Hard X-ray bursts detected by the IBIS telescope onboard the INTEGRAL observatory in 2003-2004

被引:29
作者
Chelovekov, I. V.
Grebenev, S. A.
Sunyaev, R. A.
机构
[1] Russian Acad Sci, Space Res Inst, Moscow 117810, Russia
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2006年 / 32卷 / 07期
基金
俄罗斯基础研究基金会;
关键词
neutron stars; X-ray bursts; bursters;
D O I
10.1134/S1063773706070048
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
All of the observations performed with the IBIS telescope onboard the INTEGRAL observatory during the first one and a half years of its in-orbit operation (from February 10, 2003, through July 2, 2004) have been analyzed to find X-ray bursts. The time history of the IBIS/ISGRI total count rate in the energy range 15-25 keV revealed 1077 bursts of durations from similar to 5 to similar to 500 s with a high statistical significance (over the entire period of observations, only one event could be detected by chance with a probability of 20%). A part from the events associated with cosmic gamma-ray bursts (detected in the field of view or passed through the IBIS shield), solar flares, and activity of the soft gamma repeater SGR 1806-20, we were able to localize 105 bursts and, with one exception, to identify them with previously known persistent or transient X-ray sources (96 were identified with known X-ray bursters). In one case, the burst source was a new burster in a low state that received the name IGR J17364-2711. Basic parameters of the localized bursts and their identifications are presented in the catalog of bursts. Curiously enough, 61 bursts were detected from one X-ray burster, GX 354-0. The statistical distributions of bursts in duration, maximum flux, and recurrence time have been analyzed for this source. Some of the bursts observed with the IBIS/ISGRI telescope were also detected by the JEM-X telescope onboard the INTEGRAL observatory in the standard X-ray energy range 3-20 keV.
引用
收藏
页码:456 / 477
页数:22
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