This paper describes an OH-airglow Suppressor (OHS) for the infrared Nasmyth focus of the Subaru telescope. OHS has the capability of eliminating 224 airglow-lines in the J- and H-bands, which are major sources of background radiation at near-infrared wavelengths up to 2 μm. Specifically, it is a pre-optics system installed between the telescope and an infrared camera/spectrograph (CISCO). The suppressor reduces sky background emissions to 1/25 and its throughput is 40%. As a result, the S/N gain achieved with OHS is more than 1 mag compared to the typical spectroscopic approach. The limiting magnitude measured during a test observing run was found to be H = 21.1 mag (λ/Δλ = 210, S/N = 5) in the standard 4000 s exposure sequence.
@article{arxiv.astro-ph/0101076,
title = {OHS: OH-airglow Suppressor for the Subaru Telescope},
author = {F. Iwamuro and K. Motohara and T. Maihara and R. Hata and T. Harashima},
journal= {arXiv preprint arXiv:astro-ph/0101076},
year = {2015}
}
Comments
6 pages, 9 figures. Accepted for publication in PASJ(2001)