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This page lists all entries on GRB240405A in GRBweb

Summary Fermi GBM GCN 36037 GCN 36054 GCN 36066

Summary table
Variable	Value	Source
GRB_name_Fermi	GRB240405630
T0	15:06:45.730 UTC	Fermi_GBM
ra	289.6500°	Fermi_GBM
decl	37.7900°	Fermi_GBM
pos_error	4.52e+00°	Fermi_GBM
T90	65.536 s	Fermi_GBM
T90_error	2.318 s	Fermi_GBM
T90_start	15:06:45.730 UTC	Fermi_GBM
fluence	3.88e-06 erg/cm²	Fermi_GBM
fluence_error	1.18e-07 erg/cm²	Fermi_GBM
T100	65.536 s
GBM_located	True
mjd	60405.62969594907	Fermi_GBM

Fermi GBM table
GRB_name_Fermi	GRB240405630
trigger_name	bn240405630
ra	289.6500°
decl	37.7900°
pos_error	4.52e+00°
datum	2024-04-05
t_trigger	15:06:46.498 UTC
T90	65.536 s
T90_error	2.318 s
T90_start	15:06:45.730 UTC
fluence	3.88e-06 erg/cm²
fluence_error	1.18e-07 erg/cm²
flux_1024	3.85e+00 erg/cm²/s
flux_1024_error	5.65e-01 erg/cm²/s
flux_1024_time	4.84e+01 erg/cm²/s
flux_64	1.47e+01 erg/cm²/s
flux_64_error	4.51e+00 erg/cm²/s

GCN 36037 table
GRB_name	GRB240405A
GCN_number	36037
Detection_method	Fermi GBM final loc
t_trigger	15:06:46 UTC
ra	289.6000°
decl	37.8000°
Circular_text	TITLE: GCN CIRCULAR NUMBER: 36037 SUBJECT: GRB 240405A: Fermi GBM Final Real-time Localization DATE: 24/04/05 15:17:52 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM The Fermi GBM team reports the detection of a likely LONG GRB At 15:06:46 UT on 5 Apr 2024, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 240405A (trigger 734022411.49845 / 240405630). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 289.6, Dec = 37.8 (J2000 degrees, equivalent to J2000 19h 18m, 37d 47'), with a statistical uncertainty of 5.2 degrees. The angle from the Fermi LAT boresight is 143.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2024/bn240405630/quicklook/glg_skymap_all_bn240405630.png The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2024/bn240405630/quicklook/glg_healpix_all_bn240405630.fit The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2024/bn240405630/quicklook/glg_lc_medres34_bn240405630.gif

GCN 36054 table
GRB_name	GRB240405A
GCN_number	36054
Detection_method	Fermi GBM Det
t_trigger	15:07:38.500 UTC
Circular_text	TITLE: GCN CIRCULAR NUMBER: 36054 SUBJECT: GRB 240405A: GRBAlpha detection DATE: 24/04/09 15:51:10 GMT FROM: Marianna Dafčíková at Masaryk University <500025@mail.muni.cz> M. Dafcikova, J. Ripa, M. Kolar (Masaryk U.), A. Pal (Konkoly Observatory), N. Werner (Masaryk U.), M. Ohno, H. Takahashi (Hiroshima U.), L. Meszaros, B. Csak (Konkoly Observatory), N. Husarikova, F. Munz , M. Topinka, M. Duriskova, L. Szakszonova, J.-P. Breuer, F. Hroch (Masaryk U.), T. Urbanec, M. Kasal, A. Povalac (Brno U. of Technology), J. Hudec, J. Kapus, M. Frajt (Spacemanic s.r.o), R. Laszlo, M. Koleda (Needronix s.r.o), M. Smelko, P. Hanak, P. Lipovsky (Technical U. of Kosice), G. Galgoczi (Wigner Research Center/Eotvos U.), Y. Uchida, H. Poon, H. Matake (Hiroshima U.), N. Uchida (ISAS/JAXA), T. Bozoki (Eotvos U.), G. Dalya (Eotvos U.), T. Enoto (Kyoto U.), Zs. Frei (Eotvos U.), G. Friss (Eotvos U.), Y. Fukazawa, K. Hirose (Hiroshima U.), S. Hisadomi (Nagoya U.), Y. Ichinohe (Rikkyo U.), K. Kapas (Eotvos U.), L. L. Kiss (Konkoly Observatory), T. Mizuno (Hiroshima U.), K. Nakazawa (Nagoya U.), H. Odaka (Univ of Tokyo), J. Takatsy (Eotvos U.), K. Torigoe (Hiroshima U.), N. Kogiso, M. Yoneyama (Osaka Metropolitan U.), M. Moritaki (U. Tokyo), T. Kano (U. Michigan) -- the GRBAlpha collaboration. The long-duration GRB 240405A (Fermi/GBM detection: GCN 36037) was observed by the GRBAlpha 1U CubeSat (Pal et al. 2023, A&A, 677, 40; https://ui.adsabs.harvard.edu/abs/2023A%26A...677A..40P/abstract). The detection was confirmed at the peak time 2024-04-05 15:07:38.5 UTC. The T90 duration measured by GRBAlpha is 24.0 s and the overall significance during T90 reaches 7 sigma. The light curve obtained by GRBAlpha is available here: https://grbalpha.konkoly.hu/static/share/GRB240405A_GCN.pdf All GRBAlpha detections are listed at: https://monoceros.physics.muni.cz/hea/GRBAlpha/ GRBAlpha, launched on 2021 March 22, is a demonstration mission for a future CubeSat constellation (Werner et al. Proc. SPIE 2018). The detector of GRBAlpha consists of a 75 x 75 x 5 mm3 CsI scintillator read out by a SiPM array, covering the energy range from ~50 keV to ~1000 keV. To increase the duty cycle and the downlink rate, the upgrade of the on-board data acquisition software stack is in progress. The ground segment is also supported by the radio amateur community and it takes advantage of the SatNOGS network for increased data downlink volume.

GCN 36066 table
GRB_name	GRB240405A
GCN_number	36066
Detection_method	Fermi GBM Other
Circular_text	TITLE: GCN CIRCULAR NUMBER: 36066 SUBJECT: GRB 240405A: Glowbug gamma-ray detection DATE: 24/04/11 22:51:00 GMT FROM: C.C. Cheung at Naval Research Lab 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], operating on the International Space Station, reports the detection of GRB 240405A, which was also detected by Fermi/GBM (GCN 36037) and GRBAlpha (GCN 36054). Using an adaptive window with a resolution of 32-ms, the burst onset is determined to be 2024-04-05 15:06:44.536 with a duration of 56.3 s and a total significance of about 21.2 sigma. The light curve comprises two main emission episodes from T0 to T0+1.0s and T0+48.1s to T0+56.3s. 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. The detector comprises 12 large-area (15 cm x 15 cm) CsI:Tl panels covering the surface of a half cube, and two hexagonal (5-cm diameter, 10-cm length) CLLB scintillators, giving it a large field of view (instantaneous FoV ~2/3 sky) over a wide energy band of 50 keV to >2 MeV. [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] Goldstein, A. et al. 2020, ApJ 895, 40, arXiv :1909.03006 Distribution Statement A: Approved for public release. Distribution is unlimited.