HIRDES-The High-Resolution Double-Echelle Spectrograph for WSO-UV

Details HIRDES-The High-Resolution Double-Echelle Spectrograph for WSO-UV HIRDES-The High-Resolution Double-Echelle Spectrograph for WSO-UV

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1135..338w&link_type=abstract

FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic

Computer Science

Databases

Space-Based Ultraviolet, Optical, And Infrared Telescopes, Astronomical Observations, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

We introduce the High-Resolution Double-Echelle Spectrograph (HIRDES), which is planned to be the main instrument for the World Space Observatory Ultraviolet (WSO-UV), a 1.7 m UV telescope. Within HIRDES the 102-310 nm spectral band is split to feed two echelle spectrographs covering the UV range 174-310 nm and the vacuum-UV range 102-176 nm with high spectral resolution (R>50000). The technical concept is based on the heritage of two previous ORFEUS SPAS missions. We describe results of the phase-B1 development activities.

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