INTEGRAL Galactic Bulge MonitoringRevolution 0715: Observation start 2008-08-21T01:08 = MJD 54699.048
Total Observation GTI = 12574 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 -37.849 0.5 347.749 +2.173 56.6 0.70 81.3 15.8 0.55 28.9
GX 354-0 262.987 -33.836 0.7 354.300 -0.149 17.1 0.33 51.3 5.1 0.28 18.4
IGR J17473-2721 266.830 -27.342 0.8 1.557 +0.508 13.2 0.31 42.2 5.9 0.27 21.4
GRS 1758-258 270.306 -25.752 1.0 4.502 -1.369 10.4 0.34 30.4 6.7 0.29 23.4
Ginga 1826-24 277.385 -23.802 1.1 9.275 -6.104 16.8 0.60 28.0 7.4 0.48 15.4
GX 1+4 263.000 -24.753 1.2 1.926 +4.798 8.7 0.35 24.7 0.0 0.00 0.0
1E 1740.7-2942 265.968 -29.737 1.4 359.118 -0.094 5.9 0.29 20.0 4.4 0.26 17.2
H 1820-303 275.921 -30.365 1.4 2.786 -7.917 9.0 0.45 20.2 0.0 0.00 0.0
4U 1722-30 261.890 -30.800 1.7 356.323 +2.298 6.0 0.36 16.7 1.7 0.30 5.6
GX 349+2 256.421 -36.427 1.8 349.093 +2.755 8.9 0.59 15.1 0.0 0.00 0.0
OAO 1657-415 255.212 -41.661 1.8 344.369 +0.311 23.6 1.52 15.5 4.7 1.18 4.0
1A 1742-294 266.494 -29.493 2.4 359.565 -0.356 3.3 0.00 11.4 0.0 0.00 0.0
3A 1822-371 276.445 -37.125 2.3 356.832 -11.299 6.5 0.57 11.5 0.0 0.00 0.0
GX 5-1 270.269 -25.097 3.0 5.055 -1.016 2.8 0.33 8.5 0.0 0.00 0.0
GX 3+1 267.002 -26.580 2.4 2.288 +0.771 3.4 0.31 11.0 0.0 0.00 0.0
H 1702-429 256.544 -43.033 4.1 343.880 -1.305 11.3 1.86 6.1 6.4 1.39 4.6
GX 17+2 274.028 -14.019 3.7 16.457 +1.267 16.1 2.34 6.9 0.0 0.00 0.0
GX 9+1 270.386 -20.480 4.4 9.120 +1.177 2.5 0.44 5.8 0.0 0.00 0.0
IGR J18027-2016 270.729 -20.290 0.0 9.444 +0.991 2.6 0.00 5.5 0.0 0.00 0.0
GRO J1655-40 253.454 -39.785 4.3 345.006 +2.522 6.5 1.11 5.8 0.0 0.00 0.0
SAX J1712.6-3739 258.199 -37.638 4.6 348.966 +0.894 3.1 0.56 5.4 0.0 0.00 0.0
IGR J17252-3616 261.264 -36.288 4.3 351.477 -0.335 2.7 0.46 5.8 0.0 0.00 0.0
SLX 1735-269 264.602 -26.913 5.8 0.879 +2.421 1.4 0.32 4.2 1.1 0.00 4.1
SLX 1744-299_300 266.840 -30.032 4.8 359.260 -0.893 1.6 0.30 5.2 0.0 0.00 0.0
GX 13+1 273.703 -17.183 5.5 13.527 +0.035 3.6 0.00 4.5 0.0 0.00 0.0
IGR J17354-3255 263.866 -32.906 5.3 355.480 -0.260 1.5 0.32 4.6 0.0 0.00 0.0
1E 1742.9-2849 266.562 -28.809 6.0 0.180 -0.051 1.2 0.30 4.1 0.0 0.00 0.0
Oph Cluster 258.063 -23.281 5.6 0.619 +9.361 2.1 0.00 4.4 0.0 0.00 0.0
KS 1741-293 266.116 -29.328 0.0 359.534 +0.011 1.2 0.00 4.2 1.1 0.26 4.1
XB 1832-330 278.968 -32.984 5.4 1.550 -11.395 2.8 0.62 4.5 0.0 0.00 0.0
4U 1705-32 257.212 -32.196 5.9 352.883 +4.762 1.8 0.43 4.1 0.0 0.00 0.0
1H 1746-370 267.587 -37.063 6.1 353.535 -5.034 1.9 0.47 4.0 0.0 0.00 0.0
IGR J17475-2822 266.867 -28.505 6.4 0.579 -0.122 1.1 0.30 3.8 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 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 6.8 1.26 2.2 1.19
IGR J17473-2721 266.825 -27.344 1.553 +0.510 3.4 0.49 1.8 0.29
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 4.0 0.43 0.9 0.25
GX 3+1 266.983 -26.564 2.294 +0.794 49.7 0.72 7.0 0.37
GX 5-1 270.284 -25.079 5.077 -1.019 79.6 2.31 6.2 0.97
