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[vsnet-grb-info 42816] GRB 260519C: SVOM/GRM observation
by GCN Circulars 22 May '26

22 May '26

TITLE: GCN CIRCULAR NUMBER: 44688 SUBJECT: GRB 260519C: SVOM/GRM observation DATE: 26/05/22 06:32:44 GMT FROM: renyz16607(a)163.com SVOM/GRM team: Yang-Zhao Ren, Chen-Wei Wang, Shi-Jie Zheng, Yue Huang, Shao-Lin Xiong, Shuang-Nan Zhang (IHEP) SVOM/ECLAIRs team: Feliu Lacreu (IAP) Report on behalf of the SVOM team: SVOM/GRM was triggered in-flight by GRB 260519C (SVOM trigger reference: sb26051904) at 2026-05-19T13:45:38.000 UTC (T0), which is also detected by Konus-Wind (Svinkin, GCN #44677), and NuSTAR (Waratkar et al., GCN #44672). With the event-by-event data downloaded through the X-band ground station, the GRM light curve shows that this burst consists of multiple pulses with a T90 of 26.5 +1.0/-1.0 s in the 15-5000 keV band. The SVOM/GRM light curve can be found here: https://www.bursthub.cn//admin/static/svgrb260519C.png With this localization, the time-averaged spectrum from T0-5 to T0+30 s is best fitted by a power law function with an exponential high-energy cutoff. The power law index is -0.78 +0.08/-0.09 and the cutoff energy, parameterized as Epeak, is 135 +7/-6 keV. The event fluence (10-1000 keV) in this time interval is (2.07 +0.07/-0.06)E-05 erg/cm^2. The 1s peak spectrum, measured from T0+12.5 to T0+13.5 s, if fitted by a power law function with an exponential high-energy cutoff, the power law index is -0.60 +0.19/-0.20 and the cutoff energy, parameterized as Epeak, is 93.47 +6.95/-5.93 keV. The flux (10-1000 keV) in this time interval is (1.10 +0.21/-0.06)E-06 erg/cm^2/s. The localization of GRB 260519C in the 'Amati' relation diagram is shown at: https://www.bursthub.cn//admin/static/svgrb260519C_amati.png The localization of GRB 260519C in the 'Yonetoku' relation diagram is shown at: https://www.bursthub.cn//admin/static/svgrb260519C_yonetoku.png 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. GRM is developed by the Institute of High Energy Physics (IHEP) of CAS. The SVOM point of contact for this burst is: Yang-Zhao Ren (IHEP)(renyz(a)ihep.ac.cn) View this GCN Circular online at https://gcn.nasa.gov/circulars/44688. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42815] GRB 260522A: Fermi GBM Final Real-time Localization
by GCN Circulars 22 May '26

22 May '26

TITLE: GCN CIRCULAR NUMBER: 44687 SUBJECT: GRB 260522A: Fermi GBM Final Real-time Localization DATE: 26/05/22 02:25:32 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 02:15:08 UT on 22 May 2026, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 260522A (trigger 801108913.782424 / 260522094). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 343.6, Dec = 14.1 (J2000 degrees, equivalent to J2000 22h 54m, 14d 05'), with a statistical uncertainty of 5.1 degrees. The angle from the Fermi LAT boresight is 10.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260522094/… The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260522094/… The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2026/bn260522094/… View this GCN Circular online at https://gcn.nasa.gov/circulars/44687. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42814] GRB 260511A: iTelescope T-75 optical detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44686 SUBJECT: GRB 260511A: iTelescope T-75 optical detection DATE: 26/05/21 22:55:39 GMT FROM: Takanori Sakamoto at AGU <tsakamoto(a)phys.aoyama.ac.jp> H. Ban, T. Kato, K. Hotta, Y. Kawakubo, M. Serino, T. Sakamoto (AGU) We observed the field of GRB 260511A detected by the Fermi/GBM (Fermi GBM Team, GCN Circ. 44529), the SVOM/ECLAIRs (Godet et al., GCN Circ. 44532), the NuSTAR CsI anti-coincidence shields (Waratkar et al., GCN Circ. 44555), the Konus-Wind (Ridnaia et al., GCN Circ. 44585), the Glowbug (Woolf