GRB120519A

This page lists all entries on GRB120519A in GRBweb

Summary Fermi GBM GCN 13313 GCN 13315 GCN 13350

Summary table
Variable Value Source
GRB_name_Fermi GRB120519721
T0 17:18:14.922 UTC Fermi_GBM
ra 178.3660° GCN_circulars,IPN Triangulation
decl 22.4070° GCN_circulars,IPN Triangulation
T90 1.056 s Fermi_GBM
T90_error 0.451 s Fermi_GBM
T90_start 17:18:14.922 UTC Fermi_GBM
fluence 9.59e-07 erg/cm² Fermi_GBM
fluence_error 1.67e-08 erg/cm² Fermi_GBM
T100 1.056 s
GBM_located False
mjd 56066.72100604167 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB120519721
trigger_name bn120519721
ra 180.2500°
decl 20.5500°
pos_error 4.09e+00°
datum 2012-05-19
t_trigger 17:18:14.970 UTC
T90 1.056 s
T90_error 0.451 s
T90_start 17:18:14.922 UTC
fluence 9.59e-07 erg/cm²
fluence_error 1.67e-08 erg/cm²
flux_1024 6.49e+00 erg/cm²/s
flux_1024_error 2.65e-01 erg/cm²/s
flux_1024_time -6.40e-02 erg/cm²/s
flux_64 1.27e+01 erg/cm²/s
flux_64_error 1.40e+00 erg/cm²/s
GCN 13313 table
GRB_name GRB120519A
GCN_number 13313
Detection_method IPN Triangulation
t_trigger 17:18:15 UTC
ra 178.3660°
decl 22.4070°
Circular_text TITLE: GCN CIRCULAR NUMBER: 13313 SUBJECT: IPN Triangulation of GRB 120519A (short/hard) DATE: 12/05/21 15:23:28 GMT FROM: Valentin Pal'shin at Ioffe Inst S. Golenetskii, R. Aptekar, E. Mazets, V. Pal'shin, D. Frederiks, D. Svinkin, and T. Cline on behalf of the Konus-Wind team, K. Hurley, and J. Goldsten, on behalf of the MESSENGER GRNS GRB team, V. Connaughton, M. Briggs, and C. Meegan, on behalf of the Fermi GBM team, K. Yamaoka, M. Ohno, Y. Hanabata, Y. Fukazawa, T. Takahashi, M. Tashiro, Y. Terada, T. Murakami, and K. Makishima on behalf of the Suzaku WAM team, A. von Kienlin, X. Zhang, A. Rau, V. Savchenko, E. Bozzo, and C. Ferrigno, on behalf of the INTEGRAL SPI-ACS GRB team, S. Barthelmy, J. Cummings, N. Gehrels, H. Krimm, and D. Palmer, on behalf of the Swift-BAT team, and G. Di Cocco, F. Fuschino, M. Galli, C. Labanti, and M. Marisaldi, on behalf of the AGILE MCAL team, report: The short-duration, hard GRB 120519A has been observed by Fermi (GBM trigger 359140696), Konus-Wind, Swift (BAT), MESSENGER (GRNS), INTEGRAL (SPI-ACS), Suzaku (WAM), and AGILE (MCAL), so far, at about 62295 s UT (17:18:15). 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: 178.366 (11h 53m 28s) +22.407 (+22d 24' 24") Corners: 179.899 (11h 59m 36s) +24.184 (+24d 11' 02") 178.690 (11h 54m 46s) +23.008 (+23d 00' 31") 176.909 (11h 47m 38s) +20.581 (+20d 34' 53") 178.049 (11h 52m 12s) +21.803 (+21d 48' 09") --------------------------------------------- The error box area is 0.60 sq. deg, and its maximum dimension is 4.5 deg. This box may be improved. The time history and spectrum will be given in a forthcoming GCN Circular. A triangulation map is posted at http://www.ioffe.ru/LEA/GRBs/GRB120519_T62298/IPN/
GCN 13315 table
GRB_name GRB120519A
GCN_number 13315
Detection_method Konus-Wind Det
