INTEGRAL Galactic Bulge Monitoring Revolution 0429: Observation start 2006-04-21 = MJD 53846
Total Observation GTI = 12248 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 1700-377 255.986 -37.834 0.4 347.763 +2.180 61.5 0.63 97.4 17.6 0.50 35.5 GX 354-0 262.997 -33.828 0.8 354.312 -0.152 14.5 0.35 40.9 4.0 0.30 13.3 GX 1+4 263.005 -24.737 0.8 1.942 +4.803 14.1 0.34 41.5 0.0 0.00 0.0 GRS 1758-258 270.311 -25.731 1.0 4.523 -1.362 10.9 0.33 32.5 8.5 0.28 30.7 Ginga 1826-24 277.382 -23.802 1.0 9.274 -6.102 16.3 0.54 30.4 5.6 0.42 13.3 H 1820-303 275.924 -30.357 1.1 2.794 -7.916 11.4 0.42 27.4 0.0 0.00 0.0 GX 5-1 270.284 -25.070 1.3 5.085 -1.014 7.4 0.33 22.1 0.0 0.00 0.0 GX 349+2 256.445 -36.404 1.8 349.124 +2.754 8.5 0.56 15.2 0.0 0.00 0.0 4U 1722-30 261.842 -30.812 2.4 356.289 +2.326 3.6 0.32 11.3 1.2 0.00 4.4 3A 1822-371 276.486 -37.049 2.8 356.916 -11.296 5.6 0.60 9.4 0.0 0.00 0.0 SLX 1735-269 264.562 -27.001 2.8 0.786 +2.404 2.5 0.26 9.3 1.5 0.23 6.5 GX 9+1 270.402 -20.527 2.9 9.087 +1.140 3.9 0.44 8.8 0.0 0.00 0.0 GX 3+1 266.968 -26.560 3.4 2.290 +0.807 2.3 0.30 7.6 0.0 0.00 0.0 IGR J17354-3255 263.867 -32.911 3.9 355.476 -0.263 2.2 0.34 6.4 0.0 0.00 0.0 3A 1728-169 262.933 -16.922 4.3 8.546 +9.060 3.6 0.63 5.8 0.0 0.00 0.0 1A 1743-288 266.683 -28.924 0.0 0.136 -0.201 1.4 0.00 5.1 0.0 0.00 0.0 SLX 1744-299_300 266.869 -30.011 4.7 359.291 -0.903 1.4 0.27 5.3 0.0 0.00 0.0 PKS 1830-211 278.325 -21.056 0.0 12.132 -5.634 3.2 0.00 4.4 0.0 0.00 0.0 1A 1742-294 266.495 -29.501 0.0 359.559 -0.361 1.2 0.00 4.1 0.0 0.00 0.0 Swift J174535.5-2901 266.306 -29.089 0.0 359.825 -0.006 1.0 0.00 4.0 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 4.1 0.41 0.0 0.00 1A 1742-294 266.523 -29.515 359.559 -0.389 7.3 0.46 1.6 0.27 GX 3+1 266.983 -26.564 2.294 +0.794 18.7 0.56 2.6 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 102.8 2.72 10.2 1.14
Go back to Bulge home page