December 2025 - vsnet-grb-info - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-grb-info 41174] GRB 251214B: SVOM/C-GFT optical observations
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43093 SUBJECT: GRB 251214B: SVOM/C-GFT optical observations DATE: 25/12/14 11:59:55 GMT FROM: SVOM_group <svomgroup(a)bao.ac.cn> Zhe Kang (CHO), Chao WU (NAOC), Liping Xin(NAOC), Xuhui Han(NAOC), Pinpin Zhang (NAOC), Xiaomeng Lu (NAOC), Zhenwei Li (CHO), You Lv (CHO), Ruosong Zhang (NAOC), Yujie Xiao(NAOC), Yulei Qiu(NAOC), Jing Wang (NAOC), Jinsong Deng(NAOC), Lei Huang(NAOC), Jianyan Wei (NAOC), report on behalf of the SVOM/C-GFT team: We observed the field of GRB 251214B detected by Fermi/GBM (Fermi GBM team, GCN 43088) and Swift/BAT (Eyles-Ferris et al., GCN 43089) with LATIOS on SVOM/C-GFT. Observations started at 2025-12-14T09:12:24 UTC, ~10.12 min after the trigger. The optical counterpart (Eyles-Ferris et al., GCN 43089) was clearly detected in our stacked images of band g, r , and i. The magnitudes are: |[date-obs(mid-time)] | Mid_t-T0(min) | exposure time (s) | band | mag (AB) | mag_err| |--------------------|--------------|-------------------|------|----------|--------| |2025-12-14T09:12:42 | 10.75 | 3x10 | i | 16.56 |0.070| |2025-12-14T09:26:55 | 24.64 | 5x30 | g | 18.56 |0.090| |2025-12-14T09:40:03 | 37.77 | 6x30 | r | 18.33 |0.050| The photometry was calibrated against UCAC4 catalogue and no correction for Galactic dust extinction was applied. We thank the observation assistants Chun-Lei Guo and Yin-Huai 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 arcsec x 21 arcsec 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/43093. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41173] EP251214a: COLIBRÍ optical upper limit
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43092 SUBJECT: EP251214a: COLIBRÍ optical upper limit DATE: 25/12/14 11:44:06 GMT FROM: Stephane Basa at UAR Pytheas/OHP, LAM <stephane.basa(a)lam.fr> Stéphane Basa (UAR Pytheas), Leonardo García García (UNAM), Noémie Globus (UNAM), Benjamin Schneider (LAM), Jean-Grégoire Ducoin (CPPM), William H. Lee (UNAM), Alan M. Watson (UNAM), Jean-Luc Atteia (IRAP), Camila Angulo (UNAM), Dalya Akl (NYUAD), Sarah Antier (IJCLAB), Rosa L. Becerra (UNAM), Nathaniel R. Butler (ASU), Damien Dornic (CPPM), Francis Fortin (IRAP), Ramandeep Gill (UNAM), Enrique Moreno Méndez (UNAM), Kin Ocelotl López (UNAM), Diego López-Cámara (UNAM), Francesco Magnani (CPPM), Nikos Mandarakas (LAM), Margarita Pereyra (UNAM), Ny Avo Rakotondrainibe (LAM), Fredd Sánchez Álvarez (UNAM), and Antonio de Ugarte Postigo (LAM). We imaged the field of EP251214a (Y.-H. I. Yin et al., GCN Circ. 43087) potentially associated with GRB 251214A reported by the Fermi GBM Team (GCN Circ. 43085), using the DDRAGO two-channel wide-field imager on the COLIBRÍ telescope. We observed from 2025-12-14 at 09:12:10.65 to 09:56:13.15 UTC (from 6.75 to 7.49 hr after the trigger) and obtained 32 minutes of simultaneous exposure in the r and z filters. The data were reduced, coadded and analyzed with the COLIBRÍ pipeline. The photometry was calibrated using nearby stars from the PanSTARRS DR1 catalog, is in the AB system, and was not corrected for Galactic extinction. In the stacked image, we do not detect any new source at the WXT uncertainty region (Y.-H. I. Yin et al., GCN Circ. 43087) down to the following 5-sigma limit: r > 23.1 z > 21.6 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/43092. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41172] Swift GRB 251214B: Global MASTER-Net observations report
