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	<title>The Astronomer's Telegram:  Neutron Star </title>
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	<description> Neutron Star, from The Astronomer's Telegram </description>

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<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18089" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18082" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18071" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18067" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18063" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18051" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18040" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=18039" />
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<item rdf:about="https://www.astronomerstelegram.org/?read=18089" >
	<title> ATel 18089: Detection of 205.7 s X-ray pulsations from the Be/X-ray binary pulsar LS V +44 17 during its September 2026 outburst </title>
	<link> https://www.astronomerstelegram.org/?read=18089 </link>
	<creator> Manoj Mandal, Sachindra Naik   </creator>
	<author> Manoj Mandal, Sachindra Naik   </author>
	<creatoremail> manojmandal@prl.res.in </creatoremail>
	<provenance> Credentialed by: Manoj Mandal (manojmandal@prl.res.in) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18089</identifier>
	<description> We report preliminary timing and spectral results from the XPoSat/XSPECT observations of the Be/X-ray binary pulsar LS V +44 17 (RX J0440.9+4431) during its ongoing September 2026 X-ray outburst. ... </description>
	<dc:date>2026-10-04T09:02:31-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18082" >
	<title> ATel 18082: SRG/ART-XC detection of the possible new outburst of AX J1820.5-1434 </title>
	<link> https://www.astronomerstelegram.org/?read=18082 </link>
	<creator> I. Mereminskiy, A. Semena, A. Lutovinov, S. Molkov, A. Tkachenko  </creator>
	<author> I. Mereminskiy, A. Semena, A. Lutovinov, S. Molkov, A. Tkachenko  </author>
	<creatoremail> i.a.mereminskiy@gmail.com </creatoremail>
	<provenance> Credentialed by: Andrey Semena (san@iki.rssi.ru) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18082</identifier>
	<description> During the observations of the Galactic Plane on Sept. 28, 2026, the Mikhail Pavlinsky ART-XC telescope onboard the SRG observatory detected a bright X-ray source at the position of RA, Dec = 275.1232, -14.5692 (estimated 90% containment radius of 10''), with the observed X-ray flux in 4-12 keV of (7.9+-0.2)x10^-11 erg cm-2 s-1. ... </description>
	<dc:date>2026-09-29T13:22:42-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18071" >
	<title> ATel 18071: MAXI/GSC observation of a series of X-ray outbursts with a &amp;sim;60 day interval from the Be/X-ray binary pulsar LS V +44 17 (RX J0440.9+4431) </title>
	<link> https://www.astronomerstelegram.org/?read=18071 </link>
	<creator> M. Nakajima, H. Negoro, T. Mihara, K. Saito, T. Yokoyama, M. Wada, T. Tamagawa, N. Kawai, M. Matsuoka, T. Sakamoto, M. Serino, S. Sugita, 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, T. Mihara, K. Saito, T. Yokoyama, M. Wada, T. Tamagawa, N. Kawai, M. Matsuoka, T. Sakamoto, M. Serino, S. Sugita, 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>ATel18071</identifier>
	<description> We report on anomalous X-ray activity from the Be/X-ray binary pulsar LS V +44 17 (RX J0440.9+4431). This binary system, hosting a  &amp; sim;205 sec X-ray pulsar, had previously been suggested to have an orbital period of  &amp; sim;150 days, estimated from the recurrence intervals of a series of X-ray outbursts observed in 2010-2011 (Reig 2011; Tsygankov et al. ... </description>
	<dc:date>2026-09-22T13:10:54-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18067" >
	<title> ATel 18067: The GBM Accreting Pulsar Project detects pulsations from the HMXB J0440.9+4431 (LSV+44) </title>
	<link> https://www.astronomerstelegram.org/?read=18067 </link>
	<creator> Peter Jenke, Colleen Wilson-Hodge, Christian Malacaria   </creator>
	<author> Peter Jenke, Colleen Wilson-Hodge, Christian Malacaria   </author>
	<creatoremail> peter.a.jenke@nasa.gov </creatoremail>
	<provenance> Credentialed by: Peter Jenke (peter.a.jenke@nasa.gov) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18067</identifier>
