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[vsnet-grb-info 41472] GRB 260111A: Swift ToO observations
by GCN Circulars 12 Jan '26

12 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43379 SUBJECT: GRB 260111A: Swift ToO observations DATE: 26/01/12 18:44:34 GMT FROM: Phil Evans at U of Leicester <pae9(a)star.le.ac.uk> P. A. Evans (U. Leicester) reports on behalf of the Swift team: Swift has initiated a ToO observation of the Swift/BAT-detected event GRB 260111A. Automated analysis of the XRT data will be presented online at https://www.swift.ac.uk/ToO_GRBs/00021897 Any uncatalogued X-ray sources detected in this analysis will be reported on this website and via GCN COUNTERPART notices. These are not necessarily related to the Swift/BAT event. Any X-ray source considered to be a probable afterglow candidate will be reported via a GCN Circular after manual consideration. Details of the XRT automated analysis methods are detailed in Evans et al. (2007, A&A, 469, 379; 2009, MNRAS, 397, 1177 and 2014, ApJS, 210, 8). This circular is an official product of the Swift-XRT team. View this GCN Circular online at https://gcn.nasa.gov/circulars/43379. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41471] GRB 251230A: Mondy Optical Observations
by GCN Circulars 12 Jan '26

12 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43378 SUBJECT: GRB 251230A: Mondy Optical Observations DATE: 26/01/12 15:10:09 GMT FROM: Alina Volnova at IKI RAS <alinusss(a)gmail.com> N. Pankov (HSE, IKI), A. Pozanenko (IKI), E. Klunko (ISTP), A. Volnova (IKI) report on behalf of IKI-GRB-FuN: We performed optical observations of the field of GRB 251230A (Lanava et al., GCN 43252; Wang et. al, GCN 43259; Osborne et. al, GCN 43263; Wang et. al, GCN 43272; Sbarrato et al., GCN 43275; Guo et. al, GCN 43299; Guo et. al, GCN 43301) in the R filter with the AZT-33IK 1.5-meter telescope of the Sayan Solar Observatory (SSO Mondy). The observations began on 2025-12-30 19:36:42 UT, i.e. ~0.77 days since trigger. The optical counterpart (Li et al., GCN 43255; Busmann et al., GCN 43258; Masi et al., GCN 43260; Ghosh et al., GCN 43262; Ma et al., GCN 43265; He et al., GCN 43269; Breeveld et. al, GCN 43271; He et al., GCN 43280; Antier et. al, GCN 43281; Ma et al., GCN 43282; Chatterjee et. al, GCN 43321) is not detected in the co-add image. The preliminary photometry and observation details are provided below: Date UT start t-T0 Exp. Filter OT Err. UL (mid, days) (s) (3sigma) 2025-12-30 19:36:42 0.77001 15*120 R n/d n/d 20.4 The photometry was calibrated using nearby stars from USNO-B1.0 and is not corrected for the Galactic extinction. The obtained results do not contradict the measurements reported by other teams, including upper limits (Starling et. al, GCN 43267; Tak et al., GCN 43270; Gupta et. al, GCN 43277; Sankar et al., GCN 43279). View this GCN Circular online at https://gcn.nasa.gov/circulars/43378. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41470] GRB 260111A: Swift/BAT-GUANO arcminute localization of a burst
by GCN Circulars 12 Jan '26

