The transient accreting X-ray pulsar GRO J1750-27 (AX J1749.1-2639), which became active end of January 2008 (ATel #1376), has been repeatedly observed by the INTEGRAL Galactic Bulge monitoring program since mid February (ATel #1385) on 11, 20 and 23 Feb. 2008. During the three observations, totalling about 27 ks, the source has remained bright at a roughly constant level with the following flux averaged over the 3 observations: 186+/-9 mCrab (3-10 keV), 319+/-15 mCrab (10-25 keV), 198+/-2 mCrab (18-40 keV), and 20+/-3 mCrab (40-100 keV)
We report spectral measurements of the bursting X-ray pulsar GRO J1744-28, made during a balloon fli...
We report the ASCA results of the bursting X-ray pulsar \gro, which was observed in February 1996 an...
The INTEGRAL Galactic bulge monitoring program (see ATel #438) observations obtained between 2011 Fe...
A new season of the INTEGRAL Galactic Bulge monitoring program (see ATels #438, #874, #1005; Kuulker...
INTEGRAL monitoring observations of the Galactic Bulge (e.g. ATels #438 and #1944) have been perform...
Following the detection of high energy emission from Swift J1749.4-2807 by INTEGRAL between April 10...
We report on the discovery and hard X-ray (20-70 keV) observations of the 4.45 s period transient X-...
A new season of observations for the INTEGRAL Galactic Bulge monitoring (see ATel #438) has started ...
The first of a new series of INTEGRAL Galactic bulge monitoring observations (ATel #438, #874) perfo...
The transient X-ray burster KS 1741-293 (e.g., ATel #1531, #2465, #3632, #3646) has become active ag...
The Be/X-ray binary, GRO J1750-27, is one of the farthest known galactic X-ray pulsars at a distance...
We report on the deep observations of the “bursting pulsar” GRO J1744–28, which were performed with ...
© ESO 2020. We report on the deep observations of the "bursting pulsar"GRO J1744-28, which were perf...
INTEGRAL Galactic Bulge monitoring (see ATels #438, #874, #1005, #1385) observations on UT 2008 Sep ...
Aims.The Galactic bulge region is a rich host of variable high-energy point sources. Since 2005, Feb...
We report spectral measurements of the bursting X-ray pulsar GRO J1744-28, made during a balloon fli...
We report the ASCA results of the bursting X-ray pulsar \gro, which was observed in February 1996 an...
The INTEGRAL Galactic bulge monitoring program (see ATel #438) observations obtained between 2011 Fe...
A new season of the INTEGRAL Galactic Bulge monitoring program (see ATels #438, #874, #1005; Kuulker...
INTEGRAL monitoring observations of the Galactic Bulge (e.g. ATels #438 and #1944) have been perform...
Following the detection of high energy emission from Swift J1749.4-2807 by INTEGRAL between April 10...
We report on the discovery and hard X-ray (20-70 keV) observations of the 4.45 s period transient X-...
A new season of observations for the INTEGRAL Galactic Bulge monitoring (see ATel #438) has started ...
The first of a new series of INTEGRAL Galactic bulge monitoring observations (ATel #438, #874) perfo...
The transient X-ray burster KS 1741-293 (e.g., ATel #1531, #2465, #3632, #3646) has become active ag...
The Be/X-ray binary, GRO J1750-27, is one of the farthest known galactic X-ray pulsars at a distance...
We report on the deep observations of the “bursting pulsar” GRO J1744–28, which were performed with ...
© ESO 2020. We report on the deep observations of the "bursting pulsar"GRO J1744-28, which were perf...
INTEGRAL Galactic Bulge monitoring (see ATels #438, #874, #1005, #1385) observations on UT 2008 Sep ...
Aims.The Galactic bulge region is a rich host of variable high-energy point sources. Since 2005, Feb...
We report spectral measurements of the bursting X-ray pulsar GRO J1744-28, made during a balloon fli...
We report the ASCA results of the bursting X-ray pulsar \gro, which was observed in February 1996 an...
The INTEGRAL Galactic bulge monitoring program (see ATel #438) observations obtained between 2011 Fe...