INTEGRAL Galactic Bulge MonitoringRevolution 0733: Observation start 2008-10-13T21:22 = MJD 54752.891
Total Observation GTI = 11533 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 J17464-3213 266.563 -32.235 0.5 357.253 -1.832 29.6 0.33 88.7 15.8 0.29 55.2
GX 354-0 262.987 -33.828 0.5 354.306 -0.145 25.4 0.36 70.1 8.4 0.30 28.0
Ginga 1826-24 277.364 -23.801 1.0 9.267 -6.087 18.2 0.58 31.5 6.7 0.45 14.8
1E 1740.7-2942 265.997 -29.750 1.1 359.121 -0.122 9.4 0.34 27.3 6.2 0.30 20.6
GRS 1758-258 270.314 -25.739 1.1 4.517 -1.369 9.6 0.34 28.4 7.0 0.28 24.6
4U 1700-377 256.000 -37.853 1.2 347.754 +2.160 19.6 0.80 24.5 4.4 0.63 6.9
GX 1+4 263.000 -24.741 1.5 1.937 +4.804 7.0 0.37 19.1 0.0 0.00 0.0
H 1820-303 275.923 -30.360 1.7 2.790 -7.916 7.3 0.45 16.2 0.0 0.00 0.0
4U 1722-30 261.907 -30.793 2.4 356.336 +2.290 4.1 0.36 11.4 1.7 0.30 5.7
GX 3+1 266.979 -26.546 2.9 2.307 +0.806 3.1 0.34 9.1 0.0 0.00 0.0
3A 1822-371 276.492 -37.088 3.0 356.883 -11.317 5.0 0.58 8.6 0.0 0.00 0.0
GX 349+2 256.482 -36.407 3.2 349.139 +2.729 5.4 0.67 8.0 0.0 0.00 0.0
GX 9+1 270.428 -20.499 3.8 9.123 +1.133 3.2 0.47 6.7 0.0 0.00 0.0
SLX 1744-299_300 266.884 -30.020 0.0 359.290 -0.919 2.1 0.00 6.9 0.0 0.00 0.0
1A 1742-294 266.506 -29.526 0.0 359.543 -0.382 2.0 0.00 6.0 0.0 0.00 0.0
GX 17+2 274.061 -14.050 4.8 16.446 +1.224 10.4 2.03 5.1 0.0 0.00 0.0
SLX 1735-269 264.581 -27.037 4.7 0.765 +2.370 1.9 0.00 5.3 0.0 0.00 0.0
GX 5-1 270.244 -25.055 0.0 5.081 -0.975 1.8 0.00 5.0 0.0 0.00 0.0
1E 1742.9-2849 266.499 -28.824 5.7 0.138 -0.012 1.3 0.31 4.3 0.0 0.00 0.0
MXB 1730-335 263.368 -33.453 5.5 354.794 -0.206 1.5 0.34 4.4 0.0 0.00 0.0
3A 1728-169 262.847 -16.962 6.3 8.468 +9.108 2.7 0.70 3.8 0.0 0.00 0.0
SAX J1750.8-2900 267.533 -29.096 6.7 0.373 -0.927 1.1 0.31 3.6 0.0 0.00 0.0
IGR J18135-1751 273.254 -17.872 6.6 12.717 +0.080 2.4 0.00 3.6 0.0 0.00 0.0
SAX J1712.6-3739 258.073 -37.618 5.7 348.923 +0.987 2.8 0.65 4.3 0.0 0.00 0.0
IGR J17354-3255 263.883 -32.901 7.6 355.492 -0.269 1.2 0.37 3.2 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 2.1 0.41 0.8 0.25
IGR J17464-3213 266.567 -32.229 357.260 -1.832 5.1 0.60 3.1 0.39
GX 3+1 266.983 -26.564 2.294 +0.794 39.2 0.64 5.6 0.32
GX 5-1 270.284 -25.079 5.077 -1.019 70.8 1.71 5.8 0.78
GRO J1750-27 267.303 -26.643 2.373 +0.508 9.6 1.48 0.0 0.00
