INTEGRAL Galactic Bulge Monitoring Revolution 0409: Observation start 2006-02-17 = MJD 53783
Total Observation GTI = 12264 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 1700-377 255.992 -37.846 0.4 347.755 +2.169 71.1 0.64 110.4 20.8 0.50 41.8 GRS 1758-258 270.289 -25.753 0.9 4.494 -1.356 10.5 0.28 37.2 6.1 0.23 26.2 GX 5-1 270.287 -25.092 0.9 5.067 -1.027 10.2 0.30 34.2 0.0 0.00 0.0 Ginga 1826-24 277.358 -23.793 1.0 9.272 -6.078 17.7 0.54 32.5 7.5 0.44 17.1 GX 1+4 263.004 -24.753 1.0 1.929 +4.795 10.0 0.31 32.2 0.0 0.00 0.0 1A 1742-294 266.512 -29.517 1.1 359.553 -0.382 7.2 0.26 27.8 2.2 0.22 10.0 XTE J1817-330 274.422 -33.021 1.3 359.811 -7.989 8.9 0.40 22.3 4.2 0.32 13.2 OAO 1657-415 255.166 -41.669 1.6 344.341 +0.333 21.1 1.23 17.2 6.8 0.91 7.5 GX 349+2 256.417 -36.403 1.9 349.111 +2.772 7.8 0.52 14.9 0.0 0.00 0.0 H 1820-303 275.908 -30.366 1.7 2.779 -7.907 6.6 0.41 16.2 0.0 0.00 0.0 GX 354-0 262.986 -33.829 1.8 354.306 -0.145 5.4 0.34 15.8 0.0 0.00 0.0 3A 1822-371 276.427 -37.125 2.3 356.825 -11.287 7.2 0.60 11.9 0.0 0.00 0.0 GX 17+2 274.010 -14.020 2.5 16.449 +1.282 18.5 1.77 10.5 0.0 0.00 0.0 IGR J17252-3616 261.300 -36.305 2.4 351.480 -0.368 4.5 0.41 11.1 0.0 0.00 0.0 SLX 1735-269 264.530 -26.992 3.0 0.778 +2.433 2.7 0.31 8.6 0.0 0.00 0.0 SLX 1744-299_300 266.876 -30.076 0.0 359.238 -0.942 2.6 0.00 9.0 1.0 0.24 4.2 4U 1722-30 261.875 -30.807 3.6 356.309 +2.305 2.4 0.34 7.2 1.7 0.28 6.3 GX 9+1 270.415 -20.490 3.8 9.124 +1.148 2.8 0.42 6.7 0.0 0.00 0.0 XB 1832-330 278.904 -33.010 3.5 1.503 -11.357 3.9 0.54 7.2 0.0 0.00 0.0 IGR J17456-2901 266.400 -29.008 0.0 359.937 -0.034 1.7 0.00 6.8 0.0 0.00 0.0 3A 1728-169 262.957 -16.964 3.9 8.522 +9.018 4.0 0.62 6.6 0.0 0.00 0.0 GX 13+1 273.661 -17.112 3.9 13.570 +0.103 4.6 0.70 6.6 0.0 0.00 0.0 GX 3+1 266.988 -26.632 4.7 2.237 +0.755 1.5 0.28 5.3 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 0.40 1.3 0.24 GX 354-0 262.989 -33.835 354.302 -0.150 20.9 1.54 4.7 0.96 GX 3+1 266.983 -26.564 2.294 +0.794 19.8 0.56 2.9 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 111.8 2.27 14.4 1.01
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