XDSPRES: CL-based package for Reducing OSIRIS Cross-dispersed Spectra

Details XDSPRES: CL-based package for Reducing OSIRIS Cross-dispersed Spectra XDSPRES: CL-based package for Reducing OSIRIS Cross-dispersed Spectra

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ascl.soft07010r&link_type=abstract

Astrophysics Source Code Library, record ascl:1107.010

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a description of the CL-based package XDSPRES, which aims at being a complete reducing facility for cross-dispersed spectra taken with the Ohio State Infrared Imager/Spectrometer, as installed at the SOAR telescope. This instrument provides spectra in the range between 1.2um and 2.35um in a single exposure, with resolving power of R ~ 1200. XDSPRES consists of two tasks, namely xdflat and doosiris. The former is a completely automated code for preparing normalized flat field images from raw flat field exposures. Doosiris was designed to be a complete reduction pipeline, requiring a minimum of user interaction. General steps towards a fully reduced spectrum are explained, as well as the approach adopted by our code.

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