INTEGRAL Galactic Bulge Monitoring Revolution 0413: Observation start 2006-03-01 = MJD 53795
Total Observation GTI = 12301 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 5-1 270.279 -25.087 0.6 5.068 -1.018 17.5 0.29 59.9 0.0 0.00 0.0 GRS 1758-258 270.302 -25.750 0.9 4.502 -1.365 10.4 0.29 36.4 7.6 0.23 32.4 GX 1+4 262.997 -24.749 0.9 1.928 +4.802 11.7 0.31 37.8 0.0 0.00 0.0 Ginga 1826-24 277.371 -23.802 1.0 9.269 -6.093 17.2 0.56 30.7 7.8 0.44 17.7 1A 1742-294 266.510 -29.515 1.4 359.553 -0.380 5.2 0.25 20.6 1.6 0.21 7.6 GX 354-0 263.006 -33.824 1.3 354.319 -0.156 6.7 0.30 22.3 0.0 0.00 0.0 GX 349+2 256.423 -36.421 1.6 349.099 +2.757 9.0 0.50 18.0 0.0 0.00 0.0 H 1820-303 275.905 -30.369 1.6 2.775 -7.906 7.3 0.41 17.7 0.0 0.00 0.0 XTE J1817-330 274.437 -33.009 2.0 359.828 -7.995 5.4 0.39 14.0 2.7 0.31 8.7 3A 1822-371 276.450 -37.108 2.3 356.850 -11.295 6.3 0.53 12.0 0.0 0.00 0.0 OAO 1657-415 255.201 -41.655 2.4 344.369 +0.321 15.7 1.40 11.2 0.0 0.00 0.0 GX 3+1 267.001 -26.556 2.4 2.308 +0.784 2.9 0.26 11.2 0.0 0.00 0.0 GX 9+1 270.403 -20.542 4.0 9.074 +1.132 2.5 0.40 6.3 0.0 0.00 0.0 4U 1722-30 261.856 -30.771 4.0 356.330 +2.339 1.8 0.28 6.3 0.0 0.00 0.0 1A 1743-288 266.711 -28.812 3.8 0.245 -0.165 1.7 0.25 6.6 0.0 0.00 0.0 3A 1728-169 262.931 -16.966 3.9 8.507 +9.038 4.4 0.68 6.5 0.0 0.00 0.0 GX 13+1 273.682 -17.167 4.0 13.531 +0.059 4.5 0.71 6.3 0.0 0.00 0.0 GX 17+2 274.031 -14.022 4.4 16.457 +1.263 12.9 2.25 5.7 0.0 0.00 0.0 SLX 1735-269 264.556 -27.001 4.7 0.782 +2.408 1.4 0.26 5.3 1.1 0.22 4.8 SLX 1744-299_300 266.857 -30.004 3.9 359.292 -0.891 1.7 0.26 6.5 0.0 0.00 0.0 IGR J17252-3616 261.291 -36.284 4.3 351.493 -0.350 2.2 0.38 5.9 0.0 0.00 0.0 XTE J1739-285 265.058 -28.477 4.5 359.769 +1.246 1.4 0.25 5.6 0.0 0.00 0.0 IGR J17544-2619 268.633 -26.356 5.7 3.227 -0.370 1.2 0.27 4.3 0.0 0.00 0.0 4U 1705-32 257.305 -32.377 5.0 352.784 +4.592 1.9 0.00 4.9 0.0 0.00 0.0 IGR J17488-3253 267.281 -32.948 0.0 356.954 -2.718 1.4 0.00 4.9 0.0 0.00 0.0 1H 1746-370 267.607 -37.043 5.4 353.560 -5.038 1.7 0.38 4.6 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== XTE J1739-285 264.975 -28.496 359.714 +1.298 2.9 0.39 0.5 0.22 GX 354-0 262.989 -33.835 354.302 -0.150 14.2 1.39 3.0 0.81 GX 3+1 266.983 -26.564 2.294 +0.794 22.6 0.55 3.0 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 86.6 1.99 18.0 0.99
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