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

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)