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43091 SUBJECT: Swift GRB 251214B: Global MASTER-Net observations report DATE: 25/12/14 10:37:41 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru> V.Lipunov, E.Gorbovskoy, A.Kuznetsov, K.Zhirkov, I.Panchenko, N.Tiurina, P.Balanutsa, V.Topolev, D.Vlasenko, G.Antipov, A.Sankovich, Yu.Tselik, Ya.Kechin, V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU), O.Gress, N.Budnev (ISU), C.Francile, F. Podesta, R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA), A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory), A.Sosnovskij (CrAO), A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity), D.Buckley (SAAO), R.Rebolo (The Instituto de Astrofisica de Canarias), L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez, A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory) MASTER-Tunka robotic telescope [1] located in Russia (Applied Physics Institute, Irkutsk State University) was pointed to the Swift GRB 251214B ( R. A. J. Eyles-Ferris et al., GCN 43089) errorbox 4148 sec after notice time and 4708 sec after trigger time at 2025-12-14 10:20:46 UT, with upper limit up to 17.4 mag. Observations started at twilight. The observations began at zenith distance = 61 deg. The sun altitude is -11.8 deg. The galactic latitude b = -46 deg., longitude l = 50 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3070785 We obtain a following upper limits. Tmid-T0 | Site |Filt.| Expt. | Limit| Comment _________|_____________________|_____|_______|______|________ 4739 | MASTER-Tunka | C | 60 | 16.3 | 4799 | MASTER-Tunka | C | 180 | 17.4 | Coadd 4739 | MASTER-Tunka | C | 60 | 15.9 | 4814 | MASTER-Tunka | C | 60 | 16.8 | 4814 | MASTER-Tunka | C | 60 | 16.4 | 4886 | MASTER-Tunka | C | 60 | 16.7 | 4886 | MASTER-Tunka | C | 60 | 17.0 | 4963 | MASTER-Tunka | C | 60 | 17.1 | 4963 | MASTER-Tunka | C | 60 | 16.8 | 5036 | MASTER-Tunka | C | 60 | 16.8 | 5036 | MASTER-Tunka | C | 60 | 16.5 | 5111 | MASTER-Tunka | C | 60 | 15.5 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. [1] - V.M. Lipunov, V.G. Kornilov, E.S. Gorbovskoy, N.A. Tiurina & A.S.Kuznetsov, 2023, Astronomical Robotic Networks and Operative Multichanel Astrophysics, Lomonosov MSU PRESS, 591pp. http : // www.pereplet.ru/lipunov/625.html View this GCN Circular online at https://gcn.nasa.gov/circulars/43091. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41171] EP251214.305: COLIBRÍ optical upper limit
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43090 SUBJECT: EP251214.305: COLIBRÍ optical upper limit DATE: 25/12/14 09:59:58 GMT FROM: Stephane Basa at UAR Pytheas/OHP, LAM <stephane.basa(a)lam.fr> Stéphane Basa (UAR Pytheas), Leonardo García García (UNAM), Benjamin Schneider (LAM), Jean-Grégoire Ducoin (CPPM), Noémie Globus (UNAM), William H. Lee (UNAM), Alan M. Watson (UNAM), Jean-Luc Atteia (IRAP), Camila Angulo (UNAM), Dalya Akl (NYUAD), Sarah Antier (IJCLAB), Rosa L. Becerra (UNAM), Nathaniel R. Butler (ASU), Damien Dornic (CPPM), Francis Fortin (IRAP), Ramandeep Gill (UNAM), Enrique Moreno Méndez (UNAM), Kin Ocelotl López (UNAM), Diego López-Cámara (UNAM), Francesco Magnani (CPPM), Nikos Mandarakas (LAM), Margarita Pereyra (UNAM), Ny Avo Rakotondrainibe (LAM), Fredd Sánchez Álvarez (UNAM), and Antonio de Ugarte Postigo (LAM). We imaged the field of the alert EP251214.305 using the DDRAGO two-channel wide-field imager on the COLIBRÍ telescope. We observed from 2025-12-14T08:18:20.806 to 2025-12-14T09:02:02.207 UTC (from 3478 to 6099 seconds after the trigger) and obtained 1920 seconds of simultaneous exposure in the r and z filters. The data were reduced, coadded and analyzed with the COLIBRÍ pipeline. The photometry was calibrated using nearby stars from the PanSTARRS DR1 catalog, is in the AB system, and was not corrected for Galactic extinction. In the stacked image, we do not detect any new source at the WXT uncertainty region down to the following 5-sigma limit: r > 22.69 z > 21.83 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/43090. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41170] GRB 251214B: Swift detection of a burst with an optical counterpart
