GRB230418A

This page lists all entries on GRB230418A in GRBweb

Summary Fermi GBM IPN GCN 33652 GCN 33653 GCN 33656 GCN 33657 GCN 33659 GCN 33674

Summary table
Variable Value Source
GRB_name_Fermi GRB230418883
T0 21:11:29.941 UTC GCN_circulars,Konus-Wind Det
ra 43.4417° IPN
decl -20.3500° IPN
pos_error 3.33e-01° IPN
T90 0.256 s Fermi_GBM
T90_error 0.072 s Fermi_GBM
T90_start 21:11:33.462 UTC Fermi_GBM
fluence 2.37e-06 erg/cm² Fermi_GBM
fluence_error 1.25e-08 erg/cm² Fermi_GBM
T100 3.777 s
GBM_located False
mjd 60052.88298542824 GCN_circulars,Konus-Wind Det
Fermi GBM table
GRB_name_Fermi GRB230418883
trigger_name bn230418883
ra 47.4400°
decl -12.4600°
datum 2023-04-18
t_trigger 21:11:33.494 UTC
T90 0.256 s
T90_error 0.072 s
T90_start 21:11:33.462 UTC
fluence 2.37e-06 erg/cm²
fluence_error 1.25e-08 erg/cm²
flux_1024 5.49e+00 erg/cm²/s
flux_1024_error 1.94e-01 erg/cm²/s
flux_1024_time -1.28e-01 erg/cm²/s
flux_64 3.06e+01 erg/cm²/s
flux_64_error 1.31e+00 erg/cm²/s
IPN table
GRB_name GRB230418A
ra 43.4417°
decl -20.3500°
pos_error 3.33e-01°
GCN 33652 table
GRB_name GRB230418A
GCN_number 33652
Detection_method Fermi GBM Det
t_trigger 21:11:33.490 UTC
ra 47.4000°
decl -12.5000°
Circular_text TITLE: GCN CIRCULAR NUMBER: 33652 SUBJECT: GRB 230418A: Fermi GBM Observation DATE: 23/04/19 03:51:00 GMT FROM: Oliver J Roberts at USRA/NASA O.J. Roberts (USRA/NASA-MSFC) and C. Meegan (UAH) report on behalf of the Fermi GBM Team: "At 21:11:33.49 UT on 18 April 2023, the Fermi Gamma-Ray Burst Monitor (GBM) triggered and located GRB 230418A (trigger 703545098 / 230418883). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 47.4, Dec = -12.5 (J2000 degrees, equivalent to J2000 03h 10m, -12d 30'), with a statistical uncertainty of 5.9 degrees (radius, 1-sigma containment, statistical only; there is additionally a systematic error which we have characterized as a core-plus-tail model, with 90% of GRBs having a 3.7 deg error and a small tail suffering a larger than 10 deg systematic error. [Connaughton et al. 2015, ApJS, 216, 32] ). The angle from the Fermi LAT boresight at the GBM trigger time is 71 degrees. The GBM light curve consists of single burst with a duration (T90) of about 0.25 s (50-300 keV). The time-averaged spectrum from T0-0.064 s to T0+0.256 s is best fit by a power law function with an exponential high-energy cutoff. The power law index is -0.22 +/- 0.08 and the cutoff energy, parameterized as Epeak, is 838 +/- 71 keV. The event fluence (10-1000 keV) in this time interval is (2.51 +/- 0.08)E-06 erg/cm^2. The 64 msec peak photon flux measured starting from T0+0.13 s in the 10-1000 keV band is 31 +/- 1 ph/s/cm^2. A Band function fits the spectrum equally well with Epeak = 836 +/- 75 keV, alpha = -0.22 +/- 0.08, and beta = -3.9+/- 1.9. 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/"
GCN 33653 table
GRB_name GRB230418A
GCN_number 33653
Detection_method Swift Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 33653 SUBJECT: GRB 230418A: Swift/BAT-GUANO detection outside the coded FOV DATE: 23/04/19 07:02:04 GMT FROM: Aaron Tohuvavohu at University of Toronto Samuele Ronchini (PSU), Gayathri Raman (PSU), Jamie A. Kennea (PSU), James DeLaunay (UAlabama), Aaron Tohuvavohu (U Toronto), Tyler Parsotan (UMBC/GSFC) report: Swift/BAT did not localize GRB 230418A onboard (T0: 2023-04-18T21:11:33.49 UTC, Fermi/GBM GCN 33652) The Fermi notice distributed in near real-time, triggered the Swift Mission Operations Center operated Gamma-ray Urgent Archiver for Novel Opportunities (GUANO; Tohuvavohu et al. 2020, ApJ, 900, 1). Upon trigger by this notice, GUANO sent a command to the Swift Burst Alert Telescope (BAT) to save 200 seconds of BAT event-mode data from [-50,+150] seconds around the time of the burst. All the requested event mode data was delivered to the ground. The BAT likelihood search, NITRATES (DeLaunay + Tohuvavohu 2022, ApJ, 941, 169), detects the burst with a sqrt(TS) of 31.1 in a 0.256 s analysis time bin. The burst duration as seen by BAT is ~0.25 seconds. NITRATES results indicate a burst coming from outside the FOV, with DeltaLLHOut of -20. The NITRATES best fit OFOV position is consistent with the Fermi/GBM localization (GCN 33652). See Section 9.1 and Figures 10 and 17 in the NITRATES paper for brief descriptions and interpretation of sqrt(TS), DeltaLLHPeak, and DeltaLLHOut. GUANO is a fully autonomous, extremely low latency, spacecraft commanding pipeline designed for targeted recovery of BAT event mode data around the times of compelling astrophysical events to enable more sensitive GRB searches. A live reporting of Swift/BAT event data recovered by GUANO can be found at: https://www.swift.psu.edu/guano/
GCN 33656 table
GRB_name GRB230418A
GCN_number 33656
Detection_method Fermi GBM Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 33656 SUBJECT: GRB 230418A: AGILE detection DATE: 23/04/19 20:12:42 GMT FROM: Francesco Verrecchia at SSDC,INAF-OAR G. Panebianco (Univ. Bologna - INAF/OAS Bologna), F. Verrecchia, C. Pittori (SSDC, and INAF/OAR) , N. Parmiggiani (INAF/OAS-Bologna), M. Tavani (INAF/IAPS, and Univ. Roma Tor Vergata), C. Casentini, A. Argan, M. Cardillo, Y. Evangelista, L. Foffano, E. Menegoni, G. Piano, A. Ursi (INAF/IAPS), A. Addis, L. Baroncelli, A. Bulgarelli, A. Di Piano, V. Fioretti (INAF/OAS-Bologna), F. Lucarelli (SSDC, and INAF/OAR), M. Romani (INAF/OA-Brera), M. Marisaldi (INAF/OAS-Bologna, and Bergen University), M. Pilia, A. Trois (INAF/OA-Cagliari), F. Longo (Univ. Trieste and INFN Trieste), I. Donnarumma (ASI), A. Giuliani (INAF/IASF-Mi), and P. Tempesta (TeleSpazio), report on behalf of the AGILE Team: The AGILE satellite detected the GRB 230418A at T0 = 2023-04-18 21:11:33 s (UTC), reported by Fermi GBM (GCNs #33652, #33653). The burst is clearly visible in the AGILE scientific ratemeters of the MiniCALorimeter (MCAL; 0.4-100 MeV), and AntiCoincidence (AC; 50-200 keV) detectors. The event lasted about 2 s and it released a total number of 1538 counts in the MCAL detector (above a background rate of 1100 Hz), and 7778 counts in the AC detector (above a background rate of 3659 Hz). The AGILE ratemeters light curves can be found at http://www.agilescienceapp.it/notices/GRB230418A_AGILE_RM_ND.png . Additional analysis of AGILE data is in progress. Automatic MCAL GRB alert Notices can be found at: https://gcn.gsfc.nasa.gov/agile_mcal.html
GCN 33657 table
GRB_name GRB230418A
GCN_number 33657
Detection_method AstroSat CZTI
Circular_text TITLE: GCN CIRCULAR NUMBER: 33657 SUBJECT: GRB 230418A: AstroSat CZTI detection DATE: 23/04/20 05:59:08 GMT FROM: Gaurav Waratkar at IIT,Bombay P K. Navaneeth (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 short GRB 230418A which was also detected by Fermi (O.J. Roberts, et al., GCN Circ. 33652), Swift/BAT-GUANO (S. Ronchini, et al., GCN Circ. 33653), and AGILE (G. Panebianco, et al., GCN Circ. 33656). The source was clearly detected in the 20-200 keV energy range. The light curve peaks at 2023-04-18 21:11:33.56 UTC. The measured peak count rate associated with the burst is 2120 (+893, -443) counts/s above the background in the combined data of all quadrants, with a total of 155 (+52, -45) counts. The local mean background count rate was 488 (+18, -38) counts/s. Using cumulative rates, we measure a T90 of 0.20 (+0.16, -0.06) s. The source was also clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range. 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
GCN 33659 table
GRB_name GRB230418A
GCN_number 33659
Detection_method IPN Triangulation
t_trigger 21:11:33 UTC
ra 43.4420°
decl -20.3430°
