SPIDER: a program for computing the positions of fibers for multi-objects spectroscopy.

Details SPIDER: a program for computing the positions of fibers for multi-objects spectroscopy. SPIDER: a program for computing the positions of fibers for multi-objects spectroscopy.

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pbeio..22...74s&link_type=abstract

Publications of the Beijing Astronomical Observatory, No. 22, p. 74 - 82

Physics

Optics

Fiber Optics: Control Systems

Scientific paper

This paper describes the program SPIDER, which computes x and y coordinates from right ascension and declination of objects listed in a file for positioning fibers on the star plate used at the Cassegrain focal plane of BAO 2.16 m telescope. In this program, the effects of atmospheric refraction, atmospheric dispersion, distortion at Cassegrain focal plane, air mass, temperature and pressure etc. have been considered.

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