et al., GCN Circ. 44586), and the GRID (Li et al., GCN Circ. 44664) with the iTelescope.Net (http://www.itelescope.net) T75 (ASAN250) telescope located at Rio Hurtado Valley, Chile. We took 20 images of 60 sec exposures in the Red filter starting from May 11 at 06:37:27 (UT), about 24 minutes after the Fermi/GBM trigger and stopped at 07:07:42. The afterglow (Jiang et al., GCN Circ. 44533; Akl et al., GCN Circ. 44534; Saccardi et al., GCN Circ. 44535; Zheng et al., GCN Circ. 44536; Wu et al., GCN Circ. 44538; Harper et al., GCN Circ. 44545; Brivio et al., GCN Circ. 44562; Li et al., GCN Circ. 44575; Fu et al., GCN Circ. 44579; Zhu et al., GCN Circ. 44584) is detected in the stacked image of the first eight images (total exposure of 480 s) collected between 06:37:27 and 06:49:12. The afterglow magnitude is 19.3 +- 0.6 using the USNO-B1 catalog. No afterglow was detected in the following twelve images collected between 06:49:44 and 07:07:42. The 5-sigma upper limit of the stacked image of the last twelve images (total exposure of 720 s) is 18.3 mag. View this GCN Circular online at https://gcn.nasa.gov/circulars/44686. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42813] GRB 260520B: SVOM/GRM observation
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44685 SUBJECT: GRB 260520B: SVOM/GRM observation DATE: 26/05/21 15:23:56 GMT FROM: yzh807926(a)163.com SVOM/GRM team: Zheng-Hang Yu, Chen-Wei Wang, Chao Zheng, Shi-Jie Zheng, Yue Huang, Shao-Lin Xiong, Shuang-Nan Zhang (IHEP) SVOM/ECLAIRs team: Olivier Godet (IRAP) Report on behalf of the SVOM team: SVOM/GRM was triggered on-ground by GRB 260520B at 2026-05-20T09:35:53.000 (T0), which is also detected by Fermi/GBM (Fermi GBM Team, GCN #44676). With the event-by-event data downloaded through the X-band ground station, the GRM light curve shows that this burst consists of a main episode with a single peak a T90 of 6.0 +7.0/-5.0 s in the 15-5000 keV band. The SVOM/GRM light curve can be found here: https://www.bursthub.cn//admin/static/svgrb260520B.png In addition, the position of this burst, as determined by Fermi/GBM (RA= 346.68 deg, DEC= 39.68 deg, ERR=14.4 deg, GCN#44425), is located at about 94 degrees from the SVOM optical axis, which is outside the ECLAIRs field of view. 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. GRM is developed by the Institute of High Energy Physics (IHEP) of CAS. The SVOM point of contact for this burst is: Zheng-Hang Yu (IHEP)(zhyu(a)ihep.ac.cn) View this GCN Circular online at https://gcn.nasa.gov/circulars/44685. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42812] GRB 260411B: TERI Gamma-ray detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44684 SUBJECT: GRB 260411B: TERI Gamma-ray detection DATE: 26/05/21 14:08:14 GMT FROM: nicholasjkirschner(a)gmail.com Nicholas Kirschner (a), Daniel Shy (b), C.C. Cheung (b), Bernard Phlips (b), Michael Streicher (c), James Mason (c), Douglas M. Groves (c), Feng Zhang (c), and Willy Kaye (c) (a) National Research Council Research Associate resident at the U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (b) U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (c) H3D, Inc., 812 Avis Dr., Ann Arbor, MI 48108, USA The cadmium zinc TElluride Radiation Imager (TERI) gamma-ray telescope [1], operating on the International Space Station, reports the detection of GRB 260411B, which was also detected by Fermi GBM (GCN 44262, 44266), SVOM/GRM (GCN 44268), Fermi LAT (GCN 44277), GECAM (GCN 44285), Glowbug (GCN 44312), and Konus-Wind (GCN 44332). Using 1 Hz binning, and adopting T0 = 2026-04-11T08:04:43.568 Z, we observe one peak at T0+1.5s, with peak excess count rate of 69 above the 192 cps baseline rate observed in nearby off-source intervals. The analysis results presented here are preliminary and currently lack a detailed response