Revolution 2314b: Observation start 2020-12-30T02:12 = MJD 59213.093
Total Observation GTI = 74161 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 OSA10.2
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
3A 0114+650 19.500 +65.300 2.6 125.704 +2.571 1.3 0.13 10.0 0.0 0.00 0.0
JEM-X Detected Sources 3-10 keV
Sources were detected 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 j_ima_src_locator
in 3-10 keV energy band.
/
Source Name RA dec A(cps) sigma
==================== ============= ============= ============= =============
Cas A 3.5084616E+02 5.8825695E+01 1.2593301E-03 2.7319983E+01
1H 2214+589 3.3985629E+02 6.1265472E+01 7.8526058E-04 7.3670769E+00
3A 0114+650 1.9518957E+01 6.5297279E+01 1.3520607E-03 3.3780994E+01
Gam Cas 1.4181215E+01 6.0718334E+01 5.4317072E-04 1.5006265E+01
1ES 0033+595 8.9547195E+00 5.9832493E+01 2.4384930E-04 6.1606350E+00
Go back to the INTEGRAL Galactic Plane Scanning home page