FUSE calibration pipeline version 3.0

Details FUSE calibration pipeline version 3.0 FUSE calibration pipeline version 3.0

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..348..550g&link_type=abstract

Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE ASP Conference Series, Vol. 348, Proceedings of the Confe

Astronomy and Astrophysics

Astrophysics

Scientific paper

The latest version (3.0) of the calibration pipeline for the Far Ultraviolet Spectroscopic Explorer (FUSE) is considerably faster, easier to maintain and more flexible for the end users than the older versions. It represents a major design change. Data are stored as a photon events (time of arrival, location, pulse height ...) list throughout the pipeline. This allows time dependent corrections for such effects as spacecraft jitter and mirror or grating motions. Moreover users can now select and extract subsets of the data without rerunning the pipeline.

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