ADVANCED WIDE-FIELD BROAD-PASSBAND REFRACTING FIELD CORRECTORS FOR LARGE TELESCOPES.

H. W. Epps; J. R.P. Angel; E. Anderson

doi:10.1017/s0252921100108656

ADVANCED WIDE-FIELD BROAD-PASSBAND REFRACTING FIELD CORRECTORS FOR LARGE TELESCOPES.

H. W. Epps, J. R.P. Angel, E. Anderson

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Scopus citations

Abstract

This paper describes a preliminary 30-arcmin prime focus (f/2. 0) refracting field corrector system for the University of California Ten-Meter Telescope (UC TMT), a compact 40-arcmin internal Cassegrain (f/1. 75 hyperbola to f/5. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector, suitable for imaging and multi-object spectroscopy at the UC TMT, three 60-arcmin external Cassegrain correctors for 300-inch f/1. 8 and f/2. 0 parabolic primary mirrors and a (300-inch) 40-arcmin external Cassegrain (f/1. 0 parabola to f/4. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector with ADC.

Original language	English (US)
Title of host publication	Unknown Host Publication Title
Publisher	European Southern Observatory (IAU Colloquium n 79), Garching
Pages	519-548
Number of pages	30
ISBN (Print)	3923524196, 9783923524198
DOIs	https://doi.org/10.1017/s0252921100108656
State	Published - 1984
Externally published	Yes

ASJC Scopus subject areas

General Engineering

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10.1017/s0252921100108656

Cite this

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title = "ADVANCED WIDE-FIELD BROAD-PASSBAND REFRACTING FIELD CORRECTORS FOR LARGE TELESCOPES.",

abstract = "This paper describes a preliminary 30-arcmin prime focus (f/2. 0) refracting field corrector system for the University of California Ten-Meter Telescope (UC TMT), a compact 40-arcmin internal Cassegrain (f/1. 75 hyperbola to f/5. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector, suitable for imaging and multi-object spectroscopy at the UC TMT, three 60-arcmin external Cassegrain correctors for 300-inch f/1. 8 and f/2. 0 parabolic primary mirrors and a (300-inch) 40-arcmin external Cassegrain (f/1. 0 parabola to f/4. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector with ADC.",

author = "Epps, {H. W.} and Angel, {J. R.P.} and E. Anderson",

year = "1984",

doi = "10.1017/s0252921100108656",

language = "English (US)",

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publisher = "European Southern Observatory (IAU Colloquium n 79), Garching",

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AU - Angel, J. R.P.

AU - Anderson, E.

PY - 1984

Y1 - 1984

N2 - This paper describes a preliminary 30-arcmin prime focus (f/2. 0) refracting field corrector system for the University of California Ten-Meter Telescope (UC TMT), a compact 40-arcmin internal Cassegrain (f/1. 75 hyperbola to f/5. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector, suitable for imaging and multi-object spectroscopy at the UC TMT, three 60-arcmin external Cassegrain correctors for 300-inch f/1. 8 and f/2. 0 parabolic primary mirrors and a (300-inch) 40-arcmin external Cassegrain (f/1. 0 parabola to f/4. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector with ADC.

AB - This paper describes a preliminary 30-arcmin prime focus (f/2. 0) refracting field corrector system for the University of California Ten-Meter Telescope (UC TMT), a compact 40-arcmin internal Cassegrain (f/1. 75 hyperbola to f/5. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector, suitable for imaging and multi-object spectroscopy at the UC TMT, three 60-arcmin external Cassegrain correctors for 300-inch f/1. 8 and f/2. 0 parabolic primary mirrors and a (300-inch) 40-arcmin external Cassegrain (f/1. 0 parabola to f/4. 0) broad-passband ( lambda 3300Angstrom to lambda 1. 0 mu ) corrector with ADC.

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ER -

ADVANCED WIDE-FIELD BROAD-PASSBAND REFRACTING FIELD CORRECTORS FOR LARGE TELESCOPES.

Abstract

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