INTEGRAL Galactic Bulge MonitoringRevolution 0838: Observation start 2009-08-23T23:24 = MJD 55066.976
Total Observation GTI = 12190 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 1700-377 255.983 -37.848 0.5 347.749 +2.173 58.3 0.78 74.8 15.1 0.62 24.4
GX 1+4 263.009 -24.740 0.6 1.942 +4.798 23.6 0.38 61.4 0.0 0.00 0.0
1E 1740.7-2942 265.974 -29.746 0.9 359.114 -0.103 10.5 0.31 34.3 7.0 0.27 26.3
GRS 1758-258 270.310 -25.732 1.0 4.522 -1.362 9.9 0.32 30.6 5.9 0.27 21.6
Ginga 1826-24 277.381 -23.792 1.3 9.283 -6.097 12.2 0.54 22.7 4.2 0.43 9.7
GX 5-1 270.291 -25.076 1.6 5.083 -1.022 6.1 0.34 18.2 0.0 0.00 0.0
H 1820-303 275.868 -30.345 2.0 2.782 -7.867 6.1 0.45 13.8 0.0 0.00 0.0
3A 1822-371 276.474 -37.135 2.1 356.833 -11.324 7.2 0.57 12.6 0.0 0.00 0.0
SLX 1744-299_300 266.844 -30.037 2.4 359.258 -0.898 3.5 0.31 11.4 1.1 0.27 3.9
4U 1722-30 261.880 -30.774 2.7 356.339 +2.320 3.6 0.38 9.6 0.0 0.00 0.0
GX 349+2 256.436 -36.384 2.9 349.135 +2.771 5.1 0.58 8.9 0.0 0.00 0.0
GX 9+1 270.398 -20.493 3.2 9.115 +1.161 4.0 0.49 8.1 0.0 0.00 0.0
IGR J18027-2016 270.702 -20.222 0.0 9.491 +1.046 2.5 0.00 5.0 0.0 0.00 0.0
SLX 1735-269 264.509 -26.937 4.8 0.815 +2.478 1.7 0.32 5.2 0.0 0.00 0.0
XB 1832-330 278.925 -33.051 4.5 1.473 -11.391 3.2 0.58 5.5 0.0 0.00 0.0
1A 1742-294 266.502 -29.481 0.0 359.579 -0.356 1.4 0.00 4.8 0.0 0.00 0.0
1E 1742.8-2853 266.480 -28.971 6.3 0.005 -0.074 1.2 0.32 3.9 0.0 0.00 0.0
IGR J18249-3243 276.206 -32.617 5.3 0.861 -9.145 2.0 0.43 4.6 0.0 0.00 0.0
IGR J17254-3257 261.324 -33.053 5.6 354.183 +1.439 1.8 0.41 4.4 0.0 0.00 0.0
XTE J1817-330 274.379 -33.117 5.6 359.708 -8.001 1.7 0.40 4.3 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
1A 1742-294 266.523 -29.515 359.559 -0.389 4.9 0.43 1.1 0.30
GX 3+1 266.983 -26.564 2.294 +0.794 25.8 0.65 3.2 0.35
GX 5-1 270.284 -25.079 5.077 -1.019 108.1 2.26 10.3 0.99
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Revolution 0838: Observation start 2009-08-23T23:24 = MJD 55066.976
Total Observation GTI = 12190 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 1700-377 255.983 -37.848 0.5 347.749 +2.173 58.3 0.78 74.8 15.1 0.62 24.4 GX 1+4 263.009 -24.740 0.6 1.942 +4.798 23.6 0.38 61.4 0.0 0.00 0.0 1E 1740.7-2942 265.974 -29.746 0.9 359.114 -0.103 10.5 0.31 34.3 7.0 0.27 26.3 GRS 1758-258 270.310 -25.732 1.0 4.522 -1.362 9.9 0.32 30.6 5.9 0.27 21.6 Ginga 1826-24 277.381 -23.792 1.3 9.283 -6.097 12.2 0.54 22.7 4.2 0.43 9.7 GX 5-1 270.291 -25.076 1.6 5.083 -1.022 6.1 0.34 18.2 0.0 0.00 0.0 H 1820-303 275.868 -30.345 2.0 2.782 -7.867 6.1 0.45 13.8 0.0 0.00 0.0 3A 1822-371 276.474 -37.135 2.1 356.833 -11.324 7.2 0.57 12.6 0.0 0.00 0.0 SLX 1744-299_300 266.844 -30.037 2.4 359.258 -0.898 3.5 0.31 11.4 1.1 0.27 3.9 4U 1722-30 261.880 -30.774 2.7 356.339 +2.320 3.6 0.38 9.6 0.0 0.00 0.0 GX 349+2 256.436 -36.384 2.9 349.135 +2.771 5.1 0.58 8.9 0.0 0.00 0.0 GX 9+1 270.398 -20.493 3.2 9.115 +1.161 4.0 0.49 8.1 0.0 0.00 0.0 IGR J18027-2016 270.702 -20.222 0.0 9.491 +1.046 2.5 0.00 5.0 0.0 0.00 0.0 SLX 1735-269 264.509 -26.937 4.8 0.815 +2.478 1.7 0.32 5.2 0.0 0.00 0.0 XB 1832-330 278.925 -33.051 4.5 1.473 -11.391 3.2 0.58 5.5 0.0 0.00 0.0 1A 1742-294 266.502 -29.481 0.0 359.579 -0.356 1.4 0.00 4.8 0.0 0.00 0.0 1E 1742.8-2853 266.480 -28.971 6.3 0.005 -0.074 1.2 0.32 3.9 0.0 0.00 0.0 IGR J18249-3243 276.206 -32.617 5.3 0.861 -9.145 2.0 0.43 4.6 0.0 0.00 0.0 IGR J17254-3257 261.324 -33.053 5.6 354.183 +1.439 1.8 0.41 4.4 0.0 0.00 0.0 XTE J1817-330 274.379 -33.117 5.6 359.708 -8.001 1.7 0.40 4.3 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 4.9 0.43 1.1 0.30 GX 3+1 266.983 -26.564 2.294 +0.794 25.8 0.65 3.2 0.35 GX 5-1 270.284 -25.079 5.077 -1.019 108.1 2.26 10.3 0.99
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