INTEGRAL Galactic Bulge MonitoringRevolution 0481: Observation start 2006-09-21 = MJD 53999
Total Observation GTI = 12359 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 1700-377 255.988 -37.842 0.4 347.757 +2.174 88.2 0.71 123.6 23.8 0.53 45.1
GX 354-0 262.990 -33.834 0.5 354.303 -0.150 28.8 0.38 75.5 9.2 0.30 30.4
GX 5-1 270.283 -25.079 0.6 5.077 -1.018 18.5 0.33 55.5 0.0 0.00 0.0
IGR J17497-2821 267.403 -28.349 0.7 0.955 -0.446 15.8 0.31 50.6 10.5 0.25 41.3
GX 1+4 263.010 -24.740 0.8 1.942 +4.798 15.8 0.36 44.6 0.0 0.00 0.0
Ginga 1826-24 277.371 -23.787 1.1 9.283 -6.086 15.8 0.55 28.7 6.3 0.42 15.0
GRS 1758-258 270.304 -25.749 1.2 4.504 -1.366 7.6 0.32 24.2 5.0 0.25 20.2
H 1820-303 275.919 -30.352 1.3 2.796 -7.909 9.8 0.44 22.2 0.0 0.00 0.0
1A 1742-294 266.518 -29.515 1.5 359.557 -0.385 5.7 0.29 19.7 1.8 0.24 7.6
1E 1740.7-2942 265.978 -29.750 1.4 359.112 -0.108 6.3 0.30 21.1 4.3 0.24 17.9
OAO 1657-415 255.218 -41.648 1.7 344.382 +0.316 23.5 1.47 16.0 8.5 1.06 8.0
GX 349+2 256.421 -36.423 2.1 349.096 +2.758 7.8 0.61 12.7 0.0 0.00 0.0
4U 1722-30 261.853 -30.805 2.5 356.300 +2.321 3.7 0.36 10.4 1.6 0.28 5.7
3A 1822-371 276.458 -37.133 3.2 356.829 -11.312 5.2 0.65 8.0 0.0 0.00 0.0
GX 3+1 266.975 -26.599 3.2 2.260 +0.782 2.5 0.31 8.1 0.0 0.00 0.0
GX 9+1 270.398 -20.561 3.8 9.055 +1.126 3.0 0.45 6.6 0.0 0.00 0.0
SLX 1744-299_300 266.888 -29.984 4.3 359.323 -0.903 1.9 0.33 5.8 0.0 0.00 0.0
IGR J17252-3616 261.315 -36.251 4.9 351.531 -0.348 2.3 0.45 5.0 1.5 0.00 4.3
GX 17+2 274.028 -14.042 4.4 16.438 +1.256 13.1 2.30 5.7 0.0 0.00 0.0
Swift J174535.5-2901 266.400 -29.090 0.0 359.867 -0.076 1.3 0.00 4.8 0.0 0.00 0.0
XB 1832-330 278.966 -32.914 4.5 1.614 -11.364 3.4 0.61 5.5 2.0 0.46 4.4
1E 1743.1-2843 266.588 -28.760 0.0 0.233 -0.045 1.2 0.00 4.3 0.0 0.00 0.0
NEW_0365 250.625 -34.423 5.0 347.687 +7.690 5.8 1.16 5.0 0.0 0.00 0.0
GX 13+1 273.629 -17.115 6.8 13.553 +0.129 3.1 0.87 3.5 0.0 0.00 0.0
IGR J17254-3257 261.389 -33.051 7.3 354.216 +1.396 1.2 0.37 3.3 0.0 0.00 0.0
SLX 1737-282 265.164 -28.314 5.9 359.957 +1.254 1.2 0.30 4.1 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 11.9 1.32 5.0 0.93
GX 3+1 266.983 -26.564 2.294 +0.794 25.7 0.56 4.1 0.31
GX 5-1 270.284 -25.079 5.077 -1.019 87.0 2.12 17.9 1.10
IGR J17497-2821 267.404 -28.358 0.949 -0.451 2.8 0.42 1.7 0.25
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.5 0.37 0.6 0.21
