Swinyard, Bruce M., Ade, Peter A. R. ![]() |
Official URL: http://dx.doi.org/10.1117/12.393967
Abstract
The SPIRE instrument for the FIRST mission will consist of a three band imaging submillimeter photometer and a two band imaging Fourier Transform Spectrometer (FTS) optimized for the 200 - 400 micrometers range, and with extended coverage out to 670 micrometers. The FTS will be used for follow-up spectroscopic studies of objects detected in photometric surveys by SPIRE and other facilities, and to perform medium resolving power (R approximately 500 at 250 micrometers ) imaging spectroscopy on galactic and nearby extra-galactic sources.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | The International Society for Optical Engineering |
ISBN: | 9780819436382 |
ISSN: | 0277-786X |
Last Modified: | 27 Oct 2022 09:01 |
URI: | https://orca.cardiff.ac.uk/id/eprint/64135 |
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