INTEGRAL Galactic bulge Monitoring
Revolution 0530: Observation start 2007-02-15T18:34 = MJD 54146.774
Total Observation GTI = 13253 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 354-0 262.991 -33.832 0.6 354.306 -0.150 25.5 0.36 69.8 7.5 0.29 25.7 4U 1700-377 255.986 -37.845 0.6 347.753 +2.173 38.1 0.66 57.8 10.2 0.50 20.4 GX 1+4 263.012 -24.747 0.8 1.937 +4.792 15.4 0.35 43.8 0.0 0.00 0.0 GRS 1758-258 270.302 -25.752 0.9 4.500 -1.365 12.8 0.36 35.8 7.9 0.29 27.7 1E 1740.7-2942 265.985 -29.746 1.0 359.118 -0.111 10.0 0.31 32.4 6.6 0.26 25.5 Ginga 1826-24 277.363 -23.793 1.1 9.274 -6.082 16.4 0.59 27.7 6.9 0.46 15.0 GX 349+2 256.436 -36.424 1.5 349.104 +2.747 10.5 0.55 19.2 0.0 0.00 0.0 H 1820-303 275.912 -30.374 1.8 2.774 -7.915 7.3 0.46 15.8 0.0 0.00 0.0 GX 5-1 270.287 -25.070 2.2 5.086 -1.016 4.1 0.34 12.0 0.0 0.00 0.0 3A 1822-371 276.446 -37.098 2.2 356.857 -11.289 7.0 0.58 12.2 0.0 0.00 0.0 GX 3+1 266.951 -26.564 2.6 2.278 +0.818 3.2 0.32 10.1 0.0 0.00 0.0 GX 17+2 273.996 -14.037 2.8 16.427 +1.285 22.7 2.43 9.3 0.0 0.00 0.0 4U 1722-30 261.892 -30.812 2.7 356.313 +2.290 3.3 0.34 9.8 1.7 0.27 6.0 GX 9+1 270.384 -20.525 3.2 9.079 +1.156 3.8 0.47 8.0 0.0 0.00 0.0 1E 1742.8-2853 266.390 -28.893 3.6 0.030 +0.034 2.2 0.31 7.0 0.0 0.00 0.0 IGR J17252-3616 261.332 -36.282 3.7 351.513 -0.377 2.9 0.43 6.9 0.0 0.00 0.0 SLX 1744-299_300 266.877 -29.994 0.0 359.310 -0.900 2.1 0.00 6.8 1.0 0.26 4.0 SLX 1735-269 264.541 -26.993 3.8 0.783 +2.424 2.2 0.33 6.6 1.3 0.27 4.8 SAX J1712.6-3739 258.237 -37.557 5.6 349.049 +0.917 2.5 0.56 4.4 0.0 0.00 0.0 H 1702-429 256.526 -43.072 5.4 343.841 -1.318 8.2 1.79 4.6 0.0 0.00 0.0 IGR J18135-1751 273.432 -17.889 5.8 12.783 -0.076 3.0 0.73 4.2 0.0 0.00 0.0 IGR J18173-2509 274.261 -25.182 0.0 6.727 -4.221 1.9 0.00 4.2 0.0 0.00 0.0 GRS 1734-292 264.312 -29.148 6.5 358.853 +1.441 1.1 0.31 3.7 0.0 0.00 0.0 GRS 1747-312 267.651 -31.222 0.0 358.599 -2.103 1.2 0.00 3.9 0.0 0.00 0.0 IGR J17407-2808 265.067 -28.206 6.4 0.004 +1.383 1.2 0.32 3.8 0.0 0.00 0.0 3A 1728-169 262.935 -16.939 7.1 8.532 +9.049 2.8 0.83 3.4 0.0 0.00 0.0 XB 1733-30 264.063 -30.425 6.3 357.659 +0.937 1.3 0.33 3.8 0.0 0.00 0.0 XTE J1710-281 257.562 -28.141 6.8 356.356 +6.909 1.5 0.42 3.5 0.0 0.00 0.0 4U 1708-40 258.016 -40.934 7.3 346.218 -0.932 3.4 0.00 3.3 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 1742-294 266.505 -29.523 359.544 -0.380 2.9 0.25 11.4 0.6 0.16 3.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.1 0.25 4.5 1.1 0.17 6.8 4U 1722-30 261.888 -30.802 356.320 +2.298 4.9 0.48 10.3 1.1 0.36 3.1 GX 1+4 263.009 -24.746 1.937 +4.795 3.5 0.94 3.8 2.5 0.65 3.8 GX 3+1 266.983 -26.561 2.295 +0.795 38.7 0.45 86.0 4.1 0.24 17.6 GX 354-0 262.993 -33.825 354.312 -0.147 11.9 0.88 13.4 4.8 0.77 6.2 GX 5-1 270.284 -25.079 5.077 -1.019 89.3 1.87 47.8 7.0 0.82 8.5 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.5 0.25 6.0 0.5 0.17 3.1 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.7 0.26 6.6 0.0 0.00 0.0 NEW SOURCE 269.285 -23.394 6.084 +0.611 11.9 2.49 4.8 0.0 0.00 0.0 NEW SOURCE 268.460 -23.432 5.669 +1.246 9.1 1.90 4.8 0.0 0.00 0.0 NEW SOURCE 272.804 -26.099 5.294 -3.500 15.9 3.44 4.6 0.0 0.00 0.0 NEW SOURCE 266.885 -23.188 5.140 +2.614 8.5 1.75 4.9 0.0 0.00 0.0 NEW SOURCE 271.177 -24.265 6.185 -1.324 16.5 4.00 4.1 0.0 0.00 0.0