INTEGRAL Galactic bulge Monitoring
Revolution 0595: Observation start 2007-08-28T02:31 = MJD 54340.106
Total Observation GTI = 10855 seconds
IBIS/ISGRI
IBIS/ISGRI significance mosaic images. Left: IBIS/ISGRI 18-40 keV. Right: 40-100 keV
Sources 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
OSA10.1, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 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 and NEW SOURCEs < 6σ towards the border of the image may be spurious. IBIS/ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)
Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.986 -37.844 0.4 347.754 +2.174 86.2 0.85 101.4 23.8 0.64 37.4 GX 5-1 270.283 -25.075 0.9 5.080 -1.016 15.5 0.41 38.1 0.0 0.00 0.0 Ginga 1826-24 277.371 -23.795 1.1 9.276 -6.089 19.8 0.68 29.0 7.3 0.52 14.0 GX 1+4 263.007 -24.738 1.1 1.942 +4.801 12.3 0.43 28.4 0.0 0.00 0.0 H 1820-303 275.899 -30.363 1.4 2.778 -7.899 10.4 0.51 20.4 0.0 0.00 0.0 GX 354-0 262.988 -33.840 2.1 354.298 -0.152 5.4 0.42 13.0 0.0 0.00 0.0 GRS 1758-258 270.324 -25.757 2.2 4.506 -1.385 4.8 0.39 12.3 2.9 0.31 9.2 GX 349+2 256.411 -36.420 2.2 349.094 +2.766 9.0 0.71 12.6 0.0 0.00 0.0 GX 3+1 266.961 -26.549 2.5 2.296 +0.818 3.9 0.37 10.5 0.0 0.00 0.0 3A 1822-371 276.437 -37.099 2.6 356.853 -11.282 7.2 0.70 10.2 0.0 0.00 0.0 GX 9+1 270.401 -20.516 2.7 9.095 +1.147 4.9 0.51 9.6 0.0 0.00 0.0 4U 1722-30 261.898 -30.792 3.1 356.333 +2.297 3.3 0.40 8.3 1.7 0.32 5.4 OAO 1657-415 255.211 -41.671 3.3 344.360 +0.306 17.5 2.21 7.9 0.0 0.00 0.0 SLX 1735-269 264.503 -26.988 4.5 0.769 +2.455 2.2 0.39 5.6 0.0 0.00 0.0 SLX 1744-299_300 266.831 -29.977 5.1 359.303 -0.858 1.7 0.35 4.9 0.0 0.00 0.0 1E 1742.9-2849 266.533 -28.850 5.2 0.132 -0.051 1.7 0.35 4.7 0.0 0.00 0.0 3A 1728-169 262.980 -16.986 5.6 8.516 +8.988 3.5 0.79 4.4 0.0 0.00 0.0 GX 13+1 273.635 -17.193 0.0 13.486 +0.086 4.2 0.00 4.5 0.0 0.00 0.0 H 1702-429 256.521 -43.071 5.5 343.839 -1.315 12.4 0.00 4.5 0.0 0.00 0.0 SAX J1810.8-2609 272.731 -26.154 5.2 5.213 -3.469 2.2 0.46 4.7 2.2 0.36 6.3 IGR J17091-3624 257.241 -36.421 5.5 349.494 +2.231 3.0 0.67 4.5 0.0 0.00 0.0 IGR J17454-2919 266.345 -29.332 5.3 359.635 -0.162 1.6 0.35 4.6 0.0 0.00 0.0 SAX J1712.6-3739 258.101 -37.617 6.0 348.937 +0.969 2.8 0.69 4.1 2.6 0.53 4.9 H1825-331 277.118 -33.146 6.5 0.722 -10.065 2.2 0.00 3.8 0.0 0.00 0.0 SLX 1737-282 265.198 -28.265 0.0 0.015 +1.255 1.4 0.00 3.8 0.0 0.00 0.0 Oph Cluster 258.154 -23.433 5.9 0.541 +9.205 2.1 0.51 4.1 0.0 0.00 0.0 GX 17+2 274.030 -14.053 5.8 16.429 +1.249 10.1 2.38 4.2 0.0 0.00 0.0 XTE J1709-267 257.438 -26.752 0.0 357.426 +7.811 1.7 0.00 3.5 0.0 0.00 0.0
JEM-X
JEM-X1 significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.
Sources labelled were detected in the 3-10 keV image > 6σ. The sources detected above 3σ in the 3-10 keV and/or 10-25 keV band 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 ~ 97 cps [J1], 103 cps [J2]); B = 10-25 keV (1 Crab ~ 29 cps [J1], 27 cps [J2]). NOTES: 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. The systematic noise increases towards the edge of the field of view and in the vicinity of very bright sources, such as GX 5-1;
NEW SOURCEs < 6σ towards the border of the image and/or near GX 5-1 may, therefore, be spurious.
JEM-X1 Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 4.7 0.33 14.2 1.0 0.20 5.1 GX 3+1 266.978 -26.565 2.290 +0.797 41.9 0.57 74.2 4.7 0.27 17.3 GX 354-0 262.989 -33.835 354.302 -0.150 8.4 1.23 6.9 1.9 1.01 1.9 GX 5-1 270.275 -25.083 5.070 -1.013 116.5 2.10 55.6 14.8 0.94 15.8 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.3 0.32 4.1 0.0 0.00 0.0 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.0 0.34 3.1 0.3 0.20 1.7 NEW SOURCE 270.225 -24.052 5.943 -0.462 14.1 2.90 4.9 2.2 1.53 1.4 NEW SOURCE 270.297 -24.772 5.349 -0.877 9.8 2.10 4.6 0.0 0.00 0.0 NEW SOURCE 272.483 -26.901 4.450 -3.632 8.8 1.93 4.6 0.0 0.00 0.0 NEW SOURCE 270.092 -24.619 5.390 -0.638 10.2 2.15 4.7 1.1 1.03 1.1