March 2026 - vsnet-grb-info - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-grb-info 42060] GRB 260307A: Fermi GBM Final Localization
by GCN Circulars 07 Mar '26

07 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43939 SUBJECT: GRB 260307A: Fermi GBM Final Localization DATE: 26/03/07 13:08:25 GMT FROM: A. Holzmann Airasca at University of Trento and INFN Bari <a.holzmannairasca(a)unitn.it> The Fermi GBM team reports the detection of a likely LONG GRB "At 11:27:59.32 UT on 07 March 2026, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 260307A (trigger 794575684/260307478). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 209.07, Dec = 29.03 (J2000 degrees, equivalent to J2000 13h 56m, 29d 01'), with a statistical uncertainty of 2.88 degrees. The angle from the Fermi LAT boresight is 77 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260307478/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260307478/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260307478/…" View this GCN Circular online at https://gcn.nasa.gov/circulars/43939. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42059] GRB 260211A: late-time NOT i-band observations consistent with archival flux
by GCN Circulars 07 Mar '26

07 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43938 SUBJECT: GRB 260211A: late-time NOT i-band observations consistent with archival flux DATE: 26/03/07 10:55:59 GMT FROM: Gregory Corcoran at University College Dublin <gregory.corcoran(a)ucdconnect.ie> G. Corcoran (UCD), D. B. Malesani (DAWN/NBI and Radboud), A. Martin-Carrillo (UCD), S. Bijavara Seshashayana (NOT and Malmo Univ.) report on behalf of a larger collaboration: We observed the optical counterpart (Li et al., GCN 43748) of GRB 260211A (Gotz et al., GCN 43705; Hamburg, GCN 43713) using the Nordic Optical Telescope (NOT) equipped with the ALFOSC instrument. Observations (3x300 s) were conducted in the SDSS i band, in order to reduce the effect of the large Galactic extinction towards this line of sight (A_V = 2.1 mag). Our image quality was unfortunately degraded by poor seeing (2.1"). The optical counterpart is detected in our images (mid time 23.1 days after the SVOM trigger). We measure a magnitude i = 22.5 +/- 0.2 AB, calibrated against nearby objects from the Pan-STARRS catalog, and not corrected for Galactic extinction. The source is also detected in archival imaging from the DELVE survey (Drlica-Wagner et al., 2022, doi:10.3847/1538-4365/ac78eb), for which we find a consistent magnitude to within 0.2 mag. Imagine subtraction between the two data sets yields an upper limit of i > 22.9 for any excess component at the afterglow location. Li et al. (GCN 43923) report a rebrightening of this source between 2.7 and 19.4 days after trigger, possibly suggesting the emergence of a SN. Our data cannot confirm this trend, though the different filters and the large extinction may introduce a systematic difference. View this GCN Circular online at https://gcn.nasa.gov/circulars/43938. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42058] EP260306a: refined analysis of the EP-WXT and EP-FXT observations
by GCN Circulars 07 Mar '26

07 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43937 SUBJECT: EP260306a: refined analysis of the EP-WXT and EP-FXT observations DATE: 26/03/07 02:34:23 GMT FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn> G.L. Huang, Z.X. Li (IHEP), H. Zhou (PMO, CAS) and Z.