INTEGRAL Galactic Bulge Monitoring Revolution 0406: Observation start 2006-02-09 = MJD 53775
Total Observation GTI = 7163 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 5-1 270.286 -25.082 0.9 5.076 -1.021 13.8 0.41 33.7 0.0 0.00 0.0 GX 1+4 263.010 -24.751 1.0 1.933 +4.791 12.5 0.42 29.9 0.0 0.00 0.0 Ginga 1826-24 277.375 -23.788 1.1 9.283 -6.090 18.6 0.65 28.5 6.7 0.51 13.0 GRS 1758-258 270.295 -25.742 1.1 4.506 -1.355 10.8 0.37 29.0 7.3 0.31 24.0 OAO 1657-415 255.203 -41.651 1.2 344.373 +0.323 46.7 1.84 25.4 9.4 1.34 7.0 H 1820-303 275.919 -30.352 1.6 2.797 -7.910 9.1 0.50 18.2 0.0 0.00 0.0 1A 1742-294 266.520 -29.527 2.1 359.548 -0.393 4.9 0.37 13.0 1.5 0.31 4.7 GX 354-0 263.001 -33.811 2.1 354.327 -0.145 5.2 0.41 12.6 0.0 0.00 0.0 GX 349+2 256.424 -36.387 2.4 349.127 +2.777 7.8 0.68 11.4 0.0 0.00 0.0 4U 1722-30 261.878 -30.825 3.1 356.296 +2.293 3.2 0.37 8.5 0.0 0.00 0.0 3A 1822-371 276.439 -37.132 2.9 356.823 -11.298 6.0 0.67 9.1 0.0 0.00 0.0 GX 17+2 273.954 -14.028 3.2 16.416 +1.325 18.8 2.32 8.1 0.0 0.00 0.0 XTE J1817-330 274.429 -33.019 3.2 359.816 -7.994 3.7 0.46 8.0 2.0 0.36 5.4 SLX 1735-269 264.531 -27.043 3.6 0.735 +2.404 2.7 0.38 7.1 1.8 0.00 5.8 1A 1743-288 266.791 -28.873 0.0 0.229 -0.256 2.2 0.00 6.3 0.0 0.00 0.0 GX 9+1 270.363 -20.525 3.7 9.070 +1.174 3.5 0.50 6.9 0.0 0.00 0.0 SLX 1744-299_300 266.831 -30.058 4.1 359.234 -0.900 2.4 0.40 6.1 0.0 0.00 0.0 IGR J17252-3616 261.344 -36.322 4.5 351.485 -0.407 2.9 0.53 5.5 0.0 0.00 0.0 Oph Cluster 258.179 -23.383 5.2 0.597 +9.215 2.6 0.00 4.8 0.0 0.00 0.0 GX 3+1 266.979 -26.565 5.9 2.290 +0.796 1.8 0.44 4.1 0.0 0.00 0.0 GRS 1747-312 267.609 -31.269 4.9 358.540 -2.097 1.9 0.37 5.1 0.0 0.00 0.0 IGR J17456-2901 266.415 -28.955 0.0 359.989 -0.017 1.4 0.00 4.0 0.0 0.00 0.0 XB 1832-330 278.971 -33.005 5.8 1.532 -11.406 2.8 0.66 4.2 0.0 0.00 0.0 3A 1728-169 262.920 -16.987 0.0 8.484 +9.035 3.7 0.00 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 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 6.5 0.59 0.9 0.35 GRS 1747-312 267.690 -31.292 358.555 -2.168 3.6 0.59 0.9 0.36 GX 354-0 262.989 -33.835 354.302 -0.150 19.0 2.24 4.7 1.27 GX 3+1 266.983 -26.564 2.294 +0.794 25.5 0.74 3.8 0.39 GX 5-1 270.284 -25.079 5.077 -1.019 101.3 2.44 13.2 1.06
Go back to Bulge home page