Share Email Print

Proceedings Paper

High efficiency CCD detectors at UV wavelengths
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

The Faint Intergalactic Redshifted Emission Balloon (FIREBall) is a NASA/CNES balloon-borne ultraviolet multi-object spectrograph designed to observe the diffuse gas around galaxies (the circumgalactic medium) via line emission redshifted to ~205 nm. FIREBall uses a ultraviolet-optimized delta doped e2v CCD201 with a custom designed high efficiency five layer anti-reflection coating. This combination achieves very high quantum efficiency (QE) and photon-counting capability, a first for a CCD detector in this wavelength range. We also present new work on red blocking mirror coatings to reduce red leak.

Paper Details

Date Published: 24 July 2014
PDF: 11 pages
Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91442X (24 July 2014); doi: 10.1117/12.2056204
Show Author Affiliations
Erika T. Hamden, Columbia Univ. (United States)
April D. Jewell, Jet Propulsion Lab. (United States)
Samuel Gordon, Columbia Univ. (United States)
John Hennessy, Jet Propulsion Lab. (United States)
Michael E. Hoenk, Jet Propulsion Lab. (United States)
Shouleh Nikzad, Jet Propulsion Lab. (United States)
David Schiminovich, Columbia Univ. (United States)
D. Christopher Martin, California Institute of Technology (United States)

Published in SPIE Proceedings Vol. 9144:
Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz, 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?