INTEGRAL Galactic Bulge MonitoringRevolution 0551: Observation start 2007-04-18 = MJD 54208
Total Observation GTI = 11795 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 5-1 270.293 -25.081 0.7 5.079 -1.026 17.8 0.34 52.1 0.0 0.00 0.0
GX 1+4 263.005 -24.742 0.7 1.938 +4.800 15.7 0.34 46.1 0.0 0.00 0.0
GRS 1758-258 270.301 -25.742 0.9 4.508 -1.360 12.5 0.36 34.4 8.3 0.29 28.3
Ginga 1826-24 277.372 -23.790 1.1 9.281 -6.088 16.8 0.59 28.7 7.4 0.46 16.1
1E 1740.7-2942 265.982 -29.743 1.2 359.119 -0.107 7.6 0.31 24.5 3.8 0.25 15.1
H 1820-303 275.907 -30.371 1.8 2.775 -7.909 6.7 0.43 15.6 0.0 0.00 0.0
GX 3+1 266.987 -26.523 2.1 2.331 +0.812 3.9 0.30 13.0 0.0 0.00 0.0
1A 1742-294 266.498 -29.531 2.2 359.534 -0.379 4.2 0.34 12.2 0.0 0.00 0.0
GX 354-0 262.995 -33.824 2.2 354.314 -0.148 4.4 0.37 12.1 0.0 0.00 0.0
GX 349+2 256.386 -36.407 2.5 349.093 +2.790 7.3 0.70 10.5 0.0 0.00 0.0
3A 1822-371 276.409 -37.089 2.4 356.853 -11.258 7.1 0.63 11.4 0.0 0.00 0.0
4U 1722-30 261.941 -30.786 2.6 356.358 +2.269 3.9 0.38 10.3 1.8 0.30 6.1
OAO 1657-415 255.147 -41.658 2.8 344.341 +0.352 16.9 1.79 9.5 4.8 0.00 3.5
SLX 1744-299_300 266.810 -30.040 3.1 359.240 -0.875 2.6 0.31 8.4 0.0 0.00 0.0
SLX 1735-269 264.561 -26.989 4.2 0.796 +2.410 2.1 0.34 6.0 1.0 0.00 3.6
IGR J17456-2901 266.360 -28.967 3.8 359.954 +0.018 2.2 0.33 6.7 0.0 0.00 0.0
GX 9+1 270.391 -20.515 3.8 9.092 +1.156 3.0 0.00 6.7 0.0 0.00 0.0
GX 17+2 274.003 -14.059 3.7 16.411 +1.269 13.7 2.01 6.8 0.0 0.00 0.0
4U 1700-377 256.080 -37.805 4.7 347.831 +2.139 3.9 0.74 5.3 2.2 0.56 3.9
IGR J18027-2016 270.732 -20.347 0.0 9.395 +0.960 2.4 0.00 5.1 0.0 0.00 0.0
SGR 1806-20 272.145 -20.414 5.3 9.985 -0.228 2.3 0.50 4.6 0.0 0.00 0.0
XB 1832-330 278.885 -33.017 5.0 1.490 -11.346 3.0 0.61 5.0 2.2 0.46 4.6
4U 1735-444 264.795 -44.402 5.8 346.115 -7.001 13.7 3.29 4.2 0.0 0.00 0.0
3A 1728-169 262.936 -16.916 5.1 8.553 +9.060 3.4 0.70 4.8 0.0 0.00 0.0
IGR J17407-2808 265.176 -28.185 5.4 0.071 +1.313 1.6 0.35 4.5 0.0 0.00 0.0
IGR J17252-3616 261.259 -36.291 6.5 351.473 -0.333 1.7 0.45 3.7 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
1A 1742-294 266.523 -29.515 359.559 -0.389 2.0 0.39 0.6 0.23
GX 3+1 266.983 -26.564 2.294 +0.794 23.8 0.56 3.2 0.29
GX 5-1 270.284 -25.079 5.077 -1.019 77.7 1.55 13.5 0.73
