INTEGRAL Galactic bulge Monitoring
Revolution 1589: Observation start 2015-09-19T18:30 = MJD 57284.772
Total Observation GTI = 12524 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 1700-377 255.981 -37.849 0.7 347.748 +2.174 45.8 1.00 45.8 15.4 0.59 26.1 GX 354-0 262.992 -33.844 1.0 354.295 -0.157 15.3 0.49 31.1 5.0 0.30 16.5 GRS 1758-258 270.288 -25.740 1.0 4.505 -1.349 13.8 0.46 30.1 10.2 0.29 35.3 GX 1+4 263.022 -24.757 1.6 1.934 +4.779 7.6 0.42 18.2 0.0 0.00 0.0 1E 1740.7-2942 265.976 -29.723 2.0 359.134 -0.093 5.8 0.43 13.4 5.3 0.28 18.8 GX 349+2 256.438 -36.438 2.2 349.093 +2.738 10.5 0.87 12.1 0.0 0.00 0.0 3A 1822-371 276.548 -37.091 3.8 356.899 -11.359 5.6 0.84 6.7 0.0 0.00 0.0 4U 1722-30 261.802 -30.825 4.1 356.259 +2.347 2.8 0.46 6.1 1.4 0.29 4.8 XTE J1817-330 274.477 -32.982 4.4 359.868 -8.013 2.8 0.50 5.7 0.0 0.00 0.0 SLX 1735-269 264.573 -27.047 4.9 0.752 +2.371 1.9 0.38 5.1 0.0 0.00 0.0 GX 3+1 266.920 -26.611 4.2 2.224 +0.818 2.3 0.39 6.0 0.0 0.00 0.0 Ginga 1826-24 277.349 -23.855 0.0 9.212 -6.099 3.2 0.00 5.1 0.0 0.00 0.0 Oph Cluster 258.041 -23.442 4.9 0.473 +9.285 3.0 0.00 5.1 0.0 0.00 0.0 GX 5-1 270.199 -25.043 4.8 5.071 -0.933 2.3 0.45 5.2 0.0 0.00 0.0 SAX J1750.8-2900 267.577 -29.047 0.0 0.435 -0.935 1.8 0.00 4.7 0.0 0.00 0.0 IGR J17098-3628 257.453 -36.401 0.0 349.611 +2.105 3.9 0.00 4.6 0.0 0.00 0.0 IGR J17497-2821 267.480 -28.306 0.0 1.027 -0.482 1.6 0.00 4.6 0.0 0.00 0.0 GX 17+2 273.957 -13.943 5.6 16.492 +1.364 7.3 1.67 4.4 0.0 0.00 0.0 H 1820-303 275.908 -30.325 5.9 2.816 -7.889 2.3 0.56 4.1 0.0 0.00 0.0 1A 1743-288 266.726 -28.886 5.2 0.189 -0.214 1.7 0.37 4.7 0.0 0.00 0.0 QSO B1730-130 263.192 -13.064 5.8 12.011 +10.878 9.0 0.00 4.2 0.0 0.00 0.0 H 1702-429 256.705 -43.006 5.8 343.973 -1.383 31.8 7.59 4.2 0.0 0.00 0.0 4U 1708-40 258.243 -40.808 6.0 346.421 -0.997 6.9 0.00 4.0 0.0 0.00 0.0 IGR J17475-2822 266.919 -28.389 0.0 0.702 -0.102 1.4 0.00 4.0 0.0 0.00 0.0 IGR J18135-1751 273.390 -17.936 6.3 12.723 -0.064 3.1 0.00 3.9 0.0 0.00 0.0 1A 1742-294 266.539 -29.622 0.0 359.475 -0.456 1.6 0.00 3.8 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 1742-294 266.518 -29.509 359.562 -0.382 7.4 0.26 28.0 0.9 0.14 6.5 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.6 0.29 9.1 1.0 0.16 6.2 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.0 0.25 3.8 0.3 0.13 2.0 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 0.9 0.26 3.5 0.0 0.00 0.0 GRS 1758-258 270.303 -25.741 4.511 -1.361 1.1 0.53 2.1 1.7 0.25 6.8 GX 1+4 263.009 -24.746 1.937 +4.795 2.4 0.72 3.3 1.3 0.46 2.8 GX 3+1 266.983 -26.565 2.292 +0.793 32.3 0.32 102.0 2.7 0.15 18.2 GX 5-1 270.289 -25.076 5.082 -1.021 108.6 0.78 139.2 4.0 0.30 13.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.7 0.28 9.5 0.4 0.15 2.4 SAX J1750.8-2900 267.606 -29.030 0.462 -0.948 3.1 0.26 11.8 0.6 0.14 4.5 NEW SOURCE 269.239 -33.327 357.457 -4.325 7.3 1.00 7.2 0.8 0.69 1.1