//////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 24936 SUBJECT: GRB 190701B: a long GRB detected by IBAS DATE: 19/07/01 11:18:25 GMT FROM: Diego Gotz at CEA D.Gotz (CEA, Saclay), S.Mereghetti (INAF, IASF-Milano), C.Ferrigno, E.Bozzo, V.Savchenko (ISDC, Versoix), L.Ducci (IAAT, Germany and ISDC, Versoix) and J.Borkowski (CAMK, Torun) report: a gamma ray burst lasting about 23 s has been detected by IBAS in the IBIS/ISGRI data at 10:04:58 UT of July 1st, 2019. The refined coordinates (J2000) are: R.A.= 350.4091 deg DEC.= +64.3457 deg with an uncertainty of 1.1 arcmin (90% c.l.). The burst had a peak flux of 0.1 photons/cm2/s (20-200 keV, 1-s integration time) and a fluence in the same energy range of about 5.e-8 erg/cm2. A plot of the light curve will be posted at http://ibas.iasf-milano.inaf.it/IBAS_Results.html //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 24979 SUBJECT: Konus-Wind observation of GRB 190701B DATE: 19/07/04 16:20:23 GMT FROM: Anastasia Tsvetkova at Ioffe Institute A. Tsvetkova, S. Golenetskii, R.Aptekar, D. Frederiks, M. Ulanov, D. Svinkin, A. Lysenko, A. Kozlova and T. Cline on behalf of the Konus-Wind team, report: The long-duration GRB 190701B (IBAS detection: Gotz et al., GCN 24936) triggered Konus-Wind at T0=36303.292 s UT (10:05:03.292). The burst light curve shows a multi-peaked structure which starts at ~T0-3.3 s and has a total duration of ~13 s. The emission is seen up to ~1.3 MeV. As observed by Konus-Wind, the burst had a fluence of 3.51(-0.46,+0.70)x10^-6 erg/cm2, and a 64-ms peak energy flux, measured from T0-0.072 s, of 1.39(-0.63,+0.68)x10^-6 erg/cm2/s (both in the 20 keV - 10 MeV energy range). The time-integrated spectrum of the burst (measured from T0 to T0+16.640 s) is best fit in the 20 keV - 1.3 MeV range by a power law with exponential cutoff model: dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep) with  alpha = -1.43(-0.33,+0.41), and Ep = 112(-30,+64) keV (chi2 = 48/60 dof). Fitting by the GRB (Band) model yields the same alpha and Ep, and an upper limit on the high energy photon index: beta < -2.17 (chi2 = 48/59 dof). The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB190701_T36303/ All the quoted errors are at the 90% confidence level. All the quoted values are preliminary.