Implementation of the Temperature-Dependent Dark Correction in CalnicA

Details Implementation of the Temperature-Dependent Dark Correction in CalnicA Implementation of the Temperature-Dependent Dark Correction in CalnicA

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nicm.rept....5j&link_type=abstract

Instrument Science Report NICMOS 2002-005 , 14 pages

Other

Hubble Space Telescope, Hst, Space Telescope Science Institute, Nicmos

Scientific paper

The pipeline implementation of the temperature-dependent dark correction, previously only available to users as a WWW tool, is described. The algorithm used to generate the darksisdescribed,alongwithadescriptionofhowtheIDLcodeanddatathatareusedin the WWW tool were incorporated into the usual HST pipeline model of code+reference files. This implementation necessitated the creation of a new reference file type: the Tem- perature-Dependent Dark (TDD) file. The design of this file type allowed many of the hardconstantstoberemovedfromthecodeandputintothereferencefiles,allowingmore convenient and flexible updating of the calibration parameters, if necessary.

Affiliated with

Also associated with

No associations

Rating

Implementation of the Temperature-Dependent Dark Correction in CalnicA does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Implementation of the Temperature-Dependent Dark Correction in CalnicA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Implementation of the Temperature-Dependent Dark Correction in CalnicA will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1167059