INTEGRAL Galactic Bulge Monitoring Revolution 0306: Observation start 2005-04-15 = MJD 53475
Total Observation GTI = 12311 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 1+4 263.003 -24.747 0.7 1.933 +4.799 14.4 0.28 51.1 0.0 0.00 0.0 GRS 1758-258 270.305 -25.739 0.8 4.514 -1.362 11.4 0.28 41.0 8.8 0.23 38.9 GX 349+2 256.443 -36.420 1.0 349.110 +2.745 17.1 0.55 31.0 0.0 0.00 0.0 1E 1740.7-2942 265.973 -29.744 1.0 359.115 -0.101 7.8 0.26 29.7 3.8 0.22 17.2 Ginga 1826-24 277.368 -23.800 1.1 9.270 -6.090 14.4 0.51 28.2 5.7 0.39 14.4 OAO 1657-415 255.203 -41.660 1.6 344.365 +0.317 22.5 1.26 18.0 0.0 0.00 0.0 GX 5-1 270.300 -25.071 1.6 5.091 -1.027 5.0 0.29 17.2 0.0 0.00 0.0 MXB 1730-335 263.360 -33.399 1.7 354.836 -0.171 5.1 0.32 16.2 0.0 0.00 0.0 H 1820-303 275.910 -30.355 1.6 2.791 -7.904 7.0 0.38 18.3 0.0 0.00 0.0 4U 1700-377 255.991 -37.832 1.8 347.767 +2.178 8.9 0.59 15.0 2.4 0.46 5.2 GX 354-0 263.005 -33.820 1.9 354.322 -0.153 4.3 0.29 14.7 0.0 0.00 0.0 3A 1822-371 276.431 -37.092 2.0 356.858 -11.275 7.4 0.53 14.0 2.1 0.41 5.1 4U 1722-30 261.886 -30.834 2.2 356.292 +2.282 3.4 0.28 12.1 2.0 0.23 9.0 GX 17+2 274.019 -14.036 2.4 16.439 +1.266 31.0 2.74 11.3 0.0 0.00 0.0 SLX 1735-269 264.566 -26.997 2.5 0.791 +2.402 2.9 0.27 10.7 0.9 0.23 3.9 GX 9+1 270.375 -20.500 2.9 9.098 +1.175 3.7 0.41 9.0 0.0 0.00 0.0 GX 3+1 266.984 -26.549 3.1 2.306 +0.801 2.4 0.28 8.5 0.0 0.00 0.0 1E 1742.8-2853 266.418 -28.922 2.6 0.019 -0.002 2.5 0.24 10.3 0.0 0.00 0.0 3A 1728-169 262.938 -16.955 3.4 8.521 +9.038 4.8 0.63 7.6 0.0 0.00 0.0 SLX 1744-299_300 266.923 -30.016 3.6 359.312 -0.946 1.9 0.26 7.2 0.0 0.00 0.0 XTE J1818-245 274.572 -24.521 5.2 7.445 -4.160 1.8 0.38 4.7 0.0 0.00 0.0 XB 1832-330 278.861 -32.920 4.6 1.570 -11.287 3.0 0.55 5.4 0.0 0.00 0.0 1A 1742-294 266.639 -29.462 4.5 359.657 -0.448 1.7 0.31 5.5 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== MXB 1730-335 263.350 -33.388 354.841 -0.158 19.3 1.17 4.5 0.71 GX 354-0 262.989 -33.835 354.302 -0.150 18.2 1.65 3.7 0.90 1A 1742-294 266.523 -29.515 359.559 -0.389 6.0 0.35 1.5 0.20 GRS 1758-258 270.303 -25.741 4.511 -1.361 9.9 1.67 2.0 0.70 GX 3+1 266.983 -26.564 2.294 +0.794 24.2 0.51 3.4 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 84.5 1.96 6.1 0.81
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