function. TERI is an Office of Naval Research funded technology demonstrator for large-volume pixelated CdZnTe detectors developed, built, and operated by the U.S. Naval Research Laboratory (NRL) in conjunction with H3D, Inc. The pixelated CdZnTe detectors have an energy range of 40 keV to 3 MeV per pixel. It was launched on 2025 April 21 aboard the Department of Defense Space Test Program STP-H10 to the ISS. On the ISS, it is located on the SOX external payload facility on the Columbus module. Analysis of TERI data at NRL is supported by the Office of Naval Research 6.1. [1] Shy, Daniel, et al. "Development of the cadmium zinc TElluride Radiation Imager." Journal of Astronomical Telescopes, Instruments, and Systems 10.4 (2024): 044009-044009 (arXiv:2408.04559). Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/44684. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42811] GRB 260407A: TERI Gamma-ray detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44683 SUBJECT: GRB 260407A: TERI Gamma-ray detection DATE: 26/05/21 14:07:39 GMT FROM: nicholasjkirschner(a)gmail.com Nicholas Kirschner (a), Daniel Shy (b), C.C. Cheung (b), Bernard Phlips (b), Michael Streicher (c), James Mason (c), Douglas M. Groves (c), Feng Zhang (c), and Willy Kaye (c) (a) National Research Council Research Associate resident at the U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (b) U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (c) H3D, Inc., 812 Avis Dr., Ann Arbor, MI 48108, USA The cadmium zinc TElluride Radiation Imager (TERI) gamma-ray telescope [1], operating on the International Space Station, reports the detection of GRB 260407A, which was also detected by Fermi/GBM (GCN 44226), Glowbug (GCN 44237), CALET (GCN 44242), InsightHXMT/HE (GCN 44245), and GECAM-A (GCN 44246). Using 1 Hz binning, and adopting T0 = 2026-04-07T09:11:06.112Z, we observe one peak at T0+1.5s, with peak excess count rate of 45 above the 133 cps baseline rate observed in nearby off-source intervals. The analysis results presented here are preliminary and currently lack a detailed response function. TERI is an Office of Naval Research funded technology demonstrator for large-volume pixelated CdZnTe detectors developed, built, and operated by the U.S. Naval Research Laboratory (NRL) in conjunction with H3D, Inc. The pixelated CdZnTe detectors have an energy range of 40 keV to 3 MeV per pixel. It was launched on 2025 April 21 aboard the Department of Defense Space Test Program STP-H10 to the ISS. On the ISS, it is located on the SOX external payload facility on the Columbus module. Analysis of TERI data at NRL is supported by the Office of Naval Research 6.1. [1] Shy, Daniel, et al. "Development of the cadmium zinc TElluride Radiation Imager." Journal of Astronomical Telescopes, Instruments, and Systems 10.4 (2024): 044009-044009 (arXiv:2408.04559). Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/44683. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42810] GRB 260307A: TERI Gamma-ray detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44682 SUBJECT: GRB 260307A: TERI Gamma-ray detection DATE: 26/05/21 14:06:50 GMT FROM: nicholasjkirschner(a)gmail.com Nicholas Kirschner (a), Daniel Shy (b), C.C. Cheung (b), Bernard Phlips (b), Michael Streicher (c), James Mason (c), Douglas M. Groves (c), Feng Zhang (c), and Willy Kaye (c) (a) National Research Council Research Associate resident at the U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (b) U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (c) H3D, Inc., 812 Avis Dr., Ann Arbor, MI 48108, USA The cadmium zinc TElluride Radiation Imager (TERI) gamma-ray telescope [1], operating on the International Space Station, reports the detection of GRB 260307A, which was also detected by Fermi/GBM (GCN 43939), Glowbug (GCN 43950), GECAM-B (GCN 