	<description> The GBM Accreting Pulsar Project (GAPP) is detecting pulsations from the transient Be/X-ray binary RX J0440.9+4431 (LSV+44) starting September 17, 2026. ... </description>
	<dc:date>2026-09-21T20:22:38-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18063" >
	<title> ATel 18063: EP-WXT detection of on-going X-ray brightening likely from LS V +44 17 </title>
	<link> https://www.astronomerstelegram.org/?read=18063 </link>
	<creator> Tian-Yu Liu, K. R. Ni, S. Q. Zheng, Jin-Rui Liu, G. J. Yang, B. B. Zhang and Z.-X. Ling, on behalf of the Einstein Probe  team: </creator>
	<author> Tian-Yu Liu, K. R. Ni, S. Q. Zheng, Jin-Rui Liu, G. J. Yang, B. B. Zhang and Z.-X. Ling, on behalf of the Einstein Probe  team: </author>
	<creatoremail> ep_ta@bao.ac.cn </creatoremail>
	<provenance> Credentialed by: Yuan Liu (liuyuan@bao.ac.cn) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18063</identifier>
	<description> We report on the detection of X-ray brightening, likely from LS V +44 17, by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission. ... </description>
	<dc:date>2026-09-20T18:56:46-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18051" >
	<title> ATel 18051:  Swift/XRT detects an X-ray decline in 1A 0538-66 </title>
	<link> https://www.astronomerstelegram.org/?read=18051 </link>
	<creator> G. K. Jaisawal   </creator>
	<author> G. K. Jaisawal   </author>
	<creatoremail> gaurava@space.dtu.dk </creatoremail>
	<provenance> Credentialed by: Gaurava Kumar Jaisawal (gaurava.jaisawal@gmail.com) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18051</identifier>
	<description> We report on a Swift/XRT observation of the Be/X-ray binary pulsar 1A 0538-66 following the trigger of a major X-ray outburst detected by MAXI/GSC on 2026 August 28 (ATel #18020). ... </description>
	<dc:date>2026-09-17T11:47:13-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18040" >
	<title> ATel 18040: The magnetar XTE J1810-197 remains in radio quiescence </title>
	<link> https://www.astronomerstelegram.org/?read=18040 </link>
	<creator> Marcus E. Lower, Jade Salisbury, Ryan M. Shannon, Fernando Camilo, Paul Scholz, George Younes, John E. Reynolds  and John M. Sarkissian  </creator>
	<author> Marcus E. Lower, Jade Salisbury, Ryan M. Shannon, Fernando Camilo, Paul Scholz, George Younes, John E. Reynolds  and John M. Sarkissian  </author>
	<creatoremail> mlower@swin.edu.au </creatoremail>
	<provenance> Credentialed by: Marcus Lower (mlower@swin.edu.au) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18040</identifier>
	<description> Following a reported X-ray burst from the direction of the magnetar XTE J1810-197 (PSR J1809-1943) by MAXI/GSC (ATel #18039), we triggered a search for renewed radio emission using the Ultra-Wideband Low (UWL; Hobbs et al. ... </description>
	<dc:date>2026-09-14T09:25:02-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=18039" >
	<title> ATel 18039: MAXI/GSC detection of bright X-ray burst-like activity positionally  consistent with XTE J1810-197 and XTE J1810-189 </title>
	<link> https://www.astronomerstelegram.org/?read=18039 </link>
	<creator> H. Negoro, M. Serino,  M. Nakajima, K. Saito, T. Yokoyama, M. Wada,  T. Mihara, T. Tamagawa, N. Kawai, M. Matsuoka,  T. Sakamoto, S. Sugita, 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, and S. Ogawa  </creator>
	<author> H. Negoro, M. Serino,  M. Nakajima, K. Saito, T. Yokoyama, M. Wada,  T. Mihara, T. Tamagawa, N. Kawai, M. Matsuoka,  T. Sakamoto, S. Sugita, 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, and S. Ogawa  </author>
	<creatoremail> negoro.hitoshi@nihon-u.ac.jp </creatoremail>
	<provenance> Credentialed by: Hitoshi Negoro (negoro@phys.cst.nihon-u.ac.jp) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel18039</identifier>
	<description> MAXI/GSC detected bright X-ray burst-like activity lasting more than 30 sec at 12:43 UT on September 12, 2026. Assuming that the source flux was constant over the transit, we obtain the source position at (R.A., Dec) = (272.340 deg, -19.668 deg) = (18 09 22, -19 40 05 (J2000) with a statistical 90% C.L. ... </description>
	<dc:date>2026-09-12T16:49:24-00:00</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=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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