INTEGRAL Galactic Bulge MonitoringRevolution 0718: Observation start 2008-08-30T00:29 = MJD 54708.021
Total Observation GTI = 12489 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 -37.843 0.5 347.756 +2.173 53.6 0.72 74.3 14.3 0.56 25.6
IGR J17473-2721 266.828 -27.339 0.7 1.558 +0.511 13.7 0.30 45.5 6.0 0.26 22.9
GX 354-0 262.993 -33.830 0.7 354.308 -0.150 17.5 0.36 48.6 4.4 0.29 15.1
Ginga 1826-24 277.379 -23.788 1.0 9.285 -6.093 17.7 0.57 30.8 6.3 0.44 14.3
GRS 1758-258 270.293 -25.752 1.1 4.497 -1.359 10.4 0.37 28.1 7.5 0.31 24.5
GX 5-1 270.282 -25.083 1.1 5.073 -1.019 10.1 0.38 26.8 0.0 0.00 0.0
1E 1740.7-2942 265.967 -29.746 1.3 359.110 -0.098 6.9 0.30 23.3 5.2 0.25 20.7
GX 349+2 256.416 -36.423 1.3 349.094 +2.761 13.1 0.58 22.5 0.0 0.00 0.0
OAO 1657-415 255.209 -41.661 1.5 344.367 +0.313 25.1 1.29 19.6 4.3 0.00 4.4
GX 1+4 262.992 -24.736 1.4 1.937 +4.813 8.0 0.40 20.0 0.0 0.00 0.0
4U 1722-30 261.882 -30.803 2.0 356.316 +2.302 4.7 0.34 13.5 2.5 0.28 8.8
IGR J17544-2619 268.594 -26.336 2.0 3.227 -0.329 4.3 0.31 13.8 0.0 0.00 0.0
H 1820-303 275.975 -30.375 2.7 2.798 -7.963 4.6 0.47 9.8 0.0 0.00 0.0
GX 3+1 266.990 -26.555 2.2 2.305 +0.793 3.7 0.31 12.1 0.0 0.00 0.0
3A 1822-371 276.424 -37.105 2.9 356.843 -11.276 5.8 0.65 8.9 0.0 0.00 0.0
GX 9+1 270.398 -20.512 3.0 9.098 +1.151 3.9 0.46 8.6 0.0 0.00 0.0
SLX 1735-269 264.595 -27.014 3.8 0.791 +2.372 2.2 0.33 6.6 0.0 0.00 0.0
1A 1742-294 266.480 -29.487 4.0 359.564 -0.343 1.8 0.29 6.3 0.0 0.00 0.0
GX 17+2 274.025 -13.989 3.6 16.482 +1.284 17.7 2.47 7.2 0.0 0.00 0.0
H 1702-429 256.617 -43.034 4.1 343.912 -1.348 10.8 1.75 6.2 0.0 0.00 0.0
IGR J17252-3616 261.326 -36.248 4.3 351.539 -0.353 2.6 0.44 5.8 1.5 0.36 4.1
GRS 1734-292 264.388 -29.101 4.2 358.928 +1.411 1.8 0.30 6.0 0.0 0.00 0.0
SLX 1744-299_300 266.835 -30.006 5.3 359.280 -0.875 1.3 0.29 4.6 0.0 0.00 0.0
IGR J17254-3257 261.359 -32.936 6.8 354.297 +1.481 1.3 0.37 3.6 0.0 0.00 0.0
IGR J18027-2016 270.724 -20.210 0.0 9.511 +1.035 1.8 0.00 3.7 0.0 0.00 0.0
1E 1743.1-2843 266.678 -28.753 0.0 0.281 -0.109 1.1 0.00 3.6 0.0 0.00 0.0
GX 13+1 273.618 -17.139 5.7 13.526 +0.126 3.7 0.85 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
GX 354-0 262.989 -33.835 354.302 -0.150 9.5 1.38 3.6 1.02
1A 1742-294 266.523 -29.515 359.559 -0.389 2.6 0.37 0.8 0.28
IGR J17473-2721 266.825 -27.344 1.553 +0.510 3.7 0.46 1.8 0.29
GX 3+1 266.983 -26.564 2.294 +0.794 41.2 0.68 5.8 0.36
GX 5-1 270.284 -25.079 5.077 -1.019 122.2 2.47 15.8 1.14
