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[vsnet-grb-info 41851] EP260214a: Einstein Probe detection of an X-ray transient
by GCN Circulars 15 Feb '26

15 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43742 SUBJECT: EP260214a: Einstein Probe detection of an X-ray transient DATE: 26/02/15 02:39:30 GMT FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn> A. Li (BNU), J. Yang (ZZU), Y. H. Jiang (NJU) and Y. Liu (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 EP260214a. The transient triggered EP-WXT (ID: 01709258386) at 2026-02-14T20:38:04 (UTC). The WXT position of the source is R.A. = 201.250 deg, DEC = -29.040 deg (J2000) with an uncertainty of 3 arcmin in radius (90% C.L. statistical and systematic). A follow-up observation with the Follow-up X-ray Telescope (FXT) was performed automatically. Within the WXT error circle, an uncatalogued X-ray source was detected at R.A. = 201.2326 deg, DEC = -29.0457 deg (J2000) with an uncertainty of 20 arcsec in radius (90% C.L. statistical and systematic). Further information will be updated when the telemetry data is received. Launched on January 9, 2024, EP is a space X-ray observatory to monitor the soft X-ray sky with X-ray follow-up capability (Yuan et al. 2022, Handbook of X-ray and Gamma-ray Astrophysics). View this GCN Circular online at https://gcn.nasa.gov/circulars/43742. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41850] GRB 260212A: AstroSat CZTI detection
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43741 SUBJECT: GRB 260212A: AstroSat CZTI detection DATE: 26/02/14 21:38:15 GMT FROM: Anuraag Arya at IIT Bombay <aryaanuraag910(a)gmail.com> S. Salunke (IUCAA), Harsha K. H. (IUCAA), M. Tembhurnikar (IUCAA), U. Pathak (IITB), A. Arya (IITB), A. Goyal (IITB), G. Waratkar (Caltech/IITB), A. Vibhute (IUCAA), V. Bhalerao (IITB), D. Bhattacharya (Ashoka University/IUCAA), A. R. Rao (IUCAA/TIFR), and S. Vadawale (PRL) report on behalf of the AstroSat CZTI collaboration: Analysis of AstroSat CZTI data with the CIFT framework (Sharma et al., 2021, JApA, 42, 73) showed the detection of a long GRB 260212A which was also detected by Fermi GBM (Fermi GBM Team, GCN Circ. 43716), and Glowbug (Cheung et. al., GCN Circ. 43719). The source was clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range. The light curve showed multiple peaks of emission with the strongest peak at 2026-02-12 17:49:08.04 UTC. The measured peak count rate associated with the burst is 641 (+72, -52) counts/s above the background in the combined data of all quadrants, with a total of 1727 (+302, -376) counts. The local mean background count rate was 1247 (+6, -7) counts/s. We measure a T90 of 9.7 (+1.9, -0.5) s from the cumulative Veto light curve. The source was also faintly detected in the CZT detectors in the 20-200 keV energy range. The light curve showed multiple peaks of emission with the strongest peak at 2026-02-12 17:49:08.50 UTC. The measured peak count rate associated with the burst is 44 (+28, -5) counts/s above the background in the combined data of two quadrants (out of four), with a total of 144 (+111, -95) counts. The local mean background count rate was 130 (+1, -2) counts/s. Due to poor statistics, we cannot reliably estimate the T90 from it. CZTI is built by a TIFR-led consortium of institutes across India, including VSSC, URSC, IUCAA, SAC, and PRL. The Indian Space Research Organisation funded, managed, and facilitated the project. CZTI GRB detections are reported regularly on the payload site at: http://astrosat.iucaa.in/czti/?q=grb View this GCN Circular online at https://gcn.nasa.gov/circulars/43741. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41849] GRB 260212A: Fermi GBM Observation
