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

[vsnet-grb-info 40314] GRB 251013C: ALMA detection
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42243 SUBJECT: GRB 251013C: ALMA detection DATE: 25/10/14 03:51:49 GMT FROM: Tanmoy Laskar at U of Utah <tanmoylaskar(a)gmail.com> T. Laskar (University of Utah), C. Christy, N. Franz, K. D. Alexander (University of Arizona), E. Berger (Harvard University), R. Chornock (UC Berkeley), H. J. van Eerten (University of Bath), G. Farley (U. Utah), W. Fong (Northwestern University), R. Gill (UNAM), J. Granot (Open University), R. Margutti (UC Berkeley), and P. Schady (University of Bath) report: “We observed GRB 251013C (Fermi GBM team, GCN 42221; Rakotondrainibe et al., GCN 42222) with the Atacama Large Millimeter/Submillimeter Array (ALMA) at 97.5 GHz beginning on 2025 October 13 at 23:07 UT (5.5 hours after the burst). Preliminary analysis reveals a mm source with flux density of ~ 0.3 mJy at position: RA (J2000) = 23:03:20.56 Dec (J2000) = -00:12:37.21 with an uncertainty of 0.02" in each coordinate. This is consistent with the X-ray position (Rakotondrainibe et al., GCN 42222; Evans et al., GCN 42232) and optical position (Palmerio et al., GCN 42223; Masi et al., GCN 42228). Further observations are planned. We thank the NAASC staff, P2G, AoD, JAO staff, and the entire ALMA team for their help with these observations." View this GCN Circular online at https://gcn.nasa.gov/circulars/42243. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40313] GRB 251013C: SVOM/COLIBRÍ (FM-GFT) detection of the optical counterpart
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42242 SUBJECT: GRB 251013C: SVOM/COLIBRÍ (FM-GFT) detection of the optical counterpart DATE: 25/10/14 03:33:15 GMT FROM: Diego López-Cámara at Instituto de Ciencias Nucleares, UNAM <diego(a)correo.nucleares.unam.mx> Diego López-Cámara (UNAM), Francesco Magnani (CPPM), Alan M. Watson (UNAM), Camila Angulo (UNAM), Ny Avo Rakotondrainibe (LAM), Stéphane Basa (UAR Pytheas), William H. Lee (UNAM), Jean-Luc Atteia (IRAP), Dalya Akl (NYUAD), Sarah Antier (OCA), Rosa L. Becerra (U Roma), Nathaniel R. Butler (ASU) , Damien Dornic (CPPM), Jean-Grégoire Ducoin (CPPM), Francis Fortin (IRAP), Leonardo García-García (UNAM), Ramandeep Gill (UNAM), Noémie Globus (UNAM), Kin Ocelotl López (UNAM), Enrique Moreno Méndez (UNAM), Margarita Pereyra (UNAM), Fredd Sánchez Álvarez (UNAM), Benjamin Schneider (LAM), and Antonio de Ugarte Postigo (LAM) report: We imaged the field of the SVOM GRB 251013C (Rakotondrainibe et al., GCN Circ. 42222) using the DDRAGO wide-field imager on the SVOM/COLIBRÍ (FM-GFT) telescope. We obtained a 60 seconds exposure in the r filter starting at 2025-10-14 02:18 (8.65 hours after the trigger). The image was analyzed with STDWeb/STDPipe (Karpov 2025). The photometry was calibrated using nearby stars from the PanSTARRS catalog, is in the AB system, and is not corrected for Galactic extinction. We detected the optical counterpart, (Palmerio et al., GCN Circ. 42223; Perez-Garcia et al., GCN Circ. 42225; Konno et al., GCN Circ. 42226; Martin-Carrillo et al., GCN Circ. 42227; Masi et al., GCN Circ. 42228; Palmerio et al., GCN Circ. 42229; Moskvitin et al., GCN Circ. 42230; Gompertz et al., GCN Circ. 42231; Lipunov et al., GCN Circ. 42235; and Garnavich et al., GCN Circ. 42240; Watson et al. GCN Circ. 42241) with a preliminary magnitude of: r = 18.50 +/- 0.03 Compared to the observation reported by Garnevich (GCN Circ. 42240), our observation suggests an abrupt fading between 6.4 and 8.7 hours. Further observations and analysis are 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/42242. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40312] GRB 251013C: DDOTI detection of the optical afterglow