-X. Ling (NAO, CAS) on behalf of the Einstein Probe (EP) team: The fast X-ray transient EP260306a was detected by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission (Huang et al., GCN 43930). The refined analysis of the WXT data shows that the event started at T0=2026-03-06T 01:28:20(UTC), and lasted for approximately 60 seconds, after which the WXT light curve was interrupted due to the autonomous follow-up observation. The average WXT 0.5-4 keV spectrum can be fitted with an absorbed power law with a fixed Galactic hydrogen column density (NH) of 3.24×10^20 cm^-2, a photon index of 4.01(-2.04/+3.04) and an additional absorber (z=0) of NH=6.32(-4.37/+6.21)×10^21cm^-2 to represent the comprehensive absorption of the host galaxy (z=4.773, Levan et al., GCN 43934) and the foreground galaxy (z=0.72, Globus et al., GCN 43931). The derived average unabsorbed 0.5-4 keV flux is 3.98×(-2.97/+69.04)×10^(-9) erg/s/cm^2. The Follow-up X-ray Telescope (FXT) on board EP observed this source autonomously at 2026-03-06T01:34:41(UTC, T0+261s). The exposure time of this observation is 4010s. On-ground analysis of the FXT data found an uncatalogued source at R.A. = 145.9497, DEC = 15.6942 (J2000) with an uncertainty of about 10 arcsec (radius, 90% C.L. statistical and systematic), which is consistent with the WXT position and position of the optical counterpart (Li et al, GCN 43929; Globus et al., GCN 43931; Ma et al., GCN 43933; Levan et al., GCN 43934). The average 0.5-10 keV spectrum can be fitted with an absorbed power law with a fixed Galactic hydrogen column density of 3.24×10^20 cm^-2, a photon index of 2.36(-0.38/+0.41) and an additional absorber of NH=1.53(-1.11/+1.19)×10^21 cm^-2. The derived average unabsorbed 0.5-10 keV flux is 1.37(-0.16/+0.20)×10^(-12) erg/s/cm^2. All uncertainties are reported at the 90% confidence interval. Further FXT follow-up observations have been arranged. Launched on January 9, 2024, EP is a space X-ray observatory to monitor the soft X-ray sky with X-ray follow-up capability (Yuan et al. 2022, Handbook of X-ray and Gamma-ray Astrophysics). View this GCN Circular online at https://gcn.nasa.gov/circulars/43937. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42057] GRB 260207A: TESS Detection and Possible VLA Counterpart
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43936 SUBJECT: GRB 260207A: TESS Detection and Possible VLA Counterpart DATE: 26/03/06 18:35:15 GMT FROM: Sarah Chastain at Texas Tech University <sarahichastain(a)gmail.com> S. I Chastain (TTU) and M. M. Fausnaugh (TTU) report: Approximately 93% of the Fermi GBM localization of GRB 260207A (Fermi GBM Team, GCN 43628) fell within the field of view of the Transiting Exoplanet Survey Satellite (TESS; Ricker et al. JATIS 1 2015) during observations of sector 100. We identified a counterpart consistent with the counterpart reported by MASTER-OT (C. Francile et al., GCN 43633). At around 14 days post-burst, we carried out VLA observations of this counterpart and identified a faint source within the error region with a flux of 24 +/- 4 microJy/BM at 6 GHz. The position of this source is: RA (J2000): 10:44:11.3314 ± 0.0016 seconds Declination (J2000): -33:09:36.053 ± 0.067 arcseconds This circular includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations were carried out as part of project SF171128, approved in the framework of the Fermi - NRAO joint program agreement. View this GCN Circular online at https://gcn.nasa.gov/circulars/43936. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42056] EP260302a: SVOM/VT optical observation
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43935 SUBJECT: EP260302a: SVOM/VT optical observation DATE: 26/03/06 15:17:15 GMT FROM: Yinuo Ma <mayn(a)bao.ac.cn> Y. N. Ma, L. P. Xin, H. L. Li, Z. H. Yao, Y. L. Qiu, C. Wu, X. H. Han, Y. Xu, J. Wang, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, L. Lan, J. R. Xu, J. S. Deng, J. Y. Wei (NAOC), J. Palmerio (CEA) report on behalf of the SVOM/VT team. SVOM/VT performed a Target of Opportunity observation of EP260302a detected by EP/WXT (Zhang et al., GCN 43899; Zhang et al., GCN 43906). SVOM/VT began observing the