INTEGRAL Galactic bulge Monitoring
Revolution 0966: Observation start 2010-09-10T21:56 = MJD 55449.914
Total Observation GTI = 11863 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 1+4 263.004 -24.752 0.6 1.929 +4.795 25.7 0.44 58.7 0.0 0.00 0.0 4U 1700-377 255.987 -37.862 0.9 347.741 +2.162 32.1 0.84 38.4 9.1 0.63 14.4 1E 1740.7-2942 265.980 -29.751 1.0 359.112 -0.110 10.3 0.34 30.0 5.9 0.29 20.4 GX 5-1 270.297 -25.070 1.1 5.091 -1.024 10.9 0.39 27.6 0.0 0.00 0.0 Ginga 1826-24 277.379 -23.794 1.4 9.280 -6.096 13.2 0.65 20.1 5.6 0.50 11.3 IGR J17464-3213 266.568 -32.235 1.6 357.255 -1.836 6.9 0.40 17.2 3.9 0.32 12.3 OAO 1657-415 255.191 -41.654 1.8 344.365 +0.328 32.0 2.10 15.2 0.0 0.00 0.0 GRS 1758-258 270.300 -25.742 2.5 4.508 -1.359 4.1 0.38 10.7 3.4 0.31 11.2 4U 1722-30 261.882 -30.813 2.7 356.308 +2.297 3.9 0.40 9.7 0.0 0.00 0.0 H 1820-303 275.919 -30.347 2.7 2.801 -7.907 5.4 0.55 9.8 0.0 0.00 0.0 GX 349+2 256.450 -36.489 2.8 349.058 +2.700 7.0 0.76 9.3 0.0 0.00 0.0 3A 1822-371 276.456 -37.080 3.1 356.878 -11.288 6.1 0.73 8.4 0.0 0.00 0.0 Swift J174535.5-2901 266.313 -29.001 4.3 359.902 +0.035 1.9 0.34 5.8 0.0 0.00 0.0 GX 9+1 270.404 -20.579 3.9 9.042 +1.113 3.2 0.49 6.5 0.0 0.00 0.0 GX 17+2 273.974 -13.996 4.1 16.453 +1.324 15.6 2.51 6.2 0.0 0.00 0.0 SLX 1735-269 264.629 -26.958 4.9 0.854 +2.376 1.9 0.36 5.1 0.0 0.00 0.0 1A 1742-294 266.587 -29.508 4.7 359.594 -0.433 1.8 0.34 5.3 0.0 0.00 0.0 IGR J16500-3307 252.371 -33.132 4.9 349.626 +7.406 5.1 0.00 5.1 0.0 0.00 0.0 V1223 Sgr 283.671 -31.146 5.2 4.943 -14.279 7.8 1.66 4.7 0.0 0.00 0.0 1RXS J175721.2-30440 269.452 -30.711 0.0 359.821 -3.179 1.6 0.00 4.5 0.0 0.00 0.0 GX 3+1 267.062 -26.538 0.0 2.352 +0.747 1.5 0.00 4.3 0.0 0.00 0.0 GX 354-0 263.066 -33.766 5.6 354.395 -0.166 1.9 0.42 4.4 0.0 0.00 0.0 V2400 Oph 258.149 -24.139 5.6 359.953 +8.803 2.3 0.52 4.4 0.0 0.00 0.0 H1825-331 276.999 -33.203 6.2 0.626 -10.001 2.2 0.00 3.9 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 ==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== =====