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42241 SUBJECT: GRB 251013C: DDOTI detection of the optical afterglow DATE: 25/10/14 03:26:13 GMT FROM: Alan Watson at UNAM <alan(a)astro.unam.mx> Alan M. Watson (UNAM), Camila Angulo Valdez (UNAM), Rosa L. Becerra (U Roma), Nat Butler (ASU), Simone Dichiara (Penn State University), Tsvetelina Dimitrova (ASU), Alexander Kutyrev (GSFC/UMD), William H. Lee (UNAM), Océlotl López (UNAM), Margarita Pereyra (UNAM) and Eleonora Troja (U Roma) report: We observed the field of GRB 251013C detected by Fermi/GBM (Fermi GBM Team, GCN Circ. 42221) and SVOM/ECLAIRS (Rakotondrainibe et al., GCN Circ. 42222) with the DDOTI wide-field imager at the Observatorio Astronómico Nacional on Sierra San Pedro Mártir (http://ddoti.astroscu.unam.mx) from 2025-10-14 02:41 to 03:08 (8.80 to 9.45 hours after the trigger) and obtained a total of 23 minutes of exposure in the w filter. We detect the optical afterglow (Palmerio et al., GCN Circ. 42223; Perez-Garcia et al., GCN Circ. 42225; Konno et al., GCN Circ. 42226; Martin-Carrillo et al., GCN Circ. 42227; Masi et al., GCN Circ. 42228; Palmerio et al., GCN Circ. 42229; Moskvitin et al., GCN Circ. 42230; Gompertz et al., GCN Circ. 42231; Lipunov et al., GCN Circ. 42235; and Garnavich et al., GCN Circ. 42240) with a preliminary magnitude of w = 18.95 +/- 0.04 Our photometry is calibrated against the USNO-B1 and Pan-STARRS PS1 DR2 catalogues and is not corrected for Galactic extinction. Observations are continuing. We thank the staff of the Observatorio Astronómico Nacional at the Sierra de San Pedro Mártir for their excellent support. View this GCN Circular online at https://gcn.nasa.gov/circulars/42241. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40311] GRB 20251013C: SLKT optical afterglow photometry
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42240 SUBJECT: GRB 20251013C: SLKT optical afterglow photometry DATE: 25/10/14 02:43:16 GMT FROM: Peter Garnavich at U of Notre Dame <pgarnavi(a)nd.edu> P. Garnavich (University of Notre Dame) reports: The Sarah L. Krizmanich Telescope (SLKT) obtained unfiltered observations of the SVOM/ECLAIRs source GRB 251013C (Rakotondrainibe et al., GCN 42222). Imaging was centered at 2025 October 14.002 (UT) which was 6.4 hours after the GRB trigger. Exposures totaled 320s and the afterglow was clearly detected. Compared to the nearby star at 23:03:20.64 -00:10:13.8 (2000) with a SDSS magnitude of r=14.40 mag, the afterglow had a brightness of r=17.48+/-0.06 mag. View this GCN Circular online at https://gcn.nasa.gov/circulars/42240. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40310] Swift GRB 251014A: Global MASTER-Net observations report
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42239 SUBJECT: Swift GRB 251014A: Global MASTER-Net observations report DATE: 25/10/14 00:47:01 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-SAAO robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in South Africa (South African Astronomical Observatory) was pointed to the Swift GRB 251014A ( E. Ambrosi et al., GCN 42238) errorbox 26 sec after notice time and 361 sec after trigger time at 2025-10-14 00:34:31 UT, with upper limit up to 18.5 mag. The observations began at zenith distance = 68 deg. The sun altitude is -39.4 deg. The galactic latitude b = 11 deg., longitude l = 212 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3014236 We obtain a following upper limits. Tmid-T0 | Site |Filt.| Expt. | Limit| Comment _________|_____________________|_____|_______|______|________ 391 | MASTER-SAAO | C | 60 | 18.5 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. View this GCN Circular online at https://gcn.nasa.gov/circulars/42239. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40309] GRB 251014A: Swift detection of a possibly-short burst
