INTEGRAL Galactic Bulge Monitoring Revolution 0290: Observation start 2005-02-27 = MJD 53428
Total Observation GTI = 3344 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 5-1 270.279 -25.083 1.0 5.072 -1.016 18.5 0.60 31.1 0.0 0.00 0.0 GRS 1758-258 270.296 -25.753 1.4 4.497 -1.361 12.7 0.62 20.5 9.1 0.51 17.9 1E 1740.7-2942 265.970 -29.752 1.4 359.106 -0.103 10.5 0.51 20.6 7.1 0.44 16.2 4U 1700-377 255.967 -37.850 1.4 347.741 +2.182 23.0 1.13 20.4 7.3 0.87 8.4 Ginga 1826-24 277.360 -23.812 2.0 9.256 -6.089 13.9 1.03 13.5 8.0 0.81 9.9 H 1820-303 275.946 -30.354 2.2 2.806 -7.931 8.7 0.70 12.5 0.0 0.00 0.0 GX 354-0 263.001 -33.836 2.4 354.307 -0.159 6.0 0.53 11.3 0.0 0.00 0.0 1A 1742-294 266.492 -29.478 2.5 359.577 -0.347 5.3 0.49 10.8 0.0 0.00 0.0 3A 1822-371 276.443 -37.083 2.9 356.870 -11.280 7.8 0.88 8.9 0.0 0.00 0.0 4U 1722-30 261.873 -30.798 3.3 356.316 +2.312 4.5 0.57 7.9 1.9 0.46 4.2 GX 349+2 256.473 -36.454 3.0 349.097 +2.706 8.3 0.96 8.7 0.0 0.00 0.0 OAO 1657-415 255.174 -41.685 3.9 344.333 +0.319 11.7 1.78 6.6 0.0 0.00 0.0 GRO J1655-40 253.494 -39.879 3.7 344.953 +2.439 10.1 1.47 6.9 6.8 1.16 5.8 GX 17+2 273.981 -14.011 3.7 16.443 +1.311 48.3 6.98 6.9 0.0 0.00 0.0 GX 9+1 270.347 -20.559 5.9 9.033 +1.170 3.9 0.94 4.1 0.0 0.00 0.0 SLX 1744-299_300 266.901 -30.027 6.3 359.292 -0.935 1.9 0.49 3.9 0.0 0.00 0.0 GX 1+4 263.032 -24.742 5.4 1.951 +4.779 3.2 0.70 4.5 0.0 0.00 0.0 SLX 1735-269 264.557 -27.045 6.1 0.746 +2.384 2.3 0.00 4.0 0.0 0.00 0.0 GX 3+1 266.968 -26.529 6.6 2.316 +0.824 2.2 0.60 3.7 0.0 0.00 0.0 AX J1736.4-2910 264.030 -29.087 6.4 358.772 +1.682 1.9 0.00 3.8 0.0 0.00 0.0 1E 1743.1-2843 266.666 -28.716 0.0 0.307 -0.081 1.8 0.00 3.8 0.0 0.00 0.0 SLX 1737-282 265.177 -28.341 7.3 359.940 +1.230 1.7 0.52 3.3 0.0 0.00 0.0 PKS 1830-211 278.386 -21.153 7.4 12.071 -5.728 4.4 1.35 3.2 0.0 0.00 0.0 IGR J17507-2856 267.695 -29.025 6.4 0.506 -1.012 1.7 0.45 3.8 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 with in the 3-10 keV image > 10σ 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).NOTES: Fluxes for light curves are extracted from the images using
mosaic_spec
; 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 354-0 262.989 -33.835 354.302 -0.150 22.2 2.00 5.4 1.34 GX 3+1 266.983 -26.564 2.294 +0.794 18.5 1.06 3.0 0.55 GX 5-1 270.284 -25.079 5.077 -1.019 61.1 3.10 9.9 1.39
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