INTEGRAL Galactic Bulge Monitoring Revolution 0539: Observation start 2007-03-13 = MJD 54172
Total Observation GTI = 12455 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 1700-377 255.986 -37.839 0.4 347.759 +2.177 81.0 0.70 115.6 23.7 0.53 44.8 GX 354-0 262.989 -33.832 0.4 354.305 -0.149 34.4 0.33 103.7 11.6 0.27 43.4 GX 1+4 263.010 -24.751 0.5 1.933 +4.792 22.6 0.32 71.0 0.0 0.00 0.0 1E 1740.7-2942 265.979 -29.747 0.8 359.115 -0.107 11.6 0.29 40.0 7.3 0.24 30.2 GRS 1758-258 270.313 -25.754 0.9 4.504 -1.375 11.2 0.33 33.6 7.8 0.27 29.2 H 1820-303 275.916 -30.353 1.0 2.795 -7.908 12.9 0.41 31.5 0.0 0.00 0.0 Ginga 1826-24 277.358 -23.802 1.0 9.264 -6.082 17.8 0.58 30.8 7.4 0.45 16.5 GX 349+2 256.399 -36.414 1.9 349.093 +2.777 8.0 0.55 14.6 0.0 0.00 0.0 GRS 1741.9-2853 266.275 -28.936 1.9 359.941 +0.097 3.9 0.27 14.2 1.9 0.23 8.3 1A 1742-294 266.522 -29.526 2.1 359.549 -0.394 3.8 0.29 13.3 0.0 0.00 0.0 4U 1722-30 261.843 -30.825 2.5 356.279 +2.317 3.9 0.37 10.5 2.5 0.30 8.5 GX 3+1 266.988 -26.565 2.3 2.295 +0.789 4.0 0.34 11.7 0.0 0.00 0.0 3A 1822-371 276.457 -37.120 2.8 356.841 -11.305 5.7 0.60 9.5 0.0 0.00 0.0 GX 17+2 273.991 -14.081 2.8 16.387 +1.269 22.8 2.41 9.5 0.0 0.00 0.0 OAO 1657-415 255.214 -41.661 3.3 344.370 +0.310 11.9 1.52 7.8 0.0 0.00 0.0 GX 5-1 270.207 -25.178 0.0 4.956 -1.007 2.6 0.00 7.7 0.0 0.00 0.0 GX 9+1 270.426 -20.583 4.3 9.049 +1.093 2.6 0.44 5.8 0.0 0.00 0.0 XB 1832-330 278.905 -32.962 3.9 1.547 -11.338 4.0 0.62 6.5 2.2 0.48 4.5 SLX 1735-269 264.554 -27.021 4.3 0.765 +2.399 2.0 0.00 5.9 1.1 0.28 4.0 SLX 1744-299_300 266.820 -29.992 4.3 359.286 -0.857 1.8 0.31 5.9 1.0 0.25 3.9 IGR J17252-3616 261.223 -36.232 4.6 351.505 -0.276 2.4 0.43 5.5 1.6 0.34 4.6 XTE J1716-389 258.832 -38.777 5.2 348.333 -0.176 3.0 0.00 4.7 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.9 0.38 1.5 0.25 GX 354-0 262.989 -33.835 354.302 -0.150 12.4 1.48 4.7 1.06 GX 3+1 266.983 -26.564 2.294 +0.794 37.6 0.59 5.6 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 69.3 1.96 5.3 0.81 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.8 0.40 0.9 0.27
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