INTEGRAL Galactic bulge Monitoring
Revolution 0362: Observation start 2005-09-30T09:14 = MJD 53643.385
Total Observation GTI = 11774 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 1700-377 255.979 -37.854 0.7 347.743 +2.172 35.9 0.71 50.8 9.6 0.54 17.7 GX 5-1 270.288 -25.077 0.7 5.081 -1.020 15.7 0.32 49.5 0.0 0.00 0.0 GRS 1758-258 270.312 -25.744 0.8 4.511 -1.370 13.5 0.34 39.3 8.6 0.28 30.8 Ginga 1826-24 277.374 -23.797 1.0 9.275 -6.093 17.4 0.54 32.1 6.9 0.42 16.3 1E 1740.7-2942 265.989 -29.744 1.1 359.121 -0.113 9.4 0.32 28.9 5.1 0.27 18.7 GX 1+4 263.005 -24.751 1.2 1.931 +4.795 8.3 0.32 25.6 0.0 0.00 0.0 GX 349+2 256.422 -36.409 1.4 349.108 +2.766 12.3 0.57 21.3 0.0 0.00 0.0 H 1820-303 275.938 -30.357 1.7 2.800 -7.927 8.2 0.49 16.8 0.0 0.00 0.0 GX 354-0 262.967 -33.822 1.7 354.303 -0.128 6.2 0.37 16.8 0.0 0.00 0.0 XTE J1739-285 264.976 -28.497 2.2 359.714 +1.297 3.7 0.31 12.1 1.5 0.26 5.8 3A 1822-371 276.441 -37.089 2.4 356.864 -11.281 7.1 0.63 11.2 0.0 0.00 0.0 GX 9+1 270.395 -20.524 4.1 9.086 +1.148 2.9 0.47 6.1 0.0 0.00 0.0 GX 3+1 267.030 -26.554 3.8 2.324 +0.763 2.1 0.31 6.6 0.0 0.00 0.0 SLX 1735-269 264.587 -26.885 5.4 0.896 +2.446 1.3 0.29 4.5 0.9 0.24 3.8 KS 1741-293 266.211 -29.335 0.0 359.571 -0.064 1.7 0.00 5.9 0.0 0.00 0.0 OAO 1657-415 255.098 -41.619 3.8 344.349 +0.404 9.9 1.46 6.8 0.0 0.00 0.0 SLX 1744-299_300 266.798 -30.050 5.0 359.226 -0.871 1.7 0.34 4.9 0.0 0.00 0.0 GRS 1734-292 264.376 -29.098 4.2 358.924 +1.421 1.7 0.29 6.0 0.0 0.00 0.0 IGR J18179-1621 274.576 -16.374 6.2 14.636 -0.317 4.1 1.04 3.9 0.0 0.00 0.0 XTE J1710-281 257.575 -28.227 5.5 356.291 +6.849 1.8 0.00 4.4 0.0 0.00 0.0 3A 1728-169 262.941 -16.995 6.3 8.488 +9.015 2.6 0.66 3.9 0.0 0.00 0.0 MAXI J1828-249 277.264 -25.070 6.4 8.088 -6.581 2.0 0.51 3.8 0.0 0.00 0.0 1E 1742.9-2849 266.494 -28.842 0.0 0.121 -0.017 1.2 0.00 4.2 0.0 0.00 0.0 IGR J18027-2016 270.734 -20.376 0.0 9.372 +0.945 1.9 0.00 4.0 0.0 0.00 0.0 IGR J17354-3255 263.964 -32.875 5.5 355.550 -0.312 1.4 0.30 4.5 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 4.2 0.27 15.6 0.8 0.15 5.2 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.27 7.8 0.9 0.15 5.9 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.27 3.2 0.2 0.15 1.3 4U 1722-30 261.888 -30.802 356.320 +2.298 6.0 0.59 10.2 1.2 0.39 3.1 GRS 1747-312 267.690 -31.292 358.555 -2.168 1.1 0.31 3.7 0.0 0.00 0.0 GX 3+1 266.964 -26.568 2.282 +0.806 22.5 0.42 53.3 2.4 0.21 11.7 GX 354-0 263.003 -33.843 354.301 -0.165 18.2 1.21 15.0 3.8 0.83 4.5 GX 5-1 270.278 -25.075 5.078 -1.012 130.3 1.84 71.0 14.4 0.75 19.2 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.8 0.35 5.3 0.3 0.20 1.7 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.0 0.27 7.5 0.4 0.15 2.9 XTE J1739-285 264.975 -28.496 359.714 +1.298 1.4 0.28 5.1 0.6 0.16 3.6 NEW SOURCE 272.775 -26.228 5.167 -3.539 16.9 2.94 5.7 2.0 1.45 1.4 NEW SOURCE 271.172 -26.115 4.570 -2.225 6.3 1.24 5.1 0.0 0.00 0.0 NEW SOURCE 268.247 -25.096 4.137 +0.569 3.5 0.77 4.5 0.0 0.00 0.0 NEW SOURCE 267.491 -24.221 4.539 +1.607 4.5 1.00 4.5 0.0 0.00 0.0 IGR J17419-2802 265.498 -28.036 0.348 +1.150 0.9 0.29 3.1 0.5 0.16 3.2