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Revolution 0551: Observation start 2007-04-18 = MJD 54208
Total Observation GTI = 11795 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 5-1 270.293 -25.081 0.7 5.079 -1.026 17.8 0.34 52.1 0.0 0.00 0.0 GX 1+4 263.005 -24.742 0.7 1.938 +4.800 15.7 0.34 46.1 0.0 0.00 0.0 GRS 1758-258 270.301 -25.742 0.9 4.508 -1.360 12.5 0.36 34.4 8.3 0.29 28.3 Ginga 1826-24 277.372 -23.790 1.1 9.281 -6.088 16.8 0.59 28.7 7.4 0.46 16.1 1E 1740.7-2942 265.982 -29.743 1.2 359.119 -0.107 7.6 0.31 24.5 3.8 0.25 15.1 H 1820-303 275.907 -30.371 1.8 2.775 -7.909 6.7 0.43 15.6 0.0 0.00 0.0 GX 3+1 266.987 -26.523 2.1 2.331 +0.812 3.9 0.30 13.0 0.0 0.00 0.0 1A 1742-294 266.498 -29.531 2.2 359.534 -0.379 4.2 0.34 12.2 0.0 0.00 0.0 GX 354-0 262.995 -33.824 2.2 354.314 -0.148 4.4 0.37 12.1 0.0 0.00 0.0 GX 349+2 256.386 -36.407 2.5 349.093 +2.790 7.3 0.70 10.5 0.0 0.00 0.0 3A 1822-371 276.409 -37.089 2.4 356.853 -11.258 7.1 0.63 11.4 0.0 0.00 0.0 4U 1722-30 261.941 -30.786 2.6 356.358 +2.269 3.9 0.38 10.3 1.8 0.30 6.1 OAO 1657-415 255.147 -41.658 2.8 344.341 +0.352 16.9 1.79 9.5 4.8 0.00 3.5 SLX 1744-299_300 266.810 -30.040 3.1 359.240 -0.875 2.6 0.31 8.4 0.0 0.00 0.0 SLX 1735-269 264.561 -26.989 4.2 0.796 +2.410 2.1 0.34 6.0 1.0 0.00 3.6 IGR J17456-2901 266.360 -28.967 3.8 359.954 +0.018 2.2 0.33 6.7 0.0 0.00 0.0 GX 9+1 270.391 -20.515 3.8 9.092 +1.156 3.0 0.00 6.7 0.0 0.00 0.0 GX 17+2 274.003 -14.059 3.7 16.411 +1.269 13.7 2.01 6.8 0.0 0.00 0.0 4U 1700-377 256.080 -37.805 4.7 347.831 +2.139 3.9 0.74 5.3 2.2 0.56 3.9 IGR J18027-2016 270.732 -20.347 0.0 9.395 +0.960 2.4 0.00 5.1 0.0 0.00 0.0 SGR 1806-20 272.145 -20.414 5.3 9.985 -0.228 2.3 0.50 4.6 0.0 0.00 0.0 XB 1832-330 278.885 -33.017 5.0 1.490 -11.346 3.0 0.61 5.0 2.2 0.46 4.6 4U 1735-444 264.795 -44.402 5.8 346.115 -7.001 13.7 3.29 4.2 0.0 0.00 0.0 3A 1728-169 262.936 -16.916 5.1 8.553 +9.060 3.4 0.70 4.8 0.0 0.00 0.0 IGR J17407-2808 265.176 -28.185 5.4 0.071 +1.313 1.6 0.35 4.5 0.0 0.00 0.0 IGR J17252-3616 261.259 -36.291 6.5 351.473 -0.333 1.7 0.45 3.7 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 2.0 0.39 0.6 0.23 GX 3+1 266.983 -26.564 2.294 +0.794 23.8 0.56 3.2 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 77.7 1.55 13.5 0.73
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