OHS: OH-Airglow Suppressor for the Subaru Telescope
- 25 April 2001
- journal article
- research article
- Published by Oxford University Press (OUP) in Publications of the Astronomical Society of Japan
- Vol. 53 (2) , 355-360
- https://doi.org/10.1093/pasj/53.2.355
Abstract
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 ${\mu \mathrm {m}}$. 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 ($\lambda/\Delta\lambda = 210, S/N = 5$) in the standard 4000 s exposure sequence.
All Related Versions
This publication has 8 references indexed in Scilit:
- Infrared Observations of Nebular Emission Lines from Galaxies atz≃ 3The Astrophysical Journal, 1998
- CISCO: cooled infrared spectrograph and camera for OHSPublished by SPIE-Intl Soc Optical Eng ,1998
- Near‐Infrared Spectroscopy of Powerful Radio Galaxies atz= 2.2–2.6The Astrophysical Journal, 1998
- A Panoramic View of Radio Galaxy Evolution from a Redshift of 0 to a Redshift of 4.3The Astrophysical Journal, 1996
- Observations of the OH airglow emissionPublications of the Astronomical Society of the Pacific, 1993
- Infrared spectroscopy of 11 radio galaxies at Z equals 2-4 - Evidence that some high-redshift radio galaxies may be protogalaxiesThe Astrophysical Journal, 1993
- Rotational analysis of hydroxyl vibration–rotation emission bands: Molecular constants for OH X2Π, 6 ≤ ν ≤ 10Canadian Journal of Physics, 1982
- Optimum molecular constants and term values for the X2Π(ν ≤ 5) and A2Σ+(ν ≤ 3) states of OHCanadian Journal of Physics, 1980