INTEGRAL Galactic bulge Monitoring
Revolution 0603: Observation start 2007-09-21T04:10 = MJD 54364.174
Total Observation GTI = 11856 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 SOURCEs < 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 1700-377 255.984 -37.850 0.6 347.749 +2.171 47.5 0.79 60.2 13.3 0.60 22.2 GX 5-1 270.285 -25.082 0.7 5.075 -1.020 17.7 0.36 49.5 0.0 0.00 0.0 SAX J1810.8-2609 272.688 -26.151 0.9 5.198 -3.434 13.7 0.40 34.0 5.3 0.32 16.8 GX 1+4 263.011 -24.741 0.9 1.942 +4.796 13.6 0.39 35.3 0.0 0.00 0.0 Ginga 1826-24 277.361 -23.793 1.0 9.273 -6.081 19.8 0.61 32.8 7.1 0.47 15.1 GX 349+2 256.448 -36.429 1.6 349.105 +2.737 11.9 0.68 17.5 0.0 0.00 0.0 IGR J17544-2619 268.594 -26.324 1.8 3.237 -0.323 5.3 0.34 15.7 0.0 0.00 0.0 3A 1822-371 276.489 -37.082 2.0 356.887 -11.313 9.8 0.74 13.3 0.0 0.00 0.0 GRS 1758-258 270.317 -25.746 0.0 4.513 -1.374 4.2 0.00 12.2 2.6 0.27 9.3 H 1820-303 275.923 -30.356 2.0 2.795 -7.915 7.4 0.55 13.6 0.0 0.00 0.0 GX 3+1 266.986 -26.564 2.4 2.294 +0.791 3.8 0.34 11.4 0.0 0.00 0.0 4U 1722-30 261.888 -30.823 2.5 356.302 +2.287 4.3 0.40 10.7 1.4 0.32 4.4 GX 9+1 270.345 -20.543 3.6 9.046 +1.179 3.6 0.52 7.1 0.0 0.00 0.0 GX 354-0 263.058 -33.847 3.9 354.323 -0.205 2.8 0.42 6.5 0.0 0.00 0.0 SLX 1735-269 264.574 -26.981 3.6 0.808 +2.405 2.8 0.40 7.1 0.0 0.00 0.0 1E 1743.1-2843 266.587 -28.757 0.0 0.236 -0.043 1.7 0.00 5.4 0.0 0.00 0.0 SAX J1712.6-3739 258.106 -37.580 4.6 348.970 +0.988 3.2 0.60 5.4 0.0 0.00 0.0 SLX 1744-299_300 266.774 -29.947 5.3 359.303 -0.800 1.6 0.35 4.6 0.0 0.00 0.0 GX 17+2 274.024 -14.027 5.0 16.449 +1.266 16.8 3.37 5.0 0.0 0.00 0.0 GX 13+1 273.708 -17.112 5.9 13.592 +0.064 4.2 1.01 4.1 0.0 0.00 0.0 IGR J18027-2016 270.732 -20.240 5.5 9.489 +1.013 2.4 0.53 4.4 0.0 0.00 0.0 1A 1742-294 266.569 -29.553 4.6 359.548 -0.443 1.7 0.32 5.4 0.0 0.00 0.0 Swift J174535.5-2901 266.399 -29.087 0.0 359.869 -0.074 1.3 0.00 4.2 0.0 0.00 0.0 XB 1832-330 278.870 -32.916 6.0 1.578 -11.291 2.8 0.70 4.0 0.0 0.00 0.0 IGR J17407-2808 265.277 -28.180 5.7 0.123 +1.240 1.4 0.33 4.3 0.0 0.00 0.0 H 1702-429 256.620 -43.045 5.4 343.904 -1.356 13.1 2.90 4.5 0.0 0.00 0.0 GRS 1747-312 267.766 -31.205 5.9 358.663 -2.180 1.5 0.36 4.2 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 SOURCEs < 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 1742-294 266.523 -29.515 359.559 -0.389 5.7 0.31 18.1 1.0 0.18 5.2 4U 1722-30 261.888 -30.802 356.320 +2.298 2.0 0.65 3.1 0.8 0.49 1.6 GX 3+1 266.981 -26.569 2.288 +0.792 46.1 0.53 87.3 4.9 0.26 18.8 GX 354-0 262.977 -33.820 354.308 -0.134 11.9 1.25 9.5 2.0 1.00 2.0 GX 5-1 270.287 -25.081 5.077 -1.021 109.9 1.94 56.7 18.7 0.96 19.5 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.5 0.42 3.6 0.0 0.00 0.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.0 0.31 3.2 0.0 0.00 0.0 NEW SOURCE 269.162 -23.657 5.800 +0.577 10.9 2.15 5.1 1.9 1.19 1.6 NEW SOURCE 269.354 -24.507 5.153 -0.001 6.3 1.51 4.2 1.6 0.82 1.9 NEW SOURCE 264.950 -25.626 2.137 +2.840 2.6 0.61 4.3 0.6 0.35 1.6 NEW SOURCE 271.236 -26.109 4.603 -2.272 5.8 1.37 4.2 0.0 0.00 0.0 NEW SOURCE 272.837 -25.669 5.686 -3.320 18.2 4.27 4.3 0.0 0.00 0.0 NEW SOURCE 264.530 -26.571 1.135 +2.657 2.0 0.47 4.2 0.0 0.00 0.0 IGR J17544-2619 268.599 -26.355 3.212 -0.343 1.6 0.58 2.8 1.0 0.31 3.3