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Revolution 0481: Observation start 2006-09-21 = MJD 53999
Total Observation GTI = 12359 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 1700-377 255.988 -37.842 0.4 347.757 +2.174 88.2 0.71 123.6 23.8 0.53 45.1 GX 354-0 262.990 -33.834 0.5 354.303 -0.150 28.8 0.38 75.5 9.2 0.30 30.4 GX 5-1 270.283 -25.079 0.6 5.077 -1.018 18.5 0.33 55.5 0.0 0.00 0.0 IGR J17497-2821 267.403 -28.349 0.7 0.955 -0.446 15.8 0.31 50.6 10.5 0.25 41.3 GX 1+4 263.010 -24.740 0.8 1.942 +4.798 15.8 0.36 44.6 0.0 0.00 0.0 Ginga 1826-24 277.371 -23.787 1.1 9.283 -6.086 15.8 0.55 28.7 6.3 0.42 15.0 GRS 1758-258 270.304 -25.749 1.2 4.504 -1.366 7.6 0.32 24.2 5.0 0.25 20.2 H 1820-303 275.919 -30.352 1.3 2.796 -7.909 9.8 0.44 22.2 0.0 0.00 0.0 1A 1742-294 266.518 -29.515 1.5 359.557 -0.385 5.7 0.29 19.7 1.8 0.24 7.6 1E 1740.7-2942 265.978 -29.750 1.4 359.112 -0.108 6.3 0.30 21.1 4.3 0.24 17.9 OAO 1657-415 255.218 -41.648 1.7 344.382 +0.316 23.5 1.47 16.0 8.5 1.06 8.0 GX 349+2 256.421 -36.423 2.1 349.096 +2.758 7.8 0.61 12.7 0.0 0.00 0.0 4U 1722-30 261.853 -30.805 2.5 356.300 +2.321 3.7 0.36 10.4 1.6 0.28 5.7 3A 1822-371 276.458 -37.133 3.2 356.829 -11.312 5.2 0.65 8.0 0.0 0.00 0.0 GX 3+1 266.975 -26.599 3.2 2.260 +0.782 2.5 0.31 8.1 0.0 0.00 0.0 GX 9+1 270.398 -20.561 3.8 9.055 +1.126 3.0 0.45 6.6 0.0 0.00 0.0 SLX 1744-299_300 266.888 -29.984 4.3 359.323 -0.903 1.9 0.33 5.8 0.0 0.00 0.0 IGR J17252-3616 261.315 -36.251 4.9 351.531 -0.348 2.3 0.45 5.0 1.5 0.00 4.3 GX 17+2 274.028 -14.042 4.4 16.438 +1.256 13.1 2.30 5.7 0.0 0.00 0.0 Swift J174535.5-2901 266.400 -29.090 0.0 359.867 -0.076 1.3 0.00 4.8 0.0 0.00 0.0 XB 1832-330 278.966 -32.914 4.5 1.614 -11.364 3.4 0.61 5.5 2.0 0.46 4.4 1E 1743.1-2843 266.588 -28.760 0.0 0.233 -0.045 1.2 0.00 4.3 0.0 0.00 0.0 NEW_0365 250.625 -34.423 5.0 347.687 +7.690 5.8 1.16 5.0 0.0 0.00 0.0 GX 13+1 273.629 -17.115 6.8 13.553 +0.129 3.1 0.87 3.5 0.0 0.00 0.0 IGR J17254-3257 261.389 -33.051 7.3 354.216 +1.396 1.2 0.37 3.3 0.0 0.00 0.0 SLX 1737-282 265.164 -28.314 5.9 359.957 +1.254 1.2 0.30 4.1 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 11.9 1.32 5.0 0.93 GX 3+1 266.983 -26.564 2.294 +0.794 25.7 0.56 4.1 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 87.0 2.12 17.9 1.10 IGR J17497-2821 267.404 -28.358 0.949 -0.451 2.8 0.42 1.7 0.25 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.5 0.37 0.6 0.21
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