INTEGRAL Galactic Bulge Monitoring Revolution 0415: Observation start 2006-03-08 = MJD 53802
Total Observation GTI = 12325 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 5-1 270.288 -25.083 0.7 5.076 -1.024 17.3 0.35 49.5 0.0 0.00 0.0 GX 354-0 262.997 -33.831 0.7 354.309 -0.153 15.2 0.33 46.1 2.8 0.27 10.6 GX 349+2 256.423 -36.421 0.9 349.099 +2.758 17.9 0.52 34.5 0.0 0.00 0.0 GX 1+4 263.013 -24.750 0.9 1.935 +4.789 12.7 0.35 36.5 0.0 0.00 0.0 Ginga 1826-24 277.372 -23.798 1.0 9.274 -6.092 16.7 0.53 31.7 5.9 0.40 14.5 GRS 1758-258 270.295 -25.747 1.1 4.502 -1.357 9.6 0.34 28.2 7.3 0.28 26.5 1A 1742-294 266.509 -29.515 1.5 359.553 -0.378 5.1 0.26 19.4 1.8 0.22 8.1 H 1820-303 275.884 -30.344 2.0 2.790 -7.879 5.4 0.40 13.5 0.0 0.00 0.0 1A 1743-288 266.718 -28.909 2.7 0.166 -0.220 2.5 0.26 9.6 0.0 0.00 0.0 3A 1822-371 276.426 -37.106 2.5 356.843 -11.278 5.6 0.54 10.5 0.0 0.00 0.0 GX 9+1 270.375 -20.548 2.7 9.056 +1.152 3.9 0.40 9.7 0.0 0.00 0.0 4U 1722-30 261.883 -30.799 2.9 356.320 +2.303 2.9 0.31 9.1 0.0 0.00 0.0 XTE J1817-330 274.395 -33.028 3.2 359.795 -7.972 3.1 0.39 8.0 1.3 0.31 4.0 4U 1700-377 255.940 -37.839 3.5 347.736 +2.206 4.0 0.55 7.2 0.0 0.00 0.0 SLX 1735-269 264.482 -26.949 3.0 0.792 +2.492 2.5 0.29 8.7 1.1 0.24 4.8 GX 3+1 266.948 -26.578 3.7 2.266 +0.813 2.0 0.29 7.0 0.0 0.00 0.0 SLX 1744-299_300 266.834 -30.029 4.8 359.260 -0.886 1.4 0.27 5.2 0.0 0.00 0.0 GX 17+2 274.007 -14.051 5.2 16.420 +1.270 10.5 2.22 4.7 0.0 0.00 0.0 GX 13+1 273.591 -17.112 5.0 13.538 +0.162 3.6 0.72 5.0 0.0 0.00 0.0 GRS 1747-312 267.749 -31.385 5.7 358.501 -2.259 1.3 0.00 4.3 0.0 0.00 0.0 IGR J18135-1751 273.413 -17.827 0.0 12.829 -0.031 2.6 0.00 4.2 0.0 0.00 0.0 IGR J17507-2856 267.591 -28.992 7.1 0.488 -0.917 0.9 0.27 3.4 0.0 0.00 0.0 NEW_1 278.401 -15.349 3.9 17.258 -3.095 11.7 1.80 6.5 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 9.9 1.25 3.3 0.86 GX 3+1 266.983 -26.564 2.294 +0.794 24.4 0.51 3.3 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 93.8 1.99 17.4 0.97
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