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

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<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18030" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18026" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18024" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18017" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18016" />
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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=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=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=18024" >
	<title> ATel 18024: Insight-HXMT observations of a soft X-ray flare and a possible QPO-type transition in MAXI J1750-327 </title>
	<link> https://www.astronomerstelegram.org/?read=18024 </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> chenyp@ihep.ac.cn </creatoremail>
	<provenance> Credentialed by: Yu-Peng Chen (chenyp@ihep.ac.cn) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18024</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>2026-09-01T02:15:25-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18017" >
	<title> ATel 18017: Radio flux density monitoring of MAXI J1750-327 with the Yamaguchi Interferometer (format corrected) </title>
	<link> https://www.astronomerstelegram.org/?read=18017 </link>
	<creator> Masanori Akimoto, Shogo Nohara, Hibiki Fujii, Natsuki Maekawa, Kotaro Ninuma, Kenta Fujisawa  </creator>
	<author> Masanori Akimoto, Shogo Nohara, Hibiki Fujii, Natsuki Maekawa, Kotaro Ninuma, Kenta Fujisawa  </author>
	<creatoremail> m-akimoto2025@yamaguchi-u.ac.jp </creatoremail>
	<provenance> Credentialed by: Kenta Fujisawa (kenta@yamaguchi-u.ac.jp) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18017</identifier>
	<description>  This contains the same information as ATel #18016 but is correctly formatted.   MAXI J1750-327 was discovered as a new X-ray transient by MAXI on 2026-08-13, and was also detected by Einstein Probe as EP 260812c (ATel #17963, #17964). ... </description>
	<dc:date>2026-08-28T01:19:55-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18016" >
	<title> ATel 18016: Radio flux density monitoring of MAXI J1750-327 with the Yamaguchi Interferometer </title>
	<link> https://www.astronomerstelegram.org/?read=18016 </link>
	<creator> Masanori Akimoto, Shogo Nohara, Hibiki Fujii, Natsuki Maekawa, Kotaro Ninuma, Kenta Fujisawa  </creator>
	<author> Masanori Akimoto, Shogo Nohara, Hibiki Fujii, Natsuki Maekawa, Kotaro Ninuma, Kenta Fujisawa  </author>
	<creatoremail> m-akimoto2025@yamaguchi-u.ac.jp </creatoremail>
	<provenance> Credentialed by: Kenta Fujisawa (kenta@yamaguchi-u.ac.jp) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18016</identifier>
	<description> MAXI J1750-327 was discovered as a new X-ray transient by MAXI on 2026-08-13, and was also detected by Einstein Probe as EP 260812c (ATel #17963, #17964). ... </description>
	<dc:date>2026-08-28T00:13:05-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18015" >
	<title> ATel 18015: MeerKAT monitoring reveals GX 339-4 to be in a radio quiescent state </title>
	<link> https://www.astronomerstelegram.org/?read=18015 </link>
	<creator> Miriam M. Nyamai, Rob P. Fender,, Sara Motta, Noa Grollimund  for the X-KAT collaboration </creator>
	<author> Miriam M. Nyamai, Rob P. Fender,, Sara Motta, Noa Grollimund  for the X-KAT collaboration </author>
	<creatoremail> nyamai@jive.eu </creatoremail>
	<provenance> Credentialed by: Miriam Mumbua Nyamai (nyamai@jive.eu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18015</identifier>
	<description>   As part of the X-KAT Large Survey programme with the MeerKAT telescope, the recurrent black hole X-ray binary GX 339-4 is observed weekly, usually at 1.284 GHz (L-band). ... </description>
	<dc:date>2026-08-27T17:43:45-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18010" >
	<title> ATel 18010: XSPECT observation of the newly discovered black hole transient MAXI J1750-327 / EP260812c: Detection of variable low frequency QPOs </title>
	<link> https://www.astronomerstelegram.org/?read=18010 </link>
	<creator> Rwitika Chatterjee, Vivek Kumar Agrawal, Biswajit Paul, Anuj Nandi  </creator>
	<author> Rwitika Chatterjee, Vivek Kumar Agrawal, Biswajit Paul, Anuj Nandi  </author>
	<creatoremail> rwitika@ursc.gov.in </creatoremail>
	<provenance> Credentialed by: Rwitika Chatterjee (rwitika@ursc.gov.in) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18010</identifier>
	<description> MAXI J1750-327 was discovered as a new X-ray transient by the MAXI/GSC nova alert system on 2026 August 13 (ATel #17963), with the source also detected by the EP/WXT approximately five hours earlier and designated EP260812c (ATel #17964). ... </description>
	<dc:date>2026-08-25T18:30:42-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18007" >
	<title> ATel 18007: ALMA + VLA observations of MAXI J1750-327 </title>
	<link> https://www.astronomerstelegram.org/?read=18007 </link>
	<creator> A. J. Tetarenko, E. Lescure, A. Bahramian, J. C.A. Miller-Jones,  P. Casella, N. Castro Segura, P. Gandhi, T. J. Maccarrone, A. Marino, T. D. Russell, J. van den Eijnden, and F. M. Vincentelli  </creator>
	<author> A. J. Tetarenko, E. Lescure, A. Bahramian, J. C.A. Miller-Jones,  P. Casella, N. Castro Segura, P. Gandhi, T. J. Maccarrone, A. Marino, T. D. Russell, J. van den Eijnden, and F. M. Vincentelli  </author>
	<creatoremail> alexandra.tetarenko@uleth.ca </creatoremail>
	<provenance> Credentialed by: Alexandra Tetarenko (alexandra.tetarenko@uleth.ca) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18007</identifier>
	<description> www.astronomerstelegram.org/?read=17963 &gt; 17963, #17964). Since then, it has been extensively characterized through X-ray (ATels #17969, #17974, #17983, #17993, #18004), optical/near-infrared (ATels #17971, #17977, #17988, #17990), and radio (ATel #17979) observations. ... </description>
	<dc:date>2026-08-25T10:23:37-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18004" >
	<title> ATel 18004: NuSTAR observation of the new black hole transient MAXI J1750-327/EP260812c </title>
	<link> https://www.astronomerstelegram.org/?read=18004 </link>
	<creator> S. Mandel, K. Mori, C. Hailey, M. Parra, A. Marino, N. Degenaar, R. Wijnands, J. Tomsick, M. Bachetti, P. Draghis, J. Grindlay, J. Hong, G. Ponti, M. Reynolds  </creator>
	<author> S. Mandel, K. Mori, C. Hailey, M. Parra, A. Marino, N. Degenaar, R. Wijnands, J. Tomsick, M. Bachetti, P. Draghis, J. Grindlay, J. Hong, G. Ponti, M. Reynolds  </author>
	<creatoremail> ss5018@columbia.edu </creatoremail>
	<provenance> Credentialed by: Shifra Mandel (ss5018@columbia.edu) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18004</identifier>
	<description> We report on a follow-up NuSTAR observation of the new X-ray transient MAXI J1750-327, which was detected by MAXI on Aug. 13, 2026 (ATel #17963), as well as by Einstein Probe WXT on Aug. ... </description>
	<dc:date>2026-08-25T01:43:18-00:00</dc:date></item>

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