INTEGRAL Galactic Bulge MonitoringRevolution 0476: Observation start 2006-09-06 = MJD 53984
Total Observation GTI = 12086 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 1700-377 255.983 -37.846 0.5 347.751 +2.174 52.8 0.63 83.6 18.0 0.47 38.0
GX 354-0 262.984 -33.832 0.6 354.303 -0.145 19.3 0.33 58.7 3.8 0.26 14.7
GX 5-1 270.278 -25.084 0.7 5.070 -1.016 15.4 0.31 49.6 0.0 0.00 0.0
GX 1+4 263.015 -24.750 0.8 1.937 +4.788 15.3 0.34 44.5 0.0 0.00 0.0
GX 349+2 256.415 -36.419 1.0 349.097 +2.764 17.8 0.57 31.1 0.0 0.00 0.0
Ginga 1826-24 277.379 -23.804 1.0 9.271 -6.101 17.3 0.55 31.3 5.0 0.42 12.0
1A 1742-294 266.516 -29.533 1.3 359.541 -0.393 6.1 0.27 22.6 2.7 0.22 12.4
GRS 1758-258 270.308 -25.745 1.3 4.509 -1.367 6.8 0.31 22.2 4.2 0.24 17.2
1E 1740.7-2942 265.994 -29.755 1.5 359.115 -0.123 5.1 0.27 18.6 3.3 0.22 14.7
4U 1722-30 261.879 -30.812 2.2 356.307 +2.300 3.8 0.30 12.4 1.7 0.24 7.1
H 1820-303 275.929 -30.344 2.1 2.808 -7.914 6.0 0.45 13.3 0.0 0.00 0.0
GX 3+1 267.004 -26.614 2.5 2.260 +0.752 2.9 0.28 10.5 0.0 0.00 0.0
3A 1822-371 276.442 -37.119 2.5 356.837 -11.295 6.0 0.58 10.5 0.0 0.00 0.0
GX 9+1 270.375 -20.533 3.2 9.069 +1.159 3.6 0.45 8.0 0.0 0.00 0.0
GX 17+2 274.043 -14.046 2.5 16.441 +1.241 22.0 2.10 10.5 0.0 0.00 0.0
SLX 1735-269 264.514 -26.990 3.4 0.772 +2.446 2.1 0.28 7.6 0.0 0.00 0.0
SLX 1744-299_300 266.887 -30.029 3.8 359.284 -0.926 1.8 0.27 6.8 0.0 0.00 0.0
GX 13+1 273.630 -17.168 4.3 13.507 +0.103 4.3 0.75 5.8 0.0 0.00 0.0
3A 1728-169 262.981 -16.954 4.8 8.543 +9.004 3.4 0.67 5.1 0.0 0.00 0.0
1E 1742.9-2849 266.522 -28.864 5.9 0.115 -0.050 1.1 0.27 4.1 0.0 0.00 0.0
GRS 1734-292 264.390 -29.204 5.4 358.842 +1.354 1.2 0.28 4.5 0.0 0.00 0.0
4U 1705-32 257.313 -32.335 7.3 352.822 +4.611 1.4 0.44 3.3 0.0 0.00 0.0
SAX J1712.6-3739 258.190 -37.537 7.0 349.043 +0.959 1.8 0.54 3.4 2.4 0.41 5.8
IGR J18027-2016 270.643 -20.219 0.0 9.466 +1.096 1.7 0.00 3.6 0.0 0.00 0.0
SLX 1737-282 265.130 -28.335 6.5 359.923 +1.268 1.0 0.27 3.7 0.0 0.00 0.0
NEW_1 258.203 -18.491 4.0 4.705 +11.975 4.1 0.65 6.4 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 354-0 262.989 -33.835 354.302 -0.150 12.0 1.42 4.4 1.02
GX 3+1 266.983 -26.564 2.294 +0.794 27.8 0.56 3.7 0.29
GX 5-1 270.284 -25.079 5.077 -1.019 123.5 2.37 21.3 1.15
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.29 0.5 0.21
