INTEGRAL Galactic Bulge MonitoringRevolution 0535: Observation start 2007-03-02 = MJD 54161
Total Observation GTI = 12387 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+4 263.008 -24.744 0.6 1.938 +4.797 22.2 0.32 68.5 0.0 0.00 0.0
GX 5-1 270.282 -25.085 0.8 5.071 -1.020 12.2 0.31 39.3 0.0 0.00 0.0
1E 1740.7-2942 265.984 -29.747 0.8 359.117 -0.111 11.2 0.28 40.4 7.5 0.24 31.6
GRS 1758-258 270.299 -25.747 0.8 4.504 -1.361 12.0 0.30 39.3 8.8 0.25 35.3
Ginga 1826-24 277.367 -23.805 1.0 9.265 -6.091 17.4 0.53 32.7 6.8 0.42 16.1
GX 354-0 262.998 -33.838 1.0 354.303 -0.158 10.6 0.34 31.5 2.5 0.28 9.2
H 1820-303 275.919 -30.374 1.6 2.777 -7.920 7.5 0.43 17.5 0.0 0.00 0.0
GX 349+2 256.427 -36.423 1.8 349.100 +2.754 8.5 0.56 15.1 0.0 0.00 0.0
GX 3+1 266.994 -26.575 1.7 2.289 +0.780 4.6 0.28 16.5 0.0 0.00 0.0
4U 1722-30 261.898 -30.819 2.3 356.310 +2.281 3.6 0.31 11.7 1.5 0.00 6.0
3A 1822-371 276.438 -37.108 2.3 356.845 -11.287 7.1 0.60 11.8 0.0 0.00 0.0
GX 9+1 270.377 -20.524 2.5 9.078 +1.162 4.3 0.41 10.5 0.0 0.00 0.0
GRS 1741.9-2853 266.324 -28.942 2.7 359.958 +0.058 2.6 0.27 9.6 1.6 0.23 6.7
1A 1742-294 266.494 -29.492 0.0 359.566 -0.356 2.6 0.00 9.2 0.0 0.00 0.0
OAO 1657-415 255.190 -41.671 2.9 344.351 +0.318 16.5 1.82 9.1 0.0 0.00 0.0
SLX 1735-269 264.639 -26.976 3.8 0.843 +2.359 1.9 0.28 6.7 1.4 0.24 5.9
SLX 1744-299_300 266.837 -30.012 3.2 359.276 -0.880 2.3 0.28 8.2 0.0 0.00 0.0
IGR J17391-3021 264.792 -30.329 3.9 358.077 +0.458 2.0 0.30 6.5 0.0 0.00 0.0
SLX 1737-282 265.175 -28.302 4.2 359.973 +1.252 1.7 0.28 6.0 0.0 0.00 0.0
GRS 1734-292 264.313 -29.139 4.6 358.861 +1.445 1.5 0.29 5.4 0.0 0.00 0.0
3A 1728-169 262.904 -16.968 5.3 8.491 +9.059 2.9 0.63 4.6 0.0 0.00 0.0
GX 17+2 273.996 -13.990 5.8 16.468 +1.308 8.1 1.92 4.2 0.0 0.00 0.0
4U 1700-377 255.992 -37.854 5.4 347.749 +2.164 3.0 0.66 4.6 0.0 0.00 0.0
IGR J18193-2542 274.910 -25.683 7.4 6.558 -4.974 1.3 0.41 3.2 0.0 0.00 0.0
4U 1735-444 264.704 -44.521 5.1 345.979 -7.007 26.1 5.42 4.8 0.0 0.00 0.0
1E 1743.1-2843 266.681 -28.669 0.0 0.354 -0.068 1.1 0.00 4.0 0.0 0.00 0.0
NEW_1 269.953 -13.650 4.3 14.864 +4.909 8.7 1.51 5.8 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 3+1 266.983 -26.564 2.294 +0.794 34.5 0.54 4.5 0.27
GX 5-1 270.284 -25.079 5.077 -1.019 97.8 1.77 13.1 0.79
