INTEGRAL Galactic Bulge MonitoringRevolution 0359: Observation start 2005-09-23 = MJD 53636
Total Observation GTI = 12321 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 5-1 270.286 -25.076 0.6 5.081 -1.018 20.9 0.33 63.0 0.0 0.00 0.0
4U 1700-377 255.986 -37.841 0.7 347.756 +2.176 29.8 0.59 50.7 10.7 0.45 23.7
GRS 1758-258 270.306 -25.735 0.8 4.517 -1.360 12.2 0.30 40.9 8.4 0.24 34.8
GX 354-0 262.987 -33.840 0.8 354.297 -0.152 13.8 0.32 42.6 2.9 0.26 11.1
Ginga 1826-24 277.357 -23.797 0.9 9.268 -6.079 17.6 0.52 34.1 6.1 0.40 15.2
GX 349+2 256.431 -36.410 1.0 349.112 +2.759 15.5 0.53 29.5 0.0 0.00 0.0
1E 1740.7-2942 265.963 -29.740 1.1 359.113 -0.092 8.0 0.28 28.7 4.9 0.23 21.2
GX 1+4 263.013 -24.739 1.0 1.945 +4.796 10.2 0.34 30.1 0.0 0.00 0.0
H 1820-303 275.900 -30.345 1.8 2.796 -7.892 6.1 0.40 15.4 0.0 0.00 0.0
GRO J1655-40 253.460 -39.821 2.3 344.981 +2.496 12.4 1.08 11.5 10.2 0.84 12.2
GX 9+1 270.397 -20.555 2.7 9.060 +1.131 3.9 0.40 9.7 0.0 0.00 0.0
KS 1741-293 266.211 -29.337 0.0 359.570 -0.065 2.2 0.00 8.2 0.0 0.00 0.0
IGR J17464-3213 266.567 -32.246 2.6 357.245 -1.841 2.8 0.28 10.1 2.2 0.23 9.6
SLX 1735-269 264.591 -26.992 3.1 0.807 +2.387 2.5 0.30 8.3 1.5 0.25 6.1
3A 1822-371 276.503 -37.098 3.4 356.877 -11.330 4.0 0.54 7.5 0.0 0.00 0.0
XTE J1739-285 265.020 -28.445 3.8 359.778 +1.291 1.9 0.28 6.6 0.0 0.00 0.0
GX 3+1 267.035 -26.566 3.2 2.315 +0.753 2.2 0.27 8.0 0.0 0.00 0.0
GRS 1734-292 264.347 -29.118 4.0 358.894 +1.432 1.8 0.28 6.4 0.0 0.00 0.0
GX 17+2 274.069 -14.024 4.1 16.473 +1.229 13.4 2.16 6.2 0.0 0.00 0.0
GX 13+1 273.550 -17.163 4.9 13.475 +0.172 3.9 0.77 5.1 0.0 0.00 0.0
SLX 1744-299_300 266.917 -30.039 5.5 359.289 -0.954 1.4 0.31 4.4 0.0 0.00 0.0
4U 1722-30 261.908 -30.740 5.5 356.381 +2.318 1.4 0.00 4.4 0.0 0.00 0.0
IGR J18048-1455 271.179 -14.968 4.9 14.296 +3.227 6.6 1.28 5.1 0.0 0.00 0.0
GRS 1747-312 267.775 -31.312 6.0 358.575 -2.241 1.1 0.28 4.1 0.0 0.00 0.0
V2400 Oph 258.209 -24.262 5.9 359.884 +8.687 1.7 0.40 4.1 0.0 0.00 0.0
IGR J17252-3616 261.350 -36.278 4.7 351.525 -0.387 2.1 0.39 5.2 0.0 0.00 0.0
IGR J18027-2016 270.641 -20.219 0.0 9.465 +1.098 1.6 0.00 3.7 0.0 0.00 0.0
IGR J17456-2901 266.400 -29.008 0.0 359.936 -0.033 0.9 0.00 3.7 0.0 0.00 0.0
1E 1743.1-2843 266.587 -28.679 0.0 0.303 -0.002 0.9 0.00 3.4 0.9 0.00 4.3
1A 1742-294 266.589 -29.502 0.0 359.601 -0.431 0.9 0.00 3.4 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 > 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.3 0.41 1.4 0.24
GX 354-0 262.989 -33.835 354.302 -0.150 12.9 1.42 5.0 1.00
4U 1722-30 261.888 -30.802 356.320 +2.298 5.3 0.70 0.9 0.39
1A 1742-294 266.523 -29.515 359.559 -0.389 5.0 0.33 1.0 0.19
GX 3+1 266.983 -26.564 2.294 +0.794 22.3 0.52 2.8 0.27
