The Optical Design of the 40-in Telescope and of the Irenee DuPont Telescope at Las Campanas Observatory, Chile
I. S. Bowen, A. H. Vaughan
Abstract
I. S. Bowen, A. H. Vaughan
Abstract
The optical specifications of two astronomical telescopes designed to permit wide-field photography with critical definition are presented and compared. The 40-in. (1.016-m) and DuPont 100-in. (2.54-m) telescopes use modifications of the Ritchey-Chretién design with Gascoigne correctors. By avoiding the need for field flatteners through choice of mirrors yielding zero Petzval sum (40-in. telescope) or bending of photographic plates to a moderate field curvature (100-in. telescope), it was possible to achieve monochromatic images of ? to (1/4) sec of arc over fields of 3 degrees and 2.1 degrees , respectively.
OpenAlex reports 272 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The optical specifications of two astronomical telescopes designed to permit wide-field photography with critical definition are presented and compared. The 40-in. (1.016-m) and DuPont 100-in. (2.54-m) telescopes use modifications of the Ritchey-Chretién design with Gascoigne correctors. By avoiding the need for field flatteners through choice of mirrors yielding zero Petzval sum (40-in. telescope) or bending of photographic plates to a moderate field curvature (100-in. telescope), it was possible to achieve monochromatic images of ? to (1/4) sec of arc over fields of 3 degrees and 2.1 degrees , respectively.
Key concepts: Telescope, Optics, Observatory, Optical telescope, Reflecting telescope, Physics, X-ray telescope, Active optics