July 2026 - vsnet-grb-info - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-grb-info 43451] EP260727a: Einstein Probe detection of an X-ray transient
by GCN Circulars 28 Jul '26

28 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45235 SUBJECT: EP260727a: Einstein Probe detection of an X-ray transient DATE: 26/07/28 02:19:44 GMT FROM: EP Team at NAOC/CAS <ep_ta(a)bao.ac.cn> J. W. Hu (NAO, CAS) , H. C. Ding, T. Wu (AHNU), S. Q. Jiang, Z. X. Ling (NAO, CAS) 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 EP260727a. The transient triggered EP-WXT (ID: 01709276927) at 2026-07-27T20:37:57 (UTC). The WXT position of the source is R.A. = 346.455 deg, DEC = 3.240 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 by the onboard software at R.A. = 346.4623 deg, DEC = 3.1953 deg (J2000) with an uncertainty of 20 arcsec in radius (90% C.L. statistical and systematic), which is consistent with the position of NOT likely optical counterpart (GCN 45234). 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/45235. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43450] The EP-WXT trigger 01709276927 (EP260727a?): NOT likely optical counterpart
by GCN Circulars 28 Jul '26

28 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45234 SUBJECT: The EP-WXT trigger 01709276927 (EP260727a?): NOT likely optical counterpart DATE: 26/07/28 01:53:54 GMT FROM: L. B. He at NAOC <helb(a)bao.ac.cn> L.B. He (NAOC), S.Y. Fu (HUST), Z.P. Zhu, J. An, X. Liu, S.Q. Jiang, D. Xu (NAOC), J.P.U. Fynbo (DAWN/NBI), R.H. Rasmussen, O. Stalder (NOT) report: We observed the field of EP-WXT trigger ID 01709276927 detected by EP using the 2.56m Nordic Optical Telescope (NOT) equipped with the ALFOSC camera. Observation started at 2026-07-28T00:19:16.548 UT, i.e., 3.69 hrs post-burst, and a series of Sloan r- and z-band frames were obtained. A brightened source was detected within the EP/WXT error circle at coordinates R.A. (J2000) = 23:05:50.65 (346.46104) Dec. (J2000) = +03:11:38.65 (3.19407) with an uncertainty of ~ 0.5 arcsec. The source had r = 21.98 +/- 0.08 mag at a median time of 4.18 hrs post-trigger, calibrated with Pan-STARRS DR2 and not corrected for Galactic extinction. We note that there is a faint source at that position in the Legacy Survey DR10 images with r = 23.73 +/- 0.23 and z_phot = 1.03 +/- 0.24. No NEO was at the above position at the observational time according to MPC. We thus think the source is likely the optical counterpart. View this GCN Circular online at https://gcn.nasa.gov/circulars/45234. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43449] GRB 260727A: Glowbug gamma-ray detection
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45233 SUBJECT: GRB 260727A: Glowbug gamma-ray detection DATE: 26/07/27 22:08:29 GMT FROM: C.C. Cheung at Naval Research Lab <Teddy.Cheung(a)nrl.navy.mil> C.C. Cheung, R. Woolf, M. Kerr, J.E. Grove (NRL), A. Goldstein (USRA), C.A. Wilson-Hodge, D. Kocevski (MSFC), and M.S. Briggs (UAH) report: The Glowbug gamma-ray telescope [1,2,3], operating on the International Space Station, reports the detection of GRB 260727A, which was also detected by SVOM (GCN 45220) and AstroSat (GCN 45225). Using an adaptive window with a resolution of 32-ms, the burst onset is determined to be 2026-07-27 00:21:57.592 with a duration of 22.5 s and a total significance of about 24.2 sigma. The emission seen by Glowbug corresponds to the brightest portion of the burst seen in the AstroSat light curve, and is a subset of the full emission episode observed by SVOM. The analysis results presented here are preliminary and use a response function that lacks a detailed characterization of the surrounding passive structure of the ISS. Glowbug is a NASA-funded technology demonstrator for sensitive, low-cost gamma-ray transient telescopes developed, built, and operated by the U.S. Naval Research