INTEGRAL Galactic bulge Monitoring
Revolution 1465: Observation start 2014-10-12T12:27 = MJD 56942.52
Total Observation GTI = 11872 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17464-3213 266.561 -32.237 0.7 357.250 -1.832 22.6 0.42 54.4 17.3 0.28 60.9 Ginga 1826-24 277.362 -23.778 1.0 9.287 -6.075 19.4 0.65 30.0 7.9 0.41 19.3 GRS 1758-258 270.307 -25.743 1.1 4.510 -1.366 11.6 0.43 27.2 9.0 0.28 31.7 GX 354-0 262.990 -33.887 1.7 354.259 -0.179 7.8 0.47 16.7 0.0 0.00 0.0 H 1820-303 275.897 -30.358 2.3 2.782 -7.896 6.3 0.53 11.8 0.0 0.00 0.0 4U 1700-377 255.977 -37.857 2.6 347.739 +2.171 10.1 0.98 10.2 4.2 0.61 6.9 GX 349+2 256.296 -36.426 3.0 349.033 +2.836 7.3 0.82 8.8 0.0 0.00 0.0 GX 1+4 262.976 -24.739 2.8 1.926 +4.823 3.8 0.40 9.4 0.0 0.00 0.0 SLX 1735-269 264.565 -27.004 3.6 0.785 +2.400 2.5 0.36 7.2 1.7 0.25 6.7 GX 17+2 274.060 -14.049 3.2 16.446 +1.226 16.4 2.06 7.9 0.0 0.00 0.0 3A 1822-371 276.488 -37.134 0.0 356.838 -11.334 6.3 0.00 6.7 0.0 0.00 0.0 H 1702-429 256.588 -43.047 4.2 343.888 -1.340 25.7 4.24 6.0 0.0 0.00 0.0 IGR J18027-2016 270.604 -20.291 4.6 9.385 +1.092 2.9 0.55 5.4 0.0 0.00 0.0 GX 9+1 270.367 -20.611 0.0 8.997 +1.128 2.4 0.00 4.9 0.0 0.00 0.0 4U 1722-30 261.849 -30.689 5.1 356.395 +2.388 2.0 0.42 4.8 0.0 0.00 0.0 IGR J17454-2919 266.356 -29.414 0.0 359.570 -0.213 1.9 0.00 4.7 0.0 0.00 0.0 GRS 1734-292 264.389 -29.148 4.8 358.888 +1.384 2.1 0.40 5.2 0.0 0.00 0.0 3A 1728-169 262.974 -16.970 5.0 8.526 +9.001 3.8 0.77 5.0 0.0 0.00 0.0 AX J1740.1-3102 265.004 -31.033 5.8 357.578 -0.071 1.7 0.40 4.2 0.0 0.00 0.0 1RXS J180408.9-34205 271.089 -34.393 5.1 357.279 -6.186 2.3 0.49 4.8 0.0 0.00 0.0 SGR J1745-29 266.451 -29.003 0.0 359.964 -0.069 1.8 0.00 4.2 1.2 0.29 4.0 SAX J1752.3-3138 268.222 -31.644 6.6 358.484 -2.738 1.7 0.45 3.7 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 ~ 109 cps [J1], 116 cps [J2]); B = 10-25 keV (1 Crab ~ 34 cps [J1], 32 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+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 1742-294 266.520 -29.513 359.560 -0.386 2.7 0.16 16.7 0.6 0.10 6.2 4U 1722-30 261.888 -30.802 356.320 +2.298 2.9 0.61 4.8 0.8 0.37 2.0 GRS 1739-278 265.653 -27.743 0.670 +1.189 1.8 0.14 12.9 0.0 0.00 0.0 GRS 1747-312 267.690 -31.292 358.555 -2.168 0.8 0.24 3.2 0.0 0.00 0.0 GX 3+1 266.989 -26.561 2.299 +0.791 4.3 0.14 30.1 2.2 0.15 14.8 GX 354-0 262.989 -33.835 354.302 -0.150 23.3 2.20 10.6 2.8 1.42 2.0 GX 5-1 270.284 -25.079 5.077 -1.019 2.3 0.21 10.7 2.4 0.45 5.3 IGR J17464-3213 266.567 -32.229 357.260 -1.832 4.8 0.42 11.6 1.0 0.18 5.8 SLX 1735-269 264.571 -26.994 0.796 +2.400 0.9 0.18 5.1 0.5 0.16 3.1 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 0.8 0.17 5.0 0.3 0.11 2.5 NEW SOURCE 263.342 -23.371 3.263 +5.282 4.2 1.11 3.8 0.0 0.00 0.0 NEW SOURCE 267.304 -22.083 6.287 +2.851 7.3 2.11 3.5 0.0 0.00 0.0 NEW SOURCE 266.948 -22.161 6.051 +3.094 6.1 1.93 3.2 0.0 0.00 0.0