INTEGRAL Galactic bulge Monitoring
Revolution 0537: Observation start 2007-03-07T13:37 = MJD 54166.568
Total Observation GTI = 23939 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 1700-377 255.982 -37.846 0.4 347.751 +2.176 56.4 0.52 109.2 16.7 0.38 43.5 GX 354-0 262.990 -33.833 0.4 354.304 -0.150 26.7 0.27 98.2 9.1 0.21 42.5 GX 1+4 263.008 -24.749 0.5 1.934 +4.794 22.1 0.29 76.7 0.0 0.00 0.0 1E 1740.7-2942 265.986 -29.750 0.8 359.116 -0.114 10.8 0.26 41.3 6.6 0.22 30.8 GRS 1758-258 270.308 -25.742 0.8 4.512 -1.365 11.0 0.27 41.0 7.1 0.21 33.5 Ginga 1826-24 277.356 -23.800 0.9 9.265 -6.080 17.0 0.45 38.2 7.1 0.34 21.1 H 1820-303 275.929 -30.372 1.0 2.782 -7.927 10.4 0.35 29.7 0.0 0.00 0.0 GX 349+2 256.445 -36.419 1.4 349.111 +2.744 9.8 0.47 20.9 0.0 0.00 0.0 GX 5-1 270.281 -25.091 1.4 5.066 -1.021 5.7 0.27 21.2 0.0 0.00 0.0 GRS 1741.9-2853 266.332 -28.937 2.1 359.966 +0.054 3.4 0.26 13.2 1.8 0.21 8.3 1A 1742-294 266.505 -29.499 2.0 359.565 -0.368 3.5 0.26 13.7 0.8 0.21 3.6 3A 1822-371 276.436 -37.096 1.8 356.856 -11.280 6.9 0.46 15.0 0.0 0.00 0.0 4U 1722-30 261.896 -30.787 1.9 356.336 +2.301 4.0 0.28 14.3 2.2 0.22 9.8 GX 3+1 267.006 -26.539 2.2 2.325 +0.789 3.2 0.25 12.5 0.0 0.00 0.0 GX 9+1 270.399 -20.559 2.3 9.058 +1.128 4.3 0.37 11.6 0.0 0.00 0.0 OAO 1657-415 255.171 -41.656 2.9 344.354 +0.339 8.9 1.00 8.9 0.0 0.00 0.0 SLX 1744-299_300 266.860 -30.044 4.1 359.259 -0.914 1.6 0.26 6.1 0.0 0.00 0.0 H 1702-429 256.439 -43.059 3.7 343.813 -1.260 9.1 1.30 7.0 0.0 0.00 0.0 SLX 1735-269 264.580 -26.980 3.8 0.812 +2.401 1.8 0.26 6.7 1.3 0.21 5.9 SLX 1737-282 265.187 -28.267 4.9 0.007 +1.262 1.3 0.26 5.0 0.0 0.00 0.0 GRS 1734-292 264.369 -29.142 4.9 358.885 +1.403 1.4 0.27 5.1 0.0 0.00 0.0 Swift J1753.7-2544 268.550 -25.799 5.7 3.670 -0.023 1.1 0.26 4.3 0.0 0.00 0.0 4U 1735-444 264.864 -44.486 5.5 346.069 -7.086 7.5 1.68 4.5 0.0 0.00 0.0 1A 1743-288 266.726 -28.766 0.0 0.292 -0.152 1.0 0.00 4.1 0.0 0.00 0.0 XB 1832-330 278.915 -32.939 6.1 1.573 -11.335 1.9 0.47 4.0 0.0 0.00 0.0 IGR J17475-2822 266.820 -28.437 0.0 0.616 -0.051 1.0 0.00 4.0 0.0 0.00 0.0 GX 17+2 274.037 -14.021 5.4 16.460 +1.258 12.3 2.71 4.5 0.0 0.00 0.0 Swift J165534.1-4426 253.798 -44.486 6.4 341.514 -0.636 16.0 0.00 3.8 0.0 0.00 0.0 RX J1718.4-4029 259.636 -40.417 6.0 347.354 -1.630 2.3 0.57 4.1 0.0 0.00 0.0 AX J1820.5-1434 275.138 -14.531 6.7 16.516 +0.077 6.5 1.80 3.6 0.0 0.00 0.0 1H 1746-370 267.548 -37.021 7.9 353.556 -4.986 1.0 0.34 3.0 0.0 0.00 0.0 IGR J18027-2016 270.660 -20.223 8.1 9.470 +1.080 1.1 0.38 2.9 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 1.5 0.23 6.4 0.6 0.14 4.3 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.4 0.23 10.5 1.4 0.14 10.2 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.24 3.2 0.3 0.14 2.2 4U 1722-30 261.888 -30.802 356.320 +2.298 1.7 0.40 4.2 0.8 0.30 2.8 GRS 1734-292 264.367 -29.142 358.883 +1.404 0.8 0.24 3.2 0.4 0.15 2.4 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 1.4 0.24 5.8 0.5 0.14 3.3 GX 3+1 266.983 -26.561 2.296 +0.795 35.5 0.41 85.9 3.8 0.20 18.5 GX 354-0 262.996 -33.847 354.295 -0.162 11.0 0.82 13.4 3.5 0.65 5.4 GX 5-1 270.286 -25.072 5.084 -1.016 102.4 1.50 68.3 8.8 0.65 13.6 SLX 1737-282 265.163 -28.297 359.971 +1.264 1.0 0.25 4.1 0.0 0.00 0.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.9 0.23 12.4 0.6 0.14 4.6 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.7 0.23 3.2 0.2 0.13 1.8 NEW SOURCE 270.090 -26.655 3.621 -1.648 2.9 0.63 4.7 0.0 0.00 0.0 NEW SOURCE 270.552 -26.046 4.356 -1.706 3.2 0.87 3.7 0.0 0.00 0.0 NEW SOURCE 271.979 -28.046 3.229 -3.791 3.2 0.75 4.3 0.0 0.00 0.0