Revolution 1088: Observation start 2011-09-13T09:14 = MJD 55817.386
Total Observation GTI = 12088 seconds
IBIS/ISGRI
IBIS/ISGRI significance mosaic images. Left: IBIS/ISGRI 18-40 keV. Right: 40-100 keV
Sources 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 OSA10.1
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 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 and NEW SOURCE
s < 6σ towards the border of the image may be spurious.
IBIS/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 1700-377 255.987 -37.846 0.9 347.753 +2.172 32.0 0.86 37.1 8.9 0.60 14.9
GX 5-1 270.280 -25.080 0.9 5.074 -1.016 11.9 0.33 35.7 0.0 0.00 0.0
GX 354-0 262.986 -33.831 1.0 354.304 -0.146 12.1 0.37 32.5 3.5 0.28 12.5
1E 1740.7-2942 265.977 -29.754 1.2 359.108 -0.109 7.6 0.31 24.7 4.8 0.24 20.1
Ginga 1826-24 277.392 -23.789 1.4 9.289 -6.104 10.3 0.50 20.6 5.0 0.36 13.7
GRS 1758-258 270.301 -25.726 1.5 4.523 -1.352 6.0 0.32 18.7 3.4 0.24 14.1
GX 349+2 256.430 -36.436 1.7 349.091 +2.744 11.6 0.72 16.2 0.0 0.00 0.0
H 1820-303 275.934 -30.373 1.9 2.784 -7.931 5.8 0.40 14.2 0.0 0.00 0.0
MAXI J1836-194 278.916 -19.329 2.2 13.930 -5.346 10.5 0.86 12.2 6.0 0.62 9.8
4U 1722-30 261.932 -30.774 2.9 356.364 +2.282 3.3 0.37 9.0 1.5 0.27 5.5
IGR J17454-2919 266.317 -29.311 3.2 359.640 -0.130 2.5 0.31 8.0 0.0 0.00 0.0
3A 1822-371 276.440 -37.070 3.4 356.881 -11.272 4.3 0.56 7.7 0.0 0.00 0.0
GX 3+1 266.974 -26.630 3.4 2.233 +0.766 2.3 0.31 7.5 0.0 0.00 0.0
GX 9+1 270.380 -20.522 3.5 9.081 +1.161 3.7 0.50 7.4 0.0 0.00 0.0
SLX 1744-299_300 266.843 -30.042 3.2 359.253 -0.900 2.4 0.30 8.0 1.5 0.24 6.4
1H 1746-370 267.503 -36.941 4.0 353.607 -4.915 2.9 0.46 6.4 0.0 0.00 0.0
SAX J1712.6-3739 258.113 -37.638 4.2 348.925 +0.949 4.1 0.68 6.0 0.0 0.00 0.0
SLX 1746-331 267.456 -33.233 4.5 356.784 -2.990 1.9 0.34 5.6 0.0 0.00 0.0
GX 1+4 263.009 -24.783 4.0 1.905 +4.774 2.2 0.36 6.2 0.0 0.00 0.0
MXB 1730-335 263.316 -33.380 4.8 354.831 -0.130 1.9 0.36 5.2 0.0 0.00 0.0
IGR J17353-3539 263.848 -35.614 4.8 353.192 -1.710 2.1 0.40 5.2 0.0 0.00 0.0
Swift J173203.1-3445 263.095 -34.660 5.4 353.659 -0.675 1.7 0.00 4.5 0.0 0.00 0.0
IGR J17254-3257 261.377 -33.032 6.5 354.226 +1.415 1.5 0.39 3.7 0.0 0.00 0.0
SAX J1806.5-2215 271.611 -22.204 4.5 8.179 -0.663 2.4 0.43 5.6 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined significance mosaic images.
Left: 3-10 keV. Right: 10-25 keV.
Sources labelled were detected in the 3-10 keV image > 6σ. The sources detected above 3σ in the 3-10 keV and/or 10-25 keV band 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 ~ 97 cps [J1], 103 cps [J2]); B = 10-25 keV (1 Crab ~ 29 cps [J1], 27 cps [J2]).
NOTES: 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. The systematic noise increases towards the edge of the field of view and in the vicinity of very bright sources, such as GX 5-1; NEW SOURCE
s < 6σ towards the border of the image and/or near GX 5-1 may, therefore, be spurious.
JEM-X1+2 Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- sig B(cps) +/- sig
==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== =====
1A 1742-294 266.506 -29.510 359.556 -0.374 6.1 0.25 24.6 1.0 0.15 6.6
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.0 0.25 8.1 1.0 0.16 6.3
4U 1722-30 261.888 -30.802 356.320 +2.298 2.9 0.84 3.5 0.6 0.59 1.0
GX 3+1 266.987 -26.564 2.295 +0.790 47.5 0.51 93.8 4.5 0.26 17.6
GX 354-0 262.989 -33.835 354.302 -0.150 9.6 1.94 4.9 2.2 1.48 1.5
GX 5-1 270.286 -25.074 5.083 -1.017 109.7 1.29 85.1 15.5 0.63 24.7
MXB 1730-335 263.350 -33.388 354.841 -0.158 14.4 0.98 14.7 1.8 0.71 2.5
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.0 0.24 4.1 0.3 0.14 2.4
NEW SOURCE 268.872 -25.152 4.375 +0.053 3.9 0.91 4.3 0.0 0.00 0.0
NEW SOURCE 270.035 -24.854 5.161 -0.710 4.5 1.21 3.7 0.9 0.65 1.4
NEW SOURCE 272.528 -26.447 4.868 -3.450 4.0 0.95 4.2 0.6 0.56 1.0
NEW SOURCE 272.971 -24.537 6.739 -2.884 11.8 2.91 4.1 0.0 0.00 0.0
NEW SOURCE 269.873 -23.721 6.070 -0.019 9.7 2.38 4.1 2.0 1.44 1.4
NEW SOURCE 270.754 -25.854 4.613 -1.770 2.7 0.79 3.5 0.0 0.00 0.0
KS 1741-293 266.231 -29.323 359.590 -0.072 0.8 0.26 3.0 0.5 0.15 3.1
Go back to the INTEGRAL Galactic bulge home page