GRB160521A

This page lists all entries on GRB160521A in GRBweb

Summary IPN GCN 19442 GCN 19534

Summary table
Variable Value Source
T0 3:37:20 UTC GCN_circulars,INTEGRAL
ra 129.7167° IPN
decl 46.9000° IPN
pos_error 5.33e-02° IPN
GBM_located False
mjd 57529.150925925926 GCN_circulars,INTEGRAL
IPN table
GRB_name GRB160521A
ra 129.7167°
decl 46.9000°
pos_error 5.33e-02°
GCN 19442 table
GRB_name GRB160521A
GCN_number 19442
Detection_method INTEGRAL
t_trigger 3:37:20 UTC
ra 129.7108°
decl 46.9142°
Circular_text TITLE: GCN CIRCULAR NUMBER: 19442 SUBJECT: GRB 160521A: a long GRB detected by INTEGRAL DATE: 16/05/21 04:45:52 GMT FROM: Sandro Mereghetti at IASF-Milano/INAF S.Mereghetti (IASF-Milano), D.Gotz (CEA, Saclay), C.Ferrigno, E.Bozzo, L.Di Gesu' (ISDC, Versoix), and J.Borkowski (CAMK, Torun) on behalf of the IBAS Localization Team report: a gamma ray burst lasting about 160 s has been detected by IBAS in the IBIS/ISGRI data at 03:37:20 UT of May 21, 2016. The refined coordinates (J2000) are: R.A.= 129.7108 DEC.= 46.9142 with an uncertainty of 1.5 arcmin (90% c.l.). The burst had a peak flux of 0.8 counts/cm2/s (20-200 keV, 1-s integration time) and a fluence in the same energy range of about 1.2e-6 erg/cmq. A plot of the light curve will be posted at http://ibas.iasf-milano.inaf.it/IBAS_Results.html
GCN 19534 table
GRB_name GRB160521A
GCN_number 19534
Detection_method INTEGRAL
ra 129.7138°
decl 46.9058°
Circular_text TITLE: GCN CIRCULAR NUMBER: 19534 SUBJECT: GRB 160521A: 15 GHz detections and upper limit from AMI DATE: 16/06/14 16:24:06 GMT FROM: Kunal Mooley at Oxford U K. P. Mooley, T. D. Staley, R. P. Fender (Oxford), G. E. Anderson (Curtin), T. Cantwell (Manchester), C. Rumsey, D. Titterington, S. H. Carey, J. Hickish, Y. C. Perrott, N. Razavi-Ghods, P. Scott (Cambridge), K. Grainge, A. Scaife (Manchester) We observed the INTEGRAL/IBIS GRB 160521A (Mereghetti et al., GCN 19442) with the AMI Large Array at 15 GHz on 2016 May 24.62, May 27.52, and Jun 03.61 (UT) as part of the 4pisky program. We detect a transient radio source (RA=08:38:51.3 +/-6 arcsec, Dec=+46:54:21 +/-24 arcsec) within the INTEGRAL error circle at 266+/-36 uJy and 133+/-29 uJy in the first two epochs, and obtain a 3sigma upper limit of 93 uJy in the third epoch. We thank the AMI staff for scheduling these observations. The AMI-GRB database is a log of all GRB follow up observations with the AMI, and is available at http://4pisky.org/ami-grb/.