INTEGRAL Galactic Bulge Monitoring Revolution 0469: Observation start 2006-08-16 = MJD 53963
Total Observation GTI = 12420 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 5-1 270.286 -25.085 0.7 5.073 -1.023 16.8 0.31 53.6 0.0 0.00 0.0 GX 349+2 256.443 -36.422 1.0 349.108 +2.744 16.6 0.52 32.2 0.0 0.00 0.0 Ginga 1826-24 277.379 -23.802 1.0 9.273 -6.100 17.6 0.53 33.3 5.8 0.40 14.4 GX 1+4 263.016 -24.742 1.0 1.943 +4.791 9.7 0.31 31.7 0.0 0.00 0.0 GRS 1758-258 270.314 -25.741 1.3 4.515 -1.369 8.0 0.34 23.3 2.9 0.28 10.2 1E 1740.7-2942 265.978 -29.755 1.5 359.107 -0.111 5.8 0.31 18.7 3.9 0.27 14.8 GX 17+2 274.028 -14.049 1.8 16.431 +1.253 31.9 2.02 15.8 0.0 0.00 0.0 H 1820-303 275.929 -30.358 1.8 2.795 -7.920 6.2 0.41 15.1 0.0 0.00 0.0 3A 1822-371 276.440 -37.094 2.1 356.859 -11.282 7.1 0.56 12.8 0.0 0.00 0.0 1A 1742-294 266.522 -29.505 2.3 359.568 -0.383 3.2 0.28 11.5 0.0 0.00 0.0 GX 354-0 262.970 -33.822 2.3 354.305 -0.130 4.0 0.34 11.7 0.0 0.00 0.0 GX 3+1 266.991 -26.594 3.0 2.271 +0.772 2.4 0.28 8.6 0.0 0.00 0.0 GX 13+1 273.624 -17.141 3.3 13.527 +0.121 6.2 0.80 7.8 0.0 0.00 0.0 4U 1722-30 261.927 -30.817 3.5 356.326 +2.262 2.2 0.29 7.4 0.0 0.00 0.0 GX 9+1 270.432 -20.528 3.1 9.099 +1.116 3.4 0.42 8.2 0.0 0.00 0.0 OAO 1657-415 255.187 -41.638 3.4 344.376 +0.340 10.4 1.37 7.6 0.0 0.00 0.0 SLX 1735-269 264.559 -26.959 3.1 0.820 +2.428 2.3 0.27 8.5 1.3 0.23 5.7 4U 1735-444 264.610 -44.435 5.3 346.017 -6.905 12.9 2.78 4.7 0.0 0.00 0.0 XB 1832-330 278.973 -33.004 4.0 1.533 -11.407 3.7 0.58 6.4 0.0 0.00 0.0 H 1702-429 256.510 -43.068 0.0 343.837 -1.306 9.4 0.00 5.2 0.0 0.00 0.0 1E 1742.9-2849 266.580 -28.861 5.1 0.144 -0.092 1.2 0.25 4.8 0.0 0.00 0.0 IGR J16316-4028 247.903 -40.361 5.6 341.779 +5.351 16.3 0.00 4.4 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 13.0 1.47 3.4 0.88 1A 1742-294 266.523 -29.515 359.559 -0.389 1.6 0.32 0.5 0.19 GX 3+1 266.983 -26.564 2.294 +0.794 28.2 0.61 4.5 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 107.0 2.37 18.9 1.14 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.6 0.38 0.9 0.24
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