Laboratory (NRL) with support from the University of Alabama in Huntsville, USRA, and NASA MSFC. It was launched on 2023 March 15 aboard the Department of Defense Space Test Program’s STP-H9 to the ISS and operated until 2024 April when it was put in safe storage on orbit. Glowbug was removed from storage and resumed operation on 2025 September 12. [1] Grove, J.E. et al. 2020, Proc. Yamada Conf. LXXI, arXiv:2009.11959 [2] Woolf, R.S. et al. 2022, Proc. SPIE, 12181, id. 121811O [3] Woolf, R.S. et al. 2024, Proc. SPIE, 13151, id. 1315108 Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/45233. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43448] GRB 260726A: J-band upper limit with WINTER
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45232 SUBJECT: GRB 260726A: J-band upper limit with WINTER DATE: 26/07/27 19:19:29 GMT FROM: tanishk.mohan(a)iitb.ac.in Tanishk Mohan (IITB), Geoffrey Mo (Caltech/Carnegie), Viraj Karambelkar (Columbia), Benjamin Schneider (LAM), Tomas Ahumada (NOIRLab), Robert Stein (UMD), Danielle Frostig (CfA), Nathan Lourie (MIT), Robert Simcoe (MIT), and Mansi Kasliwal (Caltech) report: We observed the field of GRB 260726A (Fermi GBM, GCN 45218; Liang et al., GCN 45219) in the near-infrared J band with the Palomar 1-m telescope, equipped with the 1.2-square degree WINTER camera (Lourie et al. 2020, Frostig et al. 2024). Observations began at 2026-07-27T04:50:12.365 UTC in the J band (5.09 hr after the Fermi trigger), consisting of 15*120 sec exposures. The images were processed using the WINTER data reduction pipeline implemented with mirar (https://github.com/winter-telescope/mirar, https://doi.org/10.5281/zenodo.13352565) We do not detect any new source at the position of SVOM/VT optical candidate (Li et al., GCN 45230) in our stacked image. We obtain the following 5-sigma upper limit: J = 18.92 mag (AB). WINTER (Wide-field INfrared Transient ExploreR) is a partnership between MIT and Caltech, housed at Palomar Observatory, and funded by NSF MRI, NSF AAG, the David and Lucile Packard Foundation, and the MIT Kavli Institute for Astrophysics and Space Research. View this GCN Circular online at https://gcn.nasa.gov/circulars/45232. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43447] GRB 260727A: J-band upper limit with WINTER
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45231 SUBJECT: GRB 260727A: J-band upper limit with WINTER DATE: 26/07/27 19:17:50 GMT FROM: tanishk.mohan(a)iitb.ac.in Tanishk Mohan (IITB), Geoffrey Mo (Caltech/Carnegie), Viraj Karambelkar (Columbia), Benjamin Schneider (LAM), Tomas Ahumada (NOIRLab), Robert Stein (UMD), Danielle Frostig (CfA), Nathan Lourie (MIT), Robert Simcoe (MIT), and Mansi Kasliwal (Caltech) report: We observed the field of GRB 260727A (Li et al., GCN 45220; Harsha et al., GCN 45225) in the near-infrared J band with the Palomar 1-m telescope, equipped with the 1.2-square degree WINTER camera (Lourie et al. 2020, Frostig et al. 2024). Observations began at 2026-07-27T04:17:32.122 UTC in the J band (3.93 hr after the SVOM/ECLAIRs trigger), consisting of 15*120 sec exposures. The images were processed using the WINTER data reduction pipeline implemented with mirar (https://github.com/winter-telescope/mirar, https://doi.org/10.5281/zenodo.13352565) We do not detect any new source in the SVOM localization (Shi et al., GCN 45223; Freeberg et al., GCN 45224; Starling et al., GCN 45226; RAPAS network, GCN 45228) in our stacked image. We obtain the following 5-sigma upper limit: J = 19.19 mag (AB). WINTER (Wide-field INfrared Transient ExploreR) is a partnership between MIT and Caltech, housed at Palomar Observatory, and funded by NSF MRI, NSF AAG, the David and Lucile Packard Foundation, and the MIT Kavli Institute for Astrophysics and Space Research. View this GCN Circular online at https://gcn.nasa.gov/circulars/45231. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43446] GRB 260726A: SVOM/VT optical candidate
