/?read=17947 </link>
	<creator> Elias Aydi, Kirill Sokolovsky, Katie Barnhart, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Bassam Debs, Omar Kilo  </creator>
	<author> Elias Aydi, Kirill Sokolovsky, Katie Barnhart, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Bassam Debs, Omar Kilo  </author>
	<creatoremail> eaydi@ttu.edu </creatoremail>
	<provenance> Credentialed by: Elias Aydi (eaydi@ttu.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel17947</identifier>
	<description>  We report photometric follow-up of the possible Galactic nova TCP J05210763+2338194, which was discovered by the NMW-TexasTech survey on 2026-08-06.4109 UT at an unfiltered magnitude of 11.2. ... </description>
	<dc:date>2026-08-07T16:55:31-00:00</dc:date></item>

</rdf:RDF>