INTEGRAL Galactic bulge Monitoring
Revolution 1276: Observation start 2013-03-26T05:12 = MJD 56377.217
Total Observation GTI = 11276 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 1700-377 255.989 -37.846 0.5 347.754 +2.171 56.4 0.64 87.7 17.5 0.43 40.4 GX 354-0 262.996 -33.830 0.7 354.309 -0.153 20.6 0.41 50.7 7.7 0.29 26.7 GX 1+4 263.010 -24.737 1.3 1.944 +4.799 9.4 0.40 23.6 0.0 0.00 0.0 GRS 1758-258 270.284 -25.751 1.5 4.494 -1.351 8.6 0.45 18.9 5.5 0.32 17.4 Ginga 1826-24 277.336 -23.808 1.5 9.249 -6.067 15.8 0.82 19.2 5.1 0.55 9.2 OAO 1657-415 255.212 -41.684 2.0 344.351 +0.297 20.0 1.45 13.8 5.8 0.92 6.3 GX 349+2 256.429 -36.370 2.3 349.143 +2.784 6.5 0.56 11.6 0.0 0.00 0.0 Swift J174510.8-2624 266.329 -26.357 2.6 2.167 +1.402 3.8 0.37 10.2 2.7 0.26 10.1 IGR J17091-3624 257.303 -36.423 2.5 349.522 +2.189 5.9 0.56 10.6 3.7 0.38 9.6 XTE J1810-189 272.548 -19.082 3.1 11.334 +0.085 7.1 0.86 8.3 2.7 0.58 4.7 3A 1822-371 276.417 -37.075 3.1 356.868 -11.258 6.6 0.79 8.3 2.5 0.55 4.5 KS 1741-293 266.229 -29.357 0.0 359.561 -0.088 2.8 0.00 6.7 0.0 0.00 0.0 H 1820-303 275.835 -30.343 3.7 2.772 -7.841 4.0 0.59 6.9 0.0 0.00 0.0 SLX 1744-299_300 266.809 -30.040 4.9 359.240 -0.874 1.7 0.34 5.1 1.5 0.25 6.1 IGR J17252-3616 261.293 -36.217 4.1 351.549 -0.314 3.1 0.50 6.2 0.0 0.00 0.0 MXB 1730-335 263.429 -33.318 4.8 354.935 -0.175 1.9 0.38 5.2 0.0 0.00 0.0 Swift J174444.9-2950 266.232 -29.851 0.0 359.141 -0.348 1.6 0.00 4.7 0.0 0.00 0.0 GX 5-1 270.241 -25.100 5.6 5.039 -0.995 1.8 0.41 4.4 0.0 0.00 0.0 4U 1722-30 261.860 -30.791 4.8 356.315 +2.325 2.1 0.39 5.2 1.4 0.28 4.9 1A 1742-294 266.607 -29.437 0.0 359.664 -0.412 1.9 0.00 4.7 0.0 0.00 0.0 GX 9+1 270.380 -20.486 5.6 9.112 +1.178 2.8 0.65 4.4 0.0 0.00 0.0 GX 3+1 267.032 -26.597 5.2 2.288 +0.739 1.8 0.38 4.8 0.0 0.00 0.0 SLX 1737-282 265.102 -28.370 5.7 359.880 +1.270 1.5 0.00 4.3 0.0 0.00 0.0 Oph Cluster 258.043 -23.276 0.0 0.612 +9.378 2.3 0.00 4.4 0.0 0.00 0.0 1RXS J175721.2-30440 269.388 -30.622 0.0 359.871 -3.087 1.9 0.00 4.2 0.0 0.00 0.0 XTE J1814-338 273.537 -33.790 6.2 358.779 -7.688 1.8 0.00 3.9 0.0 0.00 0.0 IGR J17177-3656 259.345 -36.889 0.0 350.106 +0.590 2.2 0.00 3.9 0.0 0.00 0.0 NEW SOURCE 269.585 -26.447 4.2 3.577 -1.153 2.4 0.40 6.0 0.0 0.00 0.0 NEW SOURCE 256.977 -25.852 4.4 357.919 +8.673 3.0 0.52 5.7 0.0 0.00 0.0 NEW SOURCE 269.362 -36.976 4.6 354.322 -6.218 2.7 0.51 5.4 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 1742-294 266.527 -29.526 359.552 -0.398 8.0 0.26 30.9 1.4 0.14 10.2 4U 1722-30 261.888 -30.802 356.320 +2.298 2.5 0.38 6.6 0.7 0.23 2.8 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.3 0.26 8.6 0.5 0.16 3.1 GX 1+4 263.009 -24.746 1.937 +4.795 5.1 1.24 4.1 2.1 0.72 3.0 GX 3+1 266.984 -26.562 2.295 +0.794 46.8 0.56 84.0 5.0 0.25 20.2 GX 354-0 262.984 -33.825 354.308 -0.141 10.2 0.54 19.0 4.4 0.36 12.1 GX 5-1 270.287 -25.076 5.081 -1.019 100.6 3.51 28.6 6.3 1.60 3.9 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.1 0.25 4.4 0.4 0.14 2.5 XTE J1739-285 264.975 -28.496 359.714 +1.298 7.1 0.28 25.1 0.9 0.14 6.2 NEW SOURCE 271.806 -26.921 4.141 -3.113 8.1 2.18 3.7 0.0 0.00 0.0 NEW SOURCE 267.377 -25.229 3.620 +1.178 3.4 0.97 3.5 0.7 0.46 1.4 NEW SOURCE 268.880 -25.233 4.309 +0.006 4.2 1.36 3.1 0.0 0.00 0.0