Share Email Print

Proceedings Paper

Echelle Spectroscopy With A Charge-Coupled Device (CCD)
Author(s): Donald G. York; Edward B. Jenkins; Paul Zucchino; John L. Lowrance; Donald Long; Antoinette Songaila
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

Observations made with an RCA thinned back illuminated CCD on the echelle spectrograph of the Kitt Peak 4-meter Mayall telescope are discussed. With emphasis on interstellar line measurements in bright and faint background sources, the system efficiency, spectrum format, achieved signal-to-noise, interference fringes, and overall performance are discussed. A signal-to-noise of > 100/1 has been achieved at 0.2 Å resolution in two hours on a 13.2 mag star. Projected CCD improvements should yield signal-to-noise ratios of 20/1 for 18th magnitude objects (V) in 2 hours. With appropriate gratings, 1500 Å of continuous spectrum can be obtained.

Paper Details

Date Published: 1 January 1981
PDF: 6 pages
Proc. SPIE 0290, Solid-State Imagers for Astronomy, (1 January 1981); doi: 10.1117/12.965861
Show Author Affiliations
Donald G. York, Princeton University Observatory (United States)
Edward B. Jenkins, Princeton University Observatory (United States)
Paul Zucchino, Princeton University Observatory (United States)
John L. Lowrance, Princeton University Observatory (United States)
Donald Long, Princeton University Observatory (United States)
Antoinette Songaila, Princeton University Observatory (United States)

Published in SPIE Proceedings Vol. 0290:
Solid-State Imagers for Astronomy
John C. Geary; David W. Latham, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?