12 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43377 SUBJECT: GRB 260111A: Swift/BAT-GUANO arcminute localization of a burst DATE: 26/01/12 08:48:14 GMT FROM: Samuele Ronchini at PSU <sjs8171(a)psu.edu> Samuele Ronchini (GSSI), Aaron Tohuvavohu (Cosmic Frontier), James DeLaunay (PSU), Jamie A. Kennea (PSU), Tyler Parsotan (NASA GSFC), Maia Williams (Northwestern) report: Swift/BAT did not localize GRB 260111A onboard (T0: 2026-01-11T16:33:14.01 UTC, Fermi GCN 43370). The Fermi notice, distributed in near real-time, triggered the Swift Mission Operations Center operated Gamma-ray Urgent Archiver for Novel Opportunities (GUANO; Tohuvavohu et al. 2020, ApJ, 900, 1). Upon trigger by this notice, GUANO sent a command to the Swift Burst Alert Telescope (BAT) to save 200 seconds of BAT event-mode data from [-50,+150] seconds around the time of the burst. All the requested event mode data was delivered to the ground. The position is found with the newly developed pipeline BAT-GLIMPSE: Gamma-ray Localization using Imaging and Mosaic techniques for Pointing and Slew Epochs (Ronchini et. al, in prep). The pipeline makes use of the tools from BatAnalysis (Parsotan et al. 2025). The source was detected with an SNR = 19.7 in a 8.192 s analysis time bin starting at t0 - 4.096 s. Independently, the BAT likelihood search, NITRATES (DeLaunay + Tohuvavohu 2022, ApJ, 941, 169), confirms the detection and position of the burst in a 8.192 s analysis time bin starting at T0 - 4.096 s with a sqrt(TS) of 36.98. An arcminute localization is found with DeltaLLHOut of 317.21 and a DeltaLLHPeak of 302.45. See Section 9.1 and Figures 10 and 17 in the NITRATES paper for brief descriptions and interpretations of sqrt(TS), DeltaLLHPeak, and DeltaLLHOut. The NITRATES and BAT-GLIMPSE positions are compatible. The BAT position is: RA, Dec = 229.57340, 51.97470 deg which is RA(J2000) = 15h 18m 17.6s Dec(J2000) = 51d 58' 28.9" with an estimated uncertainty of 5 arcmin radius. More details about this burst can be found on the trigger report page here: https://guano.swift.psu.edu/trigger_report?id=789842031 XRT and UVOT follow-up has been requested. Results of follow-up observations will be reported in future circulars. GUANO is a fully autonomous, extremely low latency, spacecraft commanding pipeline designed for targeted recovery of BAT event mode data around the times of compelling astrophysical events to enable more sensitive GRB searches. A live reporting of Swift/BAT event data recovered by GUANO can be found at: https://www.swift.psu.edu/guano/ View this GCN Circular online at https://gcn.nasa.gov/circulars/43377. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41469] GRB 260112A: Fermi GBM Final Real-time Localization
by GCN Circulars 12 Jan '26

12 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43376 SUBJECT: GRB 260112A: Fermi GBM Final Real-time Localization DATE: 26/01/12 05:36:31 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 05:25:50 UT on 12 Jan 2026, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 260112A (trigger 789888355.72541 / 260112226). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 326.5, Dec = -37.8 (J2000 degrees, equivalent to J2000 21h 45m, -37d 47'), with a statistical uncertainty of 18.3 degrees. The angle from the Fermi LAT boresight is 112.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260112226/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260112226/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260112226/… View this GCN Circular online at https://gcn.nasa.gov/circulars/43376. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41468] EP260110a: SVOM/VT optical upper limits
by GCN Circulars 12 Jan '26

12 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43375 SUBJECT: EP260110a: SVOM/VT optical upper limits DATE: 26/01/12 04:40:42 GMT FROM: Huali Li at at NAOC, SVOM <lhl(a)nao.cas.cn> H. L. Li, L. P. Xin, Y. L. Qiu, C. Wu, Y. N. Ma, Z. H. Yao, X. H. Han, J. Wang, P. P. Zhang, Y. Xu, 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 ToO observation on the fast X-ray transient EP260110a (Zhang et al., GCN 43363; 43367). The observation started on 2026-01-10T14:29:11 UT (i.e. 2.52 hour post trigger) in VT_B (400nm-650nm) and VT_R (650nm-1000nm) channel simultaneously. Inside the error box of the EP-FXT (Zhang et al., GCN 43367) we did not detect any new uncatalogued source, which was consistent with the non detections reported by other groups (Perez-Garcia et al., GCN 43364; Kang et al., GCN 43365; Antier et al., GCN 43366; Zheng et al., GCN 43368; Lipunov et al., GCN 43372). The 3 sigma limits in AB magnitude are derived as below: Mid time | Band | Exposure Time | 3 sigma limit magnitude 4.11 hour VT_B 52*70 sec > 23.5 4.64 hour VT_R 50*70 sec > 23.5 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/43375. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41467] IceCube-260111A - IceCube observation of a high-energy neutrino candidate track-like event
by GCN Circulars 11 Jan '26