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Revolution 0535: Observation start 2007-03-02 = MJD 54161
Total Observation GTI = 12387 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+4 263.008 -24.744 0.6 1.938 +4.797 22.2 0.32 68.5 0.0 0.00 0.0 GX 5-1 270.282 -25.085 0.8 5.071 -1.020 12.2 0.31 39.3 0.0 0.00 0.0 1E 1740.7-2942 265.984 -29.747 0.8 359.117 -0.111 11.2 0.28 40.4 7.5 0.24 31.6 GRS 1758-258 270.299 -25.747 0.8 4.504 -1.361 12.0 0.30 39.3 8.8 0.25 35.3 Ginga 1826-24 277.367 -23.805 1.0 9.265 -6.091 17.4 0.53 32.7 6.8 0.42 16.1 GX 354-0 262.998 -33.838 1.0 354.303 -0.158 10.6 0.34 31.5 2.5 0.28 9.2 H 1820-303 275.919 -30.374 1.6 2.777 -7.920 7.5 0.43 17.5 0.0 0.00 0.0 GX 349+2 256.427 -36.423 1.8 349.100 +2.754 8.5 0.56 15.1 0.0 0.00 0.0 GX 3+1 266.994 -26.575 1.7 2.289 +0.780 4.6 0.28 16.5 0.0 0.00 0.0 4U 1722-30 261.898 -30.819 2.3 356.310 +2.281 3.6 0.31 11.7 1.5 0.00 6.0 3A 1822-371 276.438 -37.108 2.3 356.845 -11.287 7.1 0.60 11.8 0.0 0.00 0.0 GX 9+1 270.377 -20.524 2.5 9.078 +1.162 4.3 0.41 10.5 0.0 0.00 0.0 GRS 1741.9-2853 266.324 -28.942 2.7 359.958 +0.058 2.6 0.27 9.6 1.6 0.23 6.7 1A 1742-294 266.494 -29.492 0.0 359.566 -0.356 2.6 0.00 9.2 0.0 0.00 0.0 OAO 1657-415 255.190 -41.671 2.9 344.351 +0.318 16.5 1.82 9.1 0.0 0.00 0.0 SLX 1735-269 264.639 -26.976 3.8 0.843 +2.359 1.9 0.28 6.7 1.4 0.24 5.9 SLX 1744-299_300 266.837 -30.012 3.2 359.276 -0.880 2.3 0.28 8.2 0.0 0.00 0.0 IGR J17391-3021 264.792 -30.329 3.9 358.077 +0.458 2.0 0.30 6.5 0.0 0.00 0.0 SLX 1737-282 265.175 -28.302 4.2 359.973 +1.252 1.7 0.28 6.0 0.0 0.00 0.0 GRS 1734-292 264.313 -29.139 4.6 358.861 +1.445 1.5 0.29 5.4 0.0 0.00 0.0 3A 1728-169 262.904 -16.968 5.3 8.491 +9.059 2.9 0.63 4.6 0.0 0.00 0.0 GX 17+2 273.996 -13.990 5.8 16.468 +1.308 8.1 1.92 4.2 0.0 0.00 0.0 4U 1700-377 255.992 -37.854 5.4 347.749 +2.164 3.0 0.66 4.6 0.0 0.00 0.0 IGR J18193-2542 274.910 -25.683 7.4 6.558 -4.974 1.3 0.41 3.2 0.0 0.00 0.0 4U 1735-444 264.704 -44.521 5.1 345.979 -7.007 26.1 5.42 4.8 0.0 0.00 0.0 1E 1743.1-2843 266.681 -28.669 0.0 0.354 -0.068 1.1 0.00 4.0 0.0 0.00 0.0 NEW_1 269.953 -13.650 4.3 14.864 +4.909 8.7 1.51 5.8 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 3+1 266.983 -26.564 2.294 +0.794 34.5 0.54 4.5 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 97.8 1.77 13.1 0.79
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