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42238 SUBJECT: GRB 251014A: Swift detection of a possibly-short burst DATE: 25/10/14 00:42:58 GMT FROM: David Palmer at LANL <palmer(a)lanl.gov> E. Ambrosi (INAF-IASFPA), V. D'Elia (SSDC & INAF-OAR), R. Gupta (NASA GSFC) and D. M. Palmer (LANL) report on behalf of the Neil Gehrels Swift Observatory Team: At 00:28:30 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 251014A (trigger=1403878). Swift did not slew immediately due to an observation constraint. The BAT on-board calculated location is RA, Dec 111.732, +6.415 which is RA(J2000) = 07h 26m 56s Dec(J2000) = +06d 24' 54" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a single peak structure with a duration of about 1.5 sec. The peak count rate was ~3000 counts/sec (15-350 keV), at ~0 sec after the trigger. Due to a Moon observing constraint, Swift cannot slew to the BAT position until 21:52 UT on 2025 October 14. There will thus be no XRT or UVOT data for this trigger before this time. Burst Advocate for this burst is E. Ambrosi (elena.ambrosi AT inaf.it). 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/42238. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40308] GRB 251014A: Fermi GBM Final Real-time Localization
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42237 SUBJECT: GRB 251014A: Fermi GBM Final Real-time Localization DATE: 25/10/14 00:39:10 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 SHORT GRB At 00:28:30 UT on 14 Oct 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 251014A (trigger 782094515.336852 / 251014020). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 114.7, Dec = 7.4 (J2000 degrees, equivalent to J2000 07h 38m, 7d 24'), with a statistical uncertainty of 8.3 degrees. The angle from the Fermi LAT boresight is 45.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251014020/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251014020/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn251014020/… View this GCN Circular online at https://gcn.nasa.gov/circulars/42237. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40307] Fermi trigger No 782044789: Global MASTER-Net observations report
by GCN Circulars 14 Oct '25

14 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42236 SUBJECT: Fermi trigger No 782044789: Global MASTER-Net observations report DATE: 25/10/14 00:15:33 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-OAFA robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in Argentina (OAFA observatory of San Juan National University) started inspect of the Fermi GRB251013.44 (trigger No 782044789,16h 21m 00.00s , -23d 58m 58.8s, R=50) errorbox 46947 sec after notice time and 46980 sec after trigger time at 2025-10-13 23:42:44 UT, with upper limit up to 19.5 mag. Observations started at twilight. The observations began at zenith distance = 6 deg. The sun altitude is -13.0 deg. The galactic latitude b = 18 deg., longitude l = 353 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3013722 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 47010 | 2025-10-13 23:42:44 | MASTER-OAFA | (20h 11m 08.20s , -31d 38m 07.6s) | C | 60 | 19.5 | 47086 | 2025-10-13 23:44:00 | MASTER-OAFA | (20h 11m 08.28s , -31d 39m 50.4s) | C | 60 | 19.3 | 47162 | 2025-10-13 23:45:15 | MASTER-OAFA | (20h 11m 12.39s , -31d 38m 20.4s) | C | 60 | 19.5 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. View this GCN Circular online at https://gcn.nasa.gov/circulars/42236. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40306] Fermi GRB 251013C: Global MASTER-Net observations report
