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	<title>The Astronomer's Telegram:  Top ATels </title>
	<link> https://www.astronomerstelegram.org </link>
	<description> For reporting and commenting upon new observations of astronomical transients  by the professional astrophysics community. </description>

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

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<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18033" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18032" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18031" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18030" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18029" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18028" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18027" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18026" />
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<item rdf:about="https://www.astronomerstelegram.org/?read=18034" >
	<title> ATel 18034: NuSTAR follow-up of 4U 1630-47 in the hard intermediate state </title>
	<link> https://www.astronomerstelegram.org/?read=18034 </link>
	<creator> Maxime Parra, Pierre-Olivier Petrucci, Stefano Bianchi, Floriane Cangemi, Alessio Marino, Poshak Gandhi, Megumi Shidatsu, et al. </creator>
	<author> Maxime Parra, Pierre-Olivier Petrucci, Stefano Bianchi, Floriane Cangemi, Alessio Marino, Poshak Gandhi, Megumi Shidatsu, et al. </author>
	<creatoremail> maxime.parrastro@gmail.com </creatoremail>
	<provenance> Credentialed by: Maxime Parra (maxime.parra@univ-grenoble-alpes.fr) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18034</identifier>
	<description> We report on a follow-up NuSTAR exposure on the Transient Black Hole LMXB candidate 4U 1630-47, obtained as part of an XMM-NuSTAR large program, following the detection of the source by SVOM (Atel #18030). ... </description>
	<dc:date>2026-09-07T18:27:22-00:00</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=18032" >
	<title> ATel 18032: Fermi-LAT detection of gamma-ray activity from the Seyfert 1 galaxy source PKS 0521-36 </title>
	<link> https://www.astronomerstelegram.org/?read=18032 </link>
	<creator> F. Casaburo, S. Ciprini  on behalf of the Fermi Large Area Telescope Collaboration </creator>
	<author> F. Casaburo, S. Ciprini  on behalf of the Fermi Large Area Telescope Collaboration </author>
	<creatoremail> fausto.casaburo@roma2.infn.it </creatoremail>
	<provenance> Credentialed by: Giovanni La Mura (giovanni.lamura@inaf.it) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18032</identifier>
	<description>   The Large Area Telescope (LAT), one of the two instruments on the Fermi Gamma-ray Space Telescope, has observed gamma-ray activity from a source positionally consistent with the Seyfert 1 galaxy PKS 0521-36, also known as 4FGL J0522.9-3628 (Abdollahi et al. ... </description>
	<dc:date>2026-09-06T20:43:58-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18031" >
	<title> ATel 18031: MAXI/GSC observation of an X-ray outburst from the Be/X-ray binary pulsar GS 0834-430 </title>
	<link> https://www.astronomerstelegram.org/?read=18031 </link>
	<creator> M. Nakajima, H. Negoro, M. Serino, S. Sugita, K. Saito, T. Yokoyama, M. Wada, T. Mihara, T. Tamagawa, N. Kawai, M. Matsuoka, T. Sakamoto, Y. Kawakubo, H. Hiramatsu, A. Yoshida, Y. Tsuboi, Y. Ishihara, H. Ogaki, M. Shidatsu, C. Kang, M. Uenishi, T. Usuki, S. Yatsuzuka, H. Aoe, I. Takahashi, Y. Yatsu, S. Nakahira, S. Ueno, H. Tomida, M. Kurihara, Y. Ueda, K. Fujiwara, S. Kobayashi, M. Yamauchi, M. Nishio, C. Hiraizumi, K. Yamaoka, M. Sugizaki, W. Iwakiri, T. Kawamuro, S. Yamada, S. Ogawa  </creator>
