INTEGRAL Galactic Bulge Monitoring Revolution 0407: Observation start 2006-02-11 = MJD 53777
Total Observation GTI = 12317 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 -37.843 0.5 347.754 +2.177 42.7 0.57 75.5 10.2 0.44 23.4 GX 5-1 270.281 -25.077 0.7 5.077 -1.015 17.1 0.31 54.9 1.2 0.25 4.9 GRS 1758-258 270.297 -25.746 0.9 4.504 -1.359 11.8 0.34 35.2 7.1 0.27 26.0 GX 1+4 263.010 -24.753 0.8 1.931 +4.791 11.8 0.30 39.2 0.0 0.00 0.0 Ginga 1826-24 277.363 -23.804 0.9 9.264 -6.088 17.9 0.52 34.6 7.8 0.40 19.3 XTE J1817-330 274.419 -33.012 1.2 359.818 -7.983 10.1 0.39 25.8 4.1 0.31 13.2 1A 1742-294 266.524 -29.521 1.5 359.555 -0.393 5.5 0.28 19.9 1.3 0.23 5.4 GX 349+2 256.439 -36.429 1.7 349.101 +2.742 8.6 0.51 16.9 0.0 0.00 0.0 H 1820-303 275.925 -30.393 1.8 2.762 -7.932 6.5 0.41 15.6 0.0 0.00 0.0 3A 1822-371 276.458 -37.115 2.0 356.846 -11.305 7.5 0.54 13.8 0.0 0.00 0.0 GX 354-0 262.991 -33.841 2.0 354.298 -0.155 4.6 0.33 14.0 0.0 0.00 0.0 4U 1722-30 261.861 -30.789 2.4 356.318 +2.325 3.1 0.28 11.0 1.6 0.23 7.0 OAO 1657-415 255.192 -41.682 2.5 344.343 +0.310 14.8 1.37 10.7 0.0 0.00 0.0 GX 17+2 273.973 -14.043 2.6 16.411 +1.302 19.6 1.92 10.2 0.0 0.00 0.0 SLX 1735-269 264.591 -26.995 2.7 0.805 +2.385 2.6 0.27 9.7 1.4 0.22 6.3 GX 9+1 270.377 -20.551 3.2 9.054 +1.149 3.3 0.41 8.0 0.0 0.00 0.0 GX 3+1 266.998 -26.565 3.0 2.299 +0.782 2.6 0.30 8.7 0.0 0.00 0.0 1E 1742.8-2853 266.437 -28.945 4.1 0.007 -0.028 1.6 0.25 6.2 0.0 0.00 0.0 GX 13+1 273.643 -17.117 3.6 13.557 +0.116 5.5 0.78 7.0 0.0 0.00 0.0 SLX 1744-299_300 266.855 -30.029 4.7 359.269 -0.902 1.6 0.31 5.3 0.0 0.00 0.0 XB 1832-330 278.940 -32.991 3.8 1.534 -11.377 3.7 0.56 6.6 0.0 0.00 0.0 3A 1728-169 262.883 -16.930 5.6 8.514 +9.096 2.9 0.67 4.4 0.0 0.00 0.0 4U 1735-444 264.743 -44.454 5.0 346.051 -6.996 14.0 2.86 4.9 0.0 0.00 0.0 XTE J1739-285 265.085 -28.427 4.8 359.825 +1.253 1.5 0.29 5.2 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 > 10σ 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).NOTES: Fluxes for light curves are extracted from the images using
mosaic_spec
; 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== XTE J1739-285 264.975 -28.496 359.714 +1.298 6.6 0.39 1.1 0.23 GRS 1747-312 267.690 -31.292 358.555 -2.168 3.4 0.52 1.0 0.32 GX 354-0 262.989 -33.835 354.302 -0.150 18.6 1.55 3.5 0.92 GX 3+1 266.983 -26.564 2.294 +0.794 23.7 0.57 3.8 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 106.5 2.26 19.8 1.07
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