INTEGRAL Galactic Bulge Monitoring Revolution 0418: Observation start 2006-03-16 = MJD 53810
Total Observation GTI = 12316 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 -37.843 0.6 347.756 +2.173 47.0 0.70 67.4 14.4 0.54 26.6 GX 5-1 270.286 -25.082 0.6 5.076 -1.022 19.5 0.30 65.1 0.0 0.00 0.0 GX 1+4 263.006 -24.745 0.8 1.936 +4.798 12.5 0.31 40.2 0.0 0.00 0.0 GRS 1758-258 270.298 -25.742 1.0 4.507 -1.357 9.8 0.30 33.0 7.0 0.24 29.3 Ginga 1826-24 277.366 -23.786 1.0 9.281 -6.082 16.7 0.53 31.3 6.2 0.41 15.1 1A 1742-294 266.513 -29.515 1.3 359.554 -0.382 6.3 0.27 23.7 2.3 0.22 10.2 H 1820-303 275.920 -30.355 1.7 2.795 -7.912 7.4 0.43 17.1 0.0 0.00 0.0 XTE J1817-330 274.451 -33.028 1.7 359.816 -8.014 6.4 0.39 16.4 3.0 0.31 9.7 GX 354-0 263.005 -33.837 1.8 354.307 -0.162 5.5 0.35 15.5 0.0 0.00 0.0 GX 349+2 256.442 -36.434 2.1 349.098 +2.738 6.9 0.54 12.7 0.0 0.00 0.0 3A 1822-371 276.420 -37.091 2.5 356.854 -11.267 6.6 0.61 10.9 0.0 0.00 0.0 1A 1743-288 266.685 -28.849 2.9 0.202 -0.164 2.4 0.26 9.1 0.8 0.22 3.6 GX 3+1 266.984 -26.560 2.9 2.298 +0.795 2.7 0.30 9.1 0.0 0.00 0.0 SLX 1744-299_300 266.858 -30.027 3.1 359.273 -0.904 2.5 0.30 8.4 0.0 0.00 0.0 GX 9+1 270.453 -20.549 4.6 9.091 +1.088 2.5 0.46 5.4 0.0 0.00 0.0 SLX 1735-269 264.569 -26.965 3.3 0.819 +2.418 2.6 0.33 7.8 0.0 0.00 0.0 SLX 1737-282 265.129 -28.392 3.5 359.875 +1.239 2.0 0.27 7.3 0.0 0.00 0.0 GX 17+2 274.022 -13.992 3.7 16.479 +1.285 16.0 2.31 6.9 0.0 0.00 0.0 3A 1728-169 262.924 -16.960 3.7 8.509 +9.047 4.8 0.69 6.9 0.0 0.00 0.0 OAO 1657-415 255.191 -41.643 3.6 344.374 +0.334 8.6 1.24 7.0 0.0 0.00 0.0 4U 1722-30 261.808 -30.776 4.1 356.303 +2.370 2.0 0.33 6.1 0.0 0.00 0.0 XB 1832-330 278.875 -32.949 4.9 1.549 -11.310 3.0 0.58 5.1 0.0 0.00 0.0 GX 13+1 273.605 -17.114 4.3 13.543 +0.150 4.6 0.78 5.9 0.0 0.00 0.0 GRS 1747-312 267.749 -31.302 0.0 358.573 -2.217 1.2 0.00 4.1 0.0 0.00 0.0 Oph Cluster 258.109 -23.320 4.9 0.611 +9.303 2.2 0.43 5.1 0.0 0.00 0.0 GRS 1734-292 264.332 -29.174 5.7 358.840 +1.413 1.2 0.28 4.3 0.0 0.00 0.0 NEW_1 257.612 -43.851 4.2 343.688 -2.415 16.2 2.52 5.9 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 18.6 1.49 4.3 1.02 GX 3+1 266.983 -26.564 2.294 +0.794 32.2 0.58 4.9 0.32 GX 5-1 270.284 -25.079 5.077 -1.019 81.4 2.02 17.7 1.03
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