INTEGRAL Galactic Bulge MonitoringRevolution 0302: Observation start 2005-04-03 = MJD 53463
Total Observation GTI = 12314 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 1700-377 255.981 -37.846 0.5 347.750 +2.176 48.7 0.69 70.4 13.9 0.51 27.2
GRS 1758-258 270.309 -25.747 0.8 4.508 -1.368 12.7 0.29 44.2 9.0 0.23 38.3
GX 349+2 256.437 -36.418 0.9 349.108 +2.750 17.6 0.52 33.9 0.0 0.00 0.0
1E 1740.7-2942 265.983 -29.739 1.1 359.123 -0.106 8.4 0.29 29.0 4.7 0.24 19.3
Ginga 1826-24 277.376 -23.805 1.1 9.269 -6.099 14.0 0.50 27.7 6.4 0.40 16.0
OAO 1657-415 255.197 -41.652 1.3 344.369 +0.325 30.1 1.28 23.5 6.5 0.96 6.8
1A 1742-294 266.495 -29.500 0.0 359.559 -0.360 4.7 0.00 16.6 2.4 0.24 10.1
GX 354-0 262.983 -33.838 1.6 354.297 -0.147 5.8 0.33 17.5 0.0 0.00 0.0
GX 5-1 270.278 -25.100 1.8 5.057 -1.024 5.1 0.32 15.8 0.0 0.00 0.0
GX 9+1 270.395 -20.544 2.0 9.068 +1.137 5.5 0.40 13.7 0.0 0.00 0.0
H 1820-303 275.931 -30.361 1.9 2.793 -7.923 5.8 0.39 14.8 0.0 0.00 0.0
GX 1+4 263.020 -24.731 2.1 1.955 +4.794 3.7 0.29 13.1 0.0 0.00 0.0
4U 1722-30 261.870 -30.783 2.2 356.327 +2.321 3.9 0.32 12.2 2.3 0.26 8.8
IGR J17252-3616 261.307 -36.289 2.0 351.496 -0.364 5.1 0.36 14.0 0.0 0.00 0.0
3A 1822-371 276.421 -37.095 2.6 356.851 -11.269 5.7 0.56 10.1 0.0 0.00 0.0
XTE J1743-363 265.767 -36.363 2.7 353.383 -3.423 3.3 0.34 9.6 0.0 0.00 0.0
GX 3+1 266.945 -26.554 3.4 2.285 +0.828 2.2 0.30 7.6 0.0 0.00 0.0
GX 17+2 274.036 -14.045 3.3 16.438 +1.248 15.8 2.06 7.7 0.0 0.00 0.0
SLX 1744-299_300 266.884 -30.048 3.6 359.266 -0.933 1.9 0.28 7.0 0.0 0.00 0.0
SLX 1735-269 264.574 -26.992 3.2 0.799 +2.399 2.1 0.26 8.0 1.3 0.23 5.8
1E 1742.8-2853 266.385 -28.893 4.5 0.028 +0.037 1.3 0.24 5.5 0.0 0.00 0.0
GX 13+1 273.677 -17.206 4.2 13.494 +0.045 4.6 0.78 6.0 0.0 0.00 0.0
KS 1741-293 266.117 -29.418 0.0 359.458 -0.037 1.2 0.00 4.6 0.0 0.00 0.0
V1223 Sgr 283.790 -31.193 5.0 4.941 -14.390 9.2 1.88 4.9 0.0 0.00 0.0
3A 1728-169 262.900 -16.904 4.9 8.545 +9.096 3.1 0.61 5.0 0.0 0.00 0.0
XTE J1818-245 274.557 -24.522 5.9 7.439 -4.148 1.6 0.37 4.2 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 with in the 3-10 keV image > 10σ 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).