	<author> M. Nakajima, H. Negoro, M. Serino, S. Sugita, K. Saito, T. Yokoyama, M. Wada, T. Mihara, T. Tamagawa, N. Kawai, M. Matsuoka, T. Sakamoto, Y. Kawakubo, H. Hiramatsu, A. Yoshida, Y. Tsuboi, Y. Ishihara, H. Ogaki, M. Shidatsu, C. Kang, M. Uenishi, T. Usuki, S. Yatsuzuka, H. Aoe, I. Takahashi, Y. Yatsu, S. Nakahira, S. Ueno, H. Tomida, M. Kurihara, Y. Ueda, K. Fujiwara, S. Kobayashi, M. Yamauchi, M. Nishio, C. Hiraizumi, K. Yamaoka, M. Sugizaki, W. Iwakiri, T. Kawamuro, S. Yamada, S. Ogawa  </author>
	<creatoremail> nakajima.motoki@nihon-u.ac.jp </creatoremail>
	<provenance> Credentialed by: Motoki Nakajima (nakajima.motoki@nihon-u.ac.jp) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18031</identifier>
	<description> The MAXI/GSC nova alert system triggered an X-ray transient source at (R.A., Dec) = (128 deg, -43 deg) on August 29, 2026 (MJD 61281). Since the source was observed during high-background orbits in late August, its position could not be precisely determined from those scans. ... </description>
	<dc:date>2026-09-06T08:02:19-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18030" >
	<title> ATel 18030: SVOM/ECLAIRs detection of a possible new outburst onset from the black hole 4U 1630-472 </title>
	<link> https://www.astronomerstelegram.org/?read=18030 </link>
	<creator> F. Cangemi, S. Le Stum, A. Coleiro, O. Godet, J. Rodriguez, Y.-H. I. Yin, R.-C. Chen, L. Tao, L. Zhang  </creator>
	<author> F. Cangemi, S. Le Stum, A. Coleiro, O. Godet, J. Rodriguez, Y.-H. I. Yin, R.-C. Chen, L. Tao, L. Zhang  </author>
	<creatoremail> cangemi@apc.in2p3.fr </creatoremail>
	<provenance> Credentialed by: Floriane Cangemi (cangemi@apc.in2p3.fr) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18030</identifier>
	<description> On 2026 September 2 at 01:59:31.116 UT, the onboard trigger software of the SVOM/ECLAIRs telescope (4-150 keV) detected and localized a source at R.A. = 248.506 deg and Dec. ... </description>
	<dc:date>2026-09-04T13:05:22-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18029" >
	<title> ATel 18029: Spectroscopic classification of AT 2026aabo as a bright nova in M31 </title>
	<link> https://www.astronomerstelegram.org/?read=18029 </link>
	<creator> Shatakshi Chamoli, Judhajeet Basu, Sudhanshu Barway, G. C. Anupama, Tanishk Mohan, Aditya Pawan Saikia,  Vishwajeet Swain, Sameer Patil, Varun Bhalerao, Srikanth Bandari  </creator>
	<author> Shatakshi Chamoli, Judhajeet Basu, Sudhanshu Barway, G. C. Anupama, Tanishk Mohan, Aditya Pawan Saikia,  Vishwajeet Swain, Sameer Patil, Varun Bhalerao, Srikanth Bandari  </author>
	<creatoremail> shatakshi.chamoli@iiap.res.in </creatoremail>
	<provenance> Credentialed by: Judhajeet Basu (judhajeet.basu@iiap.res.in) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18029</identifier>
	<description>  We report the spectroscopic classification of AT 2026aabo as a very bright and slowly evolving nova in M31.  This transient was first discovered on 2026-08-29T09:28:57 by ZTF Collaboration and reported on TNS at 18.57 mags in the ZTF-g band. ... </description>
	<dc:date>2026-09-03T07:45:36-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18028" >
	<title> ATel 18028: NuSTAR detection of shock-powered X-rays from Nova Sagittae 2026 = V488 Sge </title>
	<link> https://www.astronomerstelegram.org/?read=18028 </link>
