LEDAS  
Leicester Database and Archive Service
 
Mission
    Description
Products
    Databases
Raw Data
    Archive
Analysis Software
    Archive
Ginga Information
Ginga Gallery
Related Sites
Databases
GINGALAC
GINGABGD
GINGAFRF
GINGALOG
GINGAMODE
GINGARAW
View Ginga DBs
Line
Footer
e-mail

Gain

To provide an indication of the gain, for each observation, the 10-35 keV pulse height spectra, which include the collimator silver line, from the top- and mid-layers (all detectors combined to provide good signal-to-noise) were fitted with a model consisting of a second order polynominal plus Gaussian emission line. The best-fit energy of the Gaussian is given in the database table and is accurate to approximately 0.5 keV. In addition, four plots were produced during the extraction of data. These show the pulse height spectra from 20 to 35 keV for the top- and mid-layers and for each detector in use (two detectors per plot; see table 1). The plots can be used within QDP (Tennant 1991), which is part of the XANADU suite of software, to verify that the silver line is at the expected energy of 22.1 keV for individual layers. Individual plots may be missing if the detectors were excluded during the pipeline processing (e.g. because of electronic noise on detectors 5 & 6).


[] [Previous: Data Selection within Sortac] [Back to Pipeline Processing]
 
HOME
SEARCH
SERVICES INFO SOFTWARE ViZieR BLASTA DSS
ARCHIVES ASCA CHANDRA GINGA ROSAT ARNIE