INTEGRAL Galactic Bulge MonitoringRevolution 0492: Observation start 2006-10-23 = MJD 54031
Total Observation GTI = 12277 seconds
ISGRI
ISGRI significance mosaic images. Left: 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 OSA7, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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.
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+4 263.013 -24.742 0.6 1.942 +4.794 21.6 0.34 63.2 0.0 0.00 0.0
GX 5-1 270.290 -25.082 0.7 5.077 -1.024 16.6 0.33 50.4 1.5 0.27 5.6
4U 1700-377 255.992 -37.850 0.7 347.753 +2.167 34.9 0.71 49.0 10.2 0.56 18.4
GRS 1758-258 270.293 -25.744 1.1 4.503 -1.354 9.9 0.35 28.4 5.7 0.29 20.0
H 1820-303 275.932 -30.367 1.1 2.788 -7.926 12.1 0.43 28.3 0.0 0.00 0.0
1E 1740.7-2942 265.974 -29.755 1.2 359.106 -0.107 7.1 0.28 25.2 3.8 0.24 15.9
Ginga 1826-24 277.365 -23.795 1.3 9.273 -6.085 12.3 0.53 23.1 3.0 0.42 7.2
IGR J17497-2821 267.385 -28.344 1.7 0.952 -0.430 4.9 0.29 16.5 3.6 0.25 14.4
GX 349+2 256.436 -36.424 1.9 349.103 +2.748 8.7 0.60 14.5 0.0 0.00 0.0
4U 1722-30 261.905 -30.800 2.2 356.329 +2.288 3.9 0.31 12.4 1.8 0.25 7.3
GX 354-0 262.982 -33.818 2.1 354.313 -0.136 5.0 0.38 13.3 0.0 0.00 0.0
GX 9+1 270.397 -20.512 2.4 9.097 +1.152 4.8 0.43 11.2 0.0 0.00 0.0
3A 1822-371 276.425 -37.126 2.6 356.824 -11.285 6.0 0.59 10.2 0.0 0.00 0.0
1A 1742-294 266.497 -29.501 0.0 359.559 -0.362 2.7 0.00 8.6 0.0 0.00 0.0
GX 3+1 267.013 -26.565 3.0 2.306 +0.770 2.9 0.33 8.8 0.0 0.00 0.0
SLX 1744-299_300 266.862 -30.004 4.0 359.294 -0.895 1.8 0.29 6.3 1.1 0.24 4.6
H 1702-429 256.524 -43.084 4.1 343.831 -1.324 15.3 2.46 6.2 7.0 1.74 4.0
SLX 1735-269 264.644 -26.952 4.6 0.866 +2.368 1.6 0.29 5.4 1.4 0.23 6.0
IGR J17200-3116 260.025 -31.332 4.8 354.982 +3.320 1.8 0.34 5.2 0.0 0.00 0.0
1E 1743.1-2843 266.496 -28.760 0.0 0.192 +0.023 1.4 0.00 4.9 0.0 0.00 0.0
XB 1832-330 278.953 -32.970 5.2 1.558 -11.378 2.7 0.58 4.7 0.0 0.00 0.0
GRS 1741.9-2853 266.120 -28.925 0.0 359.880 +0.219 1.2 0.00 4.6 0.0 0.00 0.0
V2400 Oph 258.165 -24.267 0.0 359.856 +8.717 1.8 0.00 4.2 0.0 0.00 0.0
IGR J17088-4008 257.358 -40.177 0.0 346.532 -0.081 3.2 0.00 3.9 0.0 0.00 0.0
Swift J174535.5-2901 266.496 -29.090 0.0 359.911 -0.148 1.0 0.00 3.7 0.0 0.00 0.0
3A 1728-169 262.904 -16.917 6.3 8.536 +9.086 2.7 0.69 3.9 0.0 0.00 0.0
JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.
Note: Sources labelled were detected with in the 3-10 keV image > 5σ and 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 ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).