11 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43374 SUBJECT: IceCube-260111A - IceCube observation of a high-energy neutrino candidate track-like event DATE: 26/01/11 22:48:41 GMT FROM: Giacomo Sommani at Ruhr-Universität Bochum <gsommani(a)icecube.wisc.edu> The IceCube Collaboration (http://icecube.wisc.edu/) reports: On 26-01-11 at 20:10:33.91 UT IceCube detected a track-like event with a moderate probability of being of astrophysical origin. The event was selected by the ICECUBE_Astrotrack_BRONZE alert stream. The average astrophysical neutrino purity for Bronze alerts is 30%. This alert has an estimated false alarm rate of 0.7434 events per year due to atmospheric backgrounds. The IceCube detector was in a normal operating state at the time of detection. After the initial automated alert (https://gcn.gsfc.nasa.gov/notices_amon_g_b/141893_3811884.amon) more sophisticated reconstruction algorithms have been applied offline, with the direction refined to: Date: 26-01-11 Time: 20:10:33.91 UT RA: 70.88 (+1.55/-1.4 deg 90% PSF containment) J2000 Dec: 34.59 (+0.76/-0.64 deg 90% PSF containment) J2000 One gamma-ray source from the Fermi 4FGL-DR4 catalog is located within the 90% uncertainty region of this event: 4FGL J0444.6+3425, at RA = 71.16° and Dec = 34.42° (J2000), with an angular separation of 0.29° from the best-fit event position. The IceCube Neutrino Observatory is a cubic-kilometer neutrino detector operating at the geographic South Pole, Antarctica. The IceCube realtime alert point of contact can be reached at roc(a)icecube.wisc.edu View this GCN Circular online at https://gcn.nasa.gov/circulars/43374. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41466] IceCube Alert 260111.84: Global MASTER-Net observations report
by GCN Circulars 11 Jan '26

