INTEGRAL Galactic bulge Monitoring
Revolution 1395: Observation start 2014-03-19T11:00 = MJD 56735.459
Total Observation GTI = 12237 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 J1744-28 266.138 -28.742 0.2 0.043 +0.301 125.6 0.36 352.9 12.9 0.22 58.0 GRS 1739-278 265.668 -27.745 0.5 0.675 +1.176 28.3 0.39 71.9 17.1 0.24 70.5 Ginga 1826-24 277.379 -23.790 1.1 9.284 -6.094 19.5 0.71 27.3 8.4 0.41 20.7 4U 1700-377 255.998 -37.859 1.2 347.748 +2.157 26.4 1.07 24.7 8.4 0.59 14.1 GRS 1758-258 270.294 -25.733 1.2 4.513 -1.350 10.7 0.41 25.8 8.0 0.25 31.9 H 1820-303 275.947 -30.309 2.2 2.846 -7.912 6.9 0.57 12.2 0.0 0.00 0.0 GX 1+4 262.996 -24.768 2.5 1.912 +4.792 4.4 0.42 10.4 0.0 0.00 0.0 GX 5-1 270.272 -25.104 3.0 5.050 -1.021 3.5 0.40 8.8 0.0 0.00 0.0 OAO 1657-415 255.205 -41.627 2.8 344.393 +0.337 21.2 2.22 9.5 0.0 0.00 0.0 1E 1742.8-2853 266.506 -28.934 0.0 0.048 -0.075 2.9 0.00 8.2 0.0 0.00 0.0 GX 3+1 266.954 -26.548 3.9 2.293 +0.824 2.8 0.43 6.6 0.0 0.00 0.0 GX 17+2 273.991 -14.073 3.2 16.393 +1.273 22.0 2.73 8.1 0.0 0.00 0.0 GX 9+1 270.395 -20.451 4.6 9.149 +1.184 3.1 0.57 5.4 0.0 0.00 0.0 AX J1749.2-2725 267.256 -27.454 0.0 1.656 +0.126 2.3 0.00 5.5 0.0 0.00 0.0 MXB 1730-335 263.319 -33.460 4.1 354.766 -0.175 3.0 0.49 6.2 0.0 0.00 0.0 GX 349+2 256.493 -36.365 4.3 349.178 +2.747 5.0 0.84 5.9 0.0 0.00 0.0 3A 1822-371 276.307 -37.062 0.0 356.841 -11.173 3.3 0.00 4.8 0.0 0.00 0.0 SLX 1735-269 264.575 -26.940 6.5 0.844 +2.426 1.7 0.44 3.7 0.9 0.27 3.5 IGR J17204-3554 260.240 -35.858 0.0 351.364 +0.591 2.6 0.00 4.4 0.0 0.00 0.0 4U 1722-30 261.910 -30.806 5.7 356.327 +2.280 2.0 0.00 4.3 0.0 0.00 0.0 H 1702-429 256.655 -43.087 0.0 343.886 -1.402 14.4 0.00 4.3 0.0 0.00 0.0 GRO J1655-40 253.545 -39.811 5.8 345.030 +2.451 7.9 0.00 4.2 0.0 0.00 0.0 SLX 1737-282 265.202 -28.264 0.0 0.017 +1.251 1.5 0.00 4.0 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 1742-294 266.523 -29.515 359.559 -0.389 8.1 0.33 24.3 1.3 0.19 6.7 4U 1722-30 261.888 -30.802 356.320 +2.298 3.5 0.93 3.7 1.4 0.67 2.1 GRO J1744-28 266.138 -28.740 0.045 +0.302 77.5 0.40 193.6 36.2 0.23 156.5 GRS 1739-278 265.667 -27.742 0.677 +1.179 6.3 0.35 18.1 3.2 0.20 16.0 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 2.2 0.34 6.6 0.5 0.19 2.7 GRS 1758-258 270.303 -25.741 4.511 -1.361 0.0 0.00 0.0 1.4 0.36 3.9 GX 3+1 266.985 -26.570 2.289 +0.789 51.8 0.43 119.3 5.0 0.22 23.0 GX 354-0 262.989 -33.835 354.302 -0.150 12.0 2.01 6.0 4.9 1.64 3.0 GX 5-1 270.283 -25.083 5.073 -1.020 116.7 1.05 110.9 6.5 0.45 14.4 MXB 1730-335 263.350 -33.388 354.841 -0.158 7.0 1.34 5.2 0.0 0.00 0.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.1 0.42 5.0 0.8 0.24 3.4 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.3 0.33 4.0 0.0 0.00 0.0 NEW SOURCE 269.011 -23.201 6.125 +0.926 9.1 1.64 5.5 1.4 0.89 1.6 NEW SOURCE 273.076 -25.807 5.667 -3.576 10.3 2.07 5.0 1.4 1.04 1.4 NEW SOURCE 267.926 -29.007 0.625 -1.177 1.6 0.34 4.8 0.4 0.19 2.4 NEW SOURCE 267.082 -32.651 357.124 -2.422 2.7 0.57 4.8 0.0 0.00 0.0 NEW SOURCE 270.064 -24.838 5.188 -0.726 4.6 1.00 4.6 0.0 0.00 0.0 NEW SOURCE 266.143 -32.587 356.768 -1.713 2.3 0.60 3.7 1.9 0.39 4.8 NEW SOURCE 265.015 -24.526 3.102 +3.373 2.9 0.78 3.7 1.8 0.43 4.1 NEW SOURCE 260.606 -28.681 357.457 +4.408 4.2 1.25 3.4 4.0 0.98 4.1