INTEGRAL Galactic Bulge Monitoring Revolution 0302: Observation start 2005-04-03 = MJD 53463
Total Observation GTI = 12314 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 1700-377 255.981 -37.846 0.5 347.750 +2.176 48.7 0.69 70.4 13.9 0.51 27.2 GRS 1758-258 270.309 -25.747 0.8 4.508 -1.368 12.7 0.29 44.2 9.0 0.23 38.3 GX 349+2 256.437 -36.418 0.9 349.108 +2.750 17.6 0.52 33.9 0.0 0.00 0.0 1E 1740.7-2942 265.983 -29.739 1.1 359.123 -0.106 8.4 0.29 29.0 4.7 0.24 19.3 Ginga 1826-24 277.376 -23.805 1.1 9.269 -6.099 14.0 0.50 27.7 6.4 0.40 16.0 OAO 1657-415 255.197 -41.652 1.3 344.369 +0.325 30.1 1.28 23.5 6.5 0.96 6.8 1A 1742-294 266.495 -29.500 0.0 359.559 -0.360 4.7 0.00 16.6 2.4 0.24 10.1 GX 354-0 262.983 -33.838 1.6 354.297 -0.147 5.8 0.33 17.5 0.0 0.00 0.0 GX 5-1 270.278 -25.100 1.8 5.057 -1.024 5.1 0.32 15.8 0.0 0.00 0.0 GX 9+1 270.395 -20.544 2.0 9.068 +1.137 5.5 0.40 13.7 0.0 0.00 0.0 H 1820-303 275.931 -30.361 1.9 2.793 -7.923 5.8 0.39 14.8 0.0 0.00 0.0 GX 1+4 263.020 -24.731 2.1 1.955 +4.794 3.7 0.29 13.1 0.0 0.00 0.0 4U 1722-30 261.870 -30.783 2.2 356.327 +2.321 3.9 0.32 12.2 2.3 0.26 8.8 IGR J17252-3616 261.307 -36.289 2.0 351.496 -0.364 5.1 0.36 14.0 0.0 0.00 0.0 3A 1822-371 276.421 -37.095 2.6 356.851 -11.269 5.7 0.56 10.1 0.0 0.00 0.0 XTE J1743-363 265.767 -36.363 2.7 353.383 -3.423 3.3 0.34 9.6 0.0 0.00 0.0 GX 3+1 266.945 -26.554 3.4 2.285 +0.828 2.2 0.30 7.6 0.0 0.00 0.0 GX 17+2 274.036 -14.045 3.3 16.438 +1.248 15.8 2.06 7.7 0.0 0.00 0.0 SLX 1744-299_300 266.884 -30.048 3.6 359.266 -0.933 1.9 0.28 7.0 0.0 0.00 0.0 SLX 1735-269 264.574 -26.992 3.2 0.799 +2.399 2.1 0.26 8.0 1.3 0.23 5.8 1E 1742.8-2853 266.385 -28.893 4.5 0.028 +0.037 1.3 0.24 5.5 0.0 0.00 0.0 GX 13+1 273.677 -17.206 4.2 13.494 +0.045 4.6 0.78 6.0 0.0 0.00 0.0 KS 1741-293 266.117 -29.418 0.0 359.458 -0.037 1.2 0.00 4.6 0.0 0.00 0.0 V1223 Sgr 283.790 -31.193 5.0 4.941 -14.390 9.2 1.88 4.9 0.0 0.00 0.0 3A 1728-169 262.900 -16.904 4.9 8.545 +9.096 3.1 0.61 5.0 0.0 0.00 0.0 XTE J1818-245 274.557 -24.522 5.9 7.439 -4.148 1.6 0.37 4.2 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 23.7 1.49 5.0 1.00 1A 1742-294 266.523 -29.515 359.559 -0.389 1.5 0.28 0.9 0.20 GX 3+1 266.983 -26.564 2.294 +0.794 25.1 0.50 4.5 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 87.5 2.02 6.4 0.81
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