Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Analysis of the accuracy characteristics of spectroscopic observations

Not Accessible

Your library or personal account may give you access

Abstract

This paper discusses the main causes of the reduction of the accuracy of spectroscopic observations made with orbital and ground-based telescopes. An observational method is proposed that makes it possible to maintain high spectral resolution during long exposures. The method has been tested under terrestrial conditions.

PDF Article
More Like This
Special configuration of a very large Schmidt telescope for extensive astronomical spectroscopic observation

Shou-guan Wang, Ding-qiang Su, Yao-quan Chu, Xiangqun Cui, and Ya-nan Wang
Appl. Opt. 35(25) 5155-5161 (1996)

Airborne infrared astronomical observations by Fourier transform spectroscopy

Harold P. Larson
Appl. Opt. 17(9) 1352-1359 (1978)

Spectroscopic photoelectric imaging Fabry-Perot interferometer: its development and preliminary observational results

W. Hayden Smith, Joachim Born, William D. Cochran, and Jack Gelfand
Appl. Opt. 15(3) 717-724 (1976)

Cited By

You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All Rights Reserved