Focus and alignment of the Space Surveillance Telescope: Procedures and year 2 performance results

Deborah Freedman Woods, Richard L. Lambour, Walter J. Faccenda, Jessica D. Ruprecht, Eric C. Pearce, Ronak Y. Shah, Mark E. Cornell

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Scopus citations

Abstract

The Space Surveillance Telescope (SST) is a three-mirror Mersenne-Schmidt telescope with a 3.5 m primary mirror that is designed for deep, wide-area sky surveys. The SST design incorporates a camera with charge-coupled devices (CCDs) on a curved substrate to match the telescope's inherent field curvature, capturing a large field-of-view (6 square degree) with good optical performance across the focal surface. The unique design enables a compact mount construction for agile pointing, contributing to survey efficiency. However, the optical properties make the focus and alignment challenging due to an inherently small depth of focus and the additional degrees of freedom that result from having a powered tertiary mirror. Adding to the challenge, the optical focus and alignment of the mirrors must be accomplished without a dedicated wavefront sensor. Procedures created or adapted for use at the SST have enabled a successful campaign for focus and alignment, based on a five-step iterative process to (1) position the tertiary mirror along the optical axis to reduce defocus; (2) reduce spherical aberration by a coordinate move of the tertiary and secondary mirrors; (3) measure the higher order aberrations including astigmatism and coma; (4) associate the measured aberrations with the predictions of optical ray-tracing analysis; and (5) apply the mirror corrections and repeat steps 1-4 until optimal performance is achieved (Woods et al. 2013). A set of predicted mirror motions are used to maintain system performance across changes in telescope elevation pointing and in temperature conditions, both nightly and seasonally. This paper will provide an overview of the alignment procedure developed for the SST and will report on the focus performance through the telescope's second year, including lessons learned over the course of operation.

Original languageEnglish (US)
Title of host publicationObservatory Operations
Subtitle of host publicationStrategies, Processes, and Systems V
EditorsAlison B. Peck, Chris R. Benn, Robert L. Seaman
PublisherSPIE
ISBN (Electronic)9780819496171
DOIs
StatePublished - 2014
Externally publishedYes
EventObservatory Operations: Strategies, Processes, and Systems V - Montreal, Canada
Duration: Jun 25 2014Jun 27 2014

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume9149
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Other

OtherObservatory Operations: Strategies, Processes, and Systems V
Country/TerritoryCanada
CityMontreal
Period6/25/146/27/14

Keywords

  • Focus
  • Telescope alignment
  • Wavefront sensing

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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