INTEGRAL Galactic Bulge Monitoring Revolution 0307: Observation start 2005-04-19 = MJD 53479
Total Observation GTI = 12309 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 1700-377 255.987 -37.841 0.3 347.757 +2.176 132.5 0.69 191.2 43.7 0.51 84.9 GRS 1758-258 270.312 -25.735 0.8 4.520 -1.365 13.0 0.34 38.6 9.0 0.27 33.3 GX 1+4 263.008 -24.737 0.9 1.944 +4.800 10.8 0.32 33.4 0.0 0.00 0.0 Ginga 1826-24 277.366 -23.792 1.1 9.276 -6.085 14.5 0.50 29.0 7.0 0.39 17.7 GX 349+2 256.436 -36.407 1.2 349.117 +2.757 13.9 0.54 25.7 0.0 0.00 0.0 1E 1740.7-2942 265.967 -29.740 1.2 359.115 -0.094 6.8 0.26 25.9 4.3 0.22 19.9 MXB 1730-335 263.348 -33.408 1.8 354.823 -0.168 4.3 0.29 15.0 0.0 0.00 0.0 GX 5-1 270.279 -25.078 1.7 5.075 -1.014 5.0 0.30 17.0 0.0 0.00 0.0 H 1820-303 275.900 -30.351 1.7 2.790 -7.894 6.4 0.40 16.1 0.0 0.00 0.0 3A 1822-371 276.420 -37.107 1.7 356.839 -11.273 8.6 0.53 16.2 0.0 0.00 0.0 GX 9+1 270.404 -20.533 2.4 9.082 +1.136 4.2 0.37 11.2 0.0 0.00 0.0 GX 354-0 263.013 -33.812 2.4 354.332 -0.154 3.7 0.33 11.2 0.0 0.00 0.0 4U 1722-30 261.892 -30.803 2.5 356.321 +2.295 3.0 0.29 10.6 1.1 0.24 4.7 GX 3+1 266.939 -26.586 3.6 2.254 +0.816 2.3 0.32 7.1 0.0 0.00 0.0 SLX 1735-269 264.588 -26.990 2.9 0.807 +2.390 2.4 0.27 8.9 1.0 0.22 4.5 GX 17+2 274.002 -14.059 3.0 16.410 +1.270 22.0 2.55 8.6 0.0 0.00 0.0 1A 1742-294 266.495 -29.501 0.0 359.559 -0.361 2.0 0.00 6.6 0.0 0.00 0.0 SLX 1744-299_300 266.872 -29.997 3.7 359.304 -0.898 1.9 0.27 7.0 0.0 0.00 0.0 1E 1742.8-2853 266.467 -28.879 4.1 0.077 -0.017 1.6 0.25 6.1 0.0 0.00 0.0 XTE J1743-363 265.691 -36.449 4.5 353.278 -3.416 1.9 0.00 5.5 0.0 0.00 0.0 GRS 1747-312 267.665 -31.391 5.4 358.460 -2.200 1.5 0.32 4.6 0.0 0.00 0.0 IGR J17473-2721 266.720 -27.283 5.1 1.556 +0.622 1.3 0.27 4.8 0.0 0.00 0.0 NEW_1 262.944 -38.769 3.4 350.150 -2.818 3.9 0.49 7.6 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GRS 1747-312 267.690 -31.292 358.555 -2.168 2.9 0.46 0.7 0.28 MXB 1730-335 263.350 -33.388 354.841 -0.158 22.2 1.22 4.4 0.69 GX 354-0 262.989 -33.835 354.302 -0.150 14.8 1.58 3.1 0.94 1A 1742-294 266.523 -29.515 359.559 -0.389 3.1 0.37 0.9 0.22 GX 3+1 266.983 -26.564 2.294 +0.794 23.7 0.50 3.3 0.26 GX 5-1 270.284 -25.079 5.077 -1.019 86.1 1.92 6.7 0.78
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