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45230 SUBJECT: GRB 260726A: SVOM/VT optical candidate DATE: 26/07/27 17:26:25 GMT FROM: Huali Li at at NAOC, SVOM <lhl(a)nao.cas.cn> H. L. Li, L. P. Xin, Y. L. Qiu, C. Wu, J. R. Xu, Y. N. Ma, Z. H. Yao, X. H. Han, J. Wang, Y. Xu, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, J. S. Deng, J. Y. Wei (NAOC), J. T. Palmerio (CEA/Irfu), Ruizhi Li (YNAO) and Ziming Wang (BNU) report on behalf of the SVOM/VT team. SVOM/VT performed observations with automatic slew for GRB 260618B detected by SVOM/ECLAIRs (Liang et al., GCN 45219; Brunet et al., GCN 45229) and SVOM/GRM (Liang et al., GCN 45219). This burst was also detected by Fermi/GBM (Fermi GBM team, GCN 45218). The observation started at 2026-07-27T01:28:04 UTC, i.e., 1.72 hr post trigger in the VT_B (400-650 nm) and VT_R (650-1000 nm) channels simultaneously. An uncatalogued optical candidate was detected in VT_R within the errorbox of SVOM/MXT (Brunet et al., GCN 45229), compared with the PanSTARRS catalogue. The position is at R.A., Dec. = 356.883196, 52.870077 degrees, equivalent to: R.A. (J2000) = 23:47:31.93 Dec. (J2000) = +52:52:12.69 with an uncertainty of 0.5 arcsec. The following measurements are in the AB magnitude and are not corrected for Galactic extinction: Mid time | Band | Exposure Time | Brightness 1.95 hr VT_R 17*100 s 21.4 +/-0.2 mag The source showed a fading slope of about -0.2 in VT_R during the observations above. It was not detected in VT_B, even all the available data were stacked with the total exposure time of 85*100s. The 3 sigma upper limit was estimated to be 24.0 mag in VT_B at the mid time of 4.37 hr. 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/45230. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43445] GRB 260726A: SVOM ECLAIRs improved position and MXT possible detection of a counterpart
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45229 SUBJECT: GRB 260726A: SVOM ECLAIRs improved position and MXT possible detection of a counterpart DATE: 26/07/27 17:05:01 GMT FROM: SVOM_group <svomgroup(a)bao.ac.cn> M. Brunet (IRAP), P. Maggi (ObAS), D. Götz, D. Turpin (CEA), Ruizhi Li (YNAO), Ziming Wang (BNU), on behalf of the SVOM/ ECLAIRs & MXT team report: Using the full X band dataset a corrected ECLAIRs position could be derived for GRB 260726A/sb27062614 (Liang et al., GCN 45219). The improved ECLAIRs position is RA=356.770, Dec=52.851 with a 90% c.l. of 3.7 arcmin. The burst appeared very close to the Earth limb and only part of the burst signal was considered by the onboard processing, explaining the localization error. SVOM MXT observed the ECLAIRs error region starting at T0 = 2026-07-26T23:47:09 (106s after trigger time ECLAIRs T0). Using the full X band dataset, a faint fading source is recovered in the first orbit. Removing the first 150s affected by straylight, the best position is RA=356.903, Dec=52.870 corresponding to: RA (J2000) = 23h47m36.59s. Dec (J2000) = +52d52m11.7s with a statistical 90% C.L. radius of 75.4”. This detection remains tentative due to the presence of straylight possibly remaining in the MXT data. This position is 4.95 arcmin from the ECLAIRs position. This position corrects and supersedes the one reported by (Liang et al., GCN 45219). The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA), French Space Agency (CNES), and the Chinese Academy of Sciences (CAS), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. MXT was developed jointly by CEA, CNES, University of Leicester, IJCLab and MPE. ECLAIRs was developed jointly by CNES, IRAP, APC and CEA. The Burst Advocate (BA) on shift for this burst is Rui-Zhi Li: liruizhi(a)ynao.ac.cn . Please contact the BA by email if you require additional information regarding the SVOM follow-up of this burst. View this GCN Circular online at https://gcn.nasa.gov/circulars/45229. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43444] GRB 260727A / SVOM sb26072702: RAPAS optical non-detection
