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

[vsnet-grb-info 43085] GRB 260610B / AT2026owq: GRANDMA optical observations
by GCN Circulars 13 Jun '26

13 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44930 SUBJECT: GRB 260610B / AT2026owq: GRANDMA optical observations DATE: 26/06/13 13:50:34 GMT FROM: Dalya Akl at New York University Abu Dhabi <dka2010(a)nyu.edu> D. Akl (NYUAD), M. Mašek (FZU), R. Hanna (IJCLAB), P. Putsathan (KKU), Y. Rajabov (UBAI), S. Antier (IJCLAB), P. Hello (IJCLAB), M. Coughlin (UNM), S. Karpov (FZU), M. Pillas (IAP), C. Douzet (IJCLAB), A. Simon (TShNU of Kyiv), D. Rusanova (TShNU of Kyiv), V. Vasylenko (NC JASU), O. Burkhonov (UBAI), S. Ehgamberdiev (UBAI), Y. Tillayev (UBAI), P. Put (NARIT), K. Noysena (NARIT), M. Tanasan (CMU/NARIT), D. Turpin (CEA-Saclay/Irfu), M. Freeberg (KNC), A. Klotz (IRAP), C. Limonta (OCA), A. Dupin (OCA), Q. André (OCA), M. Molham (NRIAG), E. Elhosseiny (NRIAG), A. Takey (NRIAG), N. Kochiashvili (AbAO), R. Inasaridze (AbAO), V. Zhuzhunadze (AbAO) on behalf of the GRANDMA collaboration: We observed the field of the Fermi Long GRB 260610B (Fermi GBM team, GCN 44901). The observations started at 16:29:50 UTC on the 11 of June 2026, 0.7 days post the Fermi Trigger. We detected the optical afterglow candidate, reported by GOTO (O'Neill et al, GCN 44903), in several epochs, using TRT-SRO in California state, UBAI-NT60, UBAI-AZT-22 at Madainak Observatory, AZT-8 at Lisnyky Observatory, KAO-1.88m at Kottamia Astronomical Observatory, TAROT-TCA/TCH at Calern and La Silla, and Kilonova Catcher. A subset of the photometry corrected for Galactic extinction is reported in the public ACME service Skyportal/ICARE https://skyportal-icare.ijclab.in2p3.fr/source/2026owq. To access, one simply needs to create an account using your ORCID ID. The data were reduced by a single data processing pipeline, STDPipe (Karpov et al., 2022). Images obtained with the Sloan filters were calibrated using the PanSTARRS DR1 catalog. Images obtained with the Johnson-Cousins filters were calibrated using the Gaia DR3 Synphot catalog. The observations are performed under the P7 campaign of GRANDMA to monitor SVOM alerts and LSST alerts from explosive fast transients filtered by BOOM/Babamul and FINK. The results are consistent with other measurements reported (Zhu et al., GCN 44909; Akl et al., GCN 44911; O'Neill et al., GCN 44914; Moskvitin et al., GCN 44918; Jackson-Horne et al., GCN 44919; Li et al., GCN 44921; Bochenek and Perley, GCN 44927; Moskvitin et al., GCN 44929) GRANDMA is a worldwide telescope network (grandma.ijclab.in2p3.fr) devoted to the observation of transients in the context of multi-messenger astrophysics (Antier et al. 2020 MNRAS 497, 5518). Kilonova-Catcher (KNC) is the citizen science program of GRANDMA (http://kilonovacatcher.in2p3.fr/) View this GCN Circular online at https://gcn.nasa.gov/circulars/44930. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43084] GRB 260610B / AT2026owq: further SAO RAS optical observations
by GCN Circulars 13 Jun '26

13 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44929 SUBJECT: GRB 260610B / AT2026owq: further SAO RAS optical observations DATE: 26/06/13 06:35:11 GMT FROM: Alexander Moskvitin at SAO RAS <mosk(a)sao.ru> A. Moskvitin (SAO RAS), O. Spiridonova (SAO RAS), A. Pozanenko (IKI), A. Volnova (IKI), N. Pankov (IKI) report on behalf of GRB follow-up team We observed the field of GRB 260610B discovered by Fermi (The Fermi GBM team, GCN 44891; GCN 44901) with the Zeiss-1000 1-m telescope of SAO RAS + CCD photometer in BVRcIc filters on June 12. The OT (O'Neill et al., GCN 44903; Watson et al., GCN 44905; Zhu et al., GCN 44909; Gillanders et al., GCN 44910; Akl et al., GCN 44911; O'Neill et al., GCN 44914; Moskvitin et al., GCN 44918; Jackson-Horne et al., GCN 44919; Izzo, GCN 44920; Li et al., GCN 44921; Bochenek and Perley, GCN 44927) is clearly detected in our frames with the following brightness: Date, UTstart, t-T0, Exp., Filter, Mag, Err., UL (mid,d) (n*s) (3-sigma) 2026-06-12 19:21:03 2.41821 5*300 Rc 20.61 0.03 23.5 This preliminary photometry is based on nearby SDSS stars (using Lupton 2005 transformation equations) and not corrected for Galactic extinction. View this GCN Circular online at https://gcn.nasa.gov/circulars/44929. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43083] EP260605a: COLIBRÍ optical upper limits
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44928 SUBJECT: EP260605a: COLIBRÍ optical upper limits DATE: 26/06/12 19:15:05 GMT FROM: Rosa Leticia Becerra Godínez at Instituto de Astronomía, UNAM <rbecerra(a)astro.unam.mx> Rosa L. Becerra (UNAM), Massimiliano Lincetto (CPPM), Asuka Kuwata (UNAM), Sarah Antier (IJCLAB), Stéphane Basa (UAR Pytheas), William H. Lee (UNAM), Edilberto Aguilar-Ruiz (UNAM), Jean-Luc Atteia (IRAP), Camila Angulo (UNAM), Dalya Akl (NYUAD), Nathaniel R. Butler (ASU), Damien Dornic (CPPM), Jean-Grégoire Ducoin (CPPM), Francis Fortin (IRAP), Leonardo García García (UNAM), Ramandeep Gill (UNAM), Noémie Globus (UNAM), Marion Guelfand (CPPM), 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), Benjamin Schneider (LAM), Antonio de Ugarte Postigo (LAM), and Alan M. Watson (UNAM) report: We imaged the field of the EP260605a (Li et al., GCN Circ. 44847) using the DDRAGO two-channel wide-field imager on the COLIBRÍ telescope. We observed from 2026-06-06 07:27 to 08:05 UTC (from 21.93 to 22.59 hours after the trigger) and obtained 29 minutes of simultaneous exposure in the r and z filters. Given the proximity of the localization region to the Galactic bulge, we obtained additional observations to serve as templates. The field was reimaged on 2026-06-12 from 07:06 to 08:06 UTC (from 6.90 to 6.94 days after the trigger), yielding 42 minutes of simultaneous exposure in the r and z filters. The data were reduced and coadded with the COLIBRÍ pipeline and analysed with STDWeb/STDPipe (Karpov 2025). The photometry was calibrated using nearby stars from the SkyMapper catalog, is in the AB system, and is not corrected for Galactic extinction. In the image subtraction, we do not detect any new source within the FXT error region (Li et al., GCN Circ. 44867) down to the following 5-sigma limit: r > 21.4 z > 20.6 We thank the staff of the Observatorio Astronómico Nacional at Sierra de San Pedro Mártir, as well as the technical and engineering teams at CEA, CPPM, IRAP, LAM, OHP, OSU Pytheas, and UNAM. 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/44928. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43082] GRB 260610b: Liverpool Telescope optical observations
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44927 SUBJECT: GRB 260610b: Liverpool Telescope optical observations DATE: 26/06/12 18:02:21 GMT FROM: A. Bochenek at Liverpool John Moores University <a.m.bochenek(a)2023.ljmu.ac.uk> A. Bochenek, D. A. Perley (LJMU), report: We observed the field of the optical counterpart (O'Neil et al., GCN 44903) of GRB 260610b (Fu et al., GCN 44901) using the IO:O optical camera on the 2m robotic Liverpool Telescope. We obtained 5x120s exposures in SDSS griz filters, starting at 2026-06-10 23:39:02 UT, approximately 23.9 hours after trigger. We detect a source in the stacked images in all filters at the position reported by O'Neil et al. (GCN 44903), observed also by Watson et al. (GCN 44905); Zhu et al. (GCN 44909); Gillanders et al. (GCN 44910); Akl et al. (GCN 44911); O'Neill et al. (GCN 44914); Moskvitin et al. (GCN 44918); Jackson-Horne et al. (GCN 44919); Izzo, (GCN 44920), and Li et al. (GCN 44921). The photometry is: | MJD (mid) | T_mid-T_0 | Filter | Mag. (AB) | | ------------ | ------------ | ------------ | ------------ | | 61202.98947 | 23.98 h | r | 20.22 ± 0.02 | | 61202.99795 | 24.18 h | i | 19.89 ± 0.02 | | 61203.00646 | 24.38 h | z | 19.78 ± 0.05 | | 61203.01493 | 24.59 h | g | 20.66 ± 0.03 | The photometry is in the AB magnitude system, was calibrated using nearby PanSTARRS secondary standards and was not corrected for extinction. View this GCN Circular online at https://gcn.nasa.gov/circulars/44927. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43081] EP260610b: Liverpool Telescope optical upper limits
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44926 SUBJECT: EP260610b: Liverpool Telescope optical upper limits DATE: 26/06/12 17:56:45 GMT FROM: A. Bochenek at Liverpool John Moores University <a.m.bochenek(a)2023.ljmu.ac.uk> A. Bochenek, D. A. Perley (LJMU), report: We observed the field of EP260610b (Wu et al., GCN 44895, Guo et al., GCN 44912) using the IO:O optical camera on the 2m robotic Liverpool Telescope. We obtained 8x200s exposures in SDSS gri filters, starting at 2026-06-11 00:29:50.385 UT, approximately 1.46 days after trigger. We do not detect any sources at the position of the counterpart in the stacked images (Levan et al., GCN 44897; Xin et al., GCN 44900; Zhu et al., GCN 44902; Burkhonov et al., GCN 44904; Moreno Mendez et al., GCN 44906, van Hoof et al., GCN 44915) down to the three-sigma limiting magnitude of g > 23.2, r > 23.5, i > 22.9. We note that forced PSF photometry on r-band exposures gives a two-sigma detection at 23.7 ± 0.5 mag, at a mid-observation time of 1.52 days post-trigger. The photometry is in the AB magnitude system, was calibrated using nearby PanSTARRS secondary standards, and was not corrected for extinction. View this GCN Circular online at https://gcn.nasa.gov/circulars/44926. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43080] IceCube-260610A: No candidates from the Zwicky Transient Facility
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44925 SUBJECT: IceCube-260610A: No candidates from the Zwicky Transient Facility DATE: 26/06/12 17:49:32 GMT FROM: Jannis Necker at DESY <jannis.necker(a)desy.de> Jannis Necker (Leiden University), Akshay Eranhalodi (DESY), Robert Stein (JSI), Cristobal Zilleruelo Cañas (DESY), and Anna Franckowiak (Ruhr University Bochum) report, On behalf of the Zwicky Transient Facility (ZTF) and Global Relay of Observatories Watching Transients Happen (GROWTH) collaborations: As part of the ZTF neutrino follow up program (Stein et al. 2023), we observed the localization region of the neutrino event IceCube-260610A (IceCube Collaboration 2026, GCN 44899) with the Palomar 48-inch telescope, equipped with the 47 square degree ZTF camera (Bellm et al. 2019, Graham et al. 2019). We started observations in the g- and r-band beginning at 2026-06-11 06:12 UTC, approximately 10.2 hours after event time. We covered 95.9% (4.6 sq deg) of the reported localization region. This estimate accounts for chip gaps. Each exposure was 300s with a typical depth of 21.0 mag. The images were processed in real-time through the ZTF reduction and image subtraction pipelines at IPAC to search for potential counterparts (Masci et al. 2019). AMPEL (Nordin et al. 2019, Stein et al. 2021) was used to search the alerts database for candidates. We reject stellar sources (Tachibana and Miller 2018) and moving objects, and apply machine learning algorithms (Mahabal et al. 2019) . No candidate counterparts were detected. ZTF and GROWTH are worldwide collaborations comprising Caltech/IPAC, USA; University of Maryland, USA; University of California, Berkeley, USA; Cornell University, USA; Drexel University, USA; University of North Carolina at Chapel Hill, USA; Institute of Science and Technology, Austria; National Central University, Taiwan; OKC, Sweden; DZA, Germany. GROWTH acknowledges generous support of the NSF under PIRE Grant No 1545949. Alert distribution service provided by DIRAC@UW (Patterson et al. 2019). Alert database searches are done by AMPEL (Nordin et al. 2019). Alert filtering is performed with the nuztf (Stein et al. 2021, https://github.com/desy-multimessenger/nuztf ). View this GCN Circular online at https://gcn.nasa.gov/circulars/44925. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43079] IceCube-260610A: EP-FXT follow-up observation
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44924 SUBJECT: IceCube-260610A: EP-FXT follow-up observation DATE: 26/06/12 12:01:23 GMT FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn> G. J. Yang, Q. Y. Wu and Y. Liu (NAO, CAS) on behalf of the Einstein Probe (EP) team: EP-FXT conducted a follow-up observation of IceCube-260610A (GCN 44899), a Gold-track neutrino event. The observation began at 2026-06-10T21:56:33, approximately 1.9 hours after the neutrino trigger, with a total exposure of 7.9 ks. Within the neutrino localization uncertainty region, none of the detected X-ray sources exhibited significant variability compared with their historical fluxes or upper limits. The properties of the detected sources, excluding those clearly associated with stars, are summarized below. Name | RA | Dec | Flux (erg /cm^2 /s) | Flux error (erg /cm^2 /s) | SNR EPF_J203646.2+370943 | 309.1926 | 37.1612 | 6.52e-14 | 1.71e-14 | 5.14 EPF_J203731.0+370929 | 309.3791 | 37.1577 | 5.66e-14 | 1.99e-14 | 4.72 EPF_J203711.7+370245 | 309.2994 | 37.0434 | 1.05e-13 | 2.00e-14 | 8.60 EPF_J203710.6+370109 | 309.2940 | 37.0191 | 5.46e-14 | 1.38e-14 | 6.10 EPF_J203748.1+370629 | 309.4505 | 37.1080 | 5.80e-14 | 1.54e-14 | 5.06 EPF_J203709.1+365818 | 309.2880 | 36.9716 | 6.02e-14 | 1.65e-14 | 4.40 EPF_J203803.5+371737 | 309.5105 | 37.2954 | 9.50e-14 | 2.40e-14 | 5.00 EPF_J203717.9+365622 | 309.3246 | 36.9393 | 5.75e-14 | 1.67e-14 | 4.24 EPF_J203730.0+373440 | 309.3750 | 37.5779 | 1.36e-13 | 5.01e-14 | 4.84 EPF_J203737.9+365019 | 309.4045 | 36.8384 | 7.51e-14 | 2.50e-14 | 4.75 EPF_J203835.0+364342 | 309.6481 | 36.7285 | 2.01e-13 | 4.98e-14 | 6.20 EPF_J203601.0+363247 | 309.0040 | 36.5464 | 2.38e-13 | 8.65e-14 | 3.60 We note that EPF_J203835.0+364342 is associated with a CV named ASASSN -16ix. Additional follow-up observations are planned. View this GCN Circular online at https://gcn.nasa.gov/circulars/44924. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43078] GRB 260611B: CALET Gamma-Ray Burst Monitor detection
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44923 SUBJECT: GRB 260611B: CALET Gamma-Ray Burst Monitor detection DATE: 26/06/12 10:12:20 GMT FROM: Yuta Kawakubo at Aoyama Gakuin University <kawakubo(a)phys.aoyama.ac.jp> S. Nakahira (JAXA), A. Yoshida, T. Sakamoto, S. Sugita, Y. Kawakubo (AGU), K. Yamaoka (Nagoya U), Y. Asaoka (ICRR), S. Torii, Y. Akaike, K. Kobayashi (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U), N. Cannady (GSFC), M. L. Cherry (LSU), S. Ricciarini (U of Florence), P. S. Marrocchesi (U of Siena), and the CALET collaboration: The CALET Gamma-ray Burst Monitor (CGBM) detected GRB 260611B at 21:32:32.02 UTC on 11 June 2026 (trigger #1465248636; https://cgbm.calet.jp/cgbm_trigger/flight/1465248636/index.html) A CGBM Notice was distributed in near real time. This event was also reported by Fermi GBM (Fermi GBM Team., GCN #44917). The burst signal was seen by all CGBM detectors. The burst light curve shows a multi-peaked structure starting at T+0.2 s, peaking at T+14.7 s, and ending at T+28.4 s. The T90 and T50 durations measured with the SGM data are 24.7 +/- 0.9 s and 13.5 +/- 1.2 s in the 40-1000 keV band, respectively. The ground-processed light curve is available at: https://cgbm.calet.jp/cgbm_trigger/ground/1465248636/ The CALET data used in this analysis were provided by the Waseda CALET Operation Center located at Waseda University. View this GCN Circular online at https://gcn.nasa.gov/circulars/44923. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43077] The EP-WXT trigger 01709269176: SVOM/C-GFT confirmation of a stellar flare