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43089 SUBJECT: GRB 251214B: Swift detection of a burst with an optical counterpart DATE: 25/12/14 09:28:08 GMT FROM: K.L. Page at U Leicester <klp5(a)leicester.ac.uk> R. A. J. Eyles-Ferris (U Leicester), J. J. DeLaunay (PSU), R. Gupta (NASA GSFC), N. P. M. Kuin (UCL-MSSL), K. L. Page (U Leicester), D. M. Palmer (LANL) and T. M. Parsotan (GSFC) report on behalf of the Neil Gehrels Swift Observatory Team: At 09:02:17 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 251214B (trigger=1423875). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 330.217, -9.167 which is RA(J2000) = 22h 00m 52s Dec(J2000) = -09d 10' 00" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a double-peaked structure with a duration of about 10 sec. The peak count rate was ~3000 counts/sec (15-350 keV), at ~0 sec after the trigger. The XRT began observing the field at 09:03:18.2 UT, 60.7 seconds after the BAT trigger. Using promptly downlinked data we find a fading, uncatalogued X-ray source with an enhanced position: RA, Dec 330.21095, -9.16335 which is equivalent to: RA(J2000) = 22h 00m 50.63s Dec(J2000) = -09d 09' 48.1" with an uncertainty of 1.9 arcseconds (radius, 90% containment). This location is 25 arcseconds from the BAT onboard position, within the BAT error circle. This position may be improved as more data are received; the latest position is available at https://www.swift.ac.uk/sper. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density in excess of the Galactic value (4.01 x 10^20 cm^-2, Willingale et al. 2013), with an excess column of 5.2 (+2.80/-2.44) x 10^21 cm^-2 (90% confidence). UVOT took a finding chart exposure of 150 seconds with the White filter starting 63 seconds after the BAT trigger. There is a candidate afterglow in the list of sources generated on-board at RA(J2000) = 22:00:50.52 = 330.21052 DEC(J2000) = -09:09:46.7 = -9.16296 with a 90%-confidence error radius of about 1.10 arc sec. This position is 3.6 arc sec. from the center of the XRT error circle. The estimated magnitude is 17.47. No correction has been made for the expected extinction corresponding to E(B-V) of 0.039. Burst Advocate for this burst is R. A. J. Eyles-Ferris (raje1 AT leicester.ac.uk). Please contact the BA by email if you require additional information regarding Swift followup of this burst. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone (see Swift TOO web site for information: http://www.swift.psu.edu/) View this GCN Circular online at https://gcn.nasa.gov/circulars/43089. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41169] GRB 251214B: Fermi GBM Final Real-time Localization
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43088 SUBJECT: GRB 251214B: Fermi GBM Final Real-time Localization DATE: 25/12/14 09:13:00 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM <do_not_reply(a)GIOC.nsstc.nasa.gov> The Fermi GBM team reports the detection of a likely LONG GRB At 09:02:18 UT on 14 Dec 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 251214B (trigger 787395743.028482 / 251214377). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 329.6, Dec = -18.5 (J2000 degrees, equivalent to J2000 21h 58m, -18d 30'), with a statistical uncertainty of 9.3 degrees. The angle from the Fermi LAT boresight is 91.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251214377/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251214377/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251214377/… View this GCN Circular online at https://gcn.nasa.gov/circulars/43088. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41168] EP251214a: EP-WXT detection of an X-ray transient possibly associated with GRB 251214A
