An Optical Design for an Antarctic 2 m Telescope with a Near IR Imager
Publications of the Astronomical Society of Australia
19(3) 301 - 305
Published: 31 May 2002
Abstract
A study has been made of the optical performance to be expected from an Antarctic Ritchey Chrétien telescope with a 2 m diameter primary mirror imaging directly onto a detector array in the K and L infrared windows. Near diffraction limited performance is provided across a flat 30 arcmin diameter field by compensating the astigmatism and field curvature with a meniscus lens which also serves as the Dewar window. With baffling inside and Narcissus mirrors outside the Dewar, extraneous radiation can be kept to a low level.Keywords: telescopes — infrared: general — instrumentation: photometers — methods: observational
https://doi.org/10.1071/AS01071
© ASA 2002