INTEGRAL Galactic bulge Monitoring
Revolution 0350: Observation start 2005-08-25T13:00 = MJD 53607.542
Total Observation GTI = 11867 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 5-1 270.283 -25.080 0.7 5.076 -1.018 18.7 0.34 54.9 0.0 0.00 0.0 4U 1700-377 256.009 -37.845 0.7 347.765 +2.159 37.0 0.71 52.5 11.1 0.52 21.4 GRS 1758-258 270.294 -25.743 0.9 4.505 -1.355 13.7 0.36 38.3 8.4 0.28 29.7 GX 354-0 262.997 -33.835 0.9 354.306 -0.155 13.6 0.36 38.0 3.6 0.28 12.9 H 1820-303 275.922 -30.357 1.0 2.794 -7.914 16.0 0.50 32.1 3.9 0.38 10.3 Ginga 1826-24 277.369 -23.792 1.1 9.278 -6.087 18.4 0.63 29.1 6.9 0.47 14.6 IGR J17464-3213 266.562 -32.233 1.2 357.254 -1.831 8.4 0.33 25.4 4.2 0.27 15.7 1E 1740.7-2942 265.998 -29.745 1.2 359.125 -0.120 7.6 0.32 23.9 5.1 0.26 20.0 GX 349+2 256.438 -36.429 1.4 349.100 +2.743 13.2 0.63 20.8 0.0 0.00 0.0 KS 1741-293 266.213 -29.336 0.0 359.571 -0.065 4.0 0.00 13.2 1.8 0.00 7.3 GX 1+4 263.031 -24.729 1.9 1.962 +4.787 5.0 0.35 14.3 0.0 0.00 0.0 3A 1822-371 276.492 -37.087 2.9 356.883 -11.317 5.9 0.66 9.0 0.0 0.00 0.0 4U 1722-30 261.904 -30.805 3.1 356.325 +2.285 3.2 0.38 8.4 1.1 0.30 3.8 XTE J1818-245 274.623 -24.511 2.9 7.476 -4.196 4.3 0.48 8.9 1.6 0.36 4.5 IGR J17252-3616 261.290 -36.302 2.9 351.478 -0.360 4.4 0.49 9.0 0.0 0.00 0.0 SLX 1744-299_300 266.863 -30.063 3.2 359.244 -0.926 2.6 0.32 8.2 0.0 0.00 0.0 GX 9+1 270.359 -20.555 2.9 9.042 +1.162 4.3 0.47 9.0 0.0 0.00 0.0 MXB 1730-335 263.331 -33.399 3.4 354.823 -0.151 2.6 0.34 7.6 0.0 0.00 0.0 SLX 1735-269 264.588 -26.980 3.4 0.816 +2.395 3.0 0.40 7.5 1.3 0.32 4.1 GX 3+1 266.971 -26.593 4.7 2.263 +0.788 1.9 0.36 5.3 0.0 0.00 0.0 4U 1735-444 264.760 -44.527 4.7 345.994 -7.045 24.5 4.66 5.3 0.0 0.00 0.0 GX 13+1 273.598 -17.164 5.1 13.495 +0.132 4.1 0.85 4.8 0.0 0.00 0.0 Oph Cluster 258.171 -23.256 5.7 0.697 +9.294 2.3 0.54 4.3 0.0 0.00 0.0 GX 17+2 274.004 -14.059 5.2 16.412 +1.268 12.0 2.54 4.7 0.0 0.00 0.0 OAO 1657-415 255.203 -41.673 6.1 344.356 +0.309 6.7 1.69 4.0 0.0 0.00 0.0 IGR J17456-2901 266.402 -28.924 0.0 0.008 +0.009 1.2 0.00 4.1 0.0 0.00 0.0 3A 1728-169 262.953 -16.978 5.8 8.509 +9.014 3.1 0.74 4.2 0.0 0.00 0.0 QSO B1730-130 263.315 -13.109 6.5 12.036 +10.752 13.3 0.00 3.7 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 3.3 0.30 11.1 0.6 0.17 3.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.7 0.30 5.8 0.9 0.18 5.0 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.6 0.30 5.3 0.3 0.17 1.8 GX 3+1 266.973 -26.572 2.282 +0.798 15.8 0.41 38.4 1.7 0.22 7.7 GX 354-0 262.989 -33.835 354.302 -0.150 10.7 1.36 7.9 2.3 0.98 2.4 GX 5-1 270.285 -25.084 5.074 -1.022 130.9 1.77 74.1 18.8 0.80 23.4 IGR J17464-3213 266.567 -32.229 357.260 -1.832 9.5 0.46 20.7 1.2 0.28 4.2 MXB 1730-335 263.330 -33.402 354.820 -0.152 11.6 1.03 11.2 1.9 0.65 3.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.3 0.30 4.3 0.4 0.18 2.3 XTE J1739-285 264.969 -28.494 359.713 +1.303 6.5 0.31 20.9 0.9 0.18 4.9 CONFUSED ID 270.288 -25.084 5.075 -1.024 131.4 1.77 74.2 18.8 0.80 23.4 CONFUSED ID 270.253 -25.155 4.997 -1.031 32.6 1.44 22.6 5.2 0.71 7.4 NEW SOURCE 272.098 -26.261 4.846 -3.022 9.1 2.26 4.0 0.0 0.00 0.0 NEW SOURCE 268.497 -26.807 2.776 -0.493 2.1 0.44 4.7 0.0 0.00 0.0 NEW SOURCE 271.634 -26.382 4.539 -2.717 6.0 1.41 4.2 0.0 0.00 0.0 NEW SOURCE 268.856 -31.233 359.112 -2.997 0.0 0.00 0.0 0.9 0.28 3.3 KS 1741-293 266.217 -29.333 359.576 -0.067 1.0 0.29 3.4 0.5 0.17 2.7