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Revolution 0733: Observation start 2008-10-13T21:22 = MJD 54752.891
Total Observation GTI = 11533 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 J17464-3213 266.563 -32.235 0.5 357.253 -1.832 29.6 0.33 88.7 15.8 0.29 55.2 GX 354-0 262.987 -33.828 0.5 354.306 -0.145 25.4 0.36 70.1 8.4 0.30 28.0 Ginga 1826-24 277.364 -23.801 1.0 9.267 -6.087 18.2 0.58 31.5 6.7 0.45 14.8 1E 1740.7-2942 265.997 -29.750 1.1 359.121 -0.122 9.4 0.34 27.3 6.2 0.30 20.6 GRS 1758-258 270.314 -25.739 1.1 4.517 -1.369 9.6 0.34 28.4 7.0 0.28 24.6 4U 1700-377 256.000 -37.853 1.2 347.754 +2.160 19.6 0.80 24.5 4.4 0.63 6.9 GX 1+4 263.000 -24.741 1.5 1.937 +4.804 7.0 0.37 19.1 0.0 0.00 0.0 H 1820-303 275.923 -30.360 1.7 2.790 -7.916 7.3 0.45 16.2 0.0 0.00 0.0 4U 1722-30 261.907 -30.793 2.4 356.336 +2.290 4.1 0.36 11.4 1.7 0.30 5.7 GX 3+1 266.979 -26.546 2.9 2.307 +0.806 3.1 0.34 9.1 0.0 0.00 0.0 3A 1822-371 276.492 -37.088 3.0 356.883 -11.317 5.0 0.58 8.6 0.0 0.00 0.0 GX 349+2 256.482 -36.407 3.2 349.139 +2.729 5.4 0.67 8.0 0.0 0.00 0.0 GX 9+1 270.428 -20.499 3.8 9.123 +1.133 3.2 0.47 6.7 0.0 0.00 0.0 SLX 1744-299_300 266.884 -30.020 0.0 359.290 -0.919 2.1 0.00 6.9 0.0 0.00 0.0 1A 1742-294 266.506 -29.526 0.0 359.543 -0.382 2.0 0.00 6.0 0.0 0.00 0.0 GX 17+2 274.061 -14.050 4.8 16.446 +1.224 10.4 2.03 5.1 0.0 0.00 0.0 SLX 1735-269 264.581 -27.037 4.7 0.765 +2.370 1.9 0.00 5.3 0.0 0.00 0.0 GX 5-1 270.244 -25.055 0.0 5.081 -0.975 1.8 0.00 5.0 0.0 0.00 0.0 1E 1742.9-2849 266.499 -28.824 5.7 0.138 -0.012 1.3 0.31 4.3 0.0 0.00 0.0 MXB 1730-335 263.368 -33.453 5.5 354.794 -0.206 1.5 0.34 4.4 0.0 0.00 0.0 3A 1728-169 262.847 -16.962 6.3 8.468 +9.108 2.7 0.70 3.8 0.0 0.00 0.0 SAX J1750.8-2900 267.533 -29.096 6.7 0.373 -0.927 1.1 0.31 3.6 0.0 0.00 0.0 IGR J18135-1751 273.254 -17.872 6.6 12.717 +0.080 2.4 0.00 3.6 0.0 0.00 0.0 SAX J1712.6-3739 258.073 -37.618 5.7 348.923 +0.987 2.8 0.65 4.3 0.0 0.00 0.0 IGR J17354-3255 263.883 -32.901 7.6 355.492 -0.269 1.2 0.37 3.2 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 2.1 0.41 0.8 0.25 IGR J17464-3213 266.567 -32.229 357.260 -1.832 5.1 0.60 3.1 0.39 GX 3+1 266.983 -26.564 2.294 +0.794 39.2 0.64 5.6 0.32 GX 5-1 270.284 -25.079 5.077 -1.019 70.8 1.71 5.8 0.78 GRO J1750-27 267.303 -26.643 2.373 +0.508 9.6 1.48 0.0 0.00
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