	<creator> Kirill Sokolovsky, Katie Barnhart, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi, Laura Chomiuk, Peter Craig, Isabella Molina, Jennifer Sokoloski, Justin Linford, Koji Mukai  </creator>
	<author> Kirill Sokolovsky, Katie Barnhart, Darien Perla, Pragati Acharya, John Worley, Anthony Pearce, Vallia Antoniou, Elias Aydi, Laura Chomiuk, Peter Craig, Isabella Molina, Jennifer Sokoloski, Justin Linford, 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>ATel18028</identifier>
	<description>  Nova Sagittae 2026 (V488 Sge, PNV J19450648+1822422) was discovered on its rise to optical peak by the NMW-TexasTech  survey at 2026-08-25.1278 UTC having an unfiltered magnitude 9.0 (CBET #5729, ATel #18008, #18009, #18012, #18014, #18021, #18022). ... </description>
	<dc:date>2026-09-02T19:29:39-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18027" >
	<title> ATel 18027: AT 2026aabo (ZTF26abramlb, ATLAS26kqn): a bright nova candidate in M31 </title>
	<link> https://www.astronomerstelegram.org/?read=18027 </link>
	<creator> I. Perez-Fournon, F. Poidevin, A. Lopez-Oramas,  D. Aguado, N. Abreu Garcia, D. Cano-Morales, I. Correa-Plasencia,  A. E. Hernandez-Diaz, E. Lekaroz-Urriza, M. Magdalena-Rodriguez, M. Quintana-Ansaldo,  D. Rodriguez-Fernandez, and J. Uribarri-Dermit  </creator>
	<author> I. Perez-Fournon, F. Poidevin, A. Lopez-Oramas,  D. Aguado, N. Abreu Garcia, D. Cano-Morales, I. Correa-Plasencia,  A. E. Hernandez-Diaz, E. Lekaroz-Urriza, M. Magdalena-Rodriguez, M. Quintana-Ansaldo,  D. Rodriguez-Fernandez, and J. Uribarri-Dermit  </author>
	<creatoremail> ipf@iac.es </creatoremail>
	<provenance> Credentialed by: Ismael Perez-Fournon (ipf@iac.es) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18027</identifier>
	<description> We report ATLAS forced photometry of the bright nova candidate AT 2026aabo (ZTF26abramlb, ATLAS26kqn). This transient was discovered by Anirudh Salgundi on behalf of ZTF (TNS Astronomical Transient Report No. ... </description>
	<dc:date>2026-09-02T11:55:55-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18026" >
	<title> ATel 18026: Insight-HXMT observations of a soft X-ray flare and a possible QPO-type transition in MAXI J1750-327 / EP260812c (Format Corrected) </title>
	<link> https://www.astronomerstelegram.org/?read=18026 </link>
	<creator> B. Y. Chen, W. Z. Li, Q. C. Shui, Y. P. Chen, S. Zhang, S. N. Zhang, H. Feng, L. Tao, L. Zhang, S. M. Jia, X. B. Li, F. J. Lu, L. M. Song, S. J. Zheng, C. K. Li, Z. X. Li, G. L. Huang, Q. C. Zhao, on behalf of the Insight-HXMT team </creator>
	<author> B. Y. Chen, W. Z. Li, Q. C. Shui, Y. P. Chen, S. Zhang, S. N. Zhang, H. Feng, L. Tao, L. Zhang, S. M. Jia, X. B. Li, F. J. Lu, L. M. Song, S. J. Zheng, C. K. Li, Z. X. Li, G. L. Huang, Q. C. Zhao, on behalf of the Insight-HXMT team </author>
	<creatoremail> bychen@ihep.ac.cn </creatoremail>
	<provenance> Credentialed by: Yu-Peng Chen (chenyp@ihep.ac.cn) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18026</identifier>
	<description> MAXI J1750-327 / EP260812c / EP J175003.0-324244 was discovered by MAXI/GSC and Einstein Probe (ATels #17963 and #17964) and was subsequently identified as a black-hole X-ray binary candidate based on its X-ray spectral and timing properties (ATels #17969 and #17974). ... </description>
	<dc:date>2026-09-01T13:41:04-00:00</dc:date></item>
<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>

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