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43087 SUBJECT: EP251214a: EP-WXT detection of an X-ray transient possibly associated with GRB 251214A DATE: 25/12/14 08:15:25 GMT FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn> Y.-H. I. Yin (HKU), Y. H. Jiang (NJU), Y. Q. Zhao (PRIC, USTC), W. F. Wen (SZTU), H. Q. Cheng, and H. Sun (NAOC) 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 EP251214a. The source, with a signal-to-noise ratio of 6, did not trigger the WXT on-board trigger unit. The observation started at 2025-12-14T02:27:01 (UTC) and lasted for 3043 seconds. The WXT position of the source is R.A. = 148.471 deg, DEC = 21.053 deg (J2000) with an uncertainty of 3.1 arcmin in radius (90% C.L. statistical and systematic). The average WXT 0.5 - 4 keV spectrum can be fitted with an absorbed power law with a fixed Galactic hydrogen column density of 2.82 x 10^20 cm^-2 and a photon index of 1.84 (-/+0.94). The derived average unabsorbed 0.5-4 keV flux is 1.05 (-0.42/+0.70) x 10^-11 erg/s/cm^2. The position of EP251214a is around 4.86 deg away from GRB 251214A reported by the Fermi GBM Team (GCN 43085), and the observation was carried out around 2 hours after the GRB trigger. Given the temporal proximity and spatial consistency, we thus consider the EP-WXT detection the possible X-ray afterglow of GRB 251214A. EP-FXT follow-up observation has 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/43087. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41167] Fermi GRB 251214A: Global MASTER-Net observations report
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43086 SUBJECT: Fermi GRB 251214A: Global MASTER-Net observations report DATE: 25/12/14 00:45:21 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru> V.Lipunov, E.Gorbovskoy, A.Kuznetsov, K.Zhirkov, I.Panchenko, N.Tiurina, P.Balanutsa, V.Topolev, D.Vlasenko, G.Antipov, A.Sankovich, Yu.Tselik, Ya.Kechin, V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU), O.Gress, N.Budnev (ISU), C.Francile, F. Podesta, R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA), A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory), A.Sosnovskij (CrAO), A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity), D.Buckley (SAAO), R.Rebolo (The Instituto de Astrofisica de Canarias), L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez, A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory) MASTER-Tunka robotic telescope [1] located in Russia (Applied Physics Institute, Irkutsk State University) started inspect of the Fermi GRB 251214A ( Fermi GBM team, GCN 43085) errorbox 201 sec after notice time and 238 sec after trigger time at 2025-12-14 00:15:13 UT, with upper limit up to 14.7 mag. Observations started at twilight. The observations began at zenith distance = 44 deg. The sun altitude is -7.0 deg. The galactic latitude b = 52 deg., longitude l = 219 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3070442 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 239 | 2025-12-14 00:15:13 | MASTER-Tunka | (10h 12m 20.99s , +17d 57m 22.4s) | C | 1 | 14.4 | 240 | 2025-12-14 00:15:13 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.4s) | C | 3 | 14.7 | Coadd 239 | 2025-12-14 00:15:13 | MASTER-Tunka | (10h 11m 48.16s , +18d 04m 24.3s) | C | 1 | 14.2 | 245 | 2025-12-14 00:15:18 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.3s) | C | 1 | 14.3 | 245 | 2025-12-14 00:15:18 | MASTER-Tunka | (10h 11m 48.16s , +18d 04m 24.2s) | C | 1 | 14.1 | 250 | 2025-12-14 00:15:24 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.0s) | C | 1 | 14.0 | 250 | 2025-12-14 00:15:24 | MASTER-Tunka | (10h 11m 48.17s , +18d 04m 24.0s) | C | 1 | 14.0 | 256 | 2025-12-14 00:15:30 | MASTER-Tunka | (10h 11m 48.17s , +18d 04m 23.6s) | C | 1 | 13.8 | 256 | 2025-12-14 00:15:30 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 21.9s) | C | 1 | 14.0 | 257 | 2025-12-14 00:15:30 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.0s) | C | 3 | 14.4 | Coadd 262 | 2025-12-14 00:15:36 | MASTER-Tunka | (10h 12m 21.01s , +17d 57m 21.7s) | C | 1 | 13.9 | 262 | 2025-12-14 00:15:36 | MASTER-Tunka | (10h 11m 48.17s , +18d 04m 23.7s) | C | 1 | 13.8 | 267 | 2025-12-14 00:15:41 | MASTER-Tunka | (10h 11m 48.18s , +18d 04m 23.4s) | C | 1 | 13.8 | 267 | 2025-12-14 00:15:41 | MASTER-Tunka | (10h 12m 21.02s , +17d 57m 21.5s) | C | 1 | 13.9 | 273 | 2025-12-14 00:15:47 | MASTER-Tunka | (10h 12m 21.05s , +17d 57m 21.5s) | C | 1 | 13.9 | 274 | 2025-12-14 00:15:47 | MASTER-Tunka | (10h 12m 21.05s , +17d 57m 21.5s) | C | 3 | 14.4 | Coadd 273 | 2025-12-14 00:15:47 | MASTER-Tunka | (10h 11m 48.20s , +18d 04m 23.3s) | C | 1 | 13.5 | 278 | 2025-12-14 00:15:52 | MASTER-Tunka | (10h 12m 21.04s , +17d 57m 21.1s) | C | 1 | 14.0 | 279 | 2025-12-14 00:15:52 | MASTER-Tunka | (10h 11m 48.20s , +18d 04m 22.9s) | C | 1 | 13.7 | 285 | 2025-12-14 00:15:58 | MASTER-Tunka | (10h 12m 21.05s , +17d 57m 21.1s) | C | 1 | 13.9 | 285 | 2025-12-14 00:15:58 | MASTER-Tunka | (10h 11m 48.23s , +18d 04m 22.8s) | C | 1 | 13.8 | 290 | 2025-12-14 00:16:04 | MASTER-Tunka | (10h 12m 21.06s , +17d 57m 20.6s) | C | 1 | 13.8 | 291 | 2025-12-14 00:16:04 | MASTER-Tunka | (10h 12m 21.06s , +17d 57m 20.6s) | C | 3 | 14.3 | Coadd 291 | 2025-12-14 00:16:04 | MASTER-Tunka | (10h 11m 48.25s , +18d 04m 22.6s) | C | 1 | 13.8 | 296 | 2025-12-14 00:16:09 | MASTER-Tunka | (10h 12m 21.03s , +17d 57m 20.4s) | C | 1 | 13.8 | 296 | 2025-12-14 00:16:09 | MASTER-Tunka | (10h 11m 48.23s , +18d 04m 22.2s) | C | 1 | 13.5 | 302 | 2025-12-14 00:16:15 | MASTER-Tunka | (10h 12m 21.04s , +17d 57m 20.4s) | C | 1 | 13.8 | 302 | 2025-12-14 00:16:15 | MASTER-Tunka | (10h 11m 48.25s , +18d 04m 22.3s) | C | 1 | 13.5 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. [1] - V.M. Lipunov, V.G. Kornilov, E.S. Gorbovskoy, N.A. Tiurina & A.S.Kuznetsov, 2023, Astronomical Robotic Networks and Operative Multichanel Astrophysics, Lomonosov MSU PRESS, 591pp. http : // www.pereplet.ru/lipunov/625.html View this GCN Circular online at https://gcn.nasa.gov/circulars/43086. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41166] Fermi GRB 251214A: Global MASTER-Net observations report
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43086 SUBJECT: Fermi GRB 251214A: Global MASTER-Net observations report DATE: 25/12/14 00:45:21 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov(a)xray.sai.msu.ru> V.Lipunov, E.Gorbovskoy, A.Kuznetsov, K.Zhirkov, I.Panchenko, N.Tiurina, P.Balanutsa, V.Topolev, D.Vlasenko, G.Antipov, A.Sankovich, Yu.Tselik, Ya.Kechin, V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU), O.Gress, N.Budnev (ISU), C.Francile, F. Podesta, R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA), A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory), A.Sosnovskij (CrAO), A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity), D.Buckley (SAAO), R.Rebolo (The Instituto de Astrofisica de Canarias), L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez, A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory) MASTER-Tunka robotic telescope [1] located in Russia (Applied Physics Institute, Irkutsk State University) started inspect of the Fermi GRB 251214A ( Fermi GBM team, GCN 43085) errorbox 201 sec after notice time and 238 sec after trigger time at 2025-12-14 00:15:13 UT, with upper limit up to 14.7 mag. Observations started at twilight. The observations began at zenith distance = 44 deg. The sun altitude is -7.0 deg. The galactic latitude b = 52 deg., longitude l = 219 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3070442 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 239 | 2025-12-14 00:15:13 | MASTER-Tunka | (10h 12m 20.99s , +17d 57m 22.4s) | C | 1 | 14.4 | 240 | 2025-12-14 00:15:13 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.4s) | C | 3 | 14.7 | Coadd 239 | 2025-12-14 00:15:13 | MASTER-Tunka | (10h 11m 48.16s , +18d 04m 24.3s) | C | 1 | 