INTEGRAL Galactic Bulge Monitoring Revolution 0489: Observation start 2006-10-17 = MJD 54025
Total Observation GTI = 12410 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 1+4 263.009 -24.745 0.5 1.937 +4.795 25.2 0.34 73.0 0.0 0.00 0.0 4U 1700-377 255.990 -37.846 0.6 347.755 +2.170 35.3 0.62 57.1 9.6 0.47 20.4 GX 354-0 262.992 -33.835 0.8 354.303 -0.152 15.9 0.36 44.3 3.4 0.29 11.6 GX 5-1 270.286 -25.073 0.8 5.083 -1.017 13.8 0.35 38.9 0.0 0.00 0.0 GX 349+2 256.447 -36.426 0.9 349.107 +2.739 18.2 0.54 33.5 0.0 0.00 0.0 Ginga 1826-24 277.370 -23.795 1.0 9.276 -6.089 16.5 0.54 30.5 6.8 0.41 16.7 GRS 1758-258 270.313 -25.735 1.2 4.520 -1.366 7.4 0.30 24.4 5.4 0.25 21.8 H 1820-303 275.920 -30.362 1.1 2.787 -7.915 11.3 0.43 26.3 0.0 0.00 0.0 1E 1740.7-2942 265.971 -29.746 1.2 359.112 -0.101 7.5 0.29 25.5 5.1 0.24 21.0 IGR J17497-2821 267.388 -28.351 1.4 0.947 -0.435 6.5 0.32 20.2 4.4 0.27 16.3 4U 1722-30 261.876 -30.779 2.3 356.333 +2.320 3.8 0.32 11.8 2.1 0.25 8.4 3A 1822-371 276.444 -37.105 2.1 356.850 -11.290 7.6 0.59 12.8 0.0 0.00 0.0 GX 3+1 266.989 -26.579 2.4 2.283 +0.781 3.2 0.29 10.9 0.0 0.00 0.0 GX 9+1 270.395 -20.550 2.7 9.063 +1.135 4.6 0.47 9.7 0.0 0.00 0.0 1A 1742-294 266.510 -29.525 3.1 359.545 -0.385 2.7 0.32 8.3 0.0 0.00 0.0 GX 13+1 273.661 -17.179 4.1 13.511 +0.072 4.6 0.75 6.2 0.0 0.00 0.0 GX 17+2 274.050 -14.032 4.1 16.456 +1.242 18.2 2.96 6.1 0.0 0.00 0.0 SLX 1735-269 264.574 -26.961 3.9 0.825 +2.416 2.1 0.32 6.5 0.0 0.00 0.0 OAO 1657-415 255.197 -41.635 5.6 344.382 +0.336 6.3 1.44 4.4 0.0 0.00 0.0 SLX 1744-299_300 266.976 -30.014 5.1 359.337 -0.984 1.4 0.29 4.9 0.0 0.00 0.0 IGR J16500-3307 252.518 -33.217 4.8 349.638 +7.258 3.6 0.69 5.2 0.0 0.00 0.0 IGR J18027-2016 270.731 -20.298 0.0 9.438 +0.985 2.3 0.00 5.0 0.0 0.00 0.0 H 1702-429 256.498 -43.015 5.1 343.874 -1.268 10.4 2.17 4.8 0.0 0.00 0.0 XTE J1818-245 274.652 -24.503 5.7 7.495 -4.215 1.8 0.41 4.3 0.0 0.00 0.0 IGR J17204-3554 260.169 -35.806 0.0 351.374 +0.668 1.7 0.00 4.1 0.0 0.00 0.0 1E 1742.9-2849 266.471 -28.840 7.6 0.112 +0.001 0.8 0.27 3.1 0.0 0.00 0.0 Oph Cluster 258.062 -23.290 0.0 0.611 +9.356 1.8 0.00 3.9 0.0 0.00 0.0 XB 1832-330 278.831 -32.995 6.2 1.491 -11.296 2.2 0.57 3.9 0.0 0.00 0.0 IGR J16482-3036 252.041 -30.558 8.2 351.459 +9.253 2.3 0.80 2.9 0.0 0.00 0.0 IGR J17391-3021 264.825 -30.321 6.7 358.100 +0.438 1.0 0.28 3.6 0.0 0.00 0.0 3A 1728-169 263.039 -16.899 7.1 8.620 +8.986 2.4 0.00 3.4 0.0 0.00 0.0 SLX 1737-282 265.253 -28.316 7.9 359.996 +1.186 1.0 0.32 3.0 0.0 0.00 0.0 V2400 Oph 258.101 -24.250 8.6 359.837 +8.775 1.2 0.44 2.8 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 > 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 354-0 262.989 -33.835 354.302 -0.150 7.7 1.19 3.3 0.91 GX 3+1 266.983 -26.564 2.294 +0.794 30.9 0.58 4.4 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 118.7 2.35 19.5 1.14 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.35 0.4 0.27
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