INTEGRAL Galactic Bulge Monitoring Revolution 0428: Observation start 2006-04-15 = MJD 53840
Total Observation GTI = 12313 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 5-1 270.283 -25.080 0.7 5.076 -1.018 17.0 0.31 54.5 0.0 0.00 0.0 Ginga 1826-24 277.365 -23.796 0.9 9.272 -6.086 17.9 0.53 33.8 6.2 0.42 14.8 GRS 1758-258 270.302 -25.736 1.0 4.514 -1.358 8.8 0.29 30.4 7.3 0.24 30.3 GX 1+4 263.011 -24.743 0.9 1.940 +4.795 10.4 0.30 34.5 0.0 0.00 0.0 H 1820-303 275.916 -30.364 1.1 2.785 -7.913 10.7 0.40 26.7 0.0 0.00 0.0 GX 349+2 256.437 -36.417 1.3 349.110 +2.751 12.1 0.55 22.0 0.0 0.00 0.0 GX 354-0 262.997 -33.822 1.7 354.316 -0.149 4.9 0.31 16.1 0.0 0.00 0.0 4U 1722-30 261.877 -30.799 2.1 356.317 +2.308 3.8 0.29 13.2 1.7 0.24 7.2 GX 9+1 270.361 -20.515 2.5 9.078 +1.180 4.2 0.40 10.4 0.0 0.00 0.0 SLX 1735-269 264.565 -26.995 2.9 0.792 +2.405 2.5 0.29 8.8 0.0 0.00 0.0 3A 1822-371 276.455 -37.096 2.8 356.863 -11.294 4.9 0.54 9.2 0.0 0.00 0.0 GX 13+1 273.671 -17.173 3.6 13.521 +0.066 5.7 0.80 7.2 0.0 0.00 0.0 OAO 1657-415 255.208 -41.668 4.2 344.362 +0.310 7.7 1.28 6.0 0.0 0.00 0.0 GX 3+1 267.009 -26.541 4.5 2.325 +0.786 1.6 0.29 5.6 0.0 0.00 0.0 4U 1700-377 256.003 -37.822 4.5 347.780 +2.177 3.5 0.63 5.6 0.0 0.00 0.0 1A 1742-294 266.522 -29.473 6.1 359.595 -0.366 1.3 0.32 4.0 0.0 0.00 0.0 IGR J17407-2808 265.183 -28.154 5.7 0.102 +1.324 1.2 0.28 4.3 0.0 0.00 0.0 IGR J17456-2901 266.495 -29.007 0.0 359.980 -0.104 1.1 0.00 4.3 1.1 0.22 4.9 V2400 Oph 258.197 -24.293 6.1 359.851 +8.679 1.7 0.42 4.0 0.0 0.00 0.0 SLX 1744-299_300 266.814 -30.025 6.9 359.255 -0.870 0.9 0.27 3.5 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1743-288 266.761 -28.883 0.207 -0.238 6.9 0.39 0.9 0.22 GX 354-0 262.989 -33.835 354.302 -0.150 14.4 1.44 2.4 0.87 1A 1742-294 266.523 -29.515 359.559 -0.389 3.1 0.34 0.8 0.19 GX 3+1 266.983 -26.564 2.294 +0.794 22.4 0.58 3.2 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 102.5 2.24 16.0 1.01
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