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43740 SUBJECT: GRB 260212A: Fermi GBM Observation DATE: 26/02/14 20:29:37 GMT FROM: eliza.neights(a)gmail.com Eliza Neights (GWU, NASA GSFC) and C. Meegan (UAH) report on behalf of the Fermi Gamma-ray Burst Monitor Team: "At 17:49:08.21 UT on 12 February 2026, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 260212A (trigger 792611353/260212742), which was also detected by Glowbug (Cheung et al. 2026, GCN 43719), SVOM/GRM (Zhang et al. 2026, GCN 43727), and GECAM-B (Zhang et al. 2026, GCN 43736). The angle from the Fermi LAT boresight is 127 degrees. The GBM light curve consists of multiple emission episodes with a duration (T90) of about 9.7 s (50-300 keV). The time-averaged spectrum from T0-1.5 to T0+14.5 s is best fit by a power law function with an exponential high-energy cutoff. The power law index is -0.66 +/- 0.02 and the cutoff energy, parameterized as Epeak, is 107 +/- 1 keV. The event fluence (10-1000 keV) in this time interval is (7.1 +/- 0.2)E-06 erg/cm^2. The 1-sec peak photon flux measured starting from T0+8.7 s in the 10-1000 keV band is 16.2 +/- 0.6 ph/s/cm^2. A Band function fits the spectrum equally well with Epeak= 90 +/- 1 keV, alpha = -0.43 +/- 0.02 and beta = -2.52 +/- 0.04. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog: https://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html For Fermi GBM data and info, please visit the official Fermi GBM Support Page: https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/" View this GCN Circular online at https://gcn.nasa.gov/circulars/43740. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41848] EP260213a: Liverpool Telescope optical upper limits
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43739 SUBJECT: EP260213a: Liverpool Telescope optical upper limits DATE: 26/02/14 19:02:18 GMT FROM: Rob Eyles-Ferris at U of Leicester <raje1(a)leicester.ac.uk> R. A. J. Eyles-Ferris and R. L. C. Starling (Leicester) report on behalf of a larger collaboration: We observed the field of EP260213a (Yang et al., GCN 43729; Li et al., GCN 43730) with the 2m Liverpool Telescope on La Palma using the IO:O instrument. We obtained 6x150s exposures in each of the SDSS r’ and SDSS g’ filters starting at 2026-02-14 02:35:02 UT, approximately 6.6 hours after the X-ray detection. Within the EP/FXT localisation (Li et al., GCN 43730), we detect no new sources in our stacked images consistent with the results of Cotter et al. (GCN 43728), Wu et al. (GCN 43731), Maksut et al. (GCN 43732), Pankov et al. (GCN 43733), Li et al. (GCN 43734), Aryan et al. (GCN 43735), Fortin et al. (GCN 43737) and Lipunov et al. (GCN 43738). We derive 3-sigma upper limits of r’ > 23.2 and g’ > 23.5 with photometry calibrated to Pan-STARRS and not corrected for Galactic extinction. View this GCN Circular online at https://gcn.nasa.gov/circulars/43739. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41847] EP260213a: Global MASTER-Net observations report
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43738 SUBJECT: EP260213a: Global MASTER-Net observations report DATE: 26/02/14 17:27:19 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 EP260213a ( EP Team et al., GCN 43729) errorbox 46720 sec after notice time and 70986 sec after trigger time at 2026-02-14 15:41:46 UT, with upper limit up to 19.8 mag. The observations began at zenith distance = 58 deg. The sun altitude is -47.0 deg. The galactic latitude b = 56 deg., longitude l = 253 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3135046 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 71017 | 2026-02-14 15:41:46 | MASTER-Tunka | (11h 05m 53.43s , +05d 16m 04.4s) | C | 60 | 15.9 | 71017 | 2026-02-14 15:41:46 | MASTER-Tunka | (11h 06m 18.51s , +05d 10m 06.9s) | C | 60 | 19.8 | 72842 | 2026-02-14 16:12:12 | MASTER-Tunka | (11h 05m 50.85s , +05d 10m 39.1s) | C | 60 | 15.4 | 72842 | 2026-02-14 16:12:12 | MASTER-Tunka | (11h 06m 16.94s , +05d 03m 46.6s) | C | 60 | 19.6 | 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/43738. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41846] EP260213a: COLIBRÍ optical upper limits
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43737 SUBJECT: EP260213a: COLIBRÍ optical upper limits DATE: 26/02/14 16:52:46 GMT FROM: Alan Watson at UNAM <alan(a)astro.unam.mx> Francis Fortin (IRAP), Asuka Kuwata (UNAM), Alan M. Watson (UNAM), Noémie Globus (UNAM), Stéphane Basa (UAR Pytheas), William H. Lee (UNAM), Edilberto Aguilar-Ruiz (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), Jean-Grégoire Ducoin (CPPM), Leonardo García García (UNAM), Ramandeep Gill (UNAM), Nikos Mandarakas (LAM), Diego López-Cámara (UNAM), Francesco Magnani (CPPM), Enrique Moreno Méndez (UNAM), Margarita Pereyra (UNAM), Ny Avo Rakotondrainibe (LAM), Fredd Sánchez Álvarez (UNAM), Benjamin Schneider (LAM), and Antonio de Ugarte Postigo (LAM) report: We imaged the field of the EP260213a (Yang et al., GCN Circ. 43729; Li et al., GCN Circ. 43730) using the DDRAGO two-channel wide-field imager on the COLIBRÍ telescope. We observed from 2026-02-14 07:09:32 to 12:08:00 UTC (from 11.18 to 16.17 hours after the trigger) and obtained 92 minutes of simultaneous exposure in the r and z filters. The data were reduced, calibrated, and analyzed with the COLIBRÍ ASU pipeline. The photometry was calibrated using nearby stars from the PanSTARRS DR1 catalog, is in the AB system, and is not corrected for Galactic extinction. In the stacked image, and in comparison to the PS1 and Legacy Survey images (Dey et al. 2019), we do not detect any new source at the FXT source position (Li et al., GCN Circ. 43730) down to the following 5-sigma limits: r > 24.0, z > 22.6. This upper limit is consistent with the ones reported by Wu et al. (GCN Circ. 43731), Maksut et al. (GCN Circ. 43732), Pankov et al. (GCN Circ. 43733), Li et al. (GCN Circ. 43734), and Aryan et al. (GCN 43735). We have chosen to publish 5-sigma limits as the FXT region contains about 100 independent PSFs. The false-alarm probability for 3-sigma positive fluctuations in a region this size is about 0.13. For 5-sigma fluctuations, it is about 3e-5. 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/43737. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41845] GRB 260212A: GECAM-B observation
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43736 SUBJECT: GRB 260212A: GECAM-B observation DATE: 26/02/14 13:54:35 GMT FROM: zhangjinpeng(a)ihep.ac.cn Jin-Peng Zhang, Chen-Wei Wang, Shao-Lin Xiong (IHEP) report on behalf of GECAM team: GECAM-B was triggered in-flight by GRB 260212A, at 2026-02-12T17:49:07.800 UTC (denoted as T0), which is also detected by Fermi/GBM (Fermi GBM team, GCN #43716), Glowbug (C.C. Cheung et al., GCN #43719) and SVOM/GRM (Jin-Peng Zhang et al., GCN #43727). According to the GECAM-B light curves in about 70-6000 keV, this burst mainly consists of multiple pulses, with a duration (T90) of 24 +/- 7 s. The GECAM-B light curve can be found here: https://www.bursthub.cn//admin/static/gecambgrb260212A.png The time-averaged spectrum from T0 - 1.0 to T0 + 11.0 s (photon energy > 70 keV) is fitted by a power law function. The power law index is -2.53 +0.14/-0.15. The event fluence (10-1000 keV) in this time interval is (1.07 +0.09/-0.13)E-05 erg/cm^2. Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) mission originally consists of two micro-satellites (GECAM-A and GECAM-B) launched in Dec. 2020. As the third member of GECAM constellation, GECAM-C was launched onboard SATech-01 experimental satellite in July 2022. GECAM mission is funded by the Chinese Academy of Sciences (CAS). View this GCN Circular online at https://gcn.nasa.gov/circulars/43736. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41844] EP260213a: Optical upper limits with Kinder observations
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43735 SUBJECT: EP260213a: Optical upper limits with Kinder observations DATE: 26/02/14 13:48:03 GMT FROM: Amar Aryan at National Central University, Institute of Astronomy (NCUIA) <amararyan941(a)gmail.com> A. Aryan, C.-S. Lin, T.-W. Chen (all NCU), A. K. H. Kong (NTHU), J. H. Gillanders, S. J. Smartt (both Oxford), Y. J. Yang (NYUAD), Y.-H. Lee, A. Sankar.K, M.-H. Lee, C.-H. Lai, Y.-C. Pan, C.-C. Ngeow, W.-J. Hou, H.-Y. Hsiao, H.-C. Lin, J.-K. Guo (all NCU), S. Yang, Z. N. Wang, L. L. Fan, G. H. Sun (all HNAS), H.-W. Lin (UMich), H. F. Stevance, S. Srivastav, L. Rhodes (all Oxford), M. Nicholl, M. Fulton, T. Moore, K. W. Smith, C. Angus, A. Aamer (all QUB), A. Schultz, and M. Huber (both IfA, Hawaii) report: We observed the field of the fast X-ray transient EP260213a (Yang et al. GCN 43729, Li et al. GCN 43730) using the 40cm SLT at the Lulin observatory, as part of the Kinder collaboration (Chen & Yang et al. 2025, ApJ, 983, 86, doi:10.3847/1538-4357/adb428). The first SLT epoch of observations in r-band started at 20:12 UTC on 13th of February 2026 (MJD 61084.842), 0.22 hr after the EP-WXT trigger. We utilized the astroalign (Beroiz et al. 2020, A&C, 32, 100384) and astropy (Astropy Collaboration et al. 2022, ApJ, 935, 167) packages to align and stack the individual frames. We used the Python-based AutoPhOT package (Brennan & Fraser 2022, A&A, 667, A62) to perform template subtraction