INTEGRAL Galactic Bulge Monitoring Revolution 0424: Observation start 2006-04-03 = MJD 53828
Total Observation GTI = 12363 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 -37.847 0.4 347.752 +2.173 95.9 0.72 133.9 27.3 0.55 49.7 GRS 1758-258 270.302 -25.736 0.9 4.514 -1.358 10.6 0.30 35.0 7.8 0.24 32.1 Ginga 1826-24 277.375 -23.791 1.0 9.280 -6.091 16.5 0.54 30.6 6.4 0.41 15.5 GX 1+4 263.002 -24.746 1.0 1.934 +4.800 10.4 0.33 31.7 0.0 0.00 0.0 GX 5-1 270.287 -25.085 1.1 5.074 -1.024 9.9 0.34 28.8 0.0 0.00 0.0 GX 354-0 262.997 -33.825 1.1 354.314 -0.150 10.2 0.35 29.3 0.0 0.00 0.0 H 1820-303 275.910 -30.373 1.4 2.774 -7.913 9.2 0.43 21.5 0.0 0.00 0.0 GX 349+2 256.424 -36.416 2.0 349.104 +2.760 7.8 0.56 14.0 0.0 0.00 0.0 3A 1822-371 276.469 -37.126 2.2 356.839 -11.317 8.0 0.64 12.6 0.0 0.00 0.0 4U 1722-30 261.885 -30.805 2.6 356.316 +2.299 3.5 0.34 10.3 1.9 0.27 7.0 GX 9+1 270.349 -20.530 2.6 9.060 +1.182 4.4 0.43 10.2 0.0 0.00 0.0 SLX 1735-269 264.536 -27.016 3.0 0.761 +2.415 2.5 0.29 8.6 1.4 0.24 5.8 XTE J1817-330 274.388 -33.004 3.4 359.814 -7.957 2.9 0.39 7.6 2.3 0.31 7.6 GX 3+1 266.951 -26.619 3.9 2.231 +0.790 2.1 0.33 6.5 0.0 0.00 0.0 GX 13+1 273.588 -17.127 4.0 13.523 +0.157 5.5 0.87 6.3 0.0 0.00 0.0 3A 1728-169 263.020 -16.983 4.4 8.539 +8.957 3.8 0.67 5.6 0.0 0.00 0.0 IGR J17541-2252 268.490 -22.851 4.3 6.185 +1.516 1.9 0.32 5.9 0.0 0.00 0.0 GX 17+2 273.993 -14.032 5.0 16.430 +1.291 11.3 2.29 4.9 0.0 0.00 0.0 IGR J17597-2201 269.889 -22.006 4.9 7.565 +0.822 1.9 0.39 5.0 1.1 0.31 3.5 IGR J17391-3021 264.684 -30.395 5.5 357.971 +0.501 1.2 0.00 4.4 0.0 0.00 0.0 1E 1742.8-2853 266.467 -28.904 5.1 0.055 -0.029 1.3 0.26 4.8 0.0 0.00 0.0 IGR J17252-3616 261.241 -36.342 0.0 351.423 -0.350 1.6 0.00 4.2 0.0 0.00 0.0 1A 1742-294 266.495 -29.502 0.0 359.558 -0.361 1.2 0.00 3.8 0.0 0.00 0.0 AX J1749.1-2733 267.361 -27.517 6.9 1.650 +0.014 1.0 0.28 3.5 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 6.9 0.38 0.8 0.21 GX 354-0 262.989 -33.835 354.302 -0.150 16.7 1.51 4.6 0.97 1A 1742-294 266.523 -29.515 359.559 -0.389 2.2 0.35 0.8 0.21 GX 3+1 266.983 -26.564 2.294 +0.794 20.6 0.55 2.9 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 101.0 2.24 11.3 0.93 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.1 0.42 0.6 0.25
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