OHS: OH-Airglow Suppressor for the Subaru Telescope
Author(s) -
Fumihide Iwamuro,
Kentaro Motohara,
Toshinori Maihara,
Ryuji Hata,
Takashi Harashima
Publication year - 2001
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/53.2.355
Subject(s) - physics , airglow , subaru telescope , spectrograph , sky , telescope , limiting magnitude , astronomy , infrared telescope , infrared , astrophysics , spectral line
This paper describes an OH-airglow Suppressor (OHS) for the infrared Nasmythfocus of the Subaru telescope. OHS has the capability of eliminating 224airglow-lines in the $J$- and $H$-bands, which are major sources of backgroundradiation at near-infrared wavelengths up to 2 $\mu$m. Specifically, it is apre-optics system installed between the telescope and an infraredcamera/spectrograph (CISCO). The suppressor reduces sky background emissions to1/25 and its throughput is 40%. As a result, the S/N gain achieved with OHS ismore than 1 mag compared to the typical spectroscopic approach. The limitingmagnitude measured during a test observing run was found to be $H$ = 21.1 mag($\lambda/\Delta\lambda$ = 210, S/N = 5) in the standard 4000 s exposuresequence.Comment: 6 pages, 9 figures. Accepted for publication in PASJ(2001
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