INTEGRAL Galactic Bulge MonitoringRevolution 0660: Observation start 2008-03-09T12:31 = MJD 54534.522
Total Observation GTI = 11535 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRO J1750-27 267.303 -26.646 0.4 2.371 +0.506 37.1 0.36 102.2 1.6 0.30 5.5
4U 1700-377 255.991 -37.841 0.7 347.759 +2.173 28.4 0.59 47.8 6.0 0.46 13.0
GX 5-1 270.280 -25.079 0.8 5.075 -1.015 16.1 0.37 43.8 0.0 0.00 0.0
4U 1722-30 261.885 -30.805 1.1 356.316 +2.298 9.2 0.33 27.6 3.9 0.27 14.4
H 1820-303 275.913 -30.357 1.1 2.789 -7.907 12.6 0.47 27.1 0.0 0.00 0.0
Ginga 1826-24 277.379 -23.800 1.2 9.275 -6.098 17.3 0.67 25.7 7.5 0.51 14.8
GX 354-0 263.001 -33.834 1.5 354.309 -0.158 6.4 0.33 19.5 1.3 0.27 5.0
GRS 1758-258 270.290 -25.750 2.3 4.497 -1.355 4.2 0.35 12.0 2.9 0.28 10.4
1E 1740.7-2942 265.975 -29.757 2.4 359.104 -0.110 3.2 0.29 11.0 2.2 0.24 9.1
IGR J17252-3616 261.270 -36.272 2.4 351.494 -0.330 4.5 0.41 11.0 1.6 0.33 4.9
GX 349+2 256.427 -36.408 2.4 349.111 +2.762 6.3 0.57 11.1 0.0 0.00 0.0
3A 1822-371 276.439 -37.115 2.5 356.839 -11.291 6.7 0.65 10.4 0.0 0.00 0.0
GX 9+1 270.355 -20.524 2.6 9.068 +1.180 5.7 0.55 10.4 0.0 0.00 0.0
GX 3+1 266.981 -26.579 0.0 2.280 +0.788 3.0 0.00 8.2 0.0 0.00 0.0
GX 1+4 263.026 -24.750 3.3 1.941 +4.780 2.7 0.35 7.9 0.0 0.00 0.0
SLX 1744-299_300 266.828 -29.942 3.6 359.332 -0.838 2.2 0.31 7.2 0.0 0.00 0.0
SLX 1735-269 264.574 -26.975 3.7 0.814 +2.408 2.5 0.36 6.9 0.0 0.00 0.0
Swift J174535.5-2901 266.354 -29.048 0.0 359.882 -0.020 1.9 0.00 6.1 0.0 0.00 0.0
H 1702-429 256.507 -43.019 3.9 343.875 -1.275 8.2 1.27 6.4 0.0 0.00 0.0
1E 1743.1-2843 266.539 -28.717 0.0 0.248 +0.014 1.5 0.00 4.7 0.0 0.00 0.0
H 1705-440 257.242 -44.127 6.2 343.308 -2.365 6.9 1.76 3.9 0.0 0.00 0.0
V1223 Sgr 283.872 -31.189 5.7 4.973 -14.453 10.6 0.00 4.3 0.0 0.00 0.0
XTE J1710-281 257.614 -28.153 0.0 356.373 +6.865 1.8 0.00 4.4 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 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
4U 1722-30 261.888 -30.802 356.320 +2.298 3.1 0.51 1.6 0.38
GX 354-0 262.989 -33.835 354.302 -0.150 3.7 0.70 1.5 0.51
MXB 1730-335 263.350 -33.388 354.841 -0.158 5.4 0.58 1.0 0.34
1A 1742-294 266.523 -29.515 359.559 -0.389 4.6 0.39 1.2 0.27
GX 3+1 266.983 -26.564 2.294 +0.794 32.4 0.84 4.4 0.47
GX 5-1 270.284 -25.079 5.077 -1.019 76.9 4.75 12.9 2.40
GRO J1750-27 267.303 -26.643 2.373 +0.508 12.7 0.75 8.9 0.48
