INTEGRAL Galactic Bulge Monitoring Revolution 0651: Observation start 2008-02-11 = MJD 54507
Total Observation GTI = 5227 seconds
ISGRI
ISGRI significance mosaic images. Left: ISGRI 18-40 keV. Right: 40-100 keVSources 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
OSA7
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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 andNEW
sources < 6σ towards the border of the image may be spurious.
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 J1750-27 267.297 -26.646 0.5 2.368 +0.511 39.3 0.49 80.1 2.4 0.43 5.5 4U 1700-377 255.979 -37.845 0.9 347.750 +2.178 47.3 1.30 36.3 12.4 0.96 12.9 GX 354-0 262.982 -33.833 1.3 354.301 -0.144 14.2 0.60 23.4 1.6 0.48 3.3 Ginga 1826-24 277.373 -23.784 1.4 9.286 -6.086 16.5 0.78 21.2 6.6 0.60 11.0 H 1820-303 275.925 -30.355 1.7 2.796 -7.916 11.1 0.68 16.2 0.0 0.00 0.0 GX 3+1 266.971 -26.580 0.0 2.274 +0.795 5.3 0.00 10.4 0.0 0.00 0.0 OAO 1657-415 255.203 -41.668 2.8 344.359 +0.312 24.3 2.59 9.4 10.4 1.78 5.8 GX 349+2 256.449 -36.422 2.9 349.111 +2.741 10.3 1.15 8.9 0.0 0.00 0.0 3A 1822-371 276.446 -37.114 3.2 356.843 -11.295 7.2 0.90 8.0 0.0 0.00 0.0 GX 9+1 270.377 -20.519 3.5 9.082 +1.164 5.1 0.70 7.2 0.0 0.00 0.0 1E 1742.9-2849 266.489 -28.809 4.1 0.147 +0.003 2.9 0.47 6.1 0.0 0.00 0.0 SLX 1735-269 264.585 -27.036 3.7 0.768 +2.367 3.2 0.47 6.9 1.9 0.38 4.9 1A 1742-294 266.498 -29.532 3.7 359.533 -0.380 3.2 0.46 6.8 0.0 0.00 0.0 GRS 1758-258 270.294 -25.778 4.7 4.474 -1.372 2.7 0.51 5.3 1.8 0.41 4.4 IGR J17464-3213 266.546 -32.186 4.5 357.288 -1.795 2.7 0.48 5.6 2.6 0.41 6.2 4U 1722-30 261.827 -30.845 4.8 356.255 +2.318 3.0 0.58 5.1 0.0 0.00 0.0 GX 17+2 274.034 -14.066 4.4 16.420 +1.240 16.2 2.84 5.7 0.0 0.00 0.0 GX 5-1 270.323 -25.038 5.2 5.130 -1.028 2.8 0.59 4.7 0.0 0.00 0.0 IGR J17454-2703 266.273 -27.112 8.0 1.496 +1.051 1.3 0.45 3.0 0.0 0.00 0.0 SLX 1744-299_300 266.964 -30.027 6.0 359.320 -0.982 2.1 0.51 4.1 2.5 0.42 6.0 GX 1+4 263.027 -24.704 7.1 1.981 +4.804 1.8 0.54 3.4 0.0 0.00 0.0JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.Note: Sources labelled were detected in the 3-10 keV image > 5σ and 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 ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).NOTE: 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.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).Source Name RA dec l b A(cps) +/- B(cps) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 3+1 266.983 -26.564 2.294 +0.794 40.5 1.07 5.8 0.58 GX 5-1 270.284 -25.079 5.077 -1.019 79.8 2.49 7.6 1.26 GRO J1750-27 267.300 -26.647 2.368 +0.508 20.0 1.04 11.3 0.57
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