INTEGRAL Galactic Bulge MonitoringRevolution 0732: Observation start 2008-10-10T21:34 = MJD 54749.899
Total Observation GTI = 77571 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 266.566 -32.232 0.3 357.257 -1.833 30.4 0.14 223.0 16.3 0.12 140.6
4U 1700-377 255.988 -37.844 0.3 347.755 +2.173 50.5 0.26 193.7 14.1 0.21 68.9
GX 354-0 262.991 -33.834 0.3 354.304 -0.151 26.2 0.15 172.5 8.5 0.12 68.6
1E 1740.7-2942 265.981 -29.739 0.5 359.123 -0.105 9.5 0.14 70.2 5.8 0.11 51.0
OAO 1657-415 255.209 -41.648 0.6 344.378 +0.321 27.1 0.40 68.7 6.5 0.31 21.4
Ginga 1826-24 277.369 -23.796 0.5 9.273 -6.088 15.7 0.21 73.8 6.6 0.17 37.9
GX 5-1 270.284 -25.076 0.6 5.079 -1.017 10.6 0.15 69.5 0.0 0.00 0.0
GRS 1758-258 270.296 -25.739 0.6 4.509 -1.355 9.1 0.15 60.8 6.6 0.12 53.0
H 1820-303 275.914 -30.357 0.7 2.790 -7.908 7.1 0.15 47.0 0.0 0.00 0.0
GX 1+4 263.009 -24.741 0.8 1.941 +4.797 7.5 0.19 38.9 0.0 0.00 0.0
3A 1822-371 276.442 -37.095 0.9 356.858 -11.284 6.0 0.17 35.1 0.0 0.00 0.0
GX 349+2 256.440 -36.435 0.9 349.097 +2.738 8.5 0.25 33.9 0.0 0.00 0.0
4U 1722-30 261.881 -30.802 1.2 356.317 +2.303 4.1 0.16 25.4 1.3 0.13 9.9
GX 3+1 266.988 -26.561 1.3 2.298 +0.792 3.2 0.15 22.2 0.0 0.00 0.0
1A 1742-294 266.526 -29.505 0.0 359.569 -0.386 2.6 0.00 18.8 0.5 0.00 4.3
SLX 1735-269 264.572 -26.980 1.7 0.808 +2.407 2.6 0.15 16.9 1.0 0.13 8.0
GX 17+2 274.008 -14.054 1.7 16.418 +1.268 18.6 1.09 16.9 0.0 0.00 0.0
H 1702-429 256.576 -43.036 1.7 343.892 -1.326 6.0 0.38 16.0 1.8 0.30 6.0
GX 9+1 270.371 -20.518 2.0 9.080 +1.170 3.3 0.24 13.8 0.0 0.00 0.0
XB 1832-330 278.939 -32.953 2.3 1.568 -11.360 2.1 0.18 12.0 1.1 0.15 7.4
4U 1735-444 264.742 -44.447 2.5 346.056 -6.992 3.2 0.31 10.5 0.0 0.00 0.0
SLX 1744-299_300 266.871 -30.011 2.5 359.292 -0.905 1.4 0.13 10.6 0.0 0.00 0.0
MXB 1730-335 263.379 -33.349 0.0 354.886 -0.158 1.3 0.00 8.9 0.5 0.00 4.2
SAX J1712.6-3739 258.109 -37.631 3.0 348.930 +0.956 1.9 0.22 8.6 0.9 0.00 5.1
HETE J1900.1-2455 285.038 -24.909 2.6 11.317 -12.870 5.5 0.55 10.1 2.8 0.44 6.4
SAX J1750.8-2900 267.553 -29.044 3.0 0.426 -0.915 1.2 0.13 8.7 0.0 0.00 0.0
IGR J17252-3616 261.283 -36.256 3.4 351.513 -0.329 1.3 0.17 7.7 0.0 0.00 0.0
1E 1742.9-2849 266.495 -28.848 3.4 0.116 -0.021 1.1 0.14 7.6 0.0 0.00 0.0
GRS 1734-292 264.336 -29.084 4.1 358.918 +1.458 0.9 0.15 6.1 0.0 0.00 0.0
3A 1728-169 262.932 -16.878 4.0 8.584 +9.084 2.9 0.46 6.3 0.0 0.00 0.0
XTE J1716-389 258.859 -38.914 5.5 348.234 -0.273 1.1 0.00 4.5 0.0 0.00 0.0
H 1705-440 257.229 -44.028 5.8 343.382 -2.299 1.7 0.41 4.2 0.0 0.00 0.0
IGR J17200-3116 259.976 -31.315 6.0 354.972 +3.363 0.7 0.18 4.1 0.0 0.00 0.0
4U 1812-12 273.727 -12.021 6.5 18.076 +2.475 16.8 0.00 3.7 0.0 0.00 0.0
NEW_1 268.360 -23.839 2.0 5.273 +1.119 2.3 0.17 13.3 1.4 0.14 10.1
NEW_2 264.393 -30.378 2.2 357.852 +0.723 1.8 0.15 12.5 0.7 0.12 6.0
NEW_3 255.508 -40.839 3.3 345.155 +0.640 2.9 0.37 7.8 0.0 0.00 0.0
NEW_4 267.631 -50.676 0.0 341.590 -11.806 12.9 0.00 7.1 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 9.1 0.37 4.0 0.29
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.7 0.28 1.1 0.17
1A 1742-294 266.523 -29.515 359.559 -0.389 1.6 0.25 0.6 0.15
IGR J17464-3213 266.567 -32.229 357.260 -1.832 7.5 0.20 3.9 0.15
GX 5-1 270.284 -25.079 5.077 -1.019 120.1 0.89 16.1 0.39