14.2 | 245 | 2025-12-14 00:15:18 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.3s) | C | 1 | 14.3 | 245 | 2025-12-14 00:15:18 | MASTER-Tunka | (10h 11m 48.16s , +18d 04m 24.2s) | C | 1 | 14.1 | 250 | 2025-12-14 00:15:24 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.0s) | C | 1 | 14.0 | 250 | 2025-12-14 00:15:24 | MASTER-Tunka | (10h 11m 48.17s , +18d 04m 24.0s) | C | 1 | 14.0 | 256 | 2025-12-14 00:15:30 | MASTER-Tunka | (10h 11m 48.17s , +18d 04m 23.6s) | C | 1 | 13.8 | 256 | 2025-12-14 00:15:30 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 21.9s) | C | 1 | 14.0 | 257 | 2025-12-14 00:15:30 | MASTER-Tunka | (10h 12m 21.00s , +17d 57m 22.0s) | C | 3 | 14.4 | Coadd 262 | 2025-12-14 00:15:36 | MASTER-Tunka | (10h 12m 21.01s , +17d 57m 21.7s) | C | 1 | 13.9 | 262 | 2025-12-14 00:15:36 | MASTER-Tunka | (10h 11m 48.17s , +18d 04m 23.7s) | C | 1 | 13.8 | 267 | 2025-12-14 00:15:41 | MASTER-Tunka | (10h 11m 48.18s , +18d 04m 23.4s) | C | 1 | 13.8 | 267 | 2025-12-14 00:15:41 | MASTER-Tunka | (10h 12m 21.02s , +17d 57m 21.5s) | C | 1 | 13.9 | 273 | 2025-12-14 00:15:47 | MASTER-Tunka | (10h 12m 21.05s , +17d 57m 21.5s) | C | 1 | 13.9 | 274 | 2025-12-14 00:15:47 | MASTER-Tunka | (10h 12m 21.05s , +17d 57m 21.5s) | C | 3 | 14.4 | Coadd 273 | 2025-12-14 00:15:47 | MASTER-Tunka | (10h 11m 48.20s , +18d 04m 23.3s) | C | 1 | 13.5 | 278 | 2025-12-14 00:15:52 | MASTER-Tunka | (10h 12m 21.04s , +17d 57m 21.1s) | C | 1 | 14.0 | 279 | 2025-12-14 00:15:52 | MASTER-Tunka | (10h 11m 48.20s , +18d 04m 22.9s) | C | 1 | 13.7 | 285 | 2025-12-14 00:15:58 | MASTER-Tunka | (10h 12m 21.05s , +17d 57m 21.1s) | C | 1 | 13.9 | 285 | 2025-12-14 00:15:58 | MASTER-Tunka | (10h 11m 48.23s , +18d 04m 22.8s) | C | 1 | 13.8 | 290 | 2025-12-14 00:16:04 | MASTER-Tunka | (10h 12m 21.06s , +17d 57m 20.6s) | C | 1 | 13.8 | 291 | 2025-12-14 00:16:04 | MASTER-Tunka | (10h 12m 21.06s , +17d 57m 20.6s) | C | 3 | 14.3 | Coadd 291 | 2025-12-14 00:16:04 | MASTER-Tunka | (10h 11m 48.25s , +18d 04m 22.6s) | C | 1 | 13.8 | 296 | 2025-12-14 00:16:09 | MASTER-Tunka | (10h 12m 21.03s , +17d 57m 20.4s) | C | 1 | 13.8 | 296 | 2025-12-14 00:16:09 | MASTER-Tunka | (10h 11m 48.23s , +18d 04m 22.2s) | C | 1 | 13.5 | 302 | 2025-12-14 00:16:15 | MASTER-Tunka | (10h 12m 21.04s , +17d 57m 20.4s) | C | 1 | 13.8 | 302 | 2025-12-14 00:16:15 | MASTER-Tunka | (10h 11m 48.25s , +18d 04m 22.3s) | C | 1 | 13.5 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. [1] - V.M. Lipunov, V.G. Kornilov, E.S. Gorbovskoy, N.A. Tiurina & A.S.Kuznetsov, 2023, Astronomical Robotic Networks and Operative Multichanel Astrophysics, Lomonosov MSU PRESS, 591pp. http : // www.pereplet.ru/lipunov/625.html View this GCN Circular online at https://gcn.nasa.gov/circulars/43086. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41165] GRB 251214A: Fermi GBM Final Real-time Localization
by GCN Circulars 14 Dec '25

14 Dec '25

TITLE: GCN CIRCULAR NUMBER: 43085 SUBJECT: GRB 251214A: Fermi GBM Final Real-time Localization DATE: 25/12/14 00:21:49 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM <do_not_reply(a)GIOC.nsstc.nasa.gov> The Fermi GBM team reports the detection of a likely LONG GRB At 00:11:15 UT on 14 Dec 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 251214A (trigger 787363880.165798 / 251214008). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 152.4, Dec = 17.9 (J2000 degrees, equivalent to J2000 10h 09m, 17d 53'), with a statistical uncertainty of 4.9 degrees. The angle from the Fermi LAT boresight is 61.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251214008/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251214008/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251214008/… View this GCN Circular online at https://gcn.nasa.gov/circulars/43085. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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