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44922 SUBJECT: The EP-WXT trigger 01709269176: SVOM/C-GFT confirmation of a stellar flare DATE: 26/06/12 09:14:55 GMT FROM: SVOM_group <svomgroup(a)bao.ac.cn> S.J. Yin (GXU), Z. Kang (CHO), C. Wu (NAOC), L.P. Xin, X.H. Han, P.P. Zhang, X.M. Lu (NAOC), Z.W. Li, Y. Lv (CHO), R.S. Zhang, Y.J. Xiao, Y.L. Qiu, J. Wang, J.S. Deng, L. Huang, J.Y. Wei (NAOC) report on behalf of the SVOM/C-GFT team: We observed the field of EP-WXT trigger 01709269176 (Zhou et al., GCN 44913) with LATIOS on SVOM/C-GFT. Observations started at 2026-06-11T13:13:04.862 UTC, ~47.5 min after the trigger. Our observations in g,r and i bands confirmed that the reported associated star (GAIA DR3 1249275629854893952,GCN 44913 ) exhibits stellar flares. A flare is detected at ~5000 s post trigger, with an amplitude of ~1.3 mag in g-band and ~0.4 mag in i-band. The flare epoch is consistent with an X-ray flare detected by EP-FXT (EP team, private communication). The photometry was calibrated against nearby Pan-STARRS1 DR1 stars. We thank the observation assistants Chulei Guo and Yinhuai Hao at Jilin observatory for their excellent support. The Chinese Ground Follow-up Telescope (C-GFT) for the SVOM mission is located at Jilin Station, Changchun Observatory, National Astronomical Observatories, CAS. It features two instruments: (1) CATCH at the Cassegrain focus with a 21 arcmin x 21 arcmin FOV for simultaneous g/r/i-band imaging, and (2) LATIOS, a 4k x 4k CMOS camera at the prime focus with a 1.28 deg x 1.28 deg FOV that images in g, r, and i bands via filter switching. View this GCN Circular online at https://gcn.nasa.gov/circulars/44922. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0

[vsnet-grb-info 43076] GRB 260610B / AT2026owq: SVOM/VT optical observations
by GCN Circulars 12 Jun '26

12 Jun '26

TITLE: GCN CIRCULAR NUMBER: 44921 SUBJECT: GRB 260610B / AT2026owq: SVOM/VT optical observations DATE: 26/06/12 08:27:15 GMT FROM: Huali Li at at NAOC, SVOM <lhl(a)nao.cas.cn> H. L. Li, L. P. Xin, Y. L. Qiu, C. Wu, J. R. Xu, Y. N. Ma, Z. H. Yao, X. H. Han, J. Wang, Y. Xu, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, J. S. Deng, J. Y. Wei (NAOC) and J. Palmerio (CEA/Irfu) report on behalf of the SVOM/VT team. SVOM/VT performed a ToO observation of GOTO26fua/AT2026owq (O'Neil et al., GCN 44903; Watson et al., GCN 44905; Zhu et al., GCN 44909; Gillanders et al., GCN 44910; Akl et al., GCN 44911; O'Neill et al., GCN 44914; Moskvitin et al., GCN 44918; Jackson-Horne et al., GCN 44919; Izzo, GCN 44920), a possible counterpart of GRB 260610B (Fermi GBM Team, GCN 44901). The observation started at 2026-06-11T13:05:40 UTC, i.e., 13.32 hours post trigger in the VT_B (400-650 nm) and VT_R (650-1000 nm) channels simultaneously. The OT was clearly detected in both channels. The following measurements are in the AB magnitude and are not corrected for Galactic extinction: Mid time | Band | Exposure Time | Brightness 14.50 h VT_B 30*70 s 20.10 +/-0.06 mag 16.12 h VT_B 29*70 s 20.16 +/-0.06 mag 14.52 h VT_R 28*70 s 19.38 +/-0.06 mag 16.15 h VT_R 26*70 s 19.49 +/-0.06 mag 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/44921. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

1 0