INTEGRAL Galactic bulge Monitoring
Revolution 1514: Observation start 2015-03-05T02:32 = MJD 57086.106
Total Observation GTI = 12529 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 1700-377 255.985 -37.841 0.5 347.756 +2.176 61.7 0.79 78.3 23.5 0.47 50.0 1RXS J180408.9-34205 271.036 -34.355 0.6 357.292 -6.129 24.2 0.44 55.7 10.9 0.27 40.4 GX 5-1 270.283 -25.082 1.0 5.074 -1.019 13.5 0.44 30.8 0.0 0.00 0.0 Ginga 1826-24 277.368 -23.789 1.0 9.279 -6.084 21.5 0.68 31.6 9.2 0.40 23.1 GX 1+4 263.010 -24.741 1.0 1.941 +4.797 13.2 0.44 30.0 0.0 0.00 0.0 GRS 1758-258 270.311 -25.749 1.2 4.507 -1.371 10.4 0.41 25.1 7.7 0.26 30.0 GRO J1750-27 267.261 -26.643 1.2 2.353 +0.540 9.0 0.36 25.2 1.1 0.00 4.7 H 1820-303 275.917 -30.345 1.9 2.803 -7.905 8.2 0.57 14.3 1.3 0.00 3.9 GRS 1739-278 265.699 -27.786 2.8 0.655 +1.131 3.3 0.35 9.4 1.5 0.23 6.5 GX 349+2 256.363 -36.434 3.1 349.059 +2.788 6.0 0.72 8.3 0.0 0.00 0.0 4U 1722-30 261.895 -30.808 3.0 356.318 +2.289 3.5 0.40 8.8 1.6 0.25 6.3 1E 1740.7-2942 265.971 -29.737 3.2 359.120 -0.096 2.9 0.35 8.1 1.7 0.24 7.2 SLX 1735-269 264.572 -27.037 3.6 0.760 +2.377 2.6 0.37 7.2 1.1 0.23 4.7 KS 1741-293 266.228 -29.342 4.1 359.573 -0.080 2.1 0.34 6.1 0.0 0.00 0.0 IGR J17391-3021 264.841 -30.364 3.1 358.070 +0.403 3.2 0.37 8.5 1.0 0.24 4.1 GX 9+1 270.323 -20.488 3.8 9.084 +1.224 3.4 0.51 6.7 0.0 0.00 0.0 SAX J1712.6-3739 258.176 -37.667 3.7 348.932 +0.892 4.9 0.70 6.9 0.0 0.00 0.0 MXB 1730-335 263.237 -33.330 4.6 354.838 -0.047 2.3 0.42 5.4 0.0 0.00 0.0 1E 1743.1-2843 266.589 -28.760 0.0 0.235 -0.046 1.8 0.00 5.4 0.0 0.00 0.0 1A 1742-294 266.591 -29.500 0.0 359.603 -0.432 1.9 0.00 5.4 0.0 0.00 0.0 OAO 1657-415 255.255 -41.648 4.3 344.399 +0.294 10.6 1.80 5.9 0.0 0.00 0.0 GX 354-0 262.994 -33.862 4.4 354.281 -0.169 2.4 0.43 5.7 0.0 0.00 0.0 SAX J1806.5-2215 271.595 -22.126 5.3 8.240 -0.613 2.4 0.00 4.6 0.0 0.00 0.0 XTE J1818-245 274.635 -24.509 4.9 7.483 -4.205 3.1 0.61 5.0 0.0 0.00 0.0 3A 1822-371 276.431 -37.097 5.3 356.853 -11.277 3.7 0.80 4.7 0.0 0.00 0.0 SLX 1744-299_300 266.876 -29.993 0.0 359.310 -0.900 1.5 0.00 4.4 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 1742-294 266.515 -29.514 359.557 -0.383 9.8 0.24 40.7 1.6 0.14 11.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.4 0.23 6.1 0.5 0.14 3.6 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.24 3.7 0.2 0.13 1.3 4U 1722-30 261.888 -30.802 356.320 +2.298 2.6 0.48 5.5 0.7 0.32 2.3 GRO J1750-27 267.315 -26.678 2.348 +0.481 1.8 0.33 5.5 2.3 0.18 12.3 GRS 1758-258 270.303 -25.741 4.511 -1.361 2.3 0.80 2.9 1.8 0.42 4.3 GX 1+4 263.009 -24.746 1.937 +4.795 3.3 0.79 4.2 2.6 0.51 5.1 GX 3+1 266.984 -26.569 2.290 +0.790 36.9 0.35 104.6 3.7 0.18 20.3 GX 354-0 262.995 -33.838 354.302 -0.156 23.3 1.08 21.6 4.3 0.79 5.4 GX 5-1 270.289 -25.074 5.083 -1.020 116.9 1.33 87.7 19.3 0.64 30.1 IGR J17391-3021 264.791 -30.340 358.068 +0.453 1.9 0.25 7.4 0.8 0.15 5.1 MXB 1730-335 263.356 -33.383 354.848 -0.160 8.6 0.75 11.4 1.6 0.53 3.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.6 0.30 5.2 0.4 0.17 2.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.5 0.24 10.3 0.4 0.14 3.0 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.5 0.24 6.2 0.3 0.13 2.4 IGR J17451-3022 266.266 -30.380 358.705 -0.650 1.2 0.24 4.9 0.0 0.00 0.0 NEW SOURCE 272.777 -26.152 5.235 -3.504 11.6 2.42 4.8 2.4 1.75 1.4