INTEGRAL Galactic bulge Monitoring
Revolution 0594: Observation start 2007-08-25T02:43 = MJD 54337.114
Total Observation GTI = 12272 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 1700-377 255.980 -37.843 0.4 347.753 +2.178 82.1 0.79 103.6 21.8 0.60 36.3 GX 5-1 270.283 -25.081 0.7 5.075 -1.019 17.9 0.37 47.9 0.0 0.00 0.0 GX 1+4 263.008 -24.741 0.8 1.940 +4.798 15.1 0.38 39.9 0.0 0.00 0.0 Ginga 1826-24 277.366 -23.792 1.0 9.276 -6.084 18.5 0.62 29.7 6.7 0.48 13.8 H 1820-303 275.908 -30.374 1.3 2.773 -7.911 12.7 0.54 23.5 0.0 0.00 0.0 GRS 1758-258 270.295 -25.750 1.7 4.499 -1.359 6.3 0.37 17.0 3.1 0.30 10.2 3A 1822-371 276.445 -37.136 2.2 356.821 -11.304 8.2 0.67 12.3 0.0 0.00 0.0 4U 1722-30 261.876 -30.839 2.4 356.283 +2.286 4.3 0.38 11.2 1.7 0.31 5.5 GX 349+2 256.449 -36.438 2.4 349.098 +2.731 7.3 0.66 10.9 0.0 0.00 0.0 GX 9+1 270.374 -20.505 3.1 9.093 +1.175 4.0 0.48 8.3 0.0 0.00 0.0 GX 3+1 267.012 -26.585 2.7 2.289 +0.761 3.4 0.35 9.7 0.0 0.00 0.0 SAX J1810.8-2609 272.674 -26.133 3.7 5.208 -3.414 2.9 0.42 6.8 2.4 0.34 7.1 OAO 1657-415 255.204 -41.651 3.3 344.373 +0.322 13.5 1.75 7.8 0.0 0.00 0.0 1A 1742-294 266.488 -29.541 5.4 359.521 -0.376 1.4 0.30 4.5 0.0 0.00 0.0 SLX 1735-269 264.438 -27.015 4.1 0.715 +2.490 2.3 0.38 6.1 1.4 0.32 4.6 SAX J1712.6-3739 258.149 -37.575 5.1 348.993 +0.963 3.0 0.63 4.8 0.0 0.00 0.0 GX 354-0 262.912 -33.823 5.4 354.277 -0.090 1.7 0.38 4.5 0.0 0.00 0.0 IGR J17091-3624 257.268 -36.399 4.8 349.525 +2.226 3.0 0.58 5.2 2.2 0.46 4.8 H 1702-429 256.574 -43.057 6.1 343.875 -1.337 9.8 2.46 4.0 0.0 0.00 0.0 1E 1743.1-2843 266.581 -28.778 4.8 0.216 -0.050 1.6 0.31 5.2 0.0 0.00 0.0 IGR J18027-2016 270.641 -20.216 0.0 9.468 +1.099 2.1 0.00 4.2 0.0 0.00 0.0 IGR J18179-1621 274.537 -16.287 5.1 14.694 -0.242 5.8 1.20 4.9 0.0 0.00 0.0 GX 17+2 274.070 -14.075 0.0 16.427 +1.204 10.1 0.00 4.1 0.0 0.00 0.0 Swift J174535.5-2901 266.400 -29.087 0.0 359.869 -0.075 1.2 0.00 3.9 0.0 0.00 0.0 IGR J18173-2509 274.348 -25.175 0.0 6.771 -4.288 1.7 0.00 3.7 0.0 0.00 0.0 3A 1728-169 262.990 -16.937 6.4 8.563 +9.005 2.7 0.71 3.8 0.0 0.00 0.0 H 1705-440 257.247 -44.201 6.6 343.250 -2.412 13.2 0.00 3.6 0.0 0.00 0.0 IGR J17464-3213 266.497 -32.129 6.9 357.315 -1.729 1.2 0.00 3.5 0.0 0.00 0.0 SLX 1744-299_300 266.728 -30.007 6.5 359.231 -0.797 1.2 0.31 3.7 0.0 0.00 0.0 EXO 1745-248 267.123 -24.814 7.2 3.858 +1.589 1.2 0.00 3.4 0.0 0.00 0.0
JEM-X
JEM-X1 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 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 5.4 0.32 17.0 1.0 0.19 5.1 GX 3+1 266.989 -26.564 2.297 +0.789 35.3 0.51 69.0 3.8 0.26 14.5 GX 354-0 262.989 -33.835 354.302 -0.150 12.0 1.26 9.5 1.7 1.01 1.7 GX 5-1 270.284 -25.082 5.075 -1.020 116.6 1.95 59.9 17.4 0.91 19.2 NEW SOURCE 272.798 -26.104 5.286 -3.498 27.8 3.52 7.9 4.1 1.92 2.1 NEW SOURCE 270.909 -25.524 4.969 -1.729 7.8 1.73 4.5 1.0 0.86 1.2 NEW SOURCE 265.679 -29.980 358.779 -0.008 1.5 0.31 5.0 0.0 0.00 0.0 NEW SOURCE 267.672 -22.861 5.793 +2.161 12.9 2.75 4.7 1.6 1.60 1.0 NEW SOURCE 266.570 -23.192 4.987 +2.859 7.0 1.74 4.0 1.4 1.04 1.3 NEW SOURCE 272.899 -27.128 4.428 -4.066 9.3 2.20 4.3 0.0 0.00 0.0 NEW SOURCE 268.175 -26.306 3.062 +0.010 2.1 0.57 3.7 0.9 0.31 2.9 NEW SOURCE 269.727 -27.143 3.037 -1.609 1.1 0.60 1.9 1.0 0.33 3.1