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Revolution 0359: Observation start 2005-09-23 = MJD 53636
Total Observation GTI = 12321 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 5-1 270.286 -25.076 0.6 5.081 -1.018 20.9 0.33 63.0 0.0 0.00 0.0 4U 1700-377 255.986 -37.841 0.7 347.756 +2.176 29.8 0.59 50.7 10.7 0.45 23.7 GRS 1758-258 270.306 -25.735 0.8 4.517 -1.360 12.2 0.30 40.9 8.4 0.24 34.8 GX 354-0 262.987 -33.840 0.8 354.297 -0.152 13.8 0.32 42.6 2.9 0.26 11.1 Ginga 1826-24 277.357 -23.797 0.9 9.268 -6.079 17.6 0.52 34.1 6.1 0.40 15.2 GX 349+2 256.431 -36.410 1.0 349.112 +2.759 15.5 0.53 29.5 0.0 0.00 0.0 1E 1740.7-2942 265.963 -29.740 1.1 359.113 -0.092 8.0 0.28 28.7 4.9 0.23 21.2 GX 1+4 263.013 -24.739 1.0 1.945 +4.796 10.2 0.34 30.1 0.0 0.00 0.0 H 1820-303 275.900 -30.345 1.8 2.796 -7.892 6.1 0.40 15.4 0.0 0.00 0.0 GRO J1655-40 253.460 -39.821 2.3 344.981 +2.496 12.4 1.08 11.5 10.2 0.84 12.2 GX 9+1 270.397 -20.555 2.7 9.060 +1.131 3.9 0.40 9.7 0.0 0.00 0.0 KS 1741-293 266.211 -29.337 0.0 359.570 -0.065 2.2 0.00 8.2 0.0 0.00 0.0 IGR J17464-3213 266.567 -32.246 2.6 357.245 -1.841 2.8 0.28 10.1 2.2 0.23 9.6 SLX 1735-269 264.591 -26.992 3.1 0.807 +2.387 2.5 0.30 8.3 1.5 0.25 6.1 3A 1822-371 276.503 -37.098 3.4 356.877 -11.330 4.0 0.54 7.5 0.0 0.00 0.0 XTE J1739-285 265.020 -28.445 3.8 359.778 +1.291 1.9 0.28 6.6 0.0 0.00 0.0 GX 3+1 267.035 -26.566 3.2 2.315 +0.753 2.2 0.27 8.0 0.0 0.00 0.0 GRS 1734-292 264.347 -29.118 4.0 358.894 +1.432 1.8 0.28 6.4 0.0 0.00 0.0 GX 17+2 274.069 -14.024 4.1 16.473 +1.229 13.4 2.16 6.2 0.0 0.00 0.0 GX 13+1 273.550 -17.163 4.9 13.475 +0.172 3.9 0.77 5.1 0.0 0.00 0.0 SLX 1744-299_300 266.917 -30.039 5.5 359.289 -0.954 1.4 0.31 4.4 0.0 0.00 0.0 4U 1722-30 261.908 -30.740 5.5 356.381 +2.318 1.4 0.00 4.4 0.0 0.00 0.0 IGR J18048-1455 271.179 -14.968 4.9 14.296 +3.227 6.6 1.28 5.1 0.0 0.00 0.0 GRS 1747-312 267.775 -31.312 6.0 358.575 -2.241 1.1 0.28 4.1 0.0 0.00 0.0 V2400 Oph 258.209 -24.262 5.9 359.884 +8.687 1.7 0.40 4.1 0.0 0.00 0.0 IGR J17252-3616 261.350 -36.278 4.7 351.525 -0.387 2.1 0.39 5.2 0.0 0.00 0.0 IGR J18027-2016 270.641 -20.219 0.0 9.465 +1.098 1.6 0.00 3.7 0.0 0.00 0.0 IGR J17456-2901 266.400 -29.008 0.0 359.936 -0.033 0.9 0.00 3.7 0.0 0.00 0.0 1E 1743.1-2843 266.587 -28.679 0.0 0.303 -0.002 0.9 0.00 3.4 0.9 0.00 4.3 1A 1742-294 266.589 -29.502 0.0 359.601 -0.431 0.9 0.00 3.4 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 > 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.3 0.41 1.4 0.24 GX 354-0 262.989 -33.835 354.302 -0.150 12.9 1.42 5.0 1.00 4U 1722-30 261.888 -30.802 356.320 +2.298 5.3 0.70 0.9 0.39 1A 1742-294 266.523 -29.515 359.559 -0.389 5.0 0.33 1.0 0.19 GX 3+1 266.983 -26.564 2.294 +0.794 22.3 0.52 2.8 0.27
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