with the DESI Legacy Survey (Dey et al. 2019, AJ 157, 168) DR10 using the 'SFFT' (Hu et al. 2022, ApJ, 936, 157) algorithm. Either in the stacked frame or in the difference image, we do not detect any new or uncataloged sources within the 10" refined EP-FXT localization circle. Moreover, we used AutoPhOT to perform PSF photometry. The details of the observations and the measured 3-sigma upper limits (in the AB system) are as follows: Telescope | Filter | MJD (start) | t-t0 (hr) | Exposure (s) | Magnitude | avg. Seeing | med. Airmass SLT | r | 61084.842 | 0.22 | 300 * 18 | >21.6 | 2".5 | 1.70 The non-detection in our observations is consistent with those reported by Cotter et al. (GCN 43728), Wu et al. (GCN 43731), Maksut et al. (GCN 43732), Pankov et al. (GCN 43733), and Li et al. (GCN 43734). The presented magnitude is calibrated using the field stars from the ATLAS-RefCat2 catalog from MAST (Tonry J. L. et al. 2018, ApJ, 867, 105) and is not corrected for the expected Galactic foreground extinction of A_r = 0.106 mag in the direction of the transient (Schlafly & Finkbeiner 2011). The methodology, details on the Lulin observatory telescopes, and a compilation of our optical follow-up campaign for FXTs discovered within the first year of operation of the Einstein-Probe mission are presented in Aryan et al. 2025, ApJS, 281, 20, doi:10.3847/1538-4365/adfc69. View this GCN Circular online at https://gcn.nasa.gov/circulars/43735. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41843] EP260213a: SVOM/VT optical upper limit
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43734 SUBJECT: EP260213a: SVOM/VT optical upper limit DATE: 26/02/14 11:22:32 GMT FROM: Huali Li at at NAOC, SVOM <lhl(a)nao.cas.cn> H. L. Li, Y. N. Ma, L. P. Xin, Y. L. Qiu, C. Wu, Z. H. Yao, X. H. Han, Y. Xu, J. Wang, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, L. Lan, J. R. Xu, J. S. Deng, J. Y. Wei (NAOC), J. Palmerio (CEA) report on behalf of the SVOM/VT team. SVOM/VT performed a Target of Opportunity observation of EP260213a detected by Einstein Probe (Yang et al., GCN 43729; Li et al, GCN 43730). The observation started on 2026-02-13T21:19:03 UTC, 1.346 hours after the trigger, in the VT_B (400nm-650nm) and VT_R (650nm-1000nm) channels simultaneously. No uncatalogued sources were detected in stacked images within the error box of EP-FXT (Yang et al., GCN 43729; Li et al., GCN 43730). The 3 sigma limit magnitudes are derived as follows: Mid time | Band | Exposure Time | 3 sigma limit magnitude 2.38 hour VT_B 72*50 sec > 23.7 mag 2.39 hour VT_R 67*50 sec > 23.5 mag Our photometry was in AB magnitude and was not corrected for Galactic extinction. The nondetection is consistent with the results published previously (Cotter et al., GCN 43728; Wu et al., GCN 43731; Maksut et al., GCN 43732; Pankov et al., GCN 43733). 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/43734. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 41842] EP260213a: Mondy R-band optical upper limit
by GCN Circulars 14 Feb '26

14 Feb '26

TITLE: GCN CIRCULAR NUMBER: 43733 SUBJECT: EP260213a: Mondy R-band optical upper limit DATE: 26/02/14 10:48:57 GMT FROM: Nicolai Pankov at IKI <colinsergesen(a)gmail.com> N. Pankov (IKI), E. Klunko (ISTP), A. Volnova (IKI), A. Pozanenko (IKI) report on behalf of IKI-GRB-FuN: We observed the field of a fast X-ray transient EP260213a (Yang et al., GCN 43729) with the AZT-33IK 1.5m telescope of the Sayan Solar Observatory (Mondy) starting on 2026-02-13 20:08:15 (UT). A total of 30x120 sec exposures were taken in the R-band. No optical candidate was detected within refined error circle (Li et al., GCN 43730). Also, no objects from the catalogues (SDSS, PS1, WISE, LS) were found within the error circle. The preliminary photometry and observational details are presented below: Date UT start t-T0 Exp. Filter Mag. Err. UL (mid,days) (n*s) (3sigma) 2026-02-13 20:08:15 0.02797 30*120 R n/d n/d 22.2 The photometry was calibrated using nearby stars of USNO-B1.0 and has not been corrected for the Galactic extinction. Our results are consistent with the results published previously (Cotter et al., GCN 43728). View this GCN Circular online at https://gcn.nasa.gov/circulars/43733. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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