Published September 19, 2002
| Version v1
Report
Visible Imaging Fourier Transform Spectrometer: Design and Calibration
Description
We present details of the design, operation and calibration of an astronomical visible-band imaging Fourier transform spectrometer (IFTS). This type of instrument produces a spectrum for every pixel in the field of view where the spectral resolution is flexible. The instrument is a dual-input/dual-output Michelson interferometer coupled to the 3.5 meter telescope at the Apache Point Observatory. Imaging performance and interferograms and spectra from calibration sources and standard stars are discussed
Availability note (English)
Available from PURL: https://www.osti.gov/servlets/purl/15002522-mm3WJF/native/Additional details
Identifiers
Publishing Information
- Imprint Pagination
- 4.7 Megabytes
- Report number
- UCRL-JC--150957
Conference
- Title
- SPIE Astronomical Telescopes and Instrumentation
- Dates
- 22-28 Aug 2002
- Place
- Waikoloa, HI (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 35053389
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Resource subtype / Literary indicator
- Conference, Non-conventional Literature
- Descriptors DEI
- CALIBRATION; DESIGN; FOURIER TRANSFORM SPECTROMETERS; ISOCHRONOUS CYCLOTRONS; MICHELSON INTERFEROMETER; PERFORMANCE; RESOLUTION; SPECTRA; STARS; TELESCOPES
- Descriptors DEC
- ACCELERATORS; CYCLIC ACCELERATORS; CYCLOTRONS; INTERFEROMETERS; MEASURING INSTRUMENTS; SPECTROMETERS
Optional Information
- Contract/Grant/Project number
- W-7405-ENG-48
- Funding organization
- US Department of Energy (United States)