NOTE: 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.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- B(cps) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
GX 354-0 262.989 -33.835 354.302 -0.150 12.8 1.28 2.7 0.85
GX 3+1 266.983 -26.564 2.294 +0.794 21.7 0.55 3.1 0.29
GX 5-1 270.284 -25.079 5.077 -1.019 115.0 2.26 19.8 1.09
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Revolution 0492: Observation start 2006-10-23 = MJD 54031
Total Observation GTI = 12277 seconds
ISGRI
ISGRI significance mosaic images. Left: 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 OSA7, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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.
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+4 263.013 -24.742 0.6 1.942 +4.794 21.6 0.34 63.2 0.0 0.00 0.0 GX 5-1 270.290 -25.082 0.7 5.077 -1.024 16.6 0.33 50.4 1.5 0.27 5.6 4U 1700-377 255.992 -37.850 0.7 347.753 +2.167 34.9 0.71 49.0 10.2 0.56 18.4 GRS 1758-258 270.293 -25.744 1.1 4.503 -1.354 9.9 0.35 28.4 5.7 0.29 20.0 H 1820-303 275.932 -30.367 1.1 2.788 -7.926 12.1 0.43 28.3 0.0 0.00 0.0 1E 1740.7-2942 265.974 -29.755 1.2 359.106 -0.107 7.1 0.28 25.2 3.8 0.24 15.9 Ginga 1826-24 277.365 -23.795 1.3 9.273 -6.085 12.3 0.53 23.1 3.0 0.42 7.2 IGR J17497-2821 267.385 -28.344 1.7 0.952 -0.430 4.9 0.29 16.5 3.6 0.25 14.4 GX 349+2 256.436 -36.424 1.9 349.103 +2.748 8.7 0.60 14.5 0.0 0.00 0.0 4U 1722-30 261.905 -30.800 2.2 356.329 +2.288 3.9 0.31 12.4 1.8 0.25 7.3 GX 354-0 262.982 -33.818 2.1 354.313 -0.136 5.0 0.38 13.3 0.0 0.00 0.0 GX 9+1 270.397 -20.512 2.4 9.097 +1.152 4.8 0.43 11.2 0.0 0.00 0.0 3A 1822-371 276.425 -37.126 2.6 356.824 -11.285 6.0 0.59 10.2 0.0 0.00 0.0 1A 1742-294 266.497 -29.501 0.0 359.559 -0.362 2.7 0.00 8.6 0.0 0.00 0.0 GX 3+1 267.013 -26.565 3.0 2.306 +0.770 2.9 0.33 8.8 0.0 0.00 0.0 SLX 1744-299_300 266.862 -30.004 4.0 359.294 -0.895 1.8 0.29 6.3 1.1 0.24 4.6 H 1702-429 256.524 -43.084 4.1 343.831 -1.324 15.3 2.46 6.2 7.0 1.74 4.0 SLX 1735-269 264.644 -26.952 4.6 0.866 +2.368 1.6 0.29 5.4 1.4 0.23 6.0 IGR J17200-3116 260.025 -31.332 4.8 354.982 +3.320 1.8 0.34 5.2 0.0 0.00 0.0 1E 1743.1-2843 266.496 -28.760 0.0 0.192 +0.023 1.4 0.00 4.9 0.0 0.00 0.0 XB 1832-330 278.953 -32.970 5.2 1.558 -11.378 2.7 0.58 4.7 0.0 0.00 0.0 GRS 1741.9-2853 266.120 -28.925 0.0 359.880 +0.219 1.2 0.00 4.6 0.0 0.00 0.0 V2400 Oph 258.165 -24.267 0.0 359.856 +8.717 1.8 0.00 4.2 0.0 0.00 0.0 IGR J17088-4008 257.358 -40.177 0.0 346.532 -0.081 3.2 0.00 3.9 0.0 0.00 0.0 Swift J174535.5-2901 266.496 -29.090 0.0 359.911 -0.148 1.0 0.00 3.7 0.0 0.00 0.0 3A 1728-169 262.904 -16.917 6.3 8.536 +9.086 2.7 0.69 3.9 0.0 0.00 0.0
JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.
Note: Sources labelled were detected with in the 3-10 keV image > 5σ and 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 ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).
NOTE: 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.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- B(cps) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 12.8 1.28 2.7 0.85 GX 3+1 266.983 -26.564 2.294 +0.794 21.7 0.55 3.1 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 115.0 2.26 19.8 1.09
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