The case for OH suppression at near-infrared wavelengths

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 1, 2008, Pages 47-64

  Ellis, S C ^a   Bland Hawthorn, J ^b  

^a ANGLO AUSTRALIAN OBSERVATORY   (Australia)

^b UNIVERSITY OF SYDNEY   (Australia)

Author keywords

Atmospheric effects; Early Universe; Infrared: general; Instrumentation: miscellaneous

Indexed keywords

ADAPTIVE OPTICS; ASTROPHYSICS; DISPERSION (WAVES); FIBER BRAGG GRATINGS; GALAXIES; INFRARED DEVICES; OBJECT DETECTION;

ATMOSPHERIC EFFECTS; EARLY UNIVERSE; EMISSION LINES; INFRARED ASTRONOMY; INFRARED: GENERAL; INSTRUMENTATION: MISCELLANEOUS; NEAR INFRARED; NEAR-INFRARED; NEAR-INFRARED WAVELENGTH; SPECTRA'S;

LIGHT;

EID: 42449113462     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13021.x     Document Type: Article

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