INTEGRAL Galactic Bulge Monitoring Revolution 0490: Observation start 2006-10-17 = MJD 54025
Total Observation GTI = 12288 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 1+4 263.010 -24.743 0.5 1.940 +4.795 25.5 0.34 74.8 0.0 0.00 0.0 4U 1700-377 255.984 -37.846 0.6 347.751 +2.174 46.4 0.71 65.2 12.8 0.55 23.4 GX 354-0 263.000 -33.833 0.8 354.309 -0.156 15.6 0.36 42.9 3.5 0.30 11.7 GX 5-1 270.295 -25.079 1.0 5.082 -1.027 10.4 0.35 29.8 0.0 0.00 0.0 Ginga 1826-24 277.368 -23.799 1.1 9.271 -6.089 15.4 0.53 28.9 5.8 0.41 14.0 1E 1740.7-2942 265.983 -29.748 1.2 359.115 -0.111 7.5 0.30 25.4 4.9 0.25 19.6 GRS 1758-258 270.319 -25.739 1.2 4.519 -1.372 7.4 0.30 24.5 5.5 0.25 22.2 H 1820-303 275.914 -30.366 1.2 2.782 -7.912 10.4 0.44 23.9 0.0 0.00 0.0 IGR J17497-2821 267.424 -28.363 1.3 0.953 -0.469 7.3 0.32 22.6 4.3 0.27 15.7 GX 349+2 256.436 -36.423 1.7 349.104 +2.748 9.1 0.55 16.6 0.0 0.00 0.0 4U 1722-30 261.876 -30.809 1.8 356.308 +2.303 5.0 0.32 15.7 1.7 0.25 6.5 3A 1822-371 276.468 -37.074 2.3 356.887 -11.294 7.1 0.60 11.8 0.0 0.00 0.0 GX 9+1 270.392 -20.551 2.5 9.061 +1.137 4.8 0.44 10.8 0.0 0.00 0.0 GX 3+1 267.019 -26.518 3.1 2.349 +0.790 2.6 0.30 8.5 0.0 0.00 0.0 SLX 1744-299_300 266.813 -30.030 3.0 359.249 -0.872 2.5 0.29 8.5 0.0 0.00 0.0 3A 1728-169 262.927 -17.019 3.2 8.460 +9.013 5.8 0.73 8.0 0.0 0.00 0.0 1A 1742-294 266.530 -29.520 3.6 359.559 -0.397 2.4 0.33 7.1 0.0 0.00 0.0 IGR J18027-2016 270.730 -20.215 0.0 9.509 +1.027 2.7 0.00 6.1 0.0 0.00 0.0 SLX 1735-269 264.607 -26.976 3.4 0.828 +2.383 2.4 0.32 7.5 0.0 0.00 0.0 GX 13+1 273.617 -17.131 3.9 13.533 +0.131 5.3 0.81 6.6 0.0 0.00 0.0 GX 17+2 274.004 -14.077 4.2 16.396 +1.260 16.5 2.77 5.9 0.0 0.00 0.0 H 1702-429 256.586 -43.031 4.3 343.900 -1.328 14.0 2.39 5.9 0.0 0.00 0.0 IGR J18249-3243 276.269 -32.676 5.4 0.831 -9.219 2.0 0.44 4.6 0.0 0.00 0.0 SLX 1737-282 265.292 -28.295 6.4 0.033 +1.168 1.2 0.32 3.8 0.0 0.00 0.0 XB 1832-330 278.998 -33.001 6.4 1.545 -11.425 2.3 0.60 3.8 1.2 0.46 2.6JEM-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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 7.1 1.20 2.4 0.82 GX 3+1 266.983 -26.564 2.294 +0.794 25.1 0.57 3.8 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 98.1 2.21 13.9 1.02
Go back to Bulge home page