field at 2026-03-05T07:05:29 UTC, 55.435 hours after the trigger, in the VT_B (400nm-650nm) and VT_R (650nm-1000nm) channels simultaneously. With X-band data available, the optical counterpart (Li et al., GCN 43898; Pérez-García et al., GCN 43903; Corcoran et al., GCN 43904; Corcoran et al., GCN 43928; Levan et al., GCN 43932) was detected in both VT_B and VT_R bands. The AB magnitudes are: mid time (h) | exposure time (s) | band | mag (AB) -------------|-------------------|------|------------ 58.03 | 53*50 | VT_B | 21.4+-0.1 58.03 | 50*50 | VT_R | 21.2+-0.1 Our photometry was not corrected for Galactic extinction. The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA, China), National Center for Space Studies (CNES, France) and the Chinese Academy of Sciences (CAS, China), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. VT was jointly developed by Xi'an Institute of Optics and Precision Mechanics (XIOPM), CAS and National astronomical observatories (NAOC), CAS. View this GCN Circular online at https://gcn.nasa.gov/circulars/43935. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42055] EP260306a: Gemini-North redshift z = 4.773
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43934 SUBJECT: EP260306a: Gemini-North redshift z = 4.773 DATE: 26/03/06 13:36:30 GMT FROM: Daniele Bjørn Malesani at Cosmic Dawn Center, Niels Bohr Institute <daniele.malesani(a)nbi.ku.dk> A. J. Levan (Radboud), P. G. Jonker (Radboud), G. Corcoran (UCD), D. B. Malesani (DAWN/NBI and Radboud), F. E. Bauer (UTa), J. Chácon (PUC), L. Cotter (UCD), R. A. J. Eyles-Ferris (Leicester), A. Martin-Carrillo (UCD), J. Quirola-Vasquez (Radboud), report on behalf of a larger collaboration: We observed the optical counterpart (Li et al., GCN 43929; Globus et al., GCN 43931; Ma et al., GCN 43933) of the fast X-ray transient EP260306a (Huang et al., GCN 43930) using the Gemini-North telescope equipped with the GMOS-N spectrograph. Four exposures of 600 s each were obtained, using grating R400, a slit width of 1 arcsec, and covering the wavelength range 5200-9900 Å. The observation mid time was 2026 March 6.489 UT (10.2 hr after the EP/WXT trigger). Continuum is significantly detected over the red part of the spectrum, down to ~7020 Å, where a spectral break is apparent. This is due to a combination of the H I damping wing and the onset of the Lyman forest at z ~ 4.77. A number of absorption features, including fine-structure lines, are clearly visible, which we interpret as Si II, Si II*, C II, Si IV, C IV, Fe II, Al II, all at a common redshift z = 4.773, establishing it as the redshift of EP260306a. We note that, given their colors and g-band detection, the two nearby objects noted by Globus et al. (GCN 43931) are both in the foreground of the transient. We acknowledge the excellent support from the Gemini North staff in the execution of this challenging observation. View this GCN Circular online at https://gcn.nasa.gov/circulars/43934. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42054] EP260306a: SVOM/VT optical observation
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43933 SUBJECT: EP260306a: SVOM/VT optical observation DATE: 26/03/06 10:21:37 GMT FROM: Yinuo Ma <mayn(a)bao.ac.cn> Y. N. Ma, H. L. Li, Z. H. Yao, Y. L. Qiu, C. Wu, L. P. Xin, X. H. Han, Y. Xu, J. Wang, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, L. Lan, J. R. Xu, J. S. Deng, J. Y. Wei (NAOC), J. Palmerio (CEA) report on behalf of the SVOM/VT team. SVOM/VT performed a Target of Opportunity observation of EP260306a detected by EP/WXT (Huang et al., GCN 43930). SVOM/VT began observing the field at 2026-03-06T03:45:23 UTC, 2.268 hours after the trigger, in the VT_B (400nm-650nm) and VT_R (650nm-1000nm) channels simultaneously. With X-band data available, the optical counterpart (Li et