Paper
1 January 1981 Echelle Spectroscopy With A Charge-Coupled Device (CCD)
Donald G. York, Edward B. Jenkins, Paul Zucchino, John L. Lowrance, Donald Long, Antoinette Songaila
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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.
© (1981) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Donald G. York, Edward B. Jenkins, Paul Zucchino, John L. Lowrance, Donald Long, and Antoinette Songaila "Echelle Spectroscopy With A Charge-Coupled Device (CCD)", Proc. SPIE 0290, Solid-State Imagers for Astronomy, (1 January 1981); https://doi.org/10.1117/12.965861
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Cited by 6 scholarly publications and 1 patent.
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KEYWORDS
Charge-coupled devices

Spectrographs

Stars

Quartz

Signal to noise ratio

CCD cameras

Head

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