11 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43373 SUBJECT: IceCube Alert 260111.84: Global MASTER-Net observations report DATE: 26/01/11 20:39:22 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-Kislovodsk robotic telescope [1] located in Russia (Lomonosov MSU, Kislovodsk Solar Station of Pulkovo observatory) was pointed to the IceCube Alert 260111.84 (trigger No 3811884,04h 44m 30.72s , +35d 03m 43.2s, R=0.51) errorbox 12 sec after notice time and 58 sec after trigger time at 2026-01-11 20:11:32 UT, with upper limit up to 19.2 mag. The observations began at zenith distance = 21 deg. The sun altitude is -64.6 deg. MASTER-Tunka robotic telescope located in Russia (Applied Physics Institute, Irkutsk State University) was pointed to the IceCube Alert 260111.84 errorbox 26 sec after notice time and 72 sec after trigger time at 2026-01-11 20:11:46 UT, with upper limit up to 14.1 mag. The observations began at zenith distance = 61 deg. The sun altitude is -44.9 deg. MASTER-SAAO robotic telescope located in South Africa (South African Astronomical Observatory) was pointed to the IceCube Alert 260111.84 errorbox 61 sec after notice time and 107 sec after trigger time at 2026-01-11 20:12:21 UT, with upper limit up to 18.9 mag. The observations began at zenith distance = 67 deg. The sun altitude is -24.8 deg. The galactic latitude b = -6 deg., longitude l = 168 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3100219 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 64 | 2026-01-11 20:11:32 | MASTER-Kislovodsk | (04h 43m 04.86s , +35d 34m 12.2s) | P| | 10 | 15.9 | 64 | 2026-01-11 20:11:32 | MASTER-Kislovodsk | (04h 43m 29.08s , +35d 12m 14.1s) | C | 10 | 16.9 | 89 | 2026-01-11 20:11:32 | MASTER-Kislovodsk | (04h 43m 29.08s , +35d 12m 14.1s) | C | 60 | 18.0 | Coadd 78 | 2026-01-11 20:11:46 | MASTER-Tunka | (04h 43m 38.90s , +35d 16m 36.1s) | P- | 10 | 14.1 | 78 | 2026-01-11 20:11:46 | MASTER-Tunka | (04h 43m 07.38s , +35d 23m 28.3s) | P| | 10 | 13.0 | 99 | 2026-01-11 20:12:02 | MASTER-Kislovodsk | (04h 43m 04.82s , +35d 34m 09.7s) | P| | 20 | 16.4 | 99 | 2026-01-11 20:12:02 | MASTER-Kislovodsk | (04h 43m 29.04s , +35d 12m 12.1s) | C | 20 | 17.4 | 118 | 2026-01-11 20:12:21 | MASTER-SAAO | (04h 42m 05.60s , +34d 48m 35.2s) | C | 20 | 18.0 | 153 | 2026-01-11 20:12:21 | MASTER-SAAO | (04h 42m 05.60s , +34d 48m 35.2s) | C | 90 | 18.9 | 118 | 2026-01-11 20:12:21 | MASTER-SAAO | (04h 40m 03.11s , +35d 04m 27.6s) | C | 20 | 17.8 | 153 | 2026-01-11 20:12:21 | MASTER-SAAO | (04h 40m 03.11s , +35d 04m 27.6s) | C | 90 | 18.8 | 145 | 2026-01-11 20:12:43 | MASTER-Kislovodsk | (04h 43m 28.95s , +35d 12m 09.1s) | C | 30 | 17.8 | 145 | 2026-01-11 20:12:43 | MASTER-Kislovodsk | (04h 43m 04.76s , +35d 34m 06.1s) | P| | 30 | 17.0 | 162 | 2026-01-11 20:13:01 | MASTER-SAAO | (04h 42m 05.86s , +34d 48m 37.9s) | C | 30 | 18.3 | 162 | 2026-01-11 20:13:01 | MASTER-SAAO | (04h 40m 03.42s , +35d 04m 31.2s) | C | 30 | 18.2 | 200 | 2026-01-11 20:13:33 | MASTER-Kislovodsk | (04h 43m 04.72s , +35d 34m 02.5s) | P| | 40 | 16.9 | 200 | 2026-01-11 20:13:33 | MASTER-Kislovodsk | (04h 43m 28.88s , +35d 12m 06.2s) | C | 40 | 17.9 | 255 | 2026-01-11 20:13:33 | MASTER-Kislovodsk | (04h 43m 28.89s , +35d 12m 06.1s) | C | 150 | 18.7 | Coadd 216 | 2026-01-11 20:13:49 | MASTER-SAAO | (04h 42m 06.14s , +34d 48m 