al., GCN 43929; Globus et al., GCN 43931) was detected in both VT_B and VT_R bands. The AB magnitudes are: mid time (h) | exposure time (s) | band | mag (AB) -------------|-------------------|------|-------------- 2.608 | 48*50 | VT_B | 23.1+-0.2 2.642 | 53*50 | VT_R | 21.7+-0.1 Our photometry was not corrected for Galactic extinction. The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA, China), National Center for Space Studies (CNES, France) and the Chinese Academy of Sciences (CAS, China), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. VT was jointly developed by Xi'an Institute of Optics and Precision Mechanics (XIOPM), CAS and National astronomical observatories (NAOC), CAS. View this GCN Circular online at https://gcn.nasa.gov/circulars/43933. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42053] EP260302a: Gemini-South redshift z = 1.535
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43932 SUBJECT: EP260302a: Gemini-South redshift z = 1.535 DATE: 26/03/06 09:26:04 GMT FROM: Daniele Bjørn Malesani at Cosmic Dawn Center, Niels Bohr Institute <daniele.malesani(a)nbi.ku.dk> A. J. Levan (Radboud), G. Corcoran (UCD), J. Quirola-Vasquez (Radboud), D. B. Malesani (DAWN/NBI and Radboud), P. G. Jonker (Radboud), F. E. Bauer (UTa), J. Chácon (PUC), L. Cotter (UCD), R. A. J. Eyles-Ferris (Leicester), A. Martin-Carrillo (UCD), R. Ruiz (Gemini), V. Firpo (Gemini) report on behalf of a larger collaboration: Taking advantage of its rebrightening (Corcoran et al., GCN 43928), we observed the optical counterpart (Li et al., GCN 43898; Pérez-García et al., GCN 43903; Corcoran et al., GCNs 43904, 43928) of the fast X-ray transient EP260302a (Zhang et al., GCNs 43899, 43906) using Gemini-South equipped with the GMOS spectrograph. In the acquisition image (mid time 3.18 days after trigger) we measure r = 21.30 +- 0.07 AB, suggesting some fading compared with our previous observation (Corcoran et al., GCN 43928). Four exposures of 600 s each were obtained, using grating B480, a slit width of 1 arcsec, and covering the wavelength range 4470-8500 Å. The observation mid time was 2026 March 6.182 UT (3.20 days after the EP/WXT trigger). Continuum is significantly detected over the entire covered wavelength range. From the lack of Hydrogen absorption, we infer a firm upper limit z < 2.67. A number of clear absorption features are also visible, which we interpret as Fe II (2344, 2374, 2383, 2586, 2600 AA) and Mg II (2796, 2803 AA), all at a common redshift z = 1.535. Given the good S/N of the continuum, and the lack of any further unidentified features, we therefore conclude that EP260302a likely lies at this redshift. View this GCN Circular online at https://gcn.nasa.gov/circulars/43932. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42052] EP260306a: COLIBRÍ optical observations of the fading and red counterpart
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43931 SUBJECT: EP260306a: COLIBRÍ optical observations of the fading and red counterpart DATE: 26/03/06 04:38:09 GMT FROM: globus(a)astro.unam.mx Noémie Globus (UNAM), Benjamin Schneider (LAM), Rosa L. Becerra (UNAM), Alan M. Watson (UNAM), Camila Angulo (UNAM), Stéphane Basa (UAR Pytheas), William H. Lee (UNAM), Edilberto Aguilar-Ruiz (UNAM), Jean-Luc Atteia (IRAP), Dalya Akl (NYUAD), Sarah Antier (IJCLAB), Nathaniel R. Butler (ASU), Damien Dornic (CPPM), Jean-Grégoire Ducoin (CPPM), Francis Fortin (IRAP), Leonardo García García (UNAM), Ramandeep Gill (UNAM), Asuka Kuwata (UNAM), Nikos Mandarakas (LAM), Diego López-Cámara (UNAM), Francesco Magnani (CPPM), Enrique Moreno Méndez (UNAM), Margarita Pereyra (UNAM), Ny Avo Rakotondrainibe (LAM), Fredd Sánchez Álvarez (UNAM) and Antonio de Ugarte Postigo (LAM) report: We imaged the field of EP260306a (Huang et al., GCN Circ. 43930) using