INTEGRAL Galactic Bulge Monitoring Revolution 0480: Observation start 2006-09-18 = MJD 53996
Total Observation GTI = 12378 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 354-0 262.988 -33.841 0.5 354.297 -0.153 25.7 0.36 71.1 8.4 0.29 29.3 GX 5-1 270.283 -25.078 0.6 5.078 -1.017 19.1 0.31 61.5 0.0 0.00 0.0 4U 1700-377 255.983 -37.848 0.7 347.750 +2.173 33.5 0.64 52.2 10.3 0.49 21.1 GX 1+4 263.015 -24.743 0.7 1.942 +4.792 15.8 0.32 49.2 0.0 0.00 0.0 IGR J17497-2821 267.408 -28.354 1.1 0.954 -0.452 8.5 0.30 28.2 5.3 0.25 21.5 OAO 1657-415 255.196 -41.664 1.1 344.359 +0.319 44.1 1.51 29.2 10.7 1.16 9.2 Ginga 1826-24 277.383 -23.799 1.1 9.277 -6.101 16.5 0.56 29.3 6.9 0.43 16.0 GRS 1758-258 270.313 -25.748 1.3 4.509 -1.373 7.3 0.31 23.2 5.1 0.25 20.2 1E 1740.7-2942 265.984 -29.764 1.4 359.103 -0.120 6.1 0.28 21.5 4.3 0.23 18.5 1A 1742-294 266.532 -29.522 1.4 359.558 -0.399 5.7 0.28 20.6 2.4 0.23 10.7 H 1820-303 275.922 -30.365 1.4 2.786 -7.917 9.7 0.45 21.4 0.0 0.00 0.0 GX 349+2 256.422 -36.401 1.6 349.114 +2.770 10.1 0.58 17.4 0.0 0.00 0.0 3A 1822-371 276.470 -37.093 1.9 356.870 -11.303 8.2 0.57 14.4 0.0 0.00 0.0 GX 9+1 270.374 -20.545 2.2 9.058 +1.154 5.7 0.45 12.6 0.0 0.00 0.0 4U 1722-30 261.885 -30.798 2.3 356.322 +2.303 4.2 0.35 11.7 2.2 0.28 7.8 3A 1728-169 262.983 -16.950 3.0 8.548 +9.004 5.8 0.67 8.6 0.0 0.00 0.0 GX 3+1 267.024 -26.502 3.6 2.365 +0.794 2.3 0.33 7.2 0.0 0.00 0.0 GX 13+1 273.605 -17.111 4.3 13.545 +0.151 4.7 0.81 5.8 0.0 0.00 0.0 GX 17+2 274.020 -14.042 3.9 16.434 +1.263 15.0 2.30 6.5 0.0 0.00 0.0 1E 1742.9-2849 266.573 -28.856 5.3 0.145 -0.084 1.3 0.27 4.7 0.0 0.00 0.0 SLX 1744-299_300 266.862 -30.051 5.2 359.254 -0.919 1.5 0.31 4.8 0.0 0.00 0.0 AX J1749.1-2733 267.278 -27.553 6.6 1.581 +0.059 1.2 0.33 3.7 0.0 0.00 0.0 V2400 Oph 258.253 -24.272 0.0 359.899 +8.649 1.7 0.00 4.0 0.0 0.00 0.0 H 1705-250 257.068 -25.055 5.5 358.621 +9.072 2.2 0.48 4.5 0.0 0.00 0.0 SLX 1735-269 264.517 -26.944 6.7 0.813 +2.468 1.3 0.36 3.6 0.0 0.00 0.0 GRS 1734-292 264.397 -29.067 5.8 358.961 +1.422 1.2 0.30 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 > 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 8.3 1.19 3.5 0.86 GX 3+1 266.983 -26.564 2.294 +0.794 25.9 0.53 3.9 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 89.4 2.22 20.1 1.12 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.7 0.35 0.7 0.26
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