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Revolution 0715: Observation start 2008-08-21T01:08 = MJD 54699.048
Total Observation GTI = 12574 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 -37.849 0.5 347.749 +2.173 56.6 0.70 81.3 15.8 0.55 28.9 GX 354-0 262.987 -33.836 0.7 354.300 -0.149 17.1 0.33 51.3 5.1 0.28 18.4 IGR J17473-2721 266.830 -27.342 0.8 1.557 +0.508 13.2 0.31 42.2 5.9 0.27 21.4 GRS 1758-258 270.306 -25.752 1.0 4.502 -1.369 10.4 0.34 30.4 6.7 0.29 23.4 Ginga 1826-24 277.385 -23.802 1.1 9.275 -6.104 16.8 0.60 28.0 7.4 0.48 15.4 GX 1+4 263.000 -24.753 1.2 1.926 +4.798 8.7 0.35 24.7 0.0 0.00 0.0 1E 1740.7-2942 265.968 -29.737 1.4 359.118 -0.094 5.9 0.29 20.0 4.4 0.26 17.2 H 1820-303 275.921 -30.365 1.4 2.786 -7.917 9.0 0.45 20.2 0.0 0.00 0.0 4U 1722-30 261.890 -30.800 1.7 356.323 +2.298 6.0 0.36 16.7 1.7 0.30 5.6 GX 349+2 256.421 -36.427 1.8 349.093 +2.755 8.9 0.59 15.1 0.0 0.00 0.0 OAO 1657-415 255.212 -41.661 1.8 344.369 +0.311 23.6 1.52 15.5 4.7 1.18 4.0 1A 1742-294 266.494 -29.493 2.4 359.565 -0.356 3.3 0.00 11.4 0.0 0.00 0.0 3A 1822-371 276.445 -37.125 2.3 356.832 -11.299 6.5 0.57 11.5 0.0 0.00 0.0 GX 5-1 270.269 -25.097 3.0 5.055 -1.016 2.8 0.33 8.5 0.0 0.00 0.0 GX 3+1 267.002 -26.580 2.4 2.288 +0.771 3.4 0.31 11.0 0.0 0.00 0.0 H 1702-429 256.544 -43.033 4.1 343.880 -1.305 11.3 1.86 6.1 6.4 1.39 4.6 GX 17+2 274.028 -14.019 3.7 16.457 +1.267 16.1 2.34 6.9 0.0 0.00 0.0 GX 9+1 270.386 -20.480 4.4 9.120 +1.177 2.5 0.44 5.8 0.0 0.00 0.0 IGR J18027-2016 270.729 -20.290 0.0 9.444 +0.991 2.6 0.00 5.5 0.0 0.00 0.0 GRO J1655-40 253.454 -39.785 4.3 345.006 +2.522 6.5 1.11 5.8 0.0 0.00 0.0 SAX J1712.6-3739 258.199 -37.638 4.6 348.966 +0.894 3.1 0.56 5.4 0.0 0.00 0.0 IGR J17252-3616 261.264 -36.288 4.3 351.477 -0.335 2.7 0.46 5.8 0.0 0.00 0.0 SLX 1735-269 264.602 -26.913 5.8 0.879 +2.421 1.4 0.32 4.2 1.1 0.00 4.1 SLX 1744-299_300 266.840 -30.032 4.8 359.260 -0.893 1.6 0.30 5.2 0.0 0.00 0.0 GX 13+1 273.703 -17.183 5.5 13.527 +0.035 3.6 0.00 4.5 0.0 0.00 0.0 IGR J17354-3255 263.866 -32.906 5.3 355.480 -0.260 1.5 0.32 4.6 0.0 0.00 0.0 1E 1742.9-2849 266.562 -28.809 6.0 0.180 -0.051 1.2 0.30 4.1 0.0 0.00 0.0 Oph Cluster 258.063 -23.281 5.6 0.619 +9.361 2.1 0.00 4.4 0.0 0.00 0.0 KS 1741-293 266.116 -29.328 0.0 359.534 +0.011 1.2 0.00 4.2 1.1 0.26 4.1 XB 1832-330 278.968 -32.984 5.4 1.550 -11.395 2.8 0.62 4.5 0.0 0.00 0.0 4U 1705-32 257.212 -32.196 5.9 352.883 +4.762 1.8 0.43 4.1 0.0 0.00 0.0 1H 1746-370 267.587 -37.063 6.1 353.535 -5.034 1.9 0.47 4.0 0.0 0.00 0.0 IGR J17475-2822 266.867 -28.505 6.4 0.579 -0.122 1.1 0.30 3.8 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 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 6.8 1.26 2.2 1.19 IGR J17473-2721 266.825 -27.344 1.553 +0.510 3.4 0.49 1.8 0.29 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 4.0 0.43 0.9 0.25 GX 3+1 266.983 -26.564 2.294 +0.794 49.7 0.72 7.0 0.37 GX 5-1 270.284 -25.079 5.077 -1.019 79.6 2.31 6.2 0.97
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