INTEGRAL Galactic bulge Monitoring
Revolution 0602: Observation start 2007-09-18T00:57 = MJD 54361.04
Total Observation GTI = 9350 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 1700-377 255.987 -37.850 0.4 347.750 +2.170 118.3 0.96 122.9 29.4 0.73 40.4 GX 5-1 270.282 -25.074 1.1 5.080 -1.014 11.6 0.41 28.1 0.0 0.00 0.0 GX 1+4 263.000 -24.740 1.0 1.937 +4.805 11.6 0.39 30.0 0.0 0.00 0.0 Ginga 1826-24 277.372 -23.799 1.0 9.272 -6.092 21.6 0.72 30.1 7.0 0.56 12.6 SAX J1810.8-2609 272.708 -26.152 1.3 5.206 -3.450 9.8 0.44 22.2 4.6 0.35 13.0 GX 349+2 256.426 -36.427 1.6 349.095 +2.752 14.3 0.82 17.5 0.0 0.00 0.0 GRS 1758-258 270.292 -25.741 2.5 4.506 -1.352 4.6 0.42 10.8 2.2 0.35 6.3 GX 9+1 270.416 -20.497 2.8 9.119 +1.144 5.5 0.59 9.4 0.0 0.00 0.0 GX 3+1 266.989 -26.577 2.7 2.285 +0.782 4.1 0.41 9.9 0.0 0.00 0.0 OAO 1657-415 255.232 -41.616 2.5 344.413 +0.327 21.0 1.99 10.6 0.0 0.00 0.0 H 1820-303 275.882 -30.359 3.4 2.776 -7.884 4.7 0.62 7.5 0.0 0.00 0.0 3A 1822-371 276.436 -37.068 3.5 356.881 -11.268 5.6 0.77 7.3 0.0 0.00 0.0 3A 1728-169 262.958 -16.950 0.0 8.535 +9.025 5.3 0.00 6.7 0.0 0.00 0.0 4U 1722-30 261.862 -30.858 4.4 356.261 +2.286 2.7 0.49 5.6 0.0 0.00 0.0 SLX 1735-269 264.554 -26.975 5.9 0.804 +2.424 1.8 0.44 4.2 0.0 0.00 0.0 IGR J17091-3624 257.315 -36.318 4.9 349.613 +2.245 3.7 0.73 5.1 0.0 0.00 0.0 SAX J1712.6-3739 258.187 -37.691 4.4 348.917 +0.870 4.1 0.73 5.7 0.0 0.00 0.0 GRS 1741.9-2853 266.307 -28.968 0.0 359.928 +0.057 1.7 0.00 4.7 0.0 0.00 0.0 XTE J1752-223 268.077 -22.246 0.0 6.513 +2.152 1.9 0.00 4.3 0.0 0.00 0.0 GX 354-0 262.979 -33.893 4.8 354.249 -0.175 2.2 0.43 5.2 0.0 0.00 0.0 H 1702-429 256.530 -43.079 5.0 343.837 -1.325 17.6 3.52 5.0 0.0 0.00 0.0 Swift J175648.6-2544 269.147 -25.699 6.7 4.027 -0.438 1.4 0.38 3.6 0.0 0.00 0.0 Swift J1749.4-2807 267.520 -28.141 6.2 1.187 -0.427 1.4 0.00 3.9 0.0 0.00 0.0 V2400 Oph 258.164 -24.311 6.2 359.819 +8.693 2.0 0.00 3.9 0.0 0.00 0.0 AX J1820.5-1434 275.075 -14.654 6.8 16.379 +0.072 7.5 2.13 3.5 0.0 0.00 0.0 Swift J173203.1-3445 262.941 -34.843 5.6 353.437 -0.668 2.2 0.51 4.4 0.0 0.00 0.0 XB 1832-330 278.893 -32.946 6.2 1.558 -11.322 3.1 0.78 3.9 0.0 0.00 0.0 2E 1829.0-2913 278.010 -29.109 5.4 4.740 -8.980 3.0 0.66 4.5 0.0 0.00 0.0 IGR J17488-3253 267.250 -33.007 7.1 356.890 -2.727 1.2 0.37 3.4 0.0 0.00 0.0 IGR J17597-2201 269.919 -21.974 6.7 7.606 +0.814 1.7 0.00 3.6 0.0 0.00 0.0 IGR J17541-2252 268.557 -22.935 7.0 6.144 +1.420 1.6 0.48 3.4 0.0 0.00 0.0 IGR J17375-3022 264.307 -30.435 6.0 357.764 +0.755 1.7 0.41 4.0 0.0 0.00 0.0 NEW SOURCE 259.877 -31.910 4.2 354.435 +3.093 2.7 0.45 6.0 0.0 0.00 0.0 NEW SOURCE 272.037 -21.697 3.9 8.815 -0.763 3.2 0.50 6.5 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 1742-294 266.514 -29.512 359.557 -0.381 4.8 0.33 14.6 0.6 0.19 3.3 GRS 1758-258 270.303 -25.741 4.511 -1.361 5.1 1.47 3.5 0.8 0.77 1.0 GX 3+1 266.984 -26.570 2.289 +0.790 40.6 0.54 74.9 4.3 0.26 16.2 GX 354-0 262.989 -33.835 354.302 -0.150 12.6 1.68 7.5 0.0 0.00 0.0 GX 5-1 270.287 -25.073 5.084 -1.018 86.3 2.97 29.0 6.0 1.31 4.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.0 0.32 3.2 0.4 0.20 1.9 NEW SOURCE 266.338 -28.864 0.031 +0.088 1.7 0.33 5.1 0.0 0.00 0.0 NEW SOURCE 270.285 -29.672 1.081 -3.289 2.6 0.51 5.1 0.0 0.00 0.0 NEW SOURCE 267.987 -23.570 5.331 +1.550 9.4 2.14 4.4 0.0 0.00 0.0