by GCN Circulars 13 Oct '25

13 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42235 SUBJECT: Fermi GRB 251013C: Global MASTER-Net observations report DATE: 25/10/13 23:46:00 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-SAAO robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in South Africa (South African Astronomical Observatory) started inspect of the Fermi GRB 251013C ( Fermi GBM team, GCN 42221) errorbox 10000 sec after notice time and 10034 sec after trigger time at 2025-10-13 20:26:56 UT, with upper limit up to 20.4 mag. The observations began at zenith distance = 32 deg. The sun altitude is -41.1 deg. The galactic latitude b = -59 deg., longitude l = 72 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3013941 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 10064 | 2025-10-13 20:26:56 | MASTER-SAAO | (23h 02m 39.24s , -00d 30m 39.4s) | C | 60 | 18.6 | 10158 | 2025-10-13 20:28:29 | MASTER-SAAO | (23h 02m 46.41s , -00d 31m 36.1s) | C | 60 | 18.7 | 10251 | 2025-10-13 20:30:02 | MASTER-SAAO | (23h 02m 40.37s , -00d 32m 32.6s) | C | 60 | 18.9 | 10345 | 2025-10-13 20:31:37 | MASTER-SAAO | (23h 02m 47.55s , -00d 32m 05.9s) | C | 60 | 18.8 | 10441 | 2025-10-13 20:33:12 | MASTER-SAAO | (23h 02m 45.46s , -00d 30m 49.0s) | C | 60 | 18.7 | 10539 | 2025-10-13 20:34:50 | MASTER-SAAO | (23h 02m 46.25s , -00d 32m 02.3s) | C | 60 | 18.6 | 10664 | 2025-10-13 20:36:25 | MASTER-SAAO | (23h 02m 49.67s , -00d 30m 22.6s) | C | 120 | 18.9 | 10817 | 2025-10-13 20:38:58 | MASTER-SAAO | (23h 02m 45.08s , -00d 31m 17.6s) | C | 120 | 18.8 | 10980 | 2025-10-13 20:41:42 | MASTER-SAAO | (23h 02m 47.31s , -00d 30m 13.8s) | C | 120 | 19.0 | 11135 | 2025-10-13 20:44:17 | MASTER-SAAO | (23h 02m 52.66s , -00d 31m 09.8s) | C | 120 | 19.0 | 11292 | 2025-10-13 20:46:54 | MASTER-SAAO | (23h 02m 47.94s , -00d 32m 05.5s) | C | 120 | 19.2 | 11446 | 2025-10-13 20:49:27 | MASTER-SAAO | (23h 02m 55.30s , -00d 32m 00.3s) | C | 120 | 19.2 | 11630 | 2025-10-13 20:52:01 | MASTER-SAAO | (23h 02m 53.52s , -00d 30m 03.7s) | C | 180 | 19.2 | 11847 | 2025-10-13 20:55:39 | MASTER-SAAO | (23h 02m 54.71s , -00d 31m 32.8s) | C | 180 | 19.2 | 12064 | 2025-10-13 20:59:15 | MASTER-SAAO | (23h 02m 58.96s , -00d 29m 55.7s) | C | 180 | 19.4 | 12247 | 2025-10-13 21:02:48 | MASTER-SAAO | (23h 02m 53.36s , -00d 30m 39.0s) | C | 120 | 19.4 | 12399 | 2025-10-13 21:05:21 | MASTER-SAAO | (23h 02m 55.07s , -00d 29m 35.0s) | C | 120 | 19.4 | 12519 | 2025-10-13 21:05:21 | MASTER-SAAO | (23h 02m 55.07s , -00d 29m 35.0s) | C | 360 | 20.1 | Coadd 12554 | 2025-10-13 21:07:55 | MASTER-SAAO | (23h 03m 01.04s , -00d 30m 30.6s) | C | 120 | 19.4 | 12722 | 2025-10-13 21:10:43 | MASTER-SAAO | (23h 02m 55.49s , -00d 31m 25.3s) | C | 120 | 19.7 | 12875 | 2025-10-13 21:13:16 | MASTER-SAAO | (23h 03m 01.00s , -00d 31m 12.9s) | C | 120 | 19.4 | 12995 | 2025-10-13 21:13:16 | MASTER-SAAO | (23h 03m 01.00s , -00d 31m 12.9s) | C | 360 | 20.4 | Coadd 13030 | 2025-10-13 21:15:51 | MASTER-SAAO | (23h 02m 59.29s , -00d 29m 35.6s) | C | 120 | 19.7 | 13194 | 2025-10-13 21:18:36 | MASTER-SAAO | (23h 02m 59.68s , -00d 30m 53.7s) | C | 120 | 19.6 | 13347 | 2025-10-13 21:21:09 | MASTER-SAAO | (23h 03m 02.87s , -00d 29m 15.8s) | C | 120 | 19.9 | 13502 | 2025-10-13 21:23:44 | MASTER-SAAO | (23h 02m 57.06s , -00d 30m 00.8s) | C | 120 | 19.8 | 16491 | 2025-10-13 22:14:02 | MASTER-SAAO | (23h 07m 20.08s , -06d 42m 29.2s) | C | 60 | 18.9 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. View this GCN Circular online at https://gcn.nasa.gov/circulars/42235. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 40305] Fermi GRB 251013C: Global MASTER-Net observations report
