INTEGRAL Galactic Bulge Monitoring Revolution 0546: Observation start 2007-04-04 = MJD 54194
Total Observation GTI = 13827 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+4 263.012 -24.753 0.7 1.932 +4.789 15.1 0.30 51.0 0.0 0.00 0.0 GRS 1758-258 270.302 -25.741 0.8 4.510 -1.361 12.4 0.30 41.1 9.1 0.25 36.4 GX 5-1 270.285 -25.072 1.0 5.084 -1.016 10.5 0.33 31.6 0.0 0.00 0.0 1E 1740.7-2942 265.971 -29.755 1.0 359.104 -0.106 9.2 0.29 31.9 4.9 0.25 19.9 Ginga 1826-24 277.376 -23.802 1.0 9.271 -6.097 16.5 0.53 31.0 6.9 0.41 16.9 1A 1742-294 266.516 -29.518 1.3 359.554 -0.385 6.1 0.28 21.8 1.9 0.25 7.8 GX 349+2 256.398 -36.460 1.5 349.056 +2.750 8.9 0.47 19.2 0.0 0.00 0.0 GX 354-0 262.990 -33.833 1.5 354.305 -0.150 5.7 0.30 19.2 0.0 0.00 0.0 H 1820-303 275.921 -30.359 1.7 2.791 -7.914 7.0 0.41 17.0 0.0 0.00 0.0 GX 3+1 266.952 -26.559 2.0 2.283 +0.820 4.1 0.29 13.9 0.0 0.00 0.0 4U 1722-30 261.874 -30.825 2.4 356.294 +2.295 3.6 0.33 10.9 2.0 0.28 7.1 3A 1822-371 276.449 -37.081 2.7 356.874 -11.283 5.2 0.53 9.7 0.0 0.00 0.0 OAO 1657-415 255.189 -41.637 2.6 344.377 +0.340 11.7 1.17 10.0 0.0 0.00 0.0 GX 17+2 274.026 -14.007 2.6 16.468 +1.274 30.2 3.02 10.0 0.0 0.00 0.0 SLX 1735-269 264.586 -26.958 2.9 0.834 +2.408 2.4 0.27 9.1 1.3 0.23 5.6 GX 9+1 270.375 -20.516 2.7 9.083 +1.168 4.0 0.42 9.6 0.0 0.00 0.0 IGR J17252-3616 261.258 -36.278 3.9 351.484 -0.325 2.4 0.37 6.4 0.0 0.00 0.0 SLX 1744-299_300 266.822 -30.064 4.5 359.225 -0.896 1.6 0.29 5.5 0.0 0.00 0.0 3A 1728-169 262.897 -16.907 3.9 8.541 +9.097 4.7 0.73 6.4 0.0 0.00 0.0 XB 1832-330 278.954 -32.982 4.2 1.547 -11.384 3.5 0.59 6.0 0.0 0.00 0.0 GX 13+1 273.561 -17.191 5.7 13.455 +0.150 3.5 0.82 4.3 0.0 0.00 0.0 XTE J1751-305 267.812 -30.615 5.0 359.191 -1.912 1.4 0.28 5.0 0.0 0.00 0.0 1E 1742.8-2853 266.513 -28.899 6.4 0.081 -0.062 1.0 0.26 3.8 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== Swift J174535.5-2901 266.397 -29.027 359.919 -0.042 1.2 0.23 0.4 0.15 GX 354-0 262.989 -33.835 354.302 -0.150 11.7 0.79 2.3 0.53 1A 1742-294 266.523 -29.515 359.559 -0.389 1.2 0.23 0.8 0.15 GX 3+1 266.983 -26.564 2.294 +0.794 36.3 0.42 5.8 0.23 GX 5-1 270.284 -25.079 5.077 -1.019 90.0 1.80 11.0 0.86 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.1 0.28 0.6 0.17
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