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Revolution 0660: Observation start 2008-03-09T12:31 = MJD 54534.522
Total Observation GTI = 11535 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.303 -26.646 0.4 2.371 +0.506 37.1 0.36 102.2 1.6 0.30 5.5 4U 1700-377 255.991 -37.841 0.7 347.759 +2.173 28.4 0.59 47.8 6.0 0.46 13.0 GX 5-1 270.280 -25.079 0.8 5.075 -1.015 16.1 0.37 43.8 0.0 0.00 0.0 4U 1722-30 261.885 -30.805 1.1 356.316 +2.298 9.2 0.33 27.6 3.9 0.27 14.4 H 1820-303 275.913 -30.357 1.1 2.789 -7.907 12.6 0.47 27.1 0.0 0.00 0.0 Ginga 1826-24 277.379 -23.800 1.2 9.275 -6.098 17.3 0.67 25.7 7.5 0.51 14.8 GX 354-0 263.001 -33.834 1.5 354.309 -0.158 6.4 0.33 19.5 1.3 0.27 5.0 GRS 1758-258 270.290 -25.750 2.3 4.497 -1.355 4.2 0.35 12.0 2.9 0.28 10.4 1E 1740.7-2942 265.975 -29.757 2.4 359.104 -0.110 3.2 0.29 11.0 2.2 0.24 9.1 IGR J17252-3616 261.270 -36.272 2.4 351.494 -0.330 4.5 0.41 11.0 1.6 0.33 4.9 GX 349+2 256.427 -36.408 2.4 349.111 +2.762 6.3 0.57 11.1 0.0 0.00 0.0 3A 1822-371 276.439 -37.115 2.5 356.839 -11.291 6.7 0.65 10.4 0.0 0.00 0.0 GX 9+1 270.355 -20.524 2.6 9.068 +1.180 5.7 0.55 10.4 0.0 0.00 0.0 GX 3+1 266.981 -26.579 0.0 2.280 +0.788 3.0 0.00 8.2 0.0 0.00 0.0 GX 1+4 263.026 -24.750 3.3 1.941 +4.780 2.7 0.35 7.9 0.0 0.00 0.0 SLX 1744-299_300 266.828 -29.942 3.6 359.332 -0.838 2.2 0.31 7.2 0.0 0.00 0.0 SLX 1735-269 264.574 -26.975 3.7 0.814 +2.408 2.5 0.36 6.9 0.0 0.00 0.0 Swift J174535.5-2901 266.354 -29.048 0.0 359.882 -0.020 1.9 0.00 6.1 0.0 0.00 0.0 H 1702-429 256.507 -43.019 3.9 343.875 -1.275 8.2 1.27 6.4 0.0 0.00 0.0 1E 1743.1-2843 266.539 -28.717 0.0 0.248 +0.014 1.5 0.00 4.7 0.0 0.00 0.0 H 1705-440 257.242 -44.127 6.2 343.308 -2.365 6.9 1.76 3.9 0.0 0.00 0.0 V1223 Sgr 283.872 -31.189 5.7 4.973 -14.453 10.6 0.00 4.3 0.0 0.00 0.0 XTE J1710-281 257.614 -28.153 0.0 356.373 +6.865 1.8 0.00 4.4 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 4U 1722-30 261.888 -30.802 356.320 +2.298 3.1 0.51 1.6 0.38 GX 354-0 262.989 -33.835 354.302 -0.150 3.7 0.70 1.5 0.51 MXB 1730-335 263.350 -33.388 354.841 -0.158 5.4 0.58 1.0 0.34 1A 1742-294 266.523 -29.515 359.559 -0.389 4.6 0.39 1.2 0.27 GX 3+1 266.983 -26.564 2.294 +0.794 32.4 0.84 4.4 0.47 GX 5-1 270.284 -25.079 5.077 -1.019 76.9 4.75 12.9 2.40 GRO J1750-27 267.303 -26.643 2.373 +0.508 12.7 0.75 8.9 0.48
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