INTEGRAL Galactic bulge Monitoring
Revolution 0607: Observation start 1999-12-31T23:58 = MJD 51544
Total Observation GTI = 17233 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 1+4 263.005 -24.740 0.7 1.940 +4.801 14.6 0.31 47.1 0.0 0.00 0.0 GX 354-0 262.997 -33.834 0.8 354.306 -0.155 15.1 0.34 44.5 4.3 0.28 15.6 Ginga 1826-24 277.367 -23.799 0.8 9.270 -6.088 20.4 0.52 39.5 7.2 0.40 18.3 GX 5-1 270.282 -25.078 0.8 5.077 -1.016 12.3 0.31 39.2 0.0 0.00 0.0 H 1820-303 275.914 -30.354 1.3 2.793 -7.907 9.5 0.43 21.9 0.0 0.00 0.0 4U 1700-377 255.994 -37.854 1.4 347.750 +2.163 13.8 0.67 20.5 5.3 0.52 10.1 SAX J1810.8-2609 272.682 -26.147 1.4 5.199 -3.427 6.7 0.34 20.0 2.5 0.27 9.4 GX 349+2 256.444 -36.438 1.7 349.096 +2.734 9.6 0.59 16.2 0.0 0.00 0.0 3A 1822-371 276.441 -37.085 2.0 356.867 -11.279 8.5 0.60 14.0 0.0 0.00 0.0 GX 3+1 266.980 -26.563 1.9 2.293 +0.797 4.2 0.29 14.6 0.0 0.00 0.0 GX 17+2 274.007 -14.025 2.0 16.443 +1.282 23.7 1.71 13.8 0.0 0.00 0.0 4U 1722-30 261.853 -30.801 2.4 356.304 +2.324 3.2 0.29 11.0 1.6 0.23 6.7 GRS 1758-258 270.307 -25.733 2.3 4.519 -1.360 3.7 0.32 11.7 2.1 0.25 8.4 GX 9+1 270.369 -20.503 2.5 9.092 +1.180 4.1 0.40 10.4 0.0 0.00 0.0 SLX 1744-299_300 266.877 -30.017 3.0 359.289 -0.913 2.7 0.31 8.6 0.0 0.00 0.0 SLX 1735-269 264.573 -27.004 3.1 0.788 +2.393 2.3 0.28 8.4 1.4 0.23 6.2 IGR J17586-2129 269.629 -21.341 4.0 8.021 +1.363 2.3 0.36 6.3 0.0 0.00 0.0 XB 1832-330 278.904 -33.060 3.8 1.456 -11.378 3.8 0.58 6.6 0.0 0.00 0.0 1A 1742-294 266.522 -29.515 5.1 359.559 -0.388 1.4 0.30 4.8 0.0 0.00 0.0 IGR J17252-3616 261.208 -36.239 5.0 351.493 -0.270 2.2 0.45 5.0 0.0 0.00 0.0 SGR J1745-29 266.451 -28.998 0.0 359.968 -0.067 1.3 0.00 4.4 0.0 0.00 0.0 GX 13+1 273.678 -17.146 5.2 13.548 +0.072 3.2 0.67 4.8 0.0 0.00 0.0 IGR J17091-3624 257.283 -36.383 5.7 349.544 +2.226 2.3 0.53 4.3 0.0 0.00 0.0 3A 1728-169 262.892 -16.974 5.4 8.481 +9.065 2.7 0.58 4.5 0.0 0.00 0.0 AX J1700.2-4220 254.992 -42.316 5.4 343.752 +0.036 14.1 3.08 4.6 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 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 4.7 0.30 15.6 0.8 0.16 5.1 1A 1743-288 266.764 -28.882 0.210 -0.240 5.7 0.30 19.0 0.3 0.16 2.0 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.3 0.29 4.5 0.2 0.16 1.5 GRS 1758-258 270.303 -25.741 4.511 -1.361 5.8 0.89 6.5 1.3 0.44 2.9 GX 3+1 266.980 -26.567 2.289 +0.794 42.0 0.43 97.5 4.6 0.21 21.8 GX 354-0 262.989 -33.835 354.302 -0.150 11.3 2.13 5.3 4.4 1.55 2.8 GX 5-1 270.287 -25.077 5.080 -1.020 120.1 1.48 81.2 12.4 0.63 19.7 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.1 0.34 3.3 0.0 0.00 0.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.7 0.31 5.5 0.5 0.18 2.5 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.9 0.29 3.1 0.3 0.16 1.8 NEW SOURCE 265.623 -22.126 5.442 +4.161 9.7 1.89 5.1 0.0 0.00 0.0 NEW SOURCE 272.770 -26.241 5.154 -3.541 11.7 2.55 4.6 1.9 1.57 1.2 NEW SOURCE 266.095 -22.359 5.472 +3.667 8.5 1.70 5.0 1.1 0.91 1.2 NEW SOURCE 268.971 -22.326 6.863 +1.398 15.4 3.39 4.5 2.8 2.04 1.4