INTEGRAL Galactic Bulge Monitoring Revolution 0411: Observation start 2006-02-24 = MJD 53790
Total Observation GTI = 12314 seconds
ISGRI
ISGRI significance mosaic images. Left: ISGRI 18-40 keV. Right: 40-100 keVSources detected > 10σ in each band are marked on the image. The table below lists the fitted position, and statistical positional uncertainty in arcmin returned by the mosaic step of
OSA7
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 cps ) where available.NOTES: The table is constructed from the
isgri_mosa_res.fits
file - fluxes in the mosaic output are known to be systematically ~10% lower than in the ScW light-curves (see known issues). The systematic noise increases towards the edge of the field of view andNEW
sources < 6σ towards the border of the image may be spurious.
ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== XTE J1817-330 274.429 -33.026 0.6 359.810 -7.997 21.2 0.38 55.5 7.1 0.30 23.6 GX 5-1 270.285 -25.080 0.7 5.077 -1.020 16.5 0.35 47.2 0.0 0.00 0.0 4U 1700-377 255.984 -37.846 0.8 347.752 +2.174 26.4 0.59 44.5 5.8 0.46 12.7 GX 1+4 263.005 -24.750 0.8 1.931 +4.795 15.5 0.35 44.6 0.0 0.00 0.0 Ginga 1826-24 277.364 -23.790 0.9 9.277 -6.082 18.2 0.53 34.3 6.7 0.41 16.2 GRS 1758-258 270.304 -25.744 1.0 4.509 -1.363 10.5 0.34 31.1 6.9 0.27 25.3 1A 1742-294 266.522 -29.514 1.2 359.560 -0.388 6.3 0.26 24.2 2.3 0.21 10.5 OAO 1657-415 255.214 -41.663 1.2 344.368 +0.308 28.2 1.15 24.6 4.2 0.83 5.1 GX 354-0 262.988 -33.817 1.3 354.317 -0.139 7.2 0.33 21.7 0.0 0.00 0.0 H 1820-303 275.917 -30.357 1.6 2.791 -7.910 7.3 0.42 17.4 0.0 0.00 0.0 GX 349+2 256.447 -36.423 1.9 349.109 +2.741 7.7 0.52 14.7 0.0 0.00 0.0 3A 1822-371 276.458 -37.074 2.3 356.883 -11.287 6.1 0.53 11.5 0.0 0.00 0.0 1A 1743-288 266.653 -28.884 2.6 0.157 -0.159 2.6 0.26 10.2 0.0 0.00 0.0 4U 1722-30 261.881 -30.818 2.4 356.303 +2.294 3.5 0.32 11.0 1.3 0.26 5.1 GX 3+1 267.021 -26.555 3.1 2.318 +0.769 2.5 0.29 8.4 0.0 0.00 0.0 SLX 1735-269 264.548 -26.981 3.0 0.796 +2.425 2.5 0.29 8.6 1.1 0.24 4.5 SLX 1744-299_300 266.831 -29.995 3.7 359.288 -0.867 1.8 0.27 6.9 0.0 0.00 0.0 3A 1728-169 262.928 -17.011 4.5 8.468 +9.016 3.6 0.65 5.5 0.0 0.00 0.0 GX 9+1 270.396 -20.545 0.0 9.068 +1.136 2.1 0.00 5.0 0.0 0.00 0.0 Swift J174535.5-2901 266.308 -29.089 0.0 359.825 -0.007 1.1 0.00 4.3 0.0 0.00 0.0 GRS 1734-292 264.429 -29.147 6.7 358.909 +1.355 1.0 0.27 3.6 0.0 0.00 0.0 H 1705-440 257.112 -44.147 5.1 343.235 -2.303 16.8 3.47 4.8 0.0 0.00 0.0 NEW_1 268.703 -20.633 3.9 8.200 +2.466 2.5 0.39 6.5 0.0 0.00 0.0JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.Note: Sources labelled were detected with in the 3-10 keV image > 10σ and are listed in the table below. Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the source position is done), with
mosaic_spec
, in two bands: A = 3-10 keV (1 Crab ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).NOTES: Fluxes for light curves are extracted from the images using
mosaic_spec
; The object marked as SLX 1744-299_300 is used to indicate two low-mass x-ray binaries separated by 2.7 arcminutes, SLX 1744-299 and SLX 1744-300; the position for SLX 1744-299 is used, although it can not be ruled out that SLX 1744-300 may dominate the emission some of the time.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).Source Name RA dec l b A(cps) +/- B(cps) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== XTE J1739-285 264.975 -28.496 359.714 +1.298 7.0 0.40 1.2 0.23 GX 354-0 262.989 -33.835 354.302 -0.150 27.9 1.67 5.4 0.97 GX 3+1 266.983 -26.564 2.294 +0.794 21.4 0.54 2.8 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 113.0 2.30 17.2 1.03
Go back to Bulge home page