Circular_text TITLE: GCN CIRCULAR NUMBER: 33659 SUBJECT: IPN triangulation of GRB 230418A (short) DATE: 23/04/20 14:30:46 GMT FROM: Dmitry Svinkin at Ioffe Institute A.S. Kozyrev, D.V. Golovin, M.L. Litvak, I.G. Mitrofanov, and A.B. Sanin on behalf of the HEND/Mars Odyssey team, D. Svinkin, D. Frederiks, A. Ridnaia, A. Lysenko, and T. Cline on behalf of the Konus-Wind team, A. Goldstein, M. S. Briggs, C. Wilson-Hodge, and E. Burns on behalf of the Fermi GBM team, E. Bozzo and C. Ferrigno, on behalf of the INTEGRAL SPI-ACS GRB team, S. Barthelmy, J. Cummings, H. Krimm, D. Palmer, and A. Tohuvavohu on behalf of the Swift-BAT team, and W. Boynton, C. Fellows, K. Harshman, H. Enos, R. Starr, and A.S. Gardner on on behalf of the GRS-Odyssey GRB team, report: The short-duration GRB 230418A (Fermi-GBM detection: Roberts et al., GCN Circ. 33652; Swift/BAT-GUANO detection: Ronchini et al., GCN Circ. 33653; AGILE detection: Panebianco et al., GCN Circ. 33656; AstroSat-CZTI detection: Navaneeth et al., GCN Circ. 33657) was detected by Fermi (GBM trigger 703545098), Swift (BAT), Konus-Wind, INTEGRAL (SPI-ACS), AGILE (MCAL, AC), AstroSat (CZTI), and Mars-Odyssey (HEND) at about 76293 s UT (21:11:33). The burst was outside the coded field of view of the BAT. We have triangulated it to a preliminary, 3 sigma error box whose coordinates are: --------------------------------------------- RA(2000), deg Dec(2000), deg --------------------------------------------- Center: 43.442 (02h 53m 46s) -20.343 (-20d 20' 36") Corners: 43.565 (02h 54m 16s) -20.460 (-20d 27' 37") 43.510 (02h 54m 02s) -20.481 (-20d 28' 53") 43.320 (02h 53m 17s) -20.226 (-20d 13' 34") 43.375 (02h 53m 30s) -20.205 (-20d 12' 19") --------------------------------------------- The error box area is 61 sq. arcmin, and its maximum dimension is 20 arcmin (the minimum one is 3.2 arcmin). The Sun distance was 35 deg. This box may be improved. The IPN localization is consistent with, but reduces the area of, the Fermi-GBM final localization (GCN 33652). A triangulation map and HEALPix FITS file are posted at http://www.ioffe.ru/LEA/GRBs/GRB230418_T76289/IPN The Konus-Wind time history and spectrum will be given in a forthcoming GCN Circular.
GCN 33674 table
GRB_name GRB230418A
GCN_number 33674
Detection_method Konus-Wind Det
t_trigger 21:11:29.941 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 33674 SUBJECT: Konus-Wind detection of GRB 230418A DATE: 23/04/22 16:32:46 GMT FROM: Dmitry Svinkin at Ioffe Institute D. Svinkin, D. Frederiks, M. Ulanov, A. Tsvetkova, A. Lysenko, A. Ridnaia, and T. Cline on behalf of the Konus-Wind team, report: The short-duration GRB 230418A (Fermi-GBM detection: Roberts et al., GCN Circ. 33652; Swift/BAT-GUANO detection: Ronchini et al., GCN Circ. 33653; AGILE detection: Panebianco et al., GCN Circ. 33656; AstroSat-CZTI detection: Navaneeth et al., GCN Circ. 33657; IPN triangulation: Kozyrev et al., GCN Circ. 33659) triggered Konus-Wind at T0=76289.941 s UT (21:11:29.941). The burst light curve shows a multi-peaked structure which starts at ~T0 s and has a total duration of ~0.3 s. The emission is seen up to ~2 MeV. The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB230418_T76289/ As observed by Konus-Wind, the burst had a fluence of 4.13(-0.64,+0.76)x10^-6 erg/cm2, and a 16-ms peak flux, measured from T0+0.048 s, of 3.84(-1.00,+1.10)x10^-5 erg/cm2/s (both in the 20 keV - 10 MeV energy range). The time-averaged spectrum of the burst (measured from T0 to T0+0.192 s) is best fit in the 20 keV - 2 MeV range by a power law with exponential cutoff model: dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep) with alpha = -0.52(-0.20,+0.23) and Ep = 1071(-228,+335) keV (chi2 = 16/24 dof). Fitting by a GRB (Band) model yields the same alpha and Ep, and an upper limit on the high energy photon index: beta < -1.87 (chi2 = 16/23 dof). All the quoted errors are at the 90% confidence level. All the quoted values are preliminary.