INTEGRAL Galactic Bulge MonitoringRevolution 0420: Observation start 2006-03-23 = MJD 53817
Total Observation GTI = 8594 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
Ginga 1826-24 277.360 -23.808 1.0 9.259 -6.087 16.8 0.56 30.1 6.6 0.45 14.8
GRS 1758-258 270.299 -25.743 1.1 4.507 -1.359 9.6 0.35 27.4 6.6 0.29 22.6
GX 354-0 262.990 -33.825 1.2 354.311 -0.146 9.5 0.39 24.6 2.1 0.32 6.4
GX 1+4 263.013 -24.747 1.3 1.938 +4.791 9.1 0.39 23.7 0.0 0.00 0.0
4U 1700-377 255.991 -37.826 1.4 347.771 +2.182 15.2 0.75 20.2 2.9 0.59 4.8
GX 5-1 270.282 -25.065 1.6 5.089 -1.009 6.7 0.37 18.2 0.0 0.00 0.0
GX 349+2 256.451 -36.403 1.8 349.127 +2.750 10.0 0.63 15.7 0.0 0.00 0.0
H 1820-303 275.906 -30.358 1.8 2.786 -7.902 7.3 0.48 15.2 0.0 0.00 0.0
1A 1742-294 266.529 -29.488 2.4 359.585 -0.380 4.1 0.38 11.0 0.0 0.00 0.0
GX 17+2 273.990 -14.044 2.4 16.418 +1.287 24.2 2.16 11.2 0.0 0.00 0.0
1A 1743-288 266.696 -28.891 3.6 0.171 -0.194 2.4 0.34 7.0 1.4 0.30 4.9
XTE J1817-330 274.435 -33.007 2.7 359.829 -7.993 4.6 0.47 9.9 1.8 0.38 4.7
3A 1822-371 276.451 -37.102 2.9 356.855 -11.294 6.3 0.71 9.0 0.0 0.00 0.0
4U 1722-30 261.853 -30.805 2.9 356.301 +2.322 3.2 0.35 9.0 0.0 0.00 0.0
GX 3+1 267.058 -26.565 3.6 2.327 +0.736 2.7 0.38 7.0 0.0 0.00 0.0
OAO 1657-415 255.132 -41.689 3.4 344.310 +0.341 12.3 1.64 7.5 0.0 0.00 0.0
SLX 1735-269 264.567 -26.982 4.0 0.804 +2.410 2.4 0.38 6.3 0.0 0.00 0.0
Swift J174535.5-2901 266.338 -28.982 0.0 359.930 +0.026 1.8 0.00 5.1 0.0 0.00 0.0
1H 1746-370 267.624 -36.987 5.2 353.616 -5.021 2.5 0.00 4.7 0.0 0.00 0.0
GX 9+1 270.376 -20.629 3.8 8.985 +1.111 2.9 0.43 6.7 0.0 0.00 0.0
SLX 1744-299_300 266.808 -30.052 0.0 359.228 -0.880 1.6 0.00 4.7 0.0 0.00 0.0
Oph Cluster 258.144 -23.349 5.0 0.606 +9.260 2.4 0.48 4.9 0.0 0.00 0.0
AX J1749.1-2733 267.272 -27.584 0.0 1.553 +0.047 1.3 0.00 4.0 0.0 0.00 0.0
GRS 1734-292 264.374 -29.076 5.7 358.943 +1.435 1.6 0.38 4.3 0.0 0.00 0.0
XB 1832-330 278.859 -33.010 5.8 1.487 -11.323 2.6 0.62 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 10.7 1.83 2.9 1.10
GX 3+1 266.983 -26.564 2.294 +0.794 24.4 0.63 4.4 0.33
GX 5-1 270.284 -25.079 5.077 -1.019 99.6 2.14 9.1 0.90
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Revolution 0420: Observation start 2006-03-23 = MJD 53817
Total Observation GTI = 8594 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== Ginga 1826-24 277.360 -23.808 1.0 9.259 -6.087 16.8 0.56 30.1 6.6 0.45 14.8 GRS 1758-258 270.299 -25.743 1.1 4.507 -1.359 9.6 0.35 27.4 6.6 0.29 22.6 GX 354-0 262.990 -33.825 1.2 354.311 -0.146 9.5 0.39 24.6 2.1 0.32 6.4 GX 1+4 263.013 -24.747 1.3 1.938 +4.791 9.1 0.39 23.7 0.0 0.00 0.0 4U 1700-377 255.991 -37.826 1.4 347.771 +2.182 15.2 0.75 20.2 2.9 0.59 4.8 GX 5-1 270.282 -25.065 1.6 5.089 -1.009 6.7 0.37 18.2 0.0 0.00 0.0 GX 349+2 256.451 -36.403 1.8 349.127 +2.750 10.0 0.63 15.7 0.0 0.00 0.0 H 1820-303 275.906 -30.358 1.8 2.786 -7.902 7.3 0.48 15.2 0.0 0.00 0.0 1A 1742-294 266.529 -29.488 2.4 359.585 -0.380 4.1 0.38 11.0 0.0 0.00 0.0 GX 17+2 273.990 -14.044 2.4 16.418 +1.287 24.2 2.16 11.2 0.0 0.00 0.0 1A 1743-288 266.696 -28.891 3.6 0.171 -0.194 2.4 0.34 7.0 1.4 0.30 4.9 XTE J1817-330 274.435 -33.007 2.7 359.829 -7.993 4.6 0.47 9.9 1.8 0.38 4.7 3A 1822-371 276.451 -37.102 2.9 356.855 -11.294 6.3 0.71 9.0 0.0 0.00 0.0 4U 1722-30 261.853 -30.805 2.9 356.301 +2.322 3.2 0.35 9.0 0.0 0.00 0.0 GX 3+1 267.058 -26.565 3.6 2.327 +0.736 2.7 0.38 7.0 0.0 0.00 0.0 OAO 1657-415 255.132 -41.689 3.4 344.310 +0.341 12.3 1.64 7.5 0.0 0.00 0.0 SLX 1735-269 264.567 -26.982 4.0 0.804 +2.410 2.4 0.38 6.3 0.0 0.00 0.0 Swift J174535.5-2901 266.338 -28.982 0.0 359.930 +0.026 1.8 0.00 5.1 0.0 0.00 0.0 1H 1746-370 267.624 -36.987 5.2 353.616 -5.021 2.5 0.00 4.7 0.0 0.00 0.0 GX 9+1 270.376 -20.629 3.8 8.985 +1.111 2.9 0.43 6.7 0.0 0.00 0.0 SLX 1744-299_300 266.808 -30.052 0.0 359.228 -0.880 1.6 0.00 4.7 0.0 0.00 0.0 Oph Cluster 258.144 -23.349 5.0 0.606 +9.260 2.4 0.48 4.9 0.0 0.00 0.0 AX J1749.1-2733 267.272 -27.584 0.0 1.553 +0.047 1.3 0.00 4.0 0.0 0.00 0.0 GRS 1734-292 264.374 -29.076 5.7 358.943 +1.435 1.6 0.38 4.3 0.0 0.00 0.0 XB 1832-330 278.859 -33.010 5.8 1.487 -11.323 2.6 0.62 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 10.7 1.83 2.9 1.10 GX 3+1 266.983 -26.564 2.294 +0.794 24.4 0.63 4.4 0.33 GX 5-1 270.284 -25.079 5.077 -1.019 99.6 2.14 9.1 0.90
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