INTEGRAL Galactic Bulge Monitoring Revolution 0602: Observation start 2007-09-18 = MJD 54361
Total Observation GTI = 10954 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 1700-377 255.988 -37.851 0.3 347.750 +2.168 119.0 0.78 151.9 30.1 0.59 50.6 GX 1+4 263.005 -24.745 0.9 1.936 +4.798 12.0 0.34 35.5 0.0 0.00 0.0 GX 5-1 270.285 -25.075 1.0 5.081 -1.017 11.6 0.36 32.7 0.0 0.00 0.0 Ginga 1826-24 277.370 -23.799 0.9 9.271 -6.090 21.6 0.61 35.6 7.4 0.47 15.6 SAX J1810.8-2609 272.709 -26.155 1.2 5.204 -3.451 9.3 0.38 24.5 4.5 0.31 14.5 GX 349+2 256.426 -36.422 1.4 349.100 +2.755 14.1 0.67 21.2 0.0 0.00 0.0 H 1820-303 275.913 -30.377 1.8 2.772 -7.917 7.2 0.48 15.0 0.0 0.00 0.0 GRS 1758-258 270.294 -25.742 1.9 4.505 -1.354 5.4 0.36 14.7 3.1 0.30 10.3 OAO 1657-415 255.228 -41.618 1.8 344.410 +0.328 22.4 1.48 15.2 0.0 0.00 0.0 GX 9+1 270.392 -20.510 2.8 9.097 +1.157 4.7 0.51 9.3 0.0 0.00 0.0 3A 1822-371 276.453 -37.100 2.9 356.858 -11.294 5.7 0.63 9.0 0.0 0.00 0.0 GX 3+1 266.993 -26.586 2.7 2.279 +0.774 3.3 0.35 9.6 0.0 0.00 0.0 4U 1722-30 261.837 -30.827 3.5 356.275 +2.321 3.0 0.41 7.4 1.4 0.33 4.3 3A 1728-169 262.958 -16.953 4.0 8.533 +9.023 4.7 0.00 6.4 0.0 0.00 0.0 GX 354-0 262.977 -33.847 3.8 354.286 -0.149 2.4 0.36 6.7 0.0 0.00 0.0 SLX 1735-269 264.538 -27.041 4.8 0.741 +2.401 2.0 0.38 5.1 0.0 0.00 0.0 1E 1743.1-2843 266.683 -28.724 0.0 0.308 -0.097 1.7 0.00 5.6 0.0 0.00 0.0 SAX J1712.6-3739 258.124 -37.724 4.6 348.861 +0.892 3.5 0.64 5.5 1.7 0.48 3.5 GRS 1741.9-2853 266.307 -28.971 0.0 359.926 +0.055 1.4 0.00 4.8 0.0 0.00 0.0 H 1702-429 256.452 -43.061 5.3 343.817 -1.268 11.1 2.40 4.6 0.0 0.00 0.0 IGR J17541-2252 268.531 -22.893 0.0 6.168 +1.462 1.6 0.00 4.0 0.0 0.00 0.0 NEW_1 259.873 -31.919 4.2 354.426 +3.091 2.3 0.39 6.0 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 2.8 0.32 0.5 0.16 GX 3+1 266.983 -26.564 2.294 +0.794 31.1 0.58 4.1 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 74.8 3.47 6.2 1.42
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