Suppression of the near-infrared OH night-sky lines with fibre Bragg gratings - first results
Ellis, S C; Bland-Hawthorn, Joss; Lawrence, J; Horton, A J; Trinh, C; Leon-Saval, S G; Shortridge, Keith; Bryant, J.; Case, S; Colless, Matthew; Couch, Warrick; Freeman, Kenneth; Schmidt, Brian; Lawrence, J S; Gers, L; Lee, Steve; Miziarski, Stan; Zheng, Jessica
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric emission from hydroxyl molecules. We have built and commissioned a new instrument, the Gemini Near-infrared OH Suppression Integral Field Unit (IFU) System
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Ellis_Suppression_of_the_2012.pdf||1.73 MB||Adobe PDF|
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