40.7s) | C | 40 | 18.4 | 216 | 2026-01-11 20:13:50 | MASTER-SAAO | (04h 40m 03.68s , +35d 04m 34.5s) | C | 40 | 18.2 | 265 | 2026-01-11 20:14:33 | MASTER-Kislovodsk | (04h 43m 04.64s , +35d 33m 58.2s) | P| | 50 | 17.1 | 265 | 2026-01-11 20:14:33 | MASTER-Kislovodsk | (04h 43m 28.78s , +35d 12m 02.4s) | C | 50 | 18.0 | 280 | 2026-01-11 20:14:49 | MASTER-SAAO | (04h 42m 06.49s , +34d 48m 43.7s) | C | 50 | 18.5 | 280 | 2026-01-11 20:14:49 | MASTER-SAAO | (04h 40m 03.97s , +35d 04m 38.1s) | C | 50 | 18.4 | 341 | 2026-01-11 20:15:44 | MASTER-Kislovodsk | (04h 43m 28.69s , +35d 11m 58.8s) | C | 60 | 18.2 | 341 | 2026-01-11 20:15:44 | MASTER-Kislovodsk | (04h 43m 04.53s , +35d 33m 54.1s) | P| | 60 | 17.4 | 354 | 2026-01-11 20:15:58 | MASTER-SAAO | (04h 42m 06.82s , +34d 48m 46.7s) | C | 60 | 18.8 | 354 | 2026-01-11 20:15:58 | MASTER-SAAO | (04h 40m 04.29s , +35d 04m 41.7s) | C | 60 | 18.5 | 432 | 2026-01-11 20:17:05 | MASTER-Kislovodsk | (04h 43m 04.39s , +35d 33m 49.7s) | P| | 80 | 17.4 | 432 | 2026-01-11 20:17:05 | MASTER-Kislovodsk | (04h 43m 28.56s , +35d 11m 55.0s) | C | 80 | 18.4 | 542 | 2026-01-11 20:17:05 | MASTER-Kislovodsk | (04h 43m 28.56s , +35d 11m 54.9s) | C | 300 | 19.2 | Coadd 433 | 2026-01-11 20:17:17 | MASTER-SAAO | (04h 42m 07.12s , +34d 48m 50.4s) | C | 60 | 18.7 | 433 | 2026-01-11 20:17:17 | MASTER-SAAO | (04h 40m 04.61s , +35d 04m 45.6s) | C | 60 | 18.6 | 513 | 2026-01-11 20:18:36 | MASTER-SAAO | (04h 42m 07.48s , +34d 48m 53.0s) | C | 60 | 18.8 | 513 | 2026-01-11 20:18:36 | MASTER-SAAO | (04h 40m 04.97s , +35d 04m 48.8s) | C | 60 | 18.6 | 552 | 2026-01-11 20:18:56 | MASTER-Kislovodsk | (04h 43m 28.37s , +35d 11m 50.5s) | C | 100 | 18.4 | 552 | 2026-01-11 20:18:56 | MASTER-Kislovodsk | (04h 43m 04.21s , +35d 33m 44.7s) | P| | 100 | 17.6 | 592 | 2026-01-11 20:19:55 | MASTER-SAAO | (04h 42m 07.81s , +34d 48m 55.7s) | C | 60 | 18.8 | 592 | 2026-01-11 20:19:55 | MASTER-SAAO | (04h 40m 05.29s , +35d 04m 51.9s) | C | 60 | 18.6 | 683 | 2026-01-11 20:20:56 | MASTER-Kislovodsk | (04h 43m 04.05s , +35d 33m 39.6s) | P| | 120 | 17.6 | 683 | 2026-01-11 20:20:56 | MASTER-Kislovodsk | (04h 43m 28.20s , +35d 11m 46.1s) | C | 120 | 18.4 | 671 | 2026-01-11 20:21:14 | MASTER-SAAO | (04h 42m 08.14s , +34d 48m 58.6s) | C | 60 | 18.8 | 671 | 2026-01-11 20:21:14 | MASTER-SAAO | (04h 40m 05.62s , +35d 04m 55.0s) | C | 60 | 18.7 | 750 | 2026-01-11 20:22:33 | MASTER-SAAO | (04h 42m 08.48s , +34d 49m 01.7s) | C | 60 | 18.8 | 750 | 2026-01-11 20:22:33 | MASTER-SAAO | (04h 40m 05.95s , +35d 04m 58.4s) | C | 60 | 18.6 | 833 | 2026-01-11 20:23:27 | MASTER-Kislovodsk | (04h 43m 27.94s , +35d 11m 41.5s) | C | 120 | 18.5 | 840 | 2026-01-11 20:23:33 | MASTER-Kislovodsk | (04h 43m 03.83s , +35d 33m 33.8s) | P| | 120 | 17.8 | 829 | 2026-01-11 20:23:52 | MASTER-SAAO | (04h 42m 08.82s , +34d 49m 04.0s) | C | 60 | 18.8 | 829 | 2026-01-11 20:23:52 | MASTER-SAAO | (04h 40m 06.27s , +35d 05m 01.0s) | C | 60 | 18.6 | 981 | 2026-01-11 20:25:54 | MASTER-Kislovodsk | (04h 43m 03.62s , +35d 33m 28.6s) | P| | 120 | 17.6 | 981 | 2026-01-11 20:25:54 | MASTER-Kislovodsk | (04h 43m 27.69s , +35d 11m 36.9s) | C | 120 | 18.4 | 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/43373. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41465] EP260110a: Global MASTER-Net observations report
by GCN Circulars 11 Jan '26

