HIPO - A high-speed imaging photometer for occultations

E. W. Dunham*, J. L. Elliot, T. A. Bida, B. W. Taylor

*Corresponding author for this work

Research output: Contribution to journalConference articlepeer-review

37 Citations (Scopus)

Abstract

HIPO is a special purpose instrument for SOFIA, the Stratospheric Observatory For Infrared Astronomy. It is a high-speed, imaging photometer that will be used for a variety of time-resolved precise photometry observations, including stellar occultations by solar system objects and transits by extrasolar planets. HIPO has two independent CCD detectors and can also co-mount with FLITECAM, an InSb imager and spectrometer, making simultaneous photometry at three wavelengths possible. HIPO's flexible design and high-speed imaging capability make it well suited to carry out initial test observations on the completed SOFIA system, and to this end a number of additional features have been incorporated. Earlier papers have discussed the design requirements and optical design of HIPO. This paper provides an overview of the instrument, describes the instrument's features, and reviews the actual performance, in most areas, of the completed instrument.

Original languageEnglish
Pages (from-to)592-603
Number of pages12
JournalProceedings of SPIE - The International Society for Optical Engineering
Volume5492
Issue numberPART 1
DOIs
Publication statusPublished - 2004
Externally publishedYes
EventGround-based Instrumentation for Astronomy - Glasgow, United Kingdom
Duration: 21 Jun 200425 Jun 2004

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