by GCN Circulars 13 Oct '25

13 Oct '25

TITLE: GCN CIRCULAR NUMBER: 42235 SUBJECT: Fermi GRB 251013C: Global MASTER-Net observations report DATE: 25/10/13 23:46:00 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-SAAO robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in South Africa (South African Astronomical Observatory) started inspect of the Fermi GRB 251013C ( Fermi GBM team, GCN 42221) errorbox 10000 sec after notice time and 10034 sec after trigger time at 2025-10-13 20:26:56 UT, with upper limit up to 20.4 mag. The observations began at zenith distance = 32 deg. The sun altitude is -41.1 deg. The galactic latitude b = -59 deg., longitude l = 72 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3013941 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 10064 | 2025-10-13 20:26:56 | MASTER-SAAO | (23h 02m 39.24s , -00d 30m 39.4s) | C | 60 | 18.6 | 10158 | 2025-10-13 20:28:29 | MASTER-SAAO | (23h 02m 46.41s , -00d 31m 36.1s) | C | 60 | 18.7 | 10251 | 2025-10-13 20:30:02 | MASTER-SAAO | (23h 02m 40.37s , -00d 32m 32.6s) | C | 60 | 18.9 | 10345 | 2025-10-13 20:31:37 | MASTER-SAAO | (23h 02m 47.55s , -00d 32m 05.9s) | C | 60 | 18.8 | 10441 | 2025-10-13 20:33:12 | MASTER-SAAO | (23h 02m 45.46s , -00d 30m 49.0s) | C | 60 | 18.7 | 10539 | 2025-10-13 20:34:50 | MASTER-SAAO | (23h 02m 46.25s , -00d 32m 02.3s) | C | 60 | 18.6 | 10664 | 2025-10-13 20:36:25 | MASTER-SAAO | (23h 02m 49.67s , -00d 30m 22.6s) | C | 120 | 18.9 | 10817 | 2025-10-13 20:38:58 | MASTER-SAAO | (23h 02m 45.08s , -00d 31m 17.6s) | C | 120 | 18.8 | 10980 | 2025-10-13 20:41:42 | MASTER-SAAO | (23h 02m 47.31s , -00d 30m 13.8s) | C | 120 | 19.0 | 11135 | 2025-10-13 20:44:17 | MASTER-SAAO | (23h 02m 52.66s , -00d 31m 09.8s) | C | 120 | 19.0 | 11292 | 2025-10-13 20:46:54 | MASTER-SAAO | (23h 02m 47.94s , -00d 32m 05.5s) | C | 120 | 19.2 | 11446 | 2025-10-13 20:49:27 | MASTER-SAAO | (23h 02m 55.30s , -00d 32m 00.3s) | C | 120 | 19.2 | 11630 | 2025-10-13 20:52:01 | MASTER-SAAO | (23h 02m 53.52s , -00d 30m 03.7s) | C | 180 | 19.2 | 11847 | 2025-10-13 20:55:39 | MASTER-SAAO | (23h 02m 54.71s , -00d 31m 32.8s) | C | 180 | 19.2 | 12064 | 2025-10-13 20:59:15 | MASTER-SAAO | (23h 02m 58.96s , -00d 29m 55.7s) | C | 180 | 19.4 | 12247 | 2025-10-13 21:02:48 | MASTER-SAAO | (23h 02m 53.36s , -00d 30m 39.0s) | C | 120 | 19.4 | 12399 | 2025-10-13 21:05:21 | MASTER-SAAO | (23h 02m 55.07s , -00d 29m 35.0s) | C | 120 | 19.4 | 12519 | 2025-10-13 21:05:21 | MASTER-SAAO | (23h 02m 55.07s , -00d 29m 35.0s) | C | 360 | 20.1 | Coadd 12554 | 2025-10-13 21:07:55 | MASTER-SAAO | (23h 03m 01.04s , -00d 30m 30.6s) | C | 120 | 19.4 | 12722 | 2025-10-13 21:10:43 | MASTER-SAAO | (23h 02m 55.49s , -00d 31m 25.3s) | C | 120 | 19.7 | 12875 | 2025-10-13 21:13:16 | MASTER-SAAO | (23h 03m 01.00s , -00d 31m 12.9s) | C | 120 | 19.4 | 12995 | 2025-10-13 21:13:16 | MASTER-SAAO | (23h 03m 01.00s , -00d 31m 12.9s) | C | 360 | 20.4 | Coadd 13030 | 2025-10-13 21:15:51 | MASTER-SAAO | (23h 02m 59.29s , -00d 29m 35.6s) | C | 120 | 19.7 | 13194 | 2025-10-13 21:18:36 | MASTER-SAAO | (23h 02m 59.68s , -00d 30m 53.7s) | C | 120 | 19.6 | 13347 | 2025-10-13 21:21:09 | MASTER-SAAO | (23h 03m 02.87s , -00d 29m 15.8s) | C | 120 | 19.9 | 13502 | 2025-10-13 21:23:44 | MASTER-SAAO | (23h 02m 57.06s , -00d 30m 00.8s) | C | 120 | 19.8 | 16491 | 2025-10-13 22:14:02 | MASTER-SAAO | (23h 07m 20.08s , -06d 42m 29.2s) | C | 60 | 18.9 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. View this GCN Circular online at https://gcn.nasa.gov/circulars/42235. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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