the DDRAGO two-channel wide-field imager on the COLIBRÍ telescope. We observed from 2026-03-06 02:41 to 03:34 UTC (from 1.20 to 2.10 hours after the trigger) and obtained 23, 12 and 39 minutes of simultaneous exposure in the r, i, and z filters. The data were reduced, coadded, calibrated, and analysed with the COLIBRÍ ASU pipeline. The photometry was calibrated using nearby stars from the PanSTARRS DR1 catalog, is in the AB system, and is not corrected for Galactic extinction. We detect the optical counterpart reported by Li et al. (GCN Circ. 43929) at preliminary magnitudes of: r = 23.27 +/- 0.25, z = 21.58 +/- 0.12. Comparing our observations with those reported by Li et al. (GCN Circ. 43929), the transient has faded, and we estimate a temporal decay index alpha ≈ 1. A preliminary fit to the SED suggests a high-z event, with a tentative photometric redshift between z=4 and z=5, but cannot rule out an intrinsically redder source at a lower redshift. We encourage spectroscopy. We notice that at the position of the optical counterpart, there is a faint galaxy with g = 24.91 +/- 0.28, r = 23.90 +/- 0.17, i = 23.54 +/- 0.24, z = 23.30 +/- 0.26, and photo-z = 0.72 +/- 0.27 in the Legacy Survey catalog (Dey et al., 2019). Furthermore, at a distance of 17 arcsec from the source, there is a nearby (photo-z = 0.06 +/- 0.01) bright galaxy with g = 18.04 +/- 0.01, r = 17.34 +/- 0.01, i = 17.02 +/- 0.01, and z = 16.76 +/- 0.01, with a chance coincidence probability Pcc~2%. Both of these galaxies may be unrelated if the event is located at high redshift. Additional observations in g, r, i, z bands and analysis are still ongoing. We thank the staff of the Observatorio Astronómico Nacional on the Sierra de San Pedro Mártir and the COLIBRÍ and DDRAGO engineering teams. COLIBRÍ is an astronomical observatory developed and operated jointly by France (AMU, CNES and CNRS) and Mexico (UNAM and SECIHTI). It is located at the Observatorio Astronómico Nacional on the Sierra de San Pedro Mártir, Baja California, Mexico. View this GCN Circular online at https://gcn.nasa.gov/circulars/43931. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42051] EP260306a: Einstein Probe detection of an X-ray transient
by GCN Circulars 06 Mar '26

06 Mar '26

TITLE: GCN CIRCULAR NUMBER: 43930 SUBJECT: EP260306a: Einstein Probe detection of an X-ray transient DATE: 26/03/06 02:47:52 GMT FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn> G.L. Huang, Z.X. Li (IHEP), H. Zhou (PMO, CAS) and Z-.X. Ling (NAO, CAS) on behalf of the Einstein Probe (EP) team: We report on the detection of an X-ray transient by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission, designated EP260306a. The transient triggered EP-WXT (ID: 01709258759) at 2026-03-06T01:29:20 (UTC). The WXT position of the source is R.A. = 145.955 deg, DEC = 15.685 deg (J2000) with an uncertainty of 3 arcmin in radius (90% C.L. statistical and systematic). A follow-up observation with the Follow-up X-ray Telescope (FXT) was performed automatically. Within the WXT error circle, an uncatalogued X-ray source was detected at R.A. = 145.9478 deg, DEC = 15.6963 deg (J2000) with an uncertainty of 20 arcsec in radius (90% C.L. statistical and systematic). The location of the reported optical counterpart (GCN 43929) is consistent with the location of the uncatalogued X-ray source detected by FXT. Further information will be updated when the telemetry data is received. Launched on January 9, 2024, EP is a space X-ray observatory to monitor the soft X-ray sky with X-ray follow-up capability (Yuan et al. 2022, Handbook of X-ray and Gamma-ray Astrophysics). View this GCN Circular online at https://gcn.nasa.gov/circulars/43930. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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