43961), and CALET (GCN 43982). Using 1 Hz binning and adopting T0 = 2026-03-07T11:27:59.32Z, we observe three peaks at T0+1.375s, T0+3.125s, and T0+5.125s with peak excess count rate of 144, 116, 96 above the 100 cps baseline rate observed in nearby off-source intervals. The analysis results presented here are preliminary and currently lack a detailed response function. TERI is an Office of Naval Research funded technology demonstrator for large-volume pixelated CdZnTe detectors developed, built, and operated by the U.S. Naval Research Laboratory (NRL) in conjunction with H3D, Inc. The pixelated CdZnTe detectors have an energy range of 40 keV to 3 MeV per pixel. It was launched on 2025 April 21 aboard the Department of Defense Space Test Program STP-H10 to the ISS. On the ISS, it is located on the SOX external payload facility on the Columbus module. Analysis of TERI data at NRL is supported by the Office of Naval Research 6.1. [1] Shy, Daniel, et al. "Development of the cadmium zinc TElluride Radiation Imager." Journal of Astronomical Telescopes, Instruments, and Systems 10.4 (2024): 044009-044009 (arXiv:2408.04559). Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/44682. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42809] GRB 260225D: TERI Gamma-ray detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44681 SUBJECT: GRB 260225D: TERI Gamma-ray detection DATE: 26/05/21 14:06:05 GMT FROM: nicholasjkirschner(a)gmail.com Nicholas Kirschner (a), Daniel Shy (b), C.C. Cheung (b), Bernard Phlips (b), Michael Streicher (c), James Mason (c), Douglas M. Groves (c), Feng Zhang (c), and Willy Kaye (c) (a) National Research Council Research Associate resident at the U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (b) U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (c) H3D, Inc., 812 Avis Dr., Ann Arbor, MI 48108, USA The cadmium zinc TElluride Radiation Imager (TERI) gamma-ray telescope [1], operating on the International Space Station, reports the detection of GRB 260225D, which was also detected by Glowbug (GCN 43856), Konus-Wind (Trig_Time 19:51:32.84), SVOM/GRM (GCN 43885), and GRID (GCN 43890). Using 1 Hz binning and adopting T0 = 2026-02-25T19:51:28.768Z, we observe two peaks at T0+1.375s and 2.625s and peak excess count rate of 108 and 149 counts per second (cps) above the 128 cps baseline rate observed in nearby off-source intervals. The analysis results presented here are preliminary and currently lack a detailed response function. TERI is an Office of Naval Research funded technology demonstrator for large-volume pixelated CdZnTe detectors developed, built, and operated by the U.S. Naval Research Laboratory (NRL) in conjunction with H3D, Inc. The pixelated CdZnTe detectors have an energy range of 40 keV to 3 MeV per pixel. It was launched on 2025 April 21 aboard the Department of Defense Space Test Program STP-H10 to the ISS. On the ISS, it is located on the SOX external payload facility on the Columbus module. Analysis of TERI data at NRL is supported by the Office of Naval Research 6.1. [1] Shy, Daniel, et al. "Development of the cadmium zinc TElluride Radiation Imager." Journal of Astronomical Telescopes, Instruments, and Systems 10.4 (2024): 044009-044009 (arXiv:2408.04559). Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/44681. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42808] GRB 251118A: TERI Gamma-ray detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44680 SUBJECT: GRB 251118A: TERI Gamma-ray detection DATE: 26/05/21 14:05:27 GMT FROM: nicholasjkirschner(a)gmail.com Nicholas Kirschner (a), Daniel Shy (b), C.C. Cheung (b), Bernard Phlips (b), Michael Streicher (c), James Mason (c), Douglas M. Groves (c), Feng Zhang (c), and Willy Kaye (c) (a) National Research Council Research Associate resident at the U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (b) U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (c) H3D, Inc., 812 Avis Dr., Ann Arbor, MI 48108, USA The cadmium zinc TElluride Radiation Imager (TERI) gamma-ray telescope [1], operating on the International Space Station, reports the detection of GRB 251118A, which was also detected by Glowbug (GCN 42784), Fermi GBM (GCN 42743, 42745, 42783), Fermi LAT (GCN 42752), NuSTAR (GCN 42774), and GECAM-B (GCN 42779). Using 1 Hz binning, and adopting T0 = 2025-11-18T20:31:43.57Z, we observe two peaks at T0+4.5s and 40.5s. The analysis results presented here are preliminary and currently lack a detailed response function. TERI is an Office of Naval Research funded technology demonstrator for large-volume pixelated CdZnTe detectors developed, built, and operated by the U.S. Naval Research Laboratory (NRL) in conjunction with H3D, Inc. The pixelated CdZnTe detectors have an energy range of 40 keV to 3 MeV per pixel. It was launched on 2025 April 21 aboard the Department of Defense Space Test Program STP-H10 to the ISS. On the ISS, it is located on the SOX external payload facility on the Columbus module. Analysis of TERI data at NRL is supported by the Office of Naval Research 6.1. [1] Shy, Daniel, et al. "Development of the cadmium zinc TElluride Radiation Imager." Journal of Astronomical Telescopes, Instruments, and Systems 10.4 (2024): 044009-044009 (arXiv:2408.04559). Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/44680. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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[vsnet-grb-info 42807] GRB 251113A: TERI Gamma-ray detection
by GCN Circulars 21 May '26

21 May '26

TITLE: GCN CIRCULAR NUMBER: 44679 SUBJECT: GRB 251113A: TERI Gamma-ray detection DATE: 26/05/21 14:04:30 GMT FROM: nicholasjkirschner(a)gmail.com Nicholas Kirschner (a), Daniel Shy (b), C.C. Cheung (b), Bernard Phlips (b), Michael Streicher (c), James Mason (c), Douglas M. Groves (c), Feng Zhang (c), and Willy Kaye (c) (a) National Research Council Research Associate resident at the U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (b) U.S. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375 (c) H3D, Inc., 812 Avis Dr., Ann Arbor, MI 48108, USA The cadmium zinc TElluride Radiation Imager (TERI) gamma-ray telescope [1], operating on the International Space Station, reports the detection of GRB 251113A, which was also detected by Glowbug (GCN 42689), Fermi GBM (GCN 42671, 42672), and AstroSat/CZTI (GCN 42688). Using 1 Hz binning, and adopting T0 = 2025-11-13T17:37:28.512ZZ we observe one peak at T0+14.5, with peak excess count rate of 64 cps above the 83 cps baseline rate observed in nearby off-source intervals. The analysis results presented here are preliminary and currently lack a detailed response function. TERI is an Office of Naval Research funded technology demonstrator for large-volume pixelated CdZnTe detectors developed, built, and operated by the U.S. Naval Research Laboratory (NRL) in conjunction with H3D, Inc. The pixelated CdZnTe detectors have an energy range of 40 keV to 3 MeV per pixel. It was launched on 2025 April 21 aboard the Department of Defense Space Test Program STP-H10 to the ISS. On the ISS, it is located on the SOX external payload facility on the Columbus module. Analysis of TERI data at NRL is supported by the Office of Naval Research 6.1. [1] Shy, Daniel, et al. "Development of the cadmium zinc TElluride Radiation Imager." Journal of Astronomical Telescopes, Instruments, and Systems 10.4 (2024): 044009-044009 (arXiv:2408.04559). Distribution Statement A: Approved for public release. Distribution is unlimited. View this GCN Circular online at https://gcn.nasa.gov/circulars/44679. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0L…

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