NOTES: Fluxes for light curves are extracted from the images using mosaic_spec; 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 23.7 1.49 5.0 1.00
1A 1742-294 266.523 -29.515 359.559 -0.389 1.5 0.28 0.9 0.20
GX 3+1 266.983 -26.564 2.294 +0.794 25.1 0.50 4.5 0.28
GX 5-1 270.284 -25.079 5.077 -1.019 87.5 2.02 6.4 0.81
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Revolution 0302: Observation start 2005-04-03 = MJD 53463
Total Observation GTI = 12314 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 1700-377 255.981 -37.846 0.5 347.750 +2.176 48.7 0.69 70.4 13.9 0.51 27.2 GRS 1758-258 270.309 -25.747 0.8 4.508 -1.368 12.7 0.29 44.2 9.0 0.23 38.3 GX 349+2 256.437 -36.418 0.9 349.108 +2.750 17.6 0.52 33.9 0.0 0.00 0.0 1E 1740.7-2942 265.983 -29.739 1.1 359.123 -0.106 8.4 0.29 29.0 4.7 0.24 19.3 Ginga 1826-24 277.376 -23.805 1.1 9.269 -6.099 14.0 0.50 27.7 6.4 0.40 16.0 OAO 1657-415 255.197 -41.652 1.3 344.369 +0.325 30.1 1.28 23.5 6.5 0.96 6.8 1A 1742-294 266.495 -29.500 0.0 359.559 -0.360 4.7 0.00 16.6 2.4 0.24 10.1 GX 354-0 262.983 -33.838 1.6 354.297 -0.147 5.8 0.33 17.5 0.0 0.00 0.0 GX 5-1 270.278 -25.100 1.8 5.057 -1.024 5.1 0.32 15.8 0.0 0.00 0.0 GX 9+1 270.395 -20.544 2.0 9.068 +1.137 5.5 0.40 13.7 0.0 0.00 0.0 H 1820-303 275.931 -30.361 1.9 2.793 -7.923 5.8 0.39 14.8 0.0 0.00 0.0 GX 1+4 263.020 -24.731 2.1 1.955 +4.794 3.7 0.29 13.1 0.0 0.00 0.0 4U 1722-30 261.870 -30.783 2.2 356.327 +2.321 3.9 0.32 12.2 2.3 0.26 8.8 IGR J17252-3616 261.307 -36.289 2.0 351.496 -0.364 5.1 0.36 14.0 0.0 0.00 0.0 3A 1822-371 276.421 -37.095 2.6 356.851 -11.269 5.7 0.56 10.1 0.0 0.00 0.0 XTE J1743-363 265.767 -36.363 2.7 353.383 -3.423 3.3 0.34 9.6 0.0 0.00 0.0 GX 3+1 266.945 -26.554 3.4 2.285 +0.828 2.2 0.30 7.6 0.0 0.00 0.0 GX 17+2 274.036 -14.045 3.3 16.438 +1.248 15.8 2.06 7.7 0.0 0.00 0.0 SLX 1744-299_300 266.884 -30.048 3.6 359.266 -0.933 1.9 0.28 7.0 0.0 0.00 0.0 SLX 1735-269 264.574 -26.992 3.2 0.799 +2.399 2.1 0.26 8.0 1.3 0.23 5.8 1E 1742.8-2853 266.385 -28.893 4.5 0.028 +0.037 1.3 0.24 5.5 0.0 0.00 0.0 GX 13+1 273.677 -17.206 4.2 13.494 +0.045 4.6 0.78 6.0 0.0 0.00 0.0 KS 1741-293 266.117 -29.418 0.0 359.458 -0.037 1.2 0.00 4.6 0.0 0.00 0.0 V1223 Sgr 283.790 -31.193 5.0 4.941 -14.390 9.2 1.88 4.9 0.0 0.00 0.0 3A 1728-169 262.900 -16.904 4.9 8.545 +9.096 3.1 0.61 5.0 0.0 0.00 0.0 XTE J1818-245 274.557 -24.522 5.9 7.439 -4.148 1.6 0.37 4.2 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 with in the 3-10 keV image > 10σ 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).
NOTES: Fluxes for light curves are extracted from the images using mosaic_spec; 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 23.7 1.49 5.0 1.00 1A 1742-294 266.523 -29.515 359.559 -0.389 1.5 0.28 0.9 0.20 GX 3+1 266.983 -26.564 2.294 +0.794 25.1 0.50 4.5 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 87.5 2.02 6.4 0.81
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