INTEGRAL Galactic Bulge MonitoringRevolution 0673: Observation start 2008-04-17T09:35 = MJD 54573.4
Total Observation GTI = 11354 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
IGR J17473-2721 266.827 -27.341 0.3 1.556 +0.511 55.4 0.35 156.7 22.1 0.28 78.1
4U 1700-377 255.986 -37.845 0.6 347.753 +2.173 44.6 0.81 55.4 13.1 0.59 22.1
GX 5-1 270.291 -25.082 0.8 5.078 -1.026 17.5 0.39 45.0 0.0 0.00 0.0
GRO J1750-27 267.272 -26.635 0.8 2.366 +0.536 13.6 0.35 38.6 0.0 0.00 0.0
GX 354-0 262.990 -33.830 1.0 354.307 -0.148 13.2 0.40 33.3 3.9 0.31 12.7
SAX J1750.8-2900 267.609 -29.031 1.0 0.463 -0.951 10.5 0.34 30.6 4.1 0.27 14.9
Ginga 1826-24 277.379 -23.797 1.1 9.277 -6.097 18.2 0.64 28.6 7.2 0.45 16.0
GRS 1758-258 270.312 -25.730 1.5 4.524 -1.362 7.7 0.40 19.5 4.4 0.31 14.2
H 1820-303 275.912 -30.364 1.4 2.783 -7.909 9.8 0.47 20.6 0.0 0.00 0.0
4U 1722-30 261.882 -30.782 1.6 356.334 +2.314 7.7 0.43 18.0 3.4 0.33 10.4
GX 3+1 266.904 -26.582 2.5 2.241 +0.845 3.6 0.00 10.6 0.0 0.00 0.0
1E 1740.7-2942 265.988 -29.720 2.8 359.142 -0.100 3.3 0.34 9.5 3.1 0.27 11.2
3A 1822-371 276.390 -37.092 2.9 356.843 -11.246 6.0 0.65 9.2 0.0 0.00 0.0
GX 9+1 270.423 -20.489 3.0 9.129 +1.142 4.3 0.50 8.6 0.0 0.00 0.0
XTE J1810-189 272.593 -19.079 2.4 11.357 +0.049 7.5 0.67 11.1 3.9 0.51 7.7
GX 349+2 256.432 -36.422 3.1 349.103 +2.751 6.2 0.73 8.4 0.0 0.00 0.0
3A 1728-169 262.942 -16.980 4.4 8.502 +9.021 4.6 0.82 5.6 0.0 0.00 0.0
XTE J1709-267 257.362 -26.700 4.5 357.428 +7.897 2.9 0.52 5.6 0.0 0.00 0.0
Oph Cluster 258.105 -23.364 4.5 0.573 +9.281 3.2 0.56 5.6 0.0 0.00 0.0
GX 1+4 262.981 -24.735 4.6 1.932 +4.822 2.0 0.37 5.4 0.0 0.00 0.0
Swift J174535.5-2901 266.429 -29.048 0.0 359.915 -0.076 1.8 0.00 5.0 0.0 0.00 0.0
