GRB111024A

This page lists all entries on GRB111024A in GRBweb

Summary IPN GCN 12489

Summary table
Variable Value Source
T0 7:21:27 UTC GCN_circulars,MAXI Det
ra 222.1750° IPN
decl 25.8500° IPN
pos_error 3.00e-01° IPN
GBM_located False
mjd 55858.3065625 GCN_circulars,MAXI Det
IPN table
GRB_name GRB111024A
ra 222.1750°
decl 25.8500°
pos_error 3.00e-01°
GCN 12489 table
GRB_name GRB111024A
GCN_number 12489
Detection_method MAXI Det
t_trigger 7:21:27 UTC
ra 222.1800°
decl 25.8400°
Circular_text TITLE: GCN CIRCULAR NUMBER: 12489 SUBJECT: GRB 111024A: MAXI/GSC detection of a burst DATE: 11/10/24 12:17:51 GMT FROM: Motoko Suzuki at RIKEN T. Toizumi, M. Morii,(Tokyo Tech), M. Shidatsu (Kyoto U.), M. Serino(RIKEN), S. Ueno, H. Tomida, M. Kohama, M. Ishikawa (JAXA), T. Mihara, M. Sugizaki, S. Nakahira, T. Yamamoto, T. Sootome, M. Matsuoka (RIKEN), N. Kawai, K. Sugimori, R. Usui (Tokyo Tech), A. Yoshida, K. Yamaoka (AGU), H. Tsunemi, M. Kimura, H. Kitayama (Osaka U.), H. Negoro, M. Nakajima, F. Suwa (Nihon U.), Y. Ueda, K. Hiroi (Kyoto U.), Y. Tsuboi, T. Matsumura, K. Yamazaki (Chuo U.) report on behalf of the MAXI team: MAXI/GSC triggered at UT 2011-10-24T07:21:27 on a bright uncatalogued X-ray transient source. Judging from its location and spectral hardness ratio, this transient is probably a gamma-ray burst. Assuming that the source flux was constant over the transit, we obtain the source position at (R.A., Dec) = (+222.18 deg, +25.84 deg) = (14 48 42, +25 50 40)(J2000) with a rectangular error box (90%C.L.) with the following corners: (R.A., Dec) = (+222.22 deg, +25.74 deg) = (14 48 54, +25 44 11)(J2000) (R.A., Dec) = (+222.32 deg, +25.86 deg) = (14 49 16, +25 51 37)(J2000) (R.A., Dec) = (+222.13 deg, +25.95 deg) = (14 48 31, +25 57 15)(J2000) (R.A., Dec) = (+222.04 deg, +25.83 deg) = (14 48 9, +25 49 49)(J2000) There is additional systematic uncertainty of 0.2 deg (90% containment radius). The preliminary flux of the transient source was 700 mCrab (4-10 keV). There was no significant detection at the transit location in the previous orbit (92 min before the detection) with an upper limit of 20 mCrab. There is no known bright X-ray source at the detected position. Follow-up observations are encouraged.