INTEGRAL Galactic Bulge Monitoring Revolution 0482: Observation start 1999-12-31 = MJD 51544
Total Observation GTI = 22765 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 1700-377 255.984 -37.849 0.3 347.750 +2.172 76.6 0.50 152.5 21.6 0.38 57.1 GX 354-0 262.986 -33.834 0.4 354.301 -0.148 25.5 0.25 103.5 6.8 0.20 34.5 IGR J17497-2821 267.408 -28.349 0.5 0.958 -0.450 15.8 0.22 70.4 10.7 0.18 58.1 GX 1+4 263.007 -24.741 0.6 1.940 +4.799 14.4 0.23 62.9 0.0 0.00 0.0 Ginga 1826-24 277.378 -23.797 0.8 9.277 -6.096 16.9 0.41 41.6 6.4 0.31 20.5 H 1820-303 275.922 -30.357 0.8 2.793 -7.914 12.0 0.31 38.8 0.0 0.00 0.0 GX 5-1 270.288 -25.095 0.9 5.065 -1.029 8.8 0.26 34.0 0.0 0.00 0.0 GX 349+2 256.438 -36.421 1.0 349.106 +2.748 13.4 0.41 32.6 0.0 0.00 0.0 1E 1740.7-2942 265.988 -29.749 1.0 359.117 -0.115 6.5 0.21 31.1 4.4 0.17 25.5 GRS 1758-258 270.295 -25.733 1.1 4.514 -1.351 6.7 0.24 28.1 4.6 0.19 24.1 1A 1742-294 266.513 -29.510 1.1 359.559 -0.379 5.8 0.20 28.6 1.9 0.17 11.4 4U 1722-30 261.885 -30.789 1.7 356.329 +2.307 3.9 0.24 16.4 1.8 0.19 9.8 3A 1822-371 276.438 -37.090 1.9 356.862 -11.279 6.4 0.43 14.7 0.0 0.00 0.0 OAO 1657-415 255.207 -41.663 2.2 344.365 +0.313 12.3 1.00 12.3 4.2 0.75 5.5 GX 17+2 274.013 -14.029 2.5 16.441 +1.275 20.7 1.91 10.9 0.0 0.00 0.0 GX 9+1 270.406 -20.511 2.8 9.102 +1.145 3.4 0.35 9.5 0.0 0.00 0.0 GX 3+1 266.966 -26.545 2.7 2.302 +0.817 2.2 0.23 9.9 0.0 0.00 0.0 GRS 1734-292 264.352 -29.145 3.1 358.874 +1.413 2.1 0.24 8.4 1.1 0.20 5.7 SLX 1744-299_300 266.896 -30.020 0.0 359.296 -0.928 1.6 0.00 7.4 0.0 0.00 0.0 SLX 1735-269 264.586 -26.999 3.7 0.799 +2.387 1.6 0.24 6.8 0.8 0.20 3.9 IGR J17252-3616 261.290 -36.395 0.0 351.401 -0.412 2.0 0.00 6.4 0.0 0.00 0.0 IGR J18027-2016 270.734 -20.319 0.0 9.421 +0.973 2.3 0.00 6.3 0.0 0.00 0.0 3A 1728-169 262.935 -16.966 4.4 8.510 +9.035 3.2 0.57 5.6 0.0 0.00 0.0 IGR J17475-2822 266.693 -28.473 4.8 0.527 +0.025 1.1 0.00 5.2 0.0 0.00 0.0 SLX 1737-282 265.198 -28.330 5.1 359.959 +1.220 1.0 0.21 4.8 0.9 0.17 5.1 IGR J17456-2901 266.392 -28.944 0.0 359.987 +0.006 0.9 0.00 4.5 0.0 0.00 0.0 1RXS J174607.8-21333 266.541 -21.654 5.2 6.290 +3.679 1.3 0.28 4.7 0.0 0.00 0.0 GX 13+1 273.639 -17.169 4.8 13.510 +0.095 3.3 0.62 5.2 0.0 0.00 0.0 NEW_0365 250.455 -34.454 4.8 347.571 +7.776 4.3 0.82 5.2 0.0 0.00 0.0 KS 1741-293 266.093 -29.334 0.0 359.519 +0.025 0.8 0.00 3.9 0.0 0.00 0.0 XB 1832-330 278.894 -33.035 5.1 1.476 -11.361 2.1 0.43 4.8 0.0 0.00 0.0 IGR J17204-3554 260.120 -35.898 6.4 351.275 +0.648 1.2 0.32 3.8 0.0 0.00 0.0 IGR J17254-3257 261.299 -32.981 7.8 354.231 +1.497 0.7 0.24 3.1 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 > 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.8 0.35 0.9 0.17 GX 354-0 262.989 -33.835 354.302 -0.150 15.4 0.99 5.4 0.68 1A 1742-294 266.523 -29.515 359.559 -0.389 1.4 0.22 0.7 0.14 GX 3+1 266.983 -26.564 2.294 +0.794 27.1 0.47 3.5 0.25 GX 5-1 270.284 -25.079 5.077 -1.019 93.1 1.98 9.7 0.86 IGR J17497-2821 267.404 -28.358 0.949 -0.451 3.1 0.30 1.8 0.19 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.25 0.5 0.17
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