GX 17+2 274.046 -14.021 5.7 16.464 +1.251 10.5 2.46 4.3 0.0 0.00 0.0
IGR J17254-3257 261.216 -32.923 6.1 354.240 +1.588 1.6 0.39 4.0 0.0 0.00 0.0
XTE J1719-291 259.774 -29.016 6.6 356.766 +4.818 1.6 0.00 3.7 1.3 0.33 3.9
SLX 1744-299_300 266.851 -30.014 3.7 359.280 -0.892 2.3 0.33 6.8 0.0 0.00 0.0
NEW_1 284.490 -44.306 4.1 352.366 -19.671 108.5 14.63 6.2 0.0 0.00 0.0
** NOTE **: NEW_1 is found automatically by OSA in the very corner of the mosaic and is certainly not a real new source.
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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
SAX J1750.8-2900 267.603 -29.037 0.455 -0.949 2.4 0.41 1.2 0.27
1A 1742-294 266.523 -29.515 359.559 -0.389 3.3 0.41 1.0 0.27
IGR J17473-2721 266.825 -27.344 1.553 +0.510 11.0 0.53 6.4 0.33
GX 3+1 266.983 -26.564 2.294 +0.794 25.2 0.63 4.3 0.36
GX 5-1 270.284 -25.079 5.077 -1.019 84.4 1.89 15.7 0.96
GRO J1750-27 267.303 -26.643 2.373 +0.508 1.4 0.49 2.0 0.33
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Revolution 0673: Observation start 2008-04-17T09:35 = MJD 54573.4
Total Observation GTI = 11354 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17473-2721 266.827 -27.341 0.3 1.556 +0.511 55.4 0.35 156.7 22.1 0.28 78.1 4U 1700-377 255.986 -37.845 0.6 347.753 +2.173 44.6 0.81 55.4 13.1 0.59 22.1 GX 5-1 270.291 -25.082 0.8 5.078 -1.026 17.5 0.39 45.0 0.0 0.00 0.0 GRO J1750-27 267.272 -26.635 0.8 2.366 +0.536 13.6 0.35 38.6 0.0 0.00 0.0 GX 354-0 262.990 -33.830 1.0 354.307 -0.148 13.2 0.40 33.3 3.9 0.31 12.7 SAX J1750.8-2900 267.609 -29.031 1.0 0.463 -0.951 10.5 0.34 30.6 4.1 0.27 14.9 Ginga 1826-24 277.379 -23.797 1.1 9.277 -6.097 18.2 0.64 28.6 7.2 0.45 16.0 GRS 1758-258 270.312 -25.730 1.5 4.524 -1.362 7.7 0.40 19.5 4.4 0.31 14.2 H 1820-303 275.912 -30.364 1.4 2.783 -7.909 9.8 0.47 20.6 0.0 0.00 0.0 4U 1722-30 261.882 -30.782 1.6 356.334 +2.314 7.7 0.43 18.0 3.4 0.33 10.4 GX 3+1 266.904 -26.582 2.5 2.241 +0.845 3.6 0.00 10.6 0.0 0.00 0.0 1E 1740.7-2942 265.988 -29.720 2.8 359.142 -0.100 3.3 0.34 9.5 3.1 0.27 11.2 3A 1822-371 276.390 -37.092 2.9 356.843 -11.246 6.0 0.65 9.2 0.0 0.00 0.0 GX 9+1 270.423 -20.489 3.0 9.129 +1.142 4.3 0.50 8.6 0.0 0.00 0.0 XTE J1810-189 272.593 -19.079 2.4 11.357 +0.049 7.5 0.67 11.1 3.9 0.51 7.7 GX 349+2 256.432 -36.422 3.1 349.103 +2.751 6.2 0.73 8.4 0.0 0.00 0.0 3A 1728-169 262.942 -16.980 4.4 8.502 +9.021 4.6 0.82 5.6 0.0 0.00 0.0 XTE J1709-267 257.362 -26.700 4.5 357.428 +7.897 2.9 0.52 5.6 0.0 0.00 0.0 Oph Cluster 258.105 -23.364 4.5 0.573 +9.281 3.2 0.56 5.6 0.0 0.00 0.0 GX 1+4 262.981 -24.735 4.6 1.932 +4.822 2.0 0.37 5.4 0.0 0.00 0.0 Swift J174535.5-2901 266.429 -29.048 0.0 359.915 -0.076 1.8 0.00 5.0 0.0 0.00 0.0 GX 17+2 274.046 -14.021 5.7 16.464 +1.251 10.5 2.46 4.3 0.0 0.00 0.0 IGR J17254-3257 261.216 -32.923 6.1 354.240 +1.588 1.6 0.39 4.0 0.0 0.00 0.0 XTE J1719-291 259.774 -29.016 6.6 356.766 +4.818 1.6 0.00 3.7 1.3 0.33 3.9 SLX 1744-299_300 266.851 -30.014 3.7 359.280 -0.892 2.3 0.33 6.8 0.0 0.00 0.0 NEW_1 284.490 -44.306 4.1 352.366 -19.671 108.5 14.63 6.2 0.0 0.00 0.0
** NOTE **: NEW_1 is found automatically by OSA in the very corner of the mosaic and is certainly not a real new source.
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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== SAX J1750.8-2900 267.603 -29.037 0.455 -0.949 2.4 0.41 1.2 0.27 1A 1742-294 266.523 -29.515 359.559 -0.389 3.3 0.41 1.0 0.27 IGR J17473-2721 266.825 -27.344 1.553 +0.510 11.0 0.53 6.4 0.33 GX 3+1 266.983 -26.564 2.294 +0.794 25.2 0.63 4.3 0.36 GX 5-1 270.284 -25.079 5.077 -1.019 84.4 1.89 15.7 0.96 GRO J1750-27 267.303 -26.643 2.373 +0.508 1.4 0.49 2.0 0.33
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