Revolution 1611: Observation start 2015-11-18T01:28 = MJD 57344.062
Total Observation GTI = 44539 seconds
ISGRI


ISGRI significance mosaic images. Top: ISGRI 18-40 keV. Bottom: 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 OSA9
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 176 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 88 cps ) where available.
ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)
Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
Cyg X-1 299.596 +35.199 0.4 71.335 +3.062 63.0 0.49 128.5 32.6 0.31 104.2
Cyg X-3 308.112 +40.948 0.6 79.840 +0.692 22.3 0.36 61.2 5.9 0.23 25.1
GRS 1915+105 288.812 +10.939 1.1 45.366 -0.235 10.4 0.38 27.2 0.0 0.00 0.0
H 1907+097 287.387 +9.812 2.5 43.718 +0.486 4.2 0.40 10.5 0.0 0.00 0.0
4U 1909+07 287.698 +7.580 3.9 41.880 -0.817 2.8 0.43 6.5 0.0 0.00 0.0
JEM-X
Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the source position is done), with j_ima_src_locator
in 3-10 keV energy band.
Source Name RA dec A(cps) sigma
==================== ============= ============= ============= =============
Cyg X-3 3.0810730E+02 4.0948093E+01 1.0638587E-02 4.6469776E+01
IGR J21247+5058 3.2119598E+02 5.0971348E+01 4.5894849E-04 5.9397426E+00
GRS 1915+105 2.8879907E+02 1.0946445E+01 9.1042027E-02 2.5733578E+02
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