Infrared Spectroscopy In Astronomy

J. R. Houck

doi:10.1117/12.931943

27 July 1981 Infrared Spectroscopy In Astronomy

J. R. Houck

Proceedings Volume 0280, Infrared Astronomy: Scientific/Military Thrusts and Instrumentation; (1981) https://doi.org/10.1117/12.931943
Event: 1981 Technical Symposium East, 1981, Washington, D.C., United States

Abstract

The use of infrared spectroscopy in astronomy has increased dramatically in the past ten years. The broad design considerations are discussed in terns of wavelength coverage and resolution. Three rough resolution ranges,VAA % 100, 1000 and 10000, are identified in which various types of astronomical problems can be studied. Numerous existing systems are briefly discussed and references are given to more complete descriptions.

Citation Download Citation

J. R. Houck "Infrared Spectroscopy In Astronomy", Proc. SPIE 0280, Infrared Astronomy: Scientific/Military Thrusts and Instrumentation, (27 July 1981); https://doi.org/10.1117/12.931943

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE

Includes PDF, HTML & Video, when available