INTEGRAL Galactic bulge Monitoring
Revolution 1144: Observation start 2012-02-27T19:55 = MJD 55984.831
Total Observation GTI = 15372 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 1700-377 255.992 -37.852 0.6 347.751 +2.165 45.7 0.71 64.3 13.3 0.49 27.1 1E 1740.7-2942 265.986 -29.750 1.2 359.115 -0.114 7.0 0.29 24.4 3.5 0.22 15.9 GX 5-1 270.283 -25.066 1.2 5.088 -1.011 8.3 0.34 24.3 0.0 0.00 0.0 GRS 1758-258 270.314 -25.737 1.2 4.519 -1.368 8.0 0.33 24.4 5.3 0.24 22.3 Ginga 1826-24 277.370 -23.783 1.3 9.286 -6.084 11.2 0.50 22.4 4.5 0.36 12.7 GX 1+4 263.012 -24.724 2.4 1.957 +4.804 4.1 0.37 11.1 0.0 0.00 0.0 GX 354-0 262.989 -33.805 2.3 354.328 -0.134 4.0 0.35 11.6 1.2 0.25 4.8 GX 349+2 256.411 -36.405 2.4 349.106 +2.775 7.2 0.64 11.3 0.0 0.00 0.0 3A 1822-371 276.442 -37.088 3.0 356.865 -11.281 5.1 0.59 8.6 0.0 0.00 0.0 H 1820-303 275.931 -30.339 2.8 2.813 -7.913 4.2 0.44 9.5 0.0 0.00 0.0 GX 9+1 270.423 -20.459 3.8 9.156 +1.157 2.8 0.42 6.7 0.0 0.00 0.0 GX 3+1 267.001 -26.499 3.2 2.357 +0.814 2.5 0.31 8.1 0.0 0.00 0.0 1E 1742.9-2849 266.487 -28.861 3.7 0.102 -0.022 1.9 0.28 6.9 0.0 0.00 0.0 SLX 1735-269 264.569 -26.924 4.3 0.854 +2.439 1.8 0.00 5.9 0.0 0.00 0.0 IGR J17204-3554 260.057 -35.824 4.1 351.307 +0.733 3.0 0.48 6.2 0.0 0.00 0.0 IGR J17559-2612 269.055 -26.296 5.0 3.470 -0.666 1.5 0.30 4.9 0.0 0.00 0.0 H 1702-429 256.544 -43.058 4.5 343.861 -1.320 11.7 0.00 5.5 0.0 0.00 0.0 GX 13+1 273.620 -17.172 4.3 13.499 +0.109 4.4 0.76 5.8 0.0 0.00 0.0 IGR J17098-3628 257.393 -36.370 0.0 349.608 +2.162 2.9 0.00 5.4 0.0 0.00 0.0 SLX 1744-299_300 266.956 -30.007 4.5 359.333 -0.966 1.6 0.29 5.5 0.0 0.00 0.0 IGR J17252-3616 261.329 -36.238 4.9 351.548 -0.350 2.1 0.42 5.0 0.0 0.00 0.0 V4641 Sgr 274.807 -25.432 5.7 6.738 -4.774 1.8 0.43 4.3 0.0 0.00 0.0 XTE J1751-305 267.833 -30.681 5.2 359.144 -1.961 1.4 0.30 4.8 0.7 0.23 3.1 Swift J181539.7-1833 273.872 -18.528 0.0 12.421 -0.749 2.6 0.00 4.4 0.0 0.00 0.0 IGR J17354-3255 263.834 -33.031 4.8 355.360 -0.304 1.7 0.32 5.2 0.0 0.00 0.0 V1223 Sgr 283.881 -31.208 6.7 4.958 -14.468 5.7 1.58 3.6 0.0 0.00 0.0 AX J1749.2-2725 267.315 -27.479 6.0 1.662 +0.069 1.3 0.31 4.1 0.0 0.00 0.0 GRS 1734-292 264.422 -29.141 6.2 358.910 +1.364 1.1 0.00 3.9 0.0 0.00 0.0 SAX J1810.8-2609 272.635 -26.181 6.3 5.149 -3.406 1.3 0.00 3.9 0.0 0.00 0.0 SLX 1737-282 265.116 -28.235 5.4 0.002 +1.331 1.3 0.28 4.6 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined 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+2 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 1742-294 266.524 -29.511 359.563 -0.388 10.5 0.23 46.1 1.8 0.13 14.3 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.23 9.0 1.0 0.13 7.4 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.7 0.23 3.1 0.2 0.13 1.9 4U 1722-30 261.888 -30.802 356.320 +2.298 10.0 0.67 14.9 2.1 0.49 4.2 GX 3+1 266.984 -26.568 2.290 +0.791 57.8 0.39 147.9 6.6 0.18 36.1 GX 354-0 262.989 -33.835 354.302 -0.150 11.0 1.56 7.1 1.9 1.35 1.4 GX 5-1 270.285 -25.076 5.080 -1.018 149.4 1.21 123.4 16.6 0.50 33.5 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 0.7 0.21 3.6 0.3 0.12 2.1 NEW SOURCE 271.920 -27.280 3.876 -3.376 4.6 0.81 5.7 0.0 0.00 0.0