INTEGRAL Galactic Bulge Monitoring Revolution 0425: Observation start 2006-04-06 = MJD 53831
Total Observation GTI = 12326 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 1700-377 255.985 -37.838 0.4 347.758 +2.178 66.4 0.59 112.2 19.6 0.45 43.2 GRS 1758-258 270.306 -25.740 1.0 4.512 -1.363 10.9 0.34 32.4 7.8 0.28 28.0 GX 1+4 263.007 -24.740 0.9 1.941 +4.799 11.1 0.30 36.6 0.0 0.00 0.0 Ginga 1826-24 277.372 -23.795 1.0 9.276 -6.091 17.4 0.53 32.7 6.9 0.42 16.6 GX 349+2 256.433 -36.411 1.3 349.113 +2.757 11.7 0.53 21.9 0.0 0.00 0.0 H 1820-303 275.925 -30.366 1.7 2.787 -7.921 6.9 0.41 16.9 0.0 0.00 0.0 GX 354-0 262.975 -33.812 1.9 354.315 -0.128 4.9 0.34 14.1 0.0 0.00 0.0 3A 1822-371 276.459 -37.077 2.4 356.881 -11.288 6.2 0.56 10.9 0.0 0.00 0.0 GX 5-1 270.247 -25.095 2.4 5.046 -0.997 3.5 0.31 11.3 0.0 0.00 0.0 4U 1722-30 261.891 -30.805 2.6 356.318 +2.294 3.4 0.34 10.0 1.5 0.28 5.4 GX 3+1 266.963 -26.569 2.7 2.280 +0.807 2.8 0.29 9.8 0.0 0.00 0.0 GX 9+1 270.331 -20.603 3.0 8.987 +1.161 3.5 0.40 8.8 0.0 0.00 0.0 SLX 1735-269 264.554 -26.967 2.9 0.811 +2.428 2.8 0.31 8.9 1.2 0.27 4.5 XTE J1817-330 274.391 -33.007 3.9 359.813 -7.960 2.5 0.39 6.5 1.7 0.31 5.5 IGR J17456-2901 266.414 -29.006 5.0 359.945 -0.043 1.3 0.26 4.9 0.0 0.00 0.0 3A 1728-169 262.955 -16.897 5.3 8.579 +9.055 3.2 0.00 4.6 0.0 0.00 0.0 XB 1832-330 278.981 -32.982 4.9 1.557 -11.404 3.1 0.62 5.0 0.0 0.00 0.0 GX 13+1 273.644 -17.145 5.4 13.534 +0.102 3.4 0.75 4.5 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1743-288 266.761 -28.883 0.207 -0.238 7.0 0.37 0.6 0.19 GX 354-0 262.989 -33.835 354.302 -0.150 18.4 1.56 4.4 1.01 1A 1742-294 266.523 -29.515 359.559 -0.389 3.1 0.35 0.8 0.21 GX 3+1 266.983 -26.564 2.294 +0.794 21.3 0.54 3.0 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 81.1 2.11 5.2 0.83 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.8 0.43 0.6 0.22
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