Physics – Optics
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..881m&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 690, p. 881-893.
Physics
Optics
129
Astronomical Observatories, Cassegrain Optics, Design Analysis, Echelette Gratings, Absorption Spectra, Calibrating, Charge Coupled Devices, Collimators, Late Stars, Spectral Line Width, Telescopes
Scientific paper
We describe the design, construction, and performance of an efficient new flexure-compensated Cassegrain echelle spectrograph for the 2.1-m Struve reflector at McDonald Observatory. The instrument has a resolving power of 60,000 for two CCD pixels (for a reciprocal velocity dispersion of 2.5 km/s per pixel) and provides continuous wavelength coverage for less than 8000 A using a thinned backside-illuminated Reticon 1200 x 400 CCD detector. The mechanical design of the Cassegrain-mounted spectrograph incorporates a unique cantilevered counterweight system designed to drastically reduce the effects of gravitational flexure. In spite of the large physical size of the Cassegrain instrument, worst-case flexure shifts over 60 (4 hr) of telescope motion are less than 1/2 pixel and are typically on the order of 0.2 pixels or less from all sources.
Booth John
Boyd David
McCarthy James K.
Sandiford Brendan A.
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