GRB240107A

This page lists all entries on GRB240107A in GRBweb

Summary Fermi GBM IPN GCN 35495 GCN 35503

Summary table
Variable Value Source
GRB_name_Fermi GRB240107803
T0 19:15:47 UTC GCN_circulars,MAXI Det
ra 298.0125° IPN
decl -68.2333° IPN
pos_error 5.00e-01° IPN
T90 60.161 s Fermi_GBM
T90_error 4.404 s Fermi_GBM
T90_start 19:16:29.193 UTC Fermi_GBM
fluence 6.23e-06 erg/cm² Fermi_GBM
fluence_error 2.09e-07 erg/cm² Fermi_GBM
T100 102.354 s
GBM_located False
mjd 60316.80262731481 GCN_circulars,MAXI Det
Fermi GBM table
GRB_name_Fermi GRB240107803
trigger_name bn240107803
ra 292.4600°
decl -68.3000°
pos_error 5.01e+00°
datum 2024-01-07
t_trigger 19:16:29.705 UTC
T90 60.161 s
T90_error 4.404 s
T90_start 19:16:29.193 UTC
fluence 6.23e-06 erg/cm²
fluence_error 2.09e-07 erg/cm²
flux_1024 3.61e+00 erg/cm²/s
flux_1024_error 3.37e-01 erg/cm²/s
flux_1024_time 4.58e+01 erg/cm²/s
flux_64 6.03e+00 erg/cm²/s
flux_64_error 1.21e+00 erg/cm²/s
IPN table
GRB_name GRB240107A
ra 298.0125°
decl -68.2333°
pos_error 5.00e-01°
GCN 35495 table
GRB_name GRB240107A
GCN_number 35495
Detection_method MAXI Det
t_trigger 19:15:47 UTC
ra 298.0140°
decl -68.2280°
Circular_text TITLE: GCN CIRCULAR NUMBER: 35495 SUBJECT: GRB 240107A: MAXI/GSC detection DATE: 24/01/08 02:37:58 GMT FROM: Hitoshi Negoro at Nihon University/MAXI team T. Kurihara (JAXA), H. Negoro, M. Nakajima, K. Kobayashi, M. Tanaka, Y. Soejima, Y. Kudo (Nihon U.), T. Mihara, T. Kawamuro, S. Yamada, T. Tamagawa, N. Kawai, M. Matsuoka (RIKEN), T. Sakamoto, M. Serino, S. Sugita, H. Hiramatsu, H. Nishikawa, A. Yoshida (AGU), Y. Tsuboi, S. Urabe, S. Nawa, N. Nemoto, E.Goto (Chuo U.), M. Shidatsu, Y. Niida (Ehime U.), I. Takahashi, M. Niwano, S. Sato, N. Higuchi, Y. Yatsu (Tokyo Tech), S. Nakahira, S. Ueno, H. Tomida, M. Ishikawa, S. Ogawa (JAXA), Y. Ueda, K. Setoguchi, T. Yoshitake, Y. Nakatani, Y. Okada (Kyoto U.), M. Yamauchi, Y. Hagiwara, Y. Umeki, Y. Otsuki (Miyazaki U.), K. Yamaoka (Nagoya U.), Y. Kawakubo (LSU), M. Sugizaki (NAOC), and W. Iwakiri (Chiba U.) The MAXI/GSC nova alert system triggered on a bright uncatalogued X-ray transient source at 19:15:47 UT on January 7, 2023. Assuming that the source flux was constant over the transit, we obtain the source position at (R.A., Dec) = (298.014 deg, -68.228 deg) = (19 52 03, -68 13 39) (J2000) with a 90% C.L. statistical error of 0.41 deg and an additional systematic uncertainty of 0.1 deg (90% containment radius). The X-ray flux averaged over the scan was 114 +- 24 mCrab (4.0-10.0keV, 1 sigma error). Without assumptions on the source constancy, we obtain a rectangular error box for the transient source with the following corners: (R.A., Dec) = (296.278, -67.736) deg = (19 45 06, -67 44 09) (J2000) (R.A., Dec) = (296.022, -68.496) deg = (19 44 05, -68 29 45) (J2000) (R.A., Dec) = (303.762, -68.679) deg = (20 15 02, -68 40 44) (J2000) (R.A., Dec) = (303.766, -67.913) deg = (20 15 03, -67 54 46) (J2000) There was no significant excess flux in the previous transit at 17:42 UT and in the next transit at 20:48 UT with an upper limit of 20 mCrab for each.
GCN 35503 table
GRB_name GRB240107A
GCN_number 35503
Detection_method AstroSat CZTI
Circular_text TITLE: GCN CIRCULAR NUMBER: 35503 SUBJECT: GRB 240107A: AstroSat CZTI detection DATE: 24/01/09 07:01:04 GMT FROM: Gaurav Waratkar at IIT Bombay J. Joshi (IUCAA), G. Waratkar (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-duration GRB 240107A which was also detected by MAXI-GSC (Kurihara et al., GCN Circ. 35495). 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 2024-01-07 19:16:32.4 UTC. The measured peak count rate associated with the burst is 191 (+66, -13) counts/s above the background in the combined data of three quadrants (out of four), with a total of 6807 (+1623, -1781) counts. The local mean background count rate was 1088 (+3, -4) counts/s. We measure a T90 of 160 (+18, -10) s from the cumulative Veto light curve. 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