INTEGRAL Galactic Bulge MonitoringRevolution 0536: Observation start 2007-03-04 = MJD 54163
Total Observation GTI = 12289 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GX 1+4 263.009 -24.746 0.7 1.936 +4.795 19.5 0.37 53.3 0.0 0.00 0.0
GX 354-0 262.989 -33.839 0.7 354.299 -0.152 18.4 0.37 49.2 7.0 0.30 23.0
4U 1700-377 255.989 -37.842 0.9 347.757 +2.173 25.5 0.71 35.9 8.2 0.55 14.8
GRS 1758-258 270.299 -25.741 0.9 4.509 -1.357 10.7 0.30 35.6 7.4 0.24 30.5
1E 1740.7-2942 265.965 -29.746 0.9 359.109 -0.096 10.0 0.29 34.6 7.2 0.24 29.9
Ginga 1826-24 277.355 -23.801 1.0 9.264 -6.080 16.5 0.55 30.3 6.2 0.43 14.6
H 1820-303 275.910 -30.362 1.4 2.784 -7.907 9.3 0.44 20.9 0.0 0.00 0.0
GX 349+2 256.410 -36.414 1.8 349.099 +2.770 9.6 0.62 15.5 0.0 0.00 0.0
GRS 1741.9-2853 266.307 -28.918 0.0 359.971 +0.082 3.3 0.00 11.6 1.0 0.24 4.1
4U 1722-30 261.861 -30.803 2.3 356.306 +2.317 3.9 0.33 11.8 1.9 0.27 7.2
GX 9+1 270.407 -20.535 2.2 9.082 +1.133 5.3 0.44 12.0 0.0 0.00 0.0
GX 5-1 270.291 -25.079 2.4 5.080 -1.024 3.4 0.30 11.3 0.0 0.00 0.0
3A 1822-371 276.391 -37.111 3.0 356.826 -11.254 5.2 0.60 8.7 0.0 0.00 0.0
GX 3+1 267.011 -26.549 2.7 2.320 +0.780 2.9 0.30 9.8 0.0 0.00 0.0
1A 1742-294 266.492 -29.495 0.0 359.562 -0.356 2.6 0.00 9.0 0.0 0.00 0.0
OAO 1657-415 255.225 -41.659 3.0 344.377 +0.305 13.9 1.59 8.7 0.0 0.00 0.0
SLX 1735-269 264.551 -26.983 3.2 0.795 +2.421 2.4 0.30 7.9 0.0 0.00 0.0
GX 17+2 274.044 -14.027 3.7 16.458 +1.249 11.7 1.71 6.8 0.0 0.00 0.0
SLX 1744-299_300 266.861 -30.040 4.0 359.263 -0.913 1.8 0.28 6.4 1.0 0.24 4.4
XB 1832-330 278.894 -33.033 5.5 1.478 -11.360 2.4 0.00 4.5 0.0 0.00 0.0
3A 1728-169 262.920 -16.975 6.9 8.494 +9.043 2.5 0.72 3.5 0.0 0.00 0.0
HETE J1900.1-2455 284.982 -24.914 6.4 11.291 -12.825 20.9 5.55 3.8 0.0 0.00 0.0
GX 13+1 273.539 -17.198 0.0 13.439 +0.164 2.8 0.00 4.0 0.0 0.00 0.0
KS 1741-293 266.115 -29.411 0.0 359.463 -0.032 1.1 0.00 3.9 0.0 0.00 0.0
SLX 1737-282 265.247 -28.237 5.5 0.061 +1.232 1.3 0.29 4.4 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 > 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 3+1 266.983 -26.564 2.294 +0.794 29.4 0.56 4.0 0.28
GX 5-1 270.284 -25.079 5.077 -1.019 74.1 1.55 6.8 0.66
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Revolution 0536: Observation start 2007-03-04 = MJD 54163
Total Observation GTI = 12289 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 1+4 263.009 -24.746 0.7 1.936 +4.795 19.5 0.37 53.3 0.0 0.00 0.0 GX 354-0 262.989 -33.839 0.7 354.299 -0.152 18.4 0.37 49.2 7.0 0.30 23.0 4U 1700-377 255.989 -37.842 0.9 347.757 +2.173 25.5 0.71 35.9 8.2 0.55 14.8 GRS 1758-258 270.299 -25.741 0.9 4.509 -1.357 10.7 0.30 35.6 7.4 0.24 30.5 1E 1740.7-2942 265.965 -29.746 0.9 359.109 -0.096 10.0 0.29 34.6 7.2 0.24 29.9 Ginga 1826-24 277.355 -23.801 1.0 9.264 -6.080 16.5 0.55 30.3 6.2 0.43 14.6 H 1820-303 275.910 -30.362 1.4 2.784 -7.907 9.3 0.44 20.9 0.0 0.00 0.0 GX 349+2 256.410 -36.414 1.8 349.099 +2.770 9.6 0.62 15.5 0.0 0.00 0.0 GRS 1741.9-2853 266.307 -28.918 0.0 359.971 +0.082 3.3 0.00 11.6 1.0 0.24 4.1 4U 1722-30 261.861 -30.803 2.3 356.306 +2.317 3.9 0.33 11.8 1.9 0.27 7.2 GX 9+1 270.407 -20.535 2.2 9.082 +1.133 5.3 0.44 12.0 0.0 0.00 0.0 GX 5-1 270.291 -25.079 2.4 5.080 -1.024 3.4 0.30 11.3 0.0 0.00 0.0 3A 1822-371 276.391 -37.111 3.0 356.826 -11.254 5.2 0.60 8.7 0.0 0.00 0.0 GX 3+1 267.011 -26.549 2.7 2.320 +0.780 2.9 0.30 9.8 0.0 0.00 0.0 1A 1742-294 266.492 -29.495 0.0 359.562 -0.356 2.6 0.00 9.0 0.0 0.00 0.0 OAO 1657-415 255.225 -41.659 3.0 344.377 +0.305 13.9 1.59 8.7 0.0 0.00 0.0 SLX 1735-269 264.551 -26.983 3.2 0.795 +2.421 2.4 0.30 7.9 0.0 0.00 0.0 GX 17+2 274.044 -14.027 3.7 16.458 +1.249 11.7 1.71 6.8 0.0 0.00 0.0 SLX 1744-299_300 266.861 -30.040 4.0 359.263 -0.913 1.8 0.28 6.4 1.0 0.24 4.4 XB 1832-330 278.894 -33.033 5.5 1.478 -11.360 2.4 0.00 4.5 0.0 0.00 0.0 3A 1728-169 262.920 -16.975 6.9 8.494 +9.043 2.5 0.72 3.5 0.0 0.00 0.0 HETE J1900.1-2455 284.982 -24.914 6.4 11.291 -12.825 20.9 5.55 3.8 0.0 0.00 0.0 GX 13+1 273.539 -17.198 0.0 13.439 +0.164 2.8 0.00 4.0 0.0 0.00 0.0 KS 1741-293 266.115 -29.411 0.0 359.463 -0.032 1.1 0.00 3.9 0.0 0.00 0.0 SLX 1737-282 265.247 -28.237 5.5 0.061 +1.232 1.3 0.29 4.4 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 > 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 3+1 266.983 -26.564 2.294 +0.794 29.4 0.56 4.0 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 74.1 1.55 6.8 0.66
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