INTEGRAL Galactic bulge Monitoring
Revolution 0667: Observation start 2008-04-01T16:55 = MJD 54557.706
Total Observation GTI = 11516 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.294 -26.647 0.6 2.365 +0.513 19.5 0.35 55.5 0.0 0.00 0.0 4U 1700-377 255.986 -37.846 0.7 347.753 +2.173 38.6 0.78 49.5 10.1 0.58 17.5 GX 354-0 262.995 -33.830 0.8 354.308 -0.151 15.8 0.36 43.8 5.4 0.29 18.8 Ginga 1826-24 277.375 -23.800 1.1 9.273 -6.095 19.1 0.67 28.4 7.6 0.49 15.4 H 1820-303 275.917 -30.366 1.1 2.783 -7.914 12.5 0.47 26.6 0.0 0.00 0.0 4U 1722-30 261.890 -30.793 1.2 356.328 +2.302 10.3 0.42 24.6 3.2 0.32 9.9 IGR J17473-2721 266.822 -27.348 1.2 1.548 +0.511 8.4 0.35 23.9 4.2 0.29 14.8 GRS 1758-258 270.304 -25.741 1.6 4.510 -1.362 7.3 0.41 17.9 4.0 0.32 12.4 1E 1740.7-2942 265.966 -29.744 1.9 359.111 -0.096 5.3 0.36 14.5 2.8 0.30 9.5 XTE J1810-189 272.548 -19.066 2.0 11.348 +0.092 9.9 0.72 13.8 3.7 0.54 6.9 GX 3+1 266.939 -26.540 0.0 2.293 +0.840 4.0 0.00 11.4 0.0 0.00 0.0 GX 349+2 256.450 -36.402 2.3 349.127 +2.751 7.8 0.68 11.5 0.0 0.00 0.0 3A 1822-371 276.455 -37.089 2.9 356.869 -11.291 5.5 0.61 9.0 0.0 0.00 0.0 GX 9+1 270.404 -20.537 3.1 9.079 +1.134 4.9 0.60 8.2 0.0 0.00 0.0 SLX 1735-269 264.591 -26.981 3.6 0.817 +2.392 2.5 0.36 7.0 1.3 0.29 4.7 SAX J1750.8-2900 267.611 -29.090 4.2 0.413 -0.982 2.2 0.37 6.0 1.4 0.30 4.6 GX 5-1 270.295 -25.085 4.7 5.078 -1.030 2.1 0.40 5.3 0.0 0.00 0.0 OAO 1657-415 255.149 -41.626 4.9 344.367 +0.370 7.2 1.42 5.1 0.0 0.00 0.0 Swift J174510.8-2624 266.297 -26.375 0.0 2.136 +1.417 1.7 0.00 4.6 0.0 0.00 0.0 GRS 1734-292 264.394 -29.144 5.5 358.895 +1.383 1.8 0.00 4.4 0.0 0.00 0.0 XTE J1709-267 257.351 -26.671 5.1 357.446 +7.921 2.6 0.54 4.9 0.0 0.00 0.0 PKS 1830-211 278.515 -21.001 5.0 12.261 -5.767 4.5 0.92 4.9 0.0 0.00 0.0 IGR J17448-3232 266.154 -32.456 6.0 356.884 -1.652 1.5 0.00 4.1 0.0 0.00 0.0 1A 1744-361 267.031 -36.059 0.0 354.173 -4.138 1.7 0.00 4.0 0.0 0.00 0.0 Swift J1753.7-2544 268.398 -25.797 0.0 3.602 +0.096 1.5 0.00 3.9 0.0 0.00 0.0 4U 1735-444 264.796 -44.542 6.5 345.995 -7.074 6.1 0.00 3.7 0.0 0.00 0.0 1E 1742.8-2853 266.509 -28.972 7.1 0.017 -0.096 1.2 0.35 3.4 0.0 0.00 0.0 GX 1+4 263.059 -24.712 6.2 1.990 +4.775 1.5 0.39 3.9 0.0 0.00 0.0 IGR J18173-2509 274.406 -25.182 6.4 6.789 -4.337 1.9 0.50 3.8 0.0 0.00 0.0 IGR J17464-2811 266.751 -28.265 0.0 0.731 +0.090 1.1 0.00 3.4 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 1742-294 266.513 -29.509 359.560 -0.379 4.8 0.26 18.3 0.8 0.18 4.4 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 0.8 0.27 2.8 0.6 0.18 3.1 4U 1722-30 261.888 -30.802 356.320 +2.298 3.9 0.52 7.6 1.6 0.44 3.7 GRO J1750-27 267.307 -26.643 2.375 +0.505 7.6 0.52 14.6 6.2 0.33 18.8 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.1 0.25 8.1 0.5 0.18 2.7 GX 3+1 266.984 -26.558 2.299 +0.796 42.3 0.60 70.6 4.9 0.33 14.5 GX 354-0 262.983 -33.825 354.307 -0.140 6.9 0.75 9.2 2.8 0.64 4.4 GX 5-1 270.283 -25.080 5.076 -1.018 102.4 2.21 46.3 5.6 1.18 4.8 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.6 0.26 10.1 0.4 0.17 2.4 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.0 0.28 3.8 0.3 0.18 1.5 IGR J17473-2721 266.817 -27.347 1.546 +0.515 2.5 0.40 6.2 1.3 0.26 5.2 NEW SOURCE 270.210 -25.711 4.495 -1.273 6.3 1.31 4.8 0.9 0.74 1.3 SAX J1750.8-2900 267.609 -29.039 0.456 -0.955 1.1 0.28 3.9 0.5 0.19 2.4 NEW SOURCE 270.797 -25.508 4.933 -1.633 7.2 1.80 4.0 0.0 0.00 0.0 NEW SOURCE 269.691 -26.709 3.397 -1.365 2.7 0.63 4.3 0.4 0.40 1.0