INTEGRAL Galactic Bulge MonitoringRevolution 0545: Observation start 2007-03-31 = MJD 54190
Total Observation GTI = 10861 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
4U 1700-377 255.989 -37.848 0.6 347.752 +2.169 44.7 0.73 60.9 13.8 0.56 24.8
GX 1+4 263.013 -24.746 0.7 1.939 +4.791 17.7 0.39 45.7 0.0 0.00 0.0
GRS 1758-258 270.308 -25.741 1.0 4.513 -1.364 11.9 0.39 30.6 8.4 0.32 26.6
1E 1740.7-2942 265.980 -29.741 1.1 359.120 -0.105 10.3 0.35 29.3 5.8 0.29 19.7
Ginga 1826-24 277.380 -23.805 1.1 9.270 -6.102 15.7 0.58 26.9 6.7 0.46 14.6
GX 5-1 270.291 -25.084 1.5 5.076 -1.026 7.7 0.41 18.9 0.0 0.00 0.0
H 1820-303 275.901 -30.379 1.6 2.765 -7.908 7.9 0.43 18.3 0.0 0.00 0.0
GX 354-0 263.007 -33.825 1.7 354.318 -0.157 6.0 0.37 16.1 0.0 0.00 0.0
1A 1742-294 266.526 -29.512 1.8 359.564 -0.390 5.4 0.35 15.5 2.2 0.29 7.4
GX 349+2 256.444 -36.397 2.1 349.129 +2.759 7.6 0.58 13.2 0.0 0.00 0.0
OAO 1657-415 255.219 -41.640 1.9 344.389 +0.320 19.5 1.34 14.6 0.0 0.00 0.0
3A 1822-371 276.465 -37.131 2.3 356.834 -11.316 6.5 0.56 11.5 0.0 0.00 0.0
4U 1722-30 261.911 -30.783 2.7 356.346 +2.292 4.2 0.42 9.8 2.1 0.34 6.3
GX 3+1 266.981 -26.576 2.5 2.283 +0.789 3.6 0.34 10.6 0.0 0.00 0.0
GX 9+1 270.410 -20.489 3.8 9.123 +1.153 3.4 0.52 6.6 0.0 0.00 0.0
4U 1735-444 264.722 -44.419 3.3 346.073 -6.965 10.6 1.34 7.9 0.0 0.00 0.0
XB 1832-330 278.958 -33.005 3.9 1.527 -11.396 4.0 0.61 6.4 1.7 0.00 3.5
GRS 1741.9-2853 266.334 -28.958 4.1 359.949 +0.042 2.2 0.35 6.1 0.0 0.00 0.0
SLX 1744-299_300 266.849 -30.009 4.8 359.284 -0.888 1.6 0.30 5.2 0.0 0.00 0.0
SLX 1735-269 264.572 -27.009 4.8 0.784 +2.392 1.8 0.35 5.1 1.1 0.00 3.8
3A 1728-169 262.942 -16.968 4.8 8.511 +9.028 5.1 0.98 5.2 0.0 0.00 0.0
GRS 1734-292 264.412 -29.153 5.5 358.896 +1.365 1.6 0.35 4.5 0.0 0.00 0.0
NEW_1 283.871 -42.974 4.2 353.538 -18.803 18.0 3.04 6.0 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 17.3 1.23 4.4 0.84
GX 3+1 266.983 -26.564 2.294 +0.794 28.2 0.78 3.6 0.41
GX 5-1 270.284 -25.079 5.077 -1.019 81.2 2.45 9.0 1.12
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Revolution 0545: Observation start 2007-03-31 = MJD 54190
Total Observation GTI = 10861 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.989 -37.848 0.6 347.752 +2.169 44.7 0.73 60.9 13.8 0.56 24.8 GX 1+4 263.013 -24.746 0.7 1.939 +4.791 17.7 0.39 45.7 0.0 0.00 0.0 GRS 1758-258 270.308 -25.741 1.0 4.513 -1.364 11.9 0.39 30.6 8.4 0.32 26.6 1E 1740.7-2942 265.980 -29.741 1.1 359.120 -0.105 10.3 0.35 29.3 5.8 0.29 19.7 Ginga 1826-24 277.380 -23.805 1.1 9.270 -6.102 15.7 0.58 26.9 6.7 0.46 14.6 GX 5-1 270.291 -25.084 1.5 5.076 -1.026 7.7 0.41 18.9 0.0 0.00 0.0 H 1820-303 275.901 -30.379 1.6 2.765 -7.908 7.9 0.43 18.3 0.0 0.00 0.0 GX 354-0 263.007 -33.825 1.7 354.318 -0.157 6.0 0.37 16.1 0.0 0.00 0.0 1A 1742-294 266.526 -29.512 1.8 359.564 -0.390 5.4 0.35 15.5 2.2 0.29 7.4 GX 349+2 256.444 -36.397 2.1 349.129 +2.759 7.6 0.58 13.2 0.0 0.00 0.0 OAO 1657-415 255.219 -41.640 1.9 344.389 +0.320 19.5 1.34 14.6 0.0 0.00 0.0 3A 1822-371 276.465 -37.131 2.3 356.834 -11.316 6.5 0.56 11.5 0.0 0.00 0.0 4U 1722-30 261.911 -30.783 2.7 356.346 +2.292 4.2 0.42 9.8 2.1 0.34 6.3 GX 3+1 266.981 -26.576 2.5 2.283 +0.789 3.6 0.34 10.6 0.0 0.00 0.0 GX 9+1 270.410 -20.489 3.8 9.123 +1.153 3.4 0.52 6.6 0.0 0.00 0.0 4U 1735-444 264.722 -44.419 3.3 346.073 -6.965 10.6 1.34 7.9 0.0 0.00 0.0 XB 1832-330 278.958 -33.005 3.9 1.527 -11.396 4.0 0.61 6.4 1.7 0.00 3.5 GRS 1741.9-2853 266.334 -28.958 4.1 359.949 +0.042 2.2 0.35 6.1 0.0 0.00 0.0 SLX 1744-299_300 266.849 -30.009 4.8 359.284 -0.888 1.6 0.30 5.2 0.0 0.00 0.0 SLX 1735-269 264.572 -27.009 4.8 0.784 +2.392 1.8 0.35 5.1 1.1 0.00 3.8 3A 1728-169 262.942 -16.968 4.8 8.511 +9.028 5.1 0.98 5.2 0.0 0.00 0.0 GRS 1734-292 264.412 -29.153 5.5 358.896 +1.365 1.6 0.35 4.5 0.0 0.00 0.0 NEW_1 283.871 -42.974 4.2 353.538 -18.803 18.0 3.04 6.0 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 17.3 1.23 4.4 0.84 GX 3+1 266.983 -26.564 2.294 +0.794 28.2 0.78 3.6 0.41 GX 5-1 270.284 -25.079 5.077 -1.019 81.2 2.45 9.0 1.12
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