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45228 SUBJECT: GRB 260727A / SVOM sb26072702: RAPAS optical non-detection DATE: 26/07/27 15:20:56 GMT FROM: Thierry Midavaine at SAF - RAPAS <thierrymidavaine(a)sfr.fr> Pierre-Yves Lechapelain and Thierry Midavaine report on behalf of the RAPAS network: We observed the field of GRB 260727A (SVOM/ECLAIRs trigger sb26072701; Li et al., GCN 45220) in response to the overlapping SVOM broker alert sb26072702 (RA = 331.626 deg, Dec = +74.549 deg, J2000, 2.5 arcmin error radius). Observations were obtained with the RAPAS 0.25 m f/3 robotic telescope and IMX533 sensor at Observatoire de Bretagne Sud (Y80), using RAPAS filters matched to the Gaia G, Gbp, and Grp bands. Data were reduced with the STDPipe/stdweb pipeline; photometry and astrometry are calibrated to Gaia DR3 with spatially varying zero points and color terms. Observations began at 2026-07-27 00:48 UTC (T_GRB + 26 min, with T_GRB = 2026-07-27 00:22:02 UTC from GCN 45220) and continued in a G / Gbp / Grp cycle with 30 s exposures until approximately 02:44 UTC (T_GRB + 2.4 hr). We detect no optical afterglow at the sb26072702 position. Forced aperture photometry at RA = 331.626 deg, Dec = +74.549 deg shows no significant excess on the earliest G exposure (flux S/N = 1.8) or on the deep G co-add (flux S/N = 3.6, below our 5σ detection threshold). No Gaia-uncatalogued source is found within the 2.5 arcmin SVOM error circle. A comparison to Gaia DR3 in a 12 arcmin (0.2 deg) radius around the alert on the first G frame yields five marginal transient candidates at 7–11 arcmin offset; none are confirmed in deeper co-added images. Searches over the full unvignetted RAPAS field (~0.62 deg radius) reveal no plausible afterglow at the SVOM coordinates. We report 5σ limiting magnitudes (Vega, Gaia-calibrated) from the global detection limits of each reduction: Earliest epoch per band (single frame or shortest stack in the sequence): | T_mid - T_GRB | Exp | Band | Limit (5σ) | Note | |---------------|------------|------|------------|-------------| | +25 min | 1 × 30 s | G | >18.3 | | | +31 min | 2 × 30 s | G_BP | >18.6 |2-frame stack| | +36 min | 2 × 30 s | G_RP | >17.4 |2-frame stack| Co-added images from the ToO night: | Band | Co-add | Limit (5σ) | |------|-------------|------------| | G | 17 × 30 s | >20.1 | | G_BP | 18 × 30 s | >19.9 | | G_RP | 14 × 30 s | >18.6 | Mid-exposure times correspond to the first useful epoch in each band and to the weighted mean epoch of each co-added stack, respectively. Acknowledgements : RAPAS ( https://gemini.obspm.fr/20220101-rapas/ ) is a ProAm collaboration created by T. Midavaine (SAF), W. Thuillot (LTE, Obs. de Paris-PSL) and M. Dennefeld (IAP/CNRS and Sorbonne Univ.) and funded by the Paris Observatory under API ProAm of the Scientific Council. It aims at homogenizing observing procedures and filters, and is delivering to a network of french amateur observatories a set of 3 filters which have been chosen to meet the Gaia G, Gbp and Grp spectral bands. This network produces data on astrophysical alerts delivered by various Alert systems (Gaia Alerts, Atlas, ZTF, etc…) and collected by Astro-COLIBRI ( https://astro-colibri.science ). It is similarly progressing towards an homogeneous spectroscopic equipment to deliver SED. Paris Observatory PADC which is on the way to archive all the FITS files with attached processing pipeline. View this GCN Circular online at https://gcn.nasa.gov/circulars/45228. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43443] EP260723a: SVOM/ECLAIRs Upper Limit
