INTEGRAL Galactic bulge Monitoring
Revolution 0721: Observation start 2008-09-10T09:42 = MJD 54719.405
Total Observation GTI = 12379 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 1700-377 255.992 -37.840 0.8 347.760 +2.173 31.9 0.74 43.0 7.0 0.56 12.4 GX 354-0 262.996 -33.836 0.8 354.305 -0.155 16.5 0.42 39.4 4.5 0.33 13.7 GX 5-1 270.284 -25.077 1.0 5.079 -1.018 13.1 0.42 31.3 0.0 0.00 0.0 IGR J17473-2721 266.831 -27.345 1.0 1.555 +0.506 9.8 0.31 31.3 5.0 0.26 19.2 GRS 1758-258 270.306 -25.742 1.1 4.511 -1.364 11.5 0.42 27.7 7.7 0.33 23.2 H 1820-303 275.917 -30.360 1.1 2.789 -7.912 13.1 0.48 27.3 0.0 0.00 0.0 Ginga 1826-24 277.352 -23.794 1.2 9.269 -6.074 15.8 0.64 24.6 6.9 0.49 14.2 1E 1740.7-2942 265.964 -29.761 1.3 359.096 -0.103 7.4 0.32 23.0 5.2 0.26 19.5 OAO 1657-415 255.187 -41.660 1.6 344.358 +0.327 27.6 1.61 17.2 6.8 1.23 5.5 GX 1+4 262.994 -24.756 1.8 1.921 +4.800 6.9 0.44 15.6 0.0 0.00 0.0 4U 1722-30 261.871 -30.817 2.0 356.299 +2.302 5.2 0.37 13.8 1.5 0.00 5.1 GX 349+2 256.436 -36.442 2.1 349.088 +2.736 8.2 0.64 12.9 0.0 0.00 0.0 GX 3+1 266.989 -26.550 2.1 2.308 +0.796 4.2 0.33 12.7 0.0 0.00 0.0 GX 9+1 270.424 -20.503 3.7 9.118 +1.134 3.5 0.51 6.9 0.0 0.00 0.0 3A 1822-371 276.471 -37.060 3.7 356.901 -11.290 4.5 0.64 6.9 0.0 0.00 0.0 H 1702-429 256.581 -43.024 4.5 343.904 -1.321 12.8 2.30 5.6 0.0 0.00 0.0 GX 17+2 273.984 -14.022 4.0 16.435 +1.303 21.2 3.39 6.3 0.0 0.00 0.0 IGR J17454-2919 266.477 -29.358 5.0 359.672 -0.273 1.5 0.31 4.9 0.0 0.00 0.0 GRS 1747-312 267.638 -31.287 4.7 358.537 -2.128 1.8 0.35 5.3 0.0 0.00 0.0 IGR J17488-3253 267.156 -32.967 5.3 356.884 -2.638 1.7 0.37 4.7 0.0 0.00 0.0 SLX 1735-269 264.556 -26.966 5.2 0.813 +2.427 1.7 0.35 4.8 0.0 0.00 0.0 IGR J17195-4100 259.898 -40.933 5.7 347.046 -2.089 3.8 0.88 4.3 0.0 0.00 0.0 IGR J17445-2747 266.024 -27.844 6.0 0.756 +0.856 1.3 0.00 4.1 0.0 0.00 0.0 XTE J1743-363 265.788 -36.441 6.0 353.326 -3.478 1.9 0.00 4.1 0.0 0.00 0.0 MXB 1730-335 263.352 -33.394 0.0 354.836 -0.163 1.6 0.00 4.0 0.0 0.00 0.0 GRO J1655-40 253.453 -39.856 5.5 344.951 +2.478 5.3 1.20 4.5 0.0 0.00 0.0 IGR J16493-4348 252.257 -43.854 5.7 341.300 +0.619 29.3 6.85 4.3 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 5.5 0.32 17.1 0.7 0.20 3.5 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.3 0.32 4.0 1.0 0.21 4.9 4U 1722-30 261.888 -30.802 356.320 +2.298 2.9 0.66 4.4 1.3 0.51 2.5 GX 3+1 266.983 -26.566 2.291 +0.793 45.5 0.67 67.5 4.5 0.36 12.6 GX 354-0 262.989 -33.835 354.302 -0.150 11.8 1.20 9.8 4.0 1.00 4.0 GX 5-1 270.275 -25.080 5.073 -1.012 122.0 2.55 47.9 15.5 1.17 13.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.3 0.32 10.3 0.8 0.20 3.9 IGR J17473-2721 266.821 -27.343 1.552 +0.515 3.6 0.46 7.9 1.4 0.28 4.8 NEW SOURCE 271.893 -27.229 3.909 -3.330 6.2 1.26 4.9 0.0 0.00 0.0 NEW SOURCE 270.603 -24.192 5.991 -0.832 17.3 3.81 4.5 0.0 0.00 0.0 NEW SOURCE 269.867 -24.638 5.272 -0.471 11.6 2.53 4.6 0.0 0.00 0.0 NEW SOURCE 268.918 -23.489 5.833 +0.855 20.6 4.26 4.8 0.0 0.00 0.0 NEW SOURCE 271.065 -25.742 4.848 -1.959 8.8 2.01 4.4 1.2 0.99 1.2