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Revolution 0476: Observation start 2006-09-06 = MJD 53984
Total Observation GTI = 12086 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 1700-377 255.983 -37.846 0.5 347.751 +2.174 52.8 0.63 83.6 18.0 0.47 38.0 GX 354-0 262.984 -33.832 0.6 354.303 -0.145 19.3 0.33 58.7 3.8 0.26 14.7 GX 5-1 270.278 -25.084 0.7 5.070 -1.016 15.4 0.31 49.6 0.0 0.00 0.0 GX 1+4 263.015 -24.750 0.8 1.937 +4.788 15.3 0.34 44.5 0.0 0.00 0.0 GX 349+2 256.415 -36.419 1.0 349.097 +2.764 17.8 0.57 31.1 0.0 0.00 0.0 Ginga 1826-24 277.379 -23.804 1.0 9.271 -6.101 17.3 0.55 31.3 5.0 0.42 12.0 1A 1742-294 266.516 -29.533 1.3 359.541 -0.393 6.1 0.27 22.6 2.7 0.22 12.4 GRS 1758-258 270.308 -25.745 1.3 4.509 -1.367 6.8 0.31 22.2 4.2 0.24 17.2 1E 1740.7-2942 265.994 -29.755 1.5 359.115 -0.123 5.1 0.27 18.6 3.3 0.22 14.7 4U 1722-30 261.879 -30.812 2.2 356.307 +2.300 3.8 0.30 12.4 1.7 0.24 7.1 H 1820-303 275.929 -30.344 2.1 2.808 -7.914 6.0 0.45 13.3 0.0 0.00 0.0 GX 3+1 267.004 -26.614 2.5 2.260 +0.752 2.9 0.28 10.5 0.0 0.00 0.0 3A 1822-371 276.442 -37.119 2.5 356.837 -11.295 6.0 0.58 10.5 0.0 0.00 0.0 GX 9+1 270.375 -20.533 3.2 9.069 +1.159 3.6 0.45 8.0 0.0 0.00 0.0 GX 17+2 274.043 -14.046 2.5 16.441 +1.241 22.0 2.10 10.5 0.0 0.00 0.0 SLX 1735-269 264.514 -26.990 3.4 0.772 +2.446 2.1 0.28 7.6 0.0 0.00 0.0 SLX 1744-299_300 266.887 -30.029 3.8 359.284 -0.926 1.8 0.27 6.8 0.0 0.00 0.0 GX 13+1 273.630 -17.168 4.3 13.507 +0.103 4.3 0.75 5.8 0.0 0.00 0.0 3A 1728-169 262.981 -16.954 4.8 8.543 +9.004 3.4 0.67 5.1 0.0 0.00 0.0 1E 1742.9-2849 266.522 -28.864 5.9 0.115 -0.050 1.1 0.27 4.1 0.0 0.00 0.0 GRS 1734-292 264.390 -29.204 5.4 358.842 +1.354 1.2 0.28 4.5 0.0 0.00 0.0 4U 1705-32 257.313 -32.335 7.3 352.822 +4.611 1.4 0.44 3.3 0.0 0.00 0.0 SAX J1712.6-3739 258.190 -37.537 7.0 349.043 +0.959 1.8 0.54 3.4 2.4 0.41 5.8 IGR J18027-2016 270.643 -20.219 0.0 9.466 +1.096 1.7 0.00 3.6 0.0 0.00 0.0 SLX 1737-282 265.130 -28.335 6.5 359.923 +1.268 1.0 0.27 3.7 0.0 0.00 0.0 NEW_1 258.203 -18.491 4.0 4.705 +11.975 4.1 0.65 6.4 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 354-0 262.989 -33.835 354.302 -0.150 12.0 1.42 4.4 1.02 GX 3+1 266.983 -26.564 2.294 +0.794 27.8 0.56 3.7 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 123.5 2.37 21.3 1.15 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.29 0.5 0.21
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