INTEGRAL Galactic bulge Monitoring
Revolution 1986: Observation start 2018-08-11T07:44 = MJD 58341.323
Total Observation GTI = 16091 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 1700-377 255.990 -37.841 0.6 347.758 +2.173 124.6 1.84 67.8 19.9 0.57 35.2 1E 1740.7-2942 265.989 -29.756 0.9 359.112 -0.119 28.0 0.82 34.3 9.8 0.28 35.3 GRS 1758-258 270.290 -25.749 1.3 4.498 -1.355 17.5 0.79 22.2 6.6 0.26 24.9 GX 1+4 262.992 -24.736 1.8 1.937 +4.813 12.2 0.77 15.8 0.0 0.00 0.0 IGR J17591-2342 269.774 -23.715 2.7 6.030 +0.062 8.0 0.83 9.7 2.0 0.27 7.1 SLX 1735-269 264.568 -27.032 3.0 0.762 +2.383 6.8 0.79 8.6 1.1 0.00 4.2 IGR J18027-2016 270.719 -20.326 3.8 9.408 +0.981 7.1 1.07 6.6 0.0 0.00 0.0 AX J1754.2-2754 268.511 -27.930 3.5 1.815 -1.073 5.2 0.71 7.3 0.0 0.00 0.0 H 1820-303 275.915 -30.311 3.9 2.832 -7.888 7.5 1.16 6.5 0.0 0.00 0.0 3A 1822-371 276.482 -37.085 3.8 356.882 -11.308 11.3 1.70 6.6 0.0 0.00 0.0 SAX J1712.6-3739 258.131 -37.667 4.2 348.910 +0.920 9.9 1.63 6.0 0.0 0.00 0.0 Swift J174540.7-2900 266.437 -28.973 4.3 359.983 -0.043 4.6 0.79 5.8 0.0 0.00 0.0 Ginga 1826-24 277.323 -23.822 4.5 9.231 -6.063 8.0 0.00 5.6 0.0 0.00 0.0 1RXS J175113.3-20121 267.945 -20.158 4.9 8.251 +3.319 5.1 0.00 5.1 0.0 0.00 0.0 GX 17+2 274.002 -14.048 5.2 16.420 +1.275 20.0 4.20 4.8 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 ==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== =====