11 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43372 SUBJECT: EP260110a: Global MASTER-Net observations report DATE: 26/01/11 19:09:24 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-Kislovodsk robotic telescope [1] located in Russia (Lomonosov MSU, Kislovodsk Solar Station of Pulkovo observatory) was pointed to the EP260110a ( EP Team et al., GCN 43363) errorbox 1 days 21876 sec after notice time and 1 days 25310 sec after trigger time at 2026-01-11 18:58:48 UT, with upper limit up to 17.6 mag. The observations began at zenith distance = 62 deg. The sun altitude is -54.1 deg. The galactic latitude b = 51 deg., longitude l = 118 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3099928 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 111800 | 2026-01-11 18:58:48 | MASTER-Kislovodsk | (13h 17m 27.89s , +65d 50m 39.1s) | C | 180 | 16.4 | 111800 | 2026-01-11 18:58:48 | MASTER-Kislovodsk | (13h 17m 45.69s , +65d 27m 35.9s) | C | 180 | 17.6 | 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/43372. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41464] Fermi GRB 260111A: Global MASTER-Net observations report
by GCN Circulars 11 Jan '26

11 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43371 SUBJECT: Fermi GRB 260111A: Global MASTER-Net observations report DATE: 26/01/11 17:15:39 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 260111A ( Fermi GBM team, GCN 43370) errorbox 201 sec after notice time and 236 sec after trigger time at 2026-01-11 16:37:10 UT, with upper limit up to 19.5 mag. The observations began at zenith distance = 70 deg. The sun altitude is -59.9 deg. The galactic latitude b = 56 deg., longitude l = 85 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3100149 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 262 | 2026-01-11 16:37:10 | MASTER-Tunka | (14h 52m 29.86s , +46d 07m 42.6s) | C | 50 | 17.8 | 262 | 2026-01-11 16:37:10 | MASTER-Tunka | (14h 52m 01.47s , +46d 14m 15.0s) | C | 50 | 18.3 | 320 | 2026-01-11 16:38:04 | MASTER-Tunka | (14h 52m 01.36s , +46d 14m 14.7s) | C | 60 | 18.5 | 320 | 2026-01-11 16:38:04 | MASTER-Tunka | (14h 52m 29.78s , +46d 07m 43.0s) | C | 60 | 18.1 | 384 | 2026-01-11 16:39:07 | MASTER-Tunka | (14h 52m 01.23s , +46d 14m 15.1s) | C | 60 | 18.3 | 384 | 2026-01-11 16:39:07 | MASTER-Tunka | (14h 52m 29.72s , +46d 07m 43.8s) | C | 60 | 18.0 | 607 | 2026-01-11 16:42:51 | MASTER-Tunka | (14h 58m 24.98s , +50d 10m 13.5s) | C | 60 | 18.8 | 667 | 2026-01-11 16:42:51 | MASTER-Tunka | (14h 58m 24.98s , +50d 10m 13.5s) | C | 180 | 19.5 | Coadd 607 | 2026-01-11 16:42:51 | MASTER-Tunka | (14h 58m 56.47s , +50d 03m 31.9s) | C | 60 | 18.4 | 670 | 2026-01-11 16:43:54 | MASTER-Tunka | (14h 58m 56.32s , +50d 03m 33.3s) | C | 60 | 18.4 | 670 | 2026-01-11 16:43:54 | MASTER-Tunka | (14h 58m 24.82s , +50d 10m 13.4s) | C | 60 | 18.7 | 734 | 2026-01-11 16:44:58 | MASTER-Tunka | (14h 58m 24.70s , +50d 10m 13.5s) | C | 60 | 18.7 | 734 | 2026-01-11 16:44:58 | MASTER-Tunka | (14h 58m 56.28s , +50d 03m 33.8s) | C | 60 | 18.3 | 797 | 2026-01-11 16:46:01 | MASTER-Tunka | (14h 58m 24.72s , +50d 10m 13.7s) | C | 60 | 18.6 | 797 | 2026-01-11 16:46:01 | MASTER-Tunka | (14h 58m 56.30s , +50d 03m 33.8s) | C | 60 | 18.3 | 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/43371. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41463] GRB 260111A: Fermi GBM Final Real-time Localization
by GCN Circulars 11 Jan '26

11 Jan '26

TITLE: GCN CIRCULAR NUMBER: 43370 SUBJECT: GRB 260111A: Fermi GBM Final Real-time Localization DATE: 26/01/11 16:43:36 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 16:33:14 UT on 11 Jan 2026, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 260111A (trigger 789841999.012866 / 260111690). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 224.7, Dec = 50.4 (J2000 degrees, equivalent to J2000 14h 58m, 50d 23'), with a statistical uncertainty of 2.7 degrees. The angle from the Fermi LAT boresight is 12.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260111690/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260111690/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260111690/… View this GCN Circular online at https://gcn.nasa.gov/circulars/43370. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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