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45227 SUBJECT: EP260723a: SVOM/ECLAIRs Upper Limit DATE: 26/07/27 13:44:17 GMT FROM: SVOM_group <svomgroup(a)bao.ac.cn> H. Yang, M. Brunet, O. Godet, S. Guillot (IRAP) report on behalf of the SVOM team: We performed a targeted search of the X-ray transient EP260723a, detected by EP-WXT at 2026-07-23T18:56:01 UTC (T0) with a duration of about 100 s (EP team, GCN 45201), using the SVOM/ECLAIRs event-by-event data downloaded through the X-band ground station. At T0, the transient position was within the ECLAIRs field of view. No statistically significant signal was identified in the [T0 - 500 s, T0 + 3000 s] interval by the ECLAIRs image trigger performed on multiple timescales and energy bands. For the interval from T0 to T0 + 100 s, we derive a 3-sigma upper limit of 2.4e-9 erg/cm^2/s in the 4-120 keV energy band, assuming a power-law spectrum with a photon index of 1.4, as measured by EP-WXT (GCN 45201). Alternatively, assuming a “soft” spectral template (a Band function with Epeak = 25 keV, alpha = -1.5, beta = -3.0), we derive a 3-sigma upper limit of 1.5e-9 erg/cm^2/s. The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA), French Space Agency (CNES), and the Chinese Academy of Sciences (CAS), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. ECLAIRs was developed jointly by APC, CEA, CNES, and IRAP. The SVOM/ECLAIRs point of contact for this event is : Hui Yang (hui.yang(a)cnrs.fr) View this GCN Circular online at https://gcn.nasa.gov/circulars/45227. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 43442] GRB 260727A: GOTO early optical upper limit
by GCN Circulars 27 Jul '26

27 Jul '26

TITLE: GCN CIRCULAR NUMBER: 45226 SUBJECT: GRB 260727A: GOTO early optical upper limit DATE: 26/07/27 11:30:59 GMT FROM: Rhaana Starling at U of Leicester <rlcs1(a)leicester.ac.uk> R. Starling, M. Kennedy, D. O'Neill, B. P. Gompertz, G. Ramsay, A. Kumar, S. Belkin, K. Ackley, M. Dyer, J. Lyman, K. Ulaczyk, D. Steeghs, D. Galloway, V. Dhillon, P. O'Brien, K. Noysena, R. Kotak, R. Breton, J. Casares, L. Nuttall, B. Godson, T. Killestein, M. Pursiainen, I. Worssam on behalf of the GOTO collaboration We report on optical observations with the Gravitational-wave Optical Transient Observer (GOTO; Steeghs et al. 2022, Dyer et al. 2024) in response to the SVOM/ECLAIRs detected GRB 260727A (sb26072701, Li et al. 2026, GCN 45220), also detected by AstroSat (Harsha et al.2026, GCN 45225). Observations at the ECLAIRs position began at 2026-07-27 00:27:22 UT (+5.8 minutes post trigger) and continued to 2026-07-27 01:47:11 UT (+1.4h post trigger). Images consisted of 4x90s exposures in the GOTO L-band (400-700 nm). Images were processed immediately after acquisition using the GOTO pipeline. Difference imaging was performed using deeper template observations. Any source candidates are initially filtered using a classifier (Killestein et al. 2021) and cross-matched against a variety of contextual and minor planet catalogs (Lyman et al. 2026). We found no new transients that could be credibly associated with 260727A within the localisation down to a 5-sigma depth of L<20.2 AB mag. GOTO (https://goto-observatory.org) is a network of telescopes that is principally funded by the STFC and operated at the Roque de los Muchachos Observatory on La Palma, Spain, and Siding Spring Observatory in NSW, Australia, on behalf of a consortium including the University of Warwick, Monash University, Armagh Observatory & Planetarium, the University of Leicester, the University of Sheffield, the National Astronomical Research Institute of Thailand (NARIT), the University of Turku, the University of Portsmouth, the University of Manchester, the University of Birmingham and the Instituto de Astrofisica de Canarias (IAC). View this GCN Circular online at https://gcn.nasa.gov/circulars/45226. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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