Revolution 0360: Observation start 2005-09-26T19:31 = MJD 53639.814
Total Observation GTI = 13686 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRS 1758-258 270.299 -25.742 0.8 4.508 -1.359 13.3 0.34 38.9 8.0 0.28 28.9
4U 1700-377 256.000 -37.847 0.9 347.758 +2.163 23.5 0.66 35.6 7.8 0.51 15.2
Ginga 1826-24 277.361 -23.793 0.9 9.274 -6.080 20.4 0.54 37.7 7.3 0.42 17.5
GX 1+4 263.012 -24.731 1.1 1.950 +4.800 8.1 0.30 26.6 0.0 0.00 0.0
1E 1740.7-2942 265.978 -29.750 1.2 359.112 -0.108 6.9 0.29 23.8 4.2 0.24 17.3
GX 354-0 262.990 -33.838 1.3 354.300 -0.152 7.1 0.31 23.2 0.0 0.00 0.0
H 1820-303 275.935 -30.349 1.5 2.805 -7.921 8.0 0.43 18.6 0.0 0.00 0.0
3A 1822-371 276.449 -37.087 2.1 356.868 -11.286 7.7 0.58 13.1 0.0 0.00 0.0
GX 349+2 256.422 -36.406 2.2 349.111 +2.767 7.2 0.57 12.5 0.0 0.00 0.0
GX 5-1 270.266 -25.059 2.2 5.087 -0.994 3.9 0.32 12.5 0.0 0.00 0.0
IGR J17252-3616 261.296 -36.269 2.1 351.508 -0.345 5.4 0.41 13.1 0.0 0.00 0.0
OAO 1657-415 255.196 -41.661 2.6 344.362 +0.320 13.8 1.36 10.1 5.1 1.03 4.9
XTE J1739-285 264.995 -28.524 3.0 359.700 +1.269 2.5 0.28 8.7 1.3 0.23 5.5
SLX 1744-299_300 266.878 -29.979 3.3 359.323 -0.893 2.5 0.32 7.9 1.3 0.27 4.6
GX 9+1 270.374 -20.598 3.5 9.012 +1.128 3.0 0.41 7.4 0.0 0.00 0.0
SLX 1735-269 264.597 -26.960 2.8 0.837 +2.399 2.7 0.28 9.5 0.0 0.00 0.0
GRO J1655-40 253.442 -39.861 3.2 344.942 +2.482 8.5 1.06 8.0 4.8 0.78 6.2
GX 13+1 273.640 -17.115 3.7 13.558 +0.119 5.0 0.74 6.8 0.0 0.00 0.0
SGR J1745-29 266.474 -29.017 3.4 359.962 -0.093 1.9 0.25 7.5 0.0 0.00 0.0
GX 3+1 266.976 -26.514 4.4 2.333 +0.825 1.5 0.27 5.7 0.0 0.00 0.0
1RXS J163759.7-26062 249.474 -26.142 5.8 353.456 +13.811 8.4 2.00 4.2 0.0 0.00 0.0
KS 1741-293 266.212 -29.336 0.0 359.571 -0.064 1.3 0.00 4.9 0.7 0.00 3.3
AX J1749.1-2733 267.297 -27.493 4.8 1.642 +0.075 1.6 0.30 5.1 0.0 0.00 0.0
1A 1744-361 267.006 -36.045 0.0 354.175 -4.114 1.5 0.00 4.3 0.0 0.00 0.0
IGR J17464-3213 266.638 -32.192 7.0 357.323 -1.864 1.1 0.32 3.4 0.0 0.00 0.0
1E 1743.1-2843 266.588 -28.677 0.0 0.305 -0.002 1.1 0.00 4.1 0.0 0.00 0.0
1RXS J170849.0-40091 257.150 -40.160 0.0 346.451 +0.057 2.9 0.00 4.0 0.0 0.00 0.0
SLX 1746-331 267.380 -33.110 6.2 356.858 -2.873 1.1 0.00 3.9 0.0 0.00 0.0
1RXS J175721.2-30440 269.404 -30.843 6.0 359.686 -3.209 1.1 0.28 4.1 0.0 0.00 0.0
GX 17+2 274.025 -14.052 7.9 16.428 +1.254 8.9 2.96 3.0 0.0 0.00 0.0
SAX J1712.6-3739 258.115 -37.611 0.0 348.949 +0.964 1.8 0.00 3.5 0.0 0.00 0.0
GRS 1734-292 264.403 -29.077 6.7 358.955 +1.413 1.0 0.28 3.6 0.0 0.00 0.0
JEM-X
JEM-X1 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 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 1742-294 266.520 -29.513 359.560 -0.386 4.1 0.26 15.7 0.6 0.15 4.1
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.27 7.9 1.1 0.16 6.8
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.28 3.0 0.2 0.16 1.5
4U 1722-30 261.886 -30.800 356.320 +2.300 7.6 0.70 10.8 0.8 0.49 1.7
GRS 1747-312 267.690 -31.292 358.555 -2.168 1.4 0.27 5.3 0.2 0.17 1.5
GX 3+1 266.972 -26.573 2.281 +0.797 19.9 0.51 38.8 2.0 0.27 7.2
GX 354-0 262.994 -33.838 354.301 -0.155 16.8 1.24 13.5 4.6 0.92 5.1
GX 5-1 270.286 -25.082 5.075 -1.022 91.0 1.77 51.5 5.9 0.74 7.9
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 0.8 0.25 3.0 0.3 0.16 2.1
XTE J1739-285 264.975 -28.496 359.714 +1.298 1.3 0.34 3.9 0.3 0.20 1.4
NEW SOURCE 270.784 -24.193 6.072 -0.976 13.0 2.73 4.8 0.0 0.00 0.0
NEW SOURCE 269.697 -25.537 4.416 -0.786 4.2 0.87 4.8 0.0 0.00 0.0
Go back to the INTEGRAL Galactic bulge home page