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Revolution 0732: Observation start 2008-10-10T21:34 = MJD 54749.899
Total Observation GTI = 77571 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 266.566 -32.232 0.3 357.257 -1.833 30.4 0.14 223.0 16.3 0.12 140.6 4U 1700-377 255.988 -37.844 0.3 347.755 +2.173 50.5 0.26 193.7 14.1 0.21 68.9 GX 354-0 262.991 -33.834 0.3 354.304 -0.151 26.2 0.15 172.5 8.5 0.12 68.6 1E 1740.7-2942 265.981 -29.739 0.5 359.123 -0.105 9.5 0.14 70.2 5.8 0.11 51.0 OAO 1657-415 255.209 -41.648 0.6 344.378 +0.321 27.1 0.40 68.7 6.5 0.31 21.4 Ginga 1826-24 277.369 -23.796 0.5 9.273 -6.088 15.7 0.21 73.8 6.6 0.17 37.9 GX 5-1 270.284 -25.076 0.6 5.079 -1.017 10.6 0.15 69.5 0.0 0.00 0.0 GRS 1758-258 270.296 -25.739 0.6 4.509 -1.355 9.1 0.15 60.8 6.6 0.12 53.0 H 1820-303 275.914 -30.357 0.7 2.790 -7.908 7.1 0.15 47.0 0.0 0.00 0.0 GX 1+4 263.009 -24.741 0.8 1.941 +4.797 7.5 0.19 38.9 0.0 0.00 0.0 3A 1822-371 276.442 -37.095 0.9 356.858 -11.284 6.0 0.17 35.1 0.0 0.00 0.0 GX 349+2 256.440 -36.435 0.9 349.097 +2.738 8.5 0.25 33.9 0.0 0.00 0.0 4U 1722-30 261.881 -30.802 1.2 356.317 +2.303 4.1 0.16 25.4 1.3 0.13 9.9 GX 3+1 266.988 -26.561 1.3 2.298 +0.792 3.2 0.15 22.2 0.0 0.00 0.0 1A 1742-294 266.526 -29.505 0.0 359.569 -0.386 2.6 0.00 18.8 0.5 0.00 4.3 SLX 1735-269 264.572 -26.980 1.7 0.808 +2.407 2.6 0.15 16.9 1.0 0.13 8.0 GX 17+2 274.008 -14.054 1.7 16.418 +1.268 18.6 1.09 16.9 0.0 0.00 0.0 H 1702-429 256.576 -43.036 1.7 343.892 -1.326 6.0 0.38 16.0 1.8 0.30 6.0 GX 9+1 270.371 -20.518 2.0 9.080 +1.170 3.3 0.24 13.8 0.0 0.00 0.0 XB 1832-330 278.939 -32.953 2.3 1.568 -11.360 2.1 0.18 12.0 1.1 0.15 7.4 4U 1735-444 264.742 -44.447 2.5 346.056 -6.992 3.2 0.31 10.5 0.0 0.00 0.0 SLX 1744-299_300 266.871 -30.011 2.5 359.292 -0.905 1.4 0.13 10.6 0.0 0.00 0.0 MXB 1730-335 263.379 -33.349 0.0 354.886 -0.158 1.3 0.00 8.9 0.5 0.00 4.2 SAX J1712.6-3739 258.109 -37.631 3.0 348.930 +0.956 1.9 0.22 8.6 0.9 0.00 5.1 HETE J1900.1-2455 285.038 -24.909 2.6 11.317 -12.870 5.5 0.55 10.1 2.8 0.44 6.4 SAX J1750.8-2900 267.553 -29.044 3.0 0.426 -0.915 1.2 0.13 8.7 0.0 0.00 0.0 IGR J17252-3616 261.283 -36.256 3.4 351.513 -0.329 1.3 0.17 7.7 0.0 0.00 0.0 1E 1742.9-2849 266.495 -28.848 3.4 0.116 -0.021 1.1 0.14 7.6 0.0 0.00 0.0 GRS 1734-292 264.336 -29.084 4.1 358.918 +1.458 0.9 0.15 6.1 0.0 0.00 0.0 3A 1728-169 262.932 -16.878 4.0 8.584 +9.084 2.9 0.46 6.3 0.0 0.00 0.0 XTE J1716-389 258.859 -38.914 5.5 348.234 -0.273 1.1 0.00 4.5 0.0 0.00 0.0 H 1705-440 257.229 -44.028 5.8 343.382 -2.299 1.7 0.41 4.2 0.0 0.00 0.0 IGR J17200-3116 259.976 -31.315 6.0 354.972 +3.363 0.7 0.18 4.1 0.0 0.00 0.0 4U 1812-12 273.727 -12.021 6.5 18.076 +2.475 16.8 0.00 3.7 0.0 0.00 0.0 NEW_1 268.360 -23.839 2.0 5.273 +1.119 2.3 0.17 13.3 1.4 0.14 10.1 NEW_2 264.393 -30.378 2.2 357.852 +0.723 1.8 0.15 12.5 0.7 0.12 6.0 NEW_3 255.508 -40.839 3.3 345.155 +0.640 2.9 0.37 7.8 0.0 0.00 0.0 NEW_4 267.631 -50.676 0.0 341.590 -11.806 12.9 0.00 7.1 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 9.1 0.37 4.0 0.29 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.7 0.28 1.1 0.17 1A 1742-294 266.523 -29.515 359.559 -0.389 1.6 0.25 0.6 0.15 IGR J17464-3213 266.567 -32.229 357.260 -1.832 7.5 0.20 3.9 0.15 GX 5-1 270.284 -25.079 5.077 -1.019 120.1 0.89 16.1 0.39
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