INTEGRAL Galactic Bulge Monitoring Revolution 0533: Observation start 2007-02-23 = MJD 54154
Total Observation GTI = 12432 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 1700-377 255.980 -37.845 0.5 347.751 +2.177 47.4 0.61 77.1 17.1 0.48 35.7 GX 1+4 263.002 -24.745 0.7 1.934 +4.800 17.3 0.35 49.6 0.0 0.00 0.0 1E 1740.7-2942 265.979 -29.755 0.9 359.108 -0.111 10.5 0.28 37.5 6.7 0.24 28.5 GRS 1758-258 270.303 -25.749 1.0 4.503 -1.365 11.7 0.36 32.2 7.9 0.30 26.5 Ginga 1826-24 277.359 -23.800 1.1 9.266 -6.082 17.1 0.64 26.9 6.4 0.50 12.8 GX 5-1 270.288 -25.086 1.3 5.073 -1.025 7.9 0.36 21.8 0.0 0.00 0.0 OAO 1657-415 255.203 -41.660 1.5 344.366 +0.317 19.9 1.03 19.4 5.3 0.78 6.7 H 1820-303 275.918 -30.368 1.5 2.781 -7.916 9.3 0.48 19.4 0.0 0.00 0.0 GX 3+1 266.979 -26.575 1.7 2.282 +0.791 4.8 0.29 16.3 0.0 0.00 0.0 GX 354-0 262.978 -33.844 2.0 354.289 -0.147 4.5 0.33 13.8 0.0 0.00 0.0 GX 349+2 256.450 -36.386 2.0 349.141 +2.762 6.6 0.49 13.6 0.0 0.00 0.0 4U 1722-30 261.881 -30.812 2.1 356.308 +2.298 4.0 0.31 12.9 2.0 0.26 7.6 3A 1822-371 276.429 -37.092 2.5 356.856 -11.273 7.1 0.65 10.9 0.0 0.00 0.0 SLX 1744-299_300 266.863 -30.019 2.8 359.282 -0.903 2.5 0.27 9.3 0.9 0.23 4.1 GX 9+1 270.417 -20.511 3.4 9.107 +1.136 3.6 0.48 7.5 0.0 0.00 0.0 SLX 1735-269 264.546 -26.992 3.7 0.786 +2.421 2.1 0.30 6.9 1.4 0.00 5.6 1E 1742.8-2853 266.590 -28.933 0.0 0.087 -0.136 1.5 0.00 5.4 0.0 0.00 0.0 1A 1742-294 266.541 -29.487 4.1 359.592 -0.388 1.7 0.28 6.1 0.0 0.00 0.0 H 1702-429 256.504 -43.033 6.1 343.862 -1.282 5.9 1.47 4.0 0.0 0.00 0.0 GRS 1734-292 264.395 -29.087 5.2 358.943 +1.413 1.4 0.29 4.8 0.0 0.00 0.0 GRS 1741.9-2853 266.214 -28.934 0.0 359.914 +0.144 1.3 0.00 4.5 0.0 0.00 0.0 SLX 1737-282 265.180 -28.295 5.5 359.981 +1.252 1.3 0.30 4.5 0.0 0.00 0.0 XTE J1743-363 265.703 -36.308 5.6 353.403 -3.350 1.8 0.41 4.4 0.0 0.00 0.0 IGR J17254-3257 261.345 -32.967 6.5 354.265 +1.474 1.3 0.00 3.7 0.0 0.00 0.0 Oph Cluster 258.104 -23.418 0.0 0.527 +9.251 1.6 0.00 3.6 0.0 0.00 0.0 GX 13+1 273.534 -17.115 6.8 13.510 +0.209 3.0 0.00 3.6 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 14.9 1.14 3.6 0.71 GX 3+1 266.983 -26.564 2.294 +0.794 33.7 0.67 5.0 0.35 GX 5-1 270.284 -25.079 5.077 -1.019 77.5 2.67 9.1 1.17
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