ARCES: an echelle spectrograph for the Astrophysical Research Consortium (ARC) 3.5m telescope

被引：85

作者：

Wang, S ^{[1
]}

Hildebrand, RH ^{[1
]}

Hobbs, LM ^{[1
]}

Heimsath, SJ ^{[1
]}

Kelderhouse, GA ^{[1
]}

Loewenstein, RF ^{[1
]}

Lucero, S ^{[1
]}

Rockosi, CM ^{[1
]}

Sandford, DB ^{[1
]}

Sundwall, JL ^{[1
]}

Thorburn, JA ^{[1
]}

York, DG ^{[1
]}

机构：

[1] Flight Syst Inc, Sugar Grove, IL 60554 USA

来源：

INSTRUMENT DESIGN AND PERFORMANCE FOR OPTICAL/INFRARED GROUND-BASED TELESCOPES, PTS 1-3 | 2003年 / 4841卷

关键词：

D O I：

10.1117/12.461447

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

A new echelle spectrograph was commissioned in 1999 for the ARC 3.5 meter telescope. The key features of the instrument are that it has a resolution of 9 km/sec, limited by the pixel size of the CCD; has no moving parts behind the slit during observation; provides complete spectral coverage,from 3200A to 10000A, limited by the prism cross disperser material on the blue side and by the CCD sensitivity on the red side; provides blazeless spectra; achieves S/N>3000; and is remotely operable. The instrument is being used for studies of abundances in stars and for a large survey of diffuse interstellar bands.

引用

页码：1145 / 1156

页数：12

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