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Revolution 0718: Observation start 2008-08-30T00:29 = MJD 54708.021
Total Observation GTI = 12489 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 -37.843 0.5 347.756 +2.173 53.6 0.72 74.3 14.3 0.56 25.6 IGR J17473-2721 266.828 -27.339 0.7 1.558 +0.511 13.7 0.30 45.5 6.0 0.26 22.9 GX 354-0 262.993 -33.830 0.7 354.308 -0.150 17.5 0.36 48.6 4.4 0.29 15.1 Ginga 1826-24 277.379 -23.788 1.0 9.285 -6.093 17.7 0.57 30.8 6.3 0.44 14.3 GRS 1758-258 270.293 -25.752 1.1 4.497 -1.359 10.4 0.37 28.1 7.5 0.31 24.5 GX 5-1 270.282 -25.083 1.1 5.073 -1.019 10.1 0.38 26.8 0.0 0.00 0.0 1E 1740.7-2942 265.967 -29.746 1.3 359.110 -0.098 6.9 0.30 23.3 5.2 0.25 20.7 GX 349+2 256.416 -36.423 1.3 349.094 +2.761 13.1 0.58 22.5 0.0 0.00 0.0 OAO 1657-415 255.209 -41.661 1.5 344.367 +0.313 25.1 1.29 19.6 4.3 0.00 4.4 GX 1+4 262.992 -24.736 1.4 1.937 +4.813 8.0 0.40 20.0 0.0 0.00 0.0 4U 1722-30 261.882 -30.803 2.0 356.316 +2.302 4.7 0.34 13.5 2.5 0.28 8.8 IGR J17544-2619 268.594 -26.336 2.0 3.227 -0.329 4.3 0.31 13.8 0.0 0.00 0.0 H 1820-303 275.975 -30.375 2.7 2.798 -7.963 4.6 0.47 9.8 0.0 0.00 0.0 GX 3+1 266.990 -26.555 2.2 2.305 +0.793 3.7 0.31 12.1 0.0 0.00 0.0 3A 1822-371 276.424 -37.105 2.9 356.843 -11.276 5.8 0.65 8.9 0.0 0.00 0.0 GX 9+1 270.398 -20.512 3.0 9.098 +1.151 3.9 0.46 8.6 0.0 0.00 0.0 SLX 1735-269 264.595 -27.014 3.8 0.791 +2.372 2.2 0.33 6.6 0.0 0.00 0.0 1A 1742-294 266.480 -29.487 4.0 359.564 -0.343 1.8 0.29 6.3 0.0 0.00 0.0 GX 17+2 274.025 -13.989 3.6 16.482 +1.284 17.7 2.47 7.2 0.0 0.00 0.0 H 1702-429 256.617 -43.034 4.1 343.912 -1.348 10.8 1.75 6.2 0.0 0.00 0.0 IGR J17252-3616 261.326 -36.248 4.3 351.539 -0.353 2.6 0.44 5.8 1.5 0.36 4.1 GRS 1734-292 264.388 -29.101 4.2 358.928 +1.411 1.8 0.30 6.0 0.0 0.00 0.0 SLX 1744-299_300 266.835 -30.006 5.3 359.280 -0.875 1.3 0.29 4.6 0.0 0.00 0.0 IGR J17254-3257 261.359 -32.936 6.8 354.297 +1.481 1.3 0.37 3.6 0.0 0.00 0.0 IGR J18027-2016 270.724 -20.210 0.0 9.511 +1.035 1.8 0.00 3.7 0.0 0.00 0.0 1E 1743.1-2843 266.678 -28.753 0.0 0.281 -0.109 1.1 0.00 3.6 0.0 0.00 0.0 GX 13+1 273.618 -17.139 5.7 13.526 +0.126 3.7 0.85 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 9.5 1.38 3.6 1.02 1A 1742-294 266.523 -29.515 359.559 -0.389 2.6 0.37 0.8 0.28 IGR J17473-2721 266.825 -27.344 1.553 +0.510 3.7 0.46 1.8 0.29 GX 3+1 266.983 -26.564 2.294 +0.794 41.2 0.68 5.8 0.36 GX 5-1 270.284 -25.079 5.077 -1.019 122.2 2.47 15.8 1.14
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