t_trigger 17:18:18.004 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 13315 SUBJECT: Konus-Wind observation of GRB 120519A DATE: 12/05/21 16:04:56 GMT FROM: Dmitry Frederiks at Ioffe Institute S. Golenetskii, R.Aptekar, D. Frederiks, E. Mazets, V. Pal'shin, P. Oleynik, M. Ulanov, D. Svinkin, and T. Cline on behalf of the Konus-Wind team, report: The short-duration hard GRB 120519A (IPN localization: Golenetskii at al., GCN 13313) triggered Konus-Wind at T0=62298.004s UT (17:18:18.004) The light curve shows a series of overlapping pulses with a total duration of ~1.2 s. The emission is seen up to ~7.5 MeV. The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB120519_T62298/ As observed by Konus-Wind the burst had a fluence of 3.7(-1.1,+1.5)x10-6 erg/cm2, and a 16-ms peak flux, measured from T0, of 1.3(-0.4,+0.5)x10-5 erg/cm2/s (both in the 20 keV - 10 MeV energy range). The spectrum of the burst (measured from T0 to T0+0.256 s) is well fit in the 20 keV - 10 MeV range by a power law with exponential cutoff model, for which alpha = -0.5 (-0.3, +0.3), and Ep = 740(-240, +450) keV, chi2 = 22.9/22 dof. All the quoted results are preliminary. All the quoted errors are at the 90% confidence level.
GCN 13350 table
GRB_name GRB120519A
GCN_number 13350
Detection_method Suzaku WAM Det
Circular_text TITLE: GCN CIRCULAR NUMBER: 13350 SUBJECT: GRB 120519A: Suzaku WAM observation of the prompt emission DATE: 12/05/30 07:29:10 GMT FROM: Makoto Tashiro at Saitama U/Swift A. Sakamoto, M. Tashiro, Y. Terada, W. Iwakiri, T. Yasuda, K. Takahara, M. Asahina, S. Kobayashi, H. Ueno (Saitama U.), M. Akiyama, N. Ohmori, M. Yamauchi (Univ. of Miyazaki), K. Yamaoka, Y. E. Nakagawa (Waseda U.), Y. Hanabata, T. Kawano, K. Takaki, R. Nakamura, Y.Tanaka, M. Ohno, Y. Fukazawa (Hiroshima U.), S. Sugita (Nagoya U.), M. Kokubun, T. Takahashi (ISAS/JAXA), Y. Urata, P. Tsai (NCU), K. Nakazawa, K. Makishima (Univ. of Tokyo), on behalf of the Suzaku WAM team, report: The short GRB 120519A (IPN; Pal'shin et al., GCN 13313, Konus-Wind; Golenetskii et al., GCN 13315) triggered the Suzaku Wide-band All-sky Monitor (WAM) which covers an energy range of 50 keV - 5 MeV at 17:18:14.64 UT (=T0). The observed light curve shows a multi-peaked structure starting at T0-0.2 s, ending at T0+0.6 s, with a duration (T90) of about 0.72 seconds. The fluence in 100 - 1000 keV was 1.45(-0.28 +0.09) x 10^-6 erg/cm^2. The 1-s peak flux measured from T0-0.5s was 2.76(-0.33 +0.18) photons/cm^2/s in the same energy range. Preliminary result shows that the time-averaged spectrum from T0-0.5s to T0+0.5s is well fitted by a power-law with exponential cutoff model: dN/dE ~ E^{-alpha} * exp(-(2-alpha)*E/Epeak) with alpha 0.41(-0.41 +0.58), and Epeak 736(-141 +226) keV (chi^2/d.o.f. = 16.9/24). In case we fit the same spectrum by a GRB Band model with a fixed beta of 2.5, the best fit parameters and their errors are, low-energy photon index alpha: -0.10(-0.92 +1.60), and the peak energy Epeak: 611(-146 +279) keV (chi^2/d.o.f = 20.0/24). All the quoted errors are at statistical 90% confidence level, in which the systematic uncertainties are not included. ---- The light curves for this burst are available at: http://www.astro.isas.jaxa.jp/suzaku/HXD-WAM/WAM-GRB/grb/trig/grb_table.html