INTEGRAL Galactic Plane Scanning

******************* Very Preliminary results ******************

Revolution 1610: Observation start 2015-11-14T09:35 = MJD 57340.4
Total Observation GTI = 30502 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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
Vela X-1              135.520  -40.544 0.8  263.046   +3.932   26.3  0.60  43.7    6.3  0.40  15.6
H 0614+091             94.307   +9.173 0.0  200.858   -3.323    7.9  0.00   5.6    0.0  0.00   0.0

JEM-X

JEM-X1 and JEM-X2 significance mosaic images in 3-10 keV energy band.

Note: Sources labelled 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  
====================   =============   =============   =============   ============= 

Go back to the INTEGRAL Galactic Plane Scanning home page