INTEGRAL Galactic Bulge Monitoring Revolution 0476: Observation start 2006-09-06 = MJD 53984
Total Observation GTI = 12086 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 1700-377 255.983 -37.846 0.5 347.751 +2.174 52.8 0.63 83.6 18.0 0.47 38.0 GX 354-0 262.984 -33.832 0.6 354.303 -0.145 19.3 0.33 58.7 3.8 0.26 14.7 GX 5-1 270.278 -25.084 0.7 5.070 -1.016 15.4 0.31 49.6 0.0 0.00 0.0 GX 1+4 263.015 -24.750 0.8 1.937 +4.788 15.3 0.34 44.5 0.0 0.00 0.0 GX 349+2 256.415 -36.419 1.0 349.097 +2.764 17.8 0.57 31.1 0.0 0.00 0.0 Ginga 1826-24 277.379 -23.804 1.0 9.271 -6.101 17.3 0.55 31.3 5.0 0.42 12.0 1A 1742-294 266.516 -29.533 1.3 359.541 -0.393 6.1 0.27 22.6 2.7 0.22 12.4 GRS 1758-258 270.308 -25.745 1.3 4.509 -1.367 6.8 0.31 22.2 4.2 0.24 17.2 1E 1740.7-2942 265.994 -29.755 1.5 359.115 -0.123 5.1 0.27 18.6 3.3 0.22 14.7 4U 1722-30 261.879 -30.812 2.2 356.307 +2.300 3.8 0.30 12.4 1.7 0.24 7.1 H 1820-303 275.929 -30.344 2.1 2.808 -7.914 6.0 0.45 13.3 0.0 0.00 0.0 GX 3+1 267.004 -26.614 2.5 2.260 +0.752 2.9 0.28 10.5 0.0 0.00 0.0 3A 1822-371 276.442 -37.119 2.5 356.837 -11.295 6.0 0.58 10.5 0.0 0.00 0.0 GX 9+1 270.375 -20.533 3.2 9.069 +1.159 3.6 0.45 8.0 0.0 0.00 0.0 GX 17+2 274.043 -14.046 2.5 16.441 +1.241 22.0 2.10 10.5 0.0 0.00 0.0 SLX 1735-269 264.514 -26.990 3.4 0.772 +2.446 2.1 0.28 7.6 0.0 0.00 0.0 SLX 1744-299_300 266.887 -30.029 3.8 359.284 -0.926 1.8 0.27 6.8 0.0 0.00 0.0 GX 13+1 273.630 -17.168 4.3 13.507 +0.103 4.3 0.75 5.8 0.0 0.00 0.0 3A 1728-169 262.981 -16.954 4.8 8.543 +9.004 3.4 0.67 5.1 0.0 0.00 0.0 1E 1742.9-2849 266.522 -28.864 5.9 0.115 -0.050 1.1 0.27 4.1 0.0 0.00 0.0 GRS 1734-292 264.390 -29.204 5.4 358.842 +1.354 1.2 0.28 4.5 0.0 0.00 0.0 4U 1705-32 257.313 -32.335 7.3 352.822 +4.611 1.4 0.44 3.3 0.0 0.00 0.0 SAX J1712.6-3739 258.190 -37.537 7.0 349.043 +0.959 1.8 0.54 3.4 2.4 0.41 5.8 IGR J18027-2016 270.643 -20.219 0.0 9.466 +1.096 1.7 0.00 3.6 0.0 0.00 0.0 SLX 1737-282 265.130 -28.335 6.5 359.923 +1.268 1.0 0.27 3.7 0.0 0.00 0.0 NEW_1 258.203 -18.491 4.0 4.705 +11.975 4.1 0.65 6.4 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 12.0 1.42 4.4 1.02 GX 3+1 266.983 -26.564 2.294 +0.794 27.8 0.56 3.7 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 123.5 2.37 21.3 1.15 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.29 0.5 0.21
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