INTEGRAL Galactic Bulge Monitoring Revolution 0294: Observation start 2005-03-10 = MJD 53439
Total Observation GTI = 12287 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.985 -37.846 0.4 347.753 +2.173 74.7 0.58 127.9 22.8 0.44 51.7 GRO J1655-40 253.495 -39.842 0.6 344.982 +2.462 69.3 1.05 66.0 31.7 0.76 41.9 GX 5-1 270.285 -25.079 0.6 5.078 -1.019 20.2 0.30 67.4 0.0 0.00 0.0 GRS 1758-258 270.299 -25.741 0.9 4.508 -1.358 12.0 0.31 38.4 7.8 0.25 31.4 1E 1740.7-2942 265.985 -29.753 0.8 359.112 -0.114 9.9 0.26 38.5 6.5 0.21 30.4 Ginga 1826-24 277.366 -23.780 1.0 9.287 -6.079 16.7 0.52 32.0 5.6 0.40 14.1 1A 1742-294 266.503 -29.508 1.6 359.557 -0.371 4.8 0.26 18.2 1.7 0.22 7.7 GX 354-0 262.988 -33.823 1.6 354.311 -0.143 5.4 0.29 18.4 0.0 0.00 0.0 GX 349+2 256.431 -36.414 1.9 349.109 +2.757 7.3 0.51 14.3 0.0 0.00 0.0 OAO 1657-415 255.196 -41.634 1.8 344.383 +0.337 19.5 1.26 15.5 4.5 0.91 4.9 4U 1722-30 261.883 -30.790 2.0 356.328 +2.309 4.6 0.33 13.7 1.4 0.27 5.0 H 1820-303 275.963 -30.353 2.0 2.813 -7.943 5.5 0.40 14.0 0.0 0.00 0.0 3A 1822-371 276.438 -37.116 2.5 356.838 -11.291 5.9 0.55 10.7 0.0 0.00 0.0 GX 9+1 270.425 -20.478 2.8 9.140 +1.146 3.6 0.38 9.3 0.0 0.00 0.0 SLX 1735-269 264.580 -26.963 2.8 0.827 +2.410 2.8 0.30 9.2 1.0 0.25 4.1 GX 1+4 262.981 -24.782 2.7 1.892 +4.796 2.8 0.29 9.7 0.0 0.00 0.0 GX 17+2 274.033 -14.013 3.2 16.465 +1.265 15.0 1.83 8.2 0.0 0.00 0.0 GX 3+1 267.004 -26.549 3.4 2.316 +0.785 2.4 0.32 7.5 0.0 0.00 0.0 3A 1728-169 262.927 -16.951 3.5 8.518 +9.049 5.0 0.68 7.3 0.0 0.00 0.0 IGR J17456-2901 266.453 -29.028 3.9 359.944 -0.083 1.6 0.25 6.4 0.0 0.00 0.0 SLX 1744-299_300 266.839 -30.020 5.1 359.271 -0.886 1.4 0.28 4.9 0.9 0.23 3.8 SAX J1712.6-3739 258.038 -37.707 4.7 348.835 +0.956 3.1 0.58 5.3 0.0 0.00 0.0 4U 1735-444 264.761 -44.514 4.9 346.006 -7.039 14.4 0.00 5.1 0.0 0.00 0.0 IGR J18027-2016 270.769 -20.239 0.0 9.506 +0.983 1.9 0.00 4.7 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 24.1 1.53 5.5 1.13 GX 3+1 266.983 -26.564 2.294 +0.794 24.9 0.52 3.7 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 88.1 2.03 17.5 1.01
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