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	<title>The Astronomer's Telegram:  Neutron Star </title>
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<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17815" />
<rdf:li rdf:resource="https://www.astronomerstelegram.org/?read=17772" />
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<item rdf:about="https://www.astronomerstelegram.org/?read=17818" >
	<title> ATel 17818: Einstein Probe catches the onset of a new outburst from the NS LMXB MXB 1730-335 (Rapid Burster) </title>
	<link> https://www.astronomerstelegram.org/?read=17818 </link>
	<creator> Alessio Marino, Francesco Coti Zelati, Nanda Rea, Yilong Wang, Giulia Illiano, Minghao Zhang, Chen Wang, Biao Zhang, Jiapei Feng, Haiwu Pan   </creator>
	<author> Alessio Marino, Francesco Coti Zelati, Nanda Rea, Yilong Wang, Giulia Illiano, Minghao Zhang, Chen Wang, Biao Zhang, Jiapei Feng, Haiwu Pan   </author>
	<creatoremail> marino@ice.csic.es </creatoremail>
	<provenance> Credentialed by: Alessio Marino (marino@ice.csic.es) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel17818</identifier>
	<description> We report on the detection of a new outburst from the neutron star low-mass X-ray binary MXB 1730-335 (a.k.a. the Rapid Burster) with the Wide-field X-ray Telescope (WXT) onboard Einstein Probe (EP). ... </description>
	<dc:date>2026-05-27T15:18:27-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17816" >
	<title> ATel 17816: MAXI/GSC detection of an X-ray outburst from the Be/X-ray binary pulsar LS V +44 17 (RX J0440.9+4431) </title>
	<link> https://www.astronomerstelegram.org/?read=17816 </link>
	<creator> M. Nakajima, T. Mihara, H. Negoro, 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, H. Sugai, N. Nagashima, Y. Ishihara, M. Shidatsu, C. Kang, T. Nakamoto, M. Uenishi, T. Usuki, S. Yatsuzuka, 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, T. Mihara, H. Negoro, 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, H. Sugai, N. Nagashima, Y. Ishihara, M. Shidatsu, C. Kang, T. Nakamoto, M. Uenishi, T. Usuki, S. Yatsuzuka, 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>ATel17816</identifier>
	<description> The MAXI/GSC nova alert system triggered on a weak X-ray brightening from the Be/X-ray binary pulsar LS V +44 17 (RX J0440.9+4431) on 2026 May 22 (MJD 61182). ... </description>
	<dc:date>2026-05-27T02:00:01-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17815" >
	<title> ATel 17815: MAXI/GSC Observation of an X-ray Outburst from the Be/X-ray Binary Pulsar 1A 0535-66 (1A 0538-66) </title>
	<link> https://www.astronomerstelegram.org/?read=17815 </link>
	<creator> M. Nakajima, T. Mihara, M. Sugizaki, H. Negoro, 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, H. Sugai, N. Nagashima, Y. Ishihara, M. Shidatsu, C. Kang, T. Nakamoto, M. Uenishi, T. Usuki, S. Yatsuzuka, 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, W. Iwakiri, T. Kawamuro, S. Yamada, S. Ogawa  </creator>
	<author> M. Nakajima, T. Mihara, M. Sugizaki, H. Negoro, 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, H. Sugai, N. Nagashima, Y. Ishihara, M. Shidatsu, C. Kang, T. Nakamoto, M. Uenishi, T. Usuki, S. Yatsuzuka, 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, 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>ATel17815</identifier>
	<description> The MAXI/GSC nova alert system triggered on an X-ray brightening from the Be/X-ray binary pulsar 1A 0535-66 (also known as 1A 0538-66) on 2026 May 21 (MJD 61181; see the MAXI alert page at https://maxi.riken.jp/alert/novae/1181387701/1181387701.htm ). ... </description>
	<dc:date>2026-05-26T14:00:05-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17772" >
	<title> ATel 17772: MAXI/GSC detection of an X-ray burst probably from GS 0836-429 (MX 0836-42) </title>
	<link> https://www.astronomerstelegram.org/?read=17772 </link>
	<creator> H. Negoro, M. Nakajima, H. Aoe, K. Saito, T. Yokoyama, M. Wada, T. Mihara, 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, 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. Nakajima, H. Aoe, K. Saito, T. Yokoyama, M. Wada, T. Mihara, 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, 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>ATel17772</identifier>
	<description> The MAXI/GSC nova alert system triggered on a bright X-ray transient source at 08:47:31 UT on April 30, 2026. Assuming that the source flux was constant over the transit, we obtain the source position using the GSC_2 counter at (R.A., Dec) = (129.480 deg, -43.152 deg) = (08 37 55, -43 09 07) (J2000)  with a statistical 90% C.L. ... </description>
	<dc:date>2026-05-01T15:12:22-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17770" >
	<title> ATel 17770: SVOM/ECLAIRs detection of the ongoing outburst from the HMXB XTE J1859+083 </title>
	<link> https://www.astronomerstelegram.org/?read=17770 </link>
	<creator> F. Cangemi, A. Coleiro, M. Dennefeld, O. Godet, D. GÃ¶tz, S. Guillot, S. Le Stum, H.-L. Li, S. Schanne, L. Tao, L.-P. Xin, L. Zhang  </creator>
	<author> F. Cangemi, A. Coleiro, M. Dennefeld, O. Godet, D. GÃ¶tz, S. Guillot, S. Le Stum, H.-L. Li, S. Schanne, L. Tao, L.-P. Xin, 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>ATel17770</identifier>
	<description> On Monday, April 27, 2026, at 13:58:46.114 UT, the onboard trigger software of the SVOM/ECLAIRs telescope detected and localized a source at R.A. = 284.818 deg and Dec. ... </description>
	<dc:date>2026-04-30T09:35:08-00:00</dc:date></item>
<item rdf:about="https://www.astronomerstelegram.org/?read=17760" >
	<title> ATel 17760: SVOM/ECLAIRs detection of a rare type-I X-ray burst from RX J1718.4-4029 </title>
	<link> https://www.astronomerstelegram.org/?read=17760 </link>
	<creator> M. Brunet, F. Cangemi, S. Guillot, A. Coleiro, L. Zhang  </creator>
	<author> M. Brunet, F. Cangemi, S. Guillot, A. Coleiro, L. Zhang  </author>
	<creatoremail> marius.brunet@irap.omp.eu </creatoremail>
	<provenance> Credentialed by: Floriane Cangemi (cangemi@apc.in2p3.fr) </provenance>
	<publisher> The Astronomer's Telegram  </publisher>
	<identifier>ATel17760</identifier>
	<description> On Tuesday, April 19th 2026, at 01:02:07.9 UTC (T0), the SVOM/ECLAIRs (4-150 keV) coded-mask telescope detected a Type I burst via an offline search with the event-by-event data downloaded through the X-band ground station. ... </description>
	<dc:date>2026-04-21T13:16:55-00:00</dc:date></item>

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