INTEGRAL Galactic Bulge Monitoring Revolution 0542: Observation start 1999-12-31 = MJD 51544
Total Observation GTI = 9439 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+4 263.011 -24.742 0.6 1.941 +4.795 21.7 0.36 60.8 0.0 0.00 0.0 GX 5-1 270.285 -25.080 0.7 5.077 -1.020 18.2 0.37 48.6 0.0 0.00 0.0 1E 1740.7-2942 265.983 -29.750 1.0 359.114 -0.111 10.1 0.33 31.1 6.5 0.27 24.1 GRS 1758-258 270.298 -25.736 1.0 4.512 -1.355 12.5 0.40 31.3 8.9 0.32 27.7 Ginga 1826-24 277.371 -23.803 1.2 9.268 -6.094 15.7 0.63 24.9 6.3 0.49 12.8 GX 354-0 263.001 -33.840 1.4 354.303 -0.161 8.4 0.41 20.4 0.0 0.00 0.0 GX 349+2 256.437 -36.417 1.5 349.109 +2.751 13.1 0.67 19.5 0.0 0.00 0.0 H 1820-303 275.923 -30.360 1.7 2.791 -7.916 8.9 0.53 16.6 0.0 0.00 0.0 1A 1742-294 266.490 -29.459 2.8 359.592 -0.335 3.2 0.34 9.4 0.0 0.00 0.0 GRS 1741.9-2853 266.313 -28.948 3.1 359.948 +0.063 3.1 0.37 8.3 0.0 0.00 0.0 GX 9+1 270.378 -20.559 2.9 9.047 +1.144 4.1 0.45 9.1 0.0 0.00 0.0 3A 1728-169 262.931 -16.943 3.3 8.527 +9.051 5.4 0.69 7.9 0.0 0.00 0.0 OAO 1657-415 255.205 -41.668 2.9 344.361 +0.311 20.9 2.32 9.0 0.0 0.00 0.0 GX 13+1 273.601 -17.169 3.4 13.492 +0.126 6.2 0.81 7.6 0.0 0.00 0.0 4U 1722-30 261.911 -30.814 2.8 356.321 +2.275 4.0 0.42 9.5 2.0 0.35 5.8 GX 3+1 267.016 -26.581 3.2 2.294 +0.760 3.0 0.38 8.0 0.0 0.00 0.0 3A 1822-371 276.477 -37.082 3.8 356.883 -11.304 5.2 0.78 6.7 0.0 0.00 0.0 XB 1832-330 278.946 -33.029 3.8 1.501 -11.397 4.8 0.72 6.7 2.6 0.55 4.7 IGR J17252-3616 261.254 -36.272 4.8 351.486 -0.319 2.8 0.54 5.2 0.0 0.00 0.0 GX 17+2 274.057 -14.027 4.4 16.464 +1.238 9.6 1.70 5.7 0.0 0.00 0.0 SLX 1744-299_300 266.970 -29.998 9.9 359.347 -0.972 0.8 0.34 2.4 0.0 0.00 0.0 SLX 1735-269 264.581 -26.951 6.1 0.837 +2.415 1.5 0.00 4.0 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 > 5σ 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).NOTE: 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 19.4 2.72 5.2 1.89 GX 3+1 266.983 -26.564 2.294 +0.794 32.9 0.58 4.6 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 83.0 1.81 16.7 0.92
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