Paper
17 September 2012 The Astronomical Telescope of New York: a new 12-meter astronomical telescope
T. Sebring, R. Junquist, C. Stutzki, P. Sebring, S. Baum
Author Affiliations +
Abstract
The Astronomical Corporation of New York has commissioned a study of a 12-meter class telescope to be developed by a group of NY universities. The telescope concept builds on the basic principles established by the Keck telescopes; segmented primary mirror, Ritchey Chretien Nasmyth instrument layout, and light weight structures. New, lightweight, and low cost approaches are proposed for the primary mirror architecture, dome structure and mechanisms, telescope mount approach, and adaptive optics. Work on the design is supported by several NY based corporations and universities. The design offers a substantially larger aperture than any existing Visible/IR wavelength telescope at historically low cost. The concept employs an adaptive secondary mirror and laser guide star adaptive optics. Two First Light instruments are proposed; A High resolution near infrared spectrograph and a near infrared Integral field spectrograph/imager.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
T. Sebring, R. Junquist, C. Stutzki, P. Sebring, and S. Baum "The Astronomical Telescope of New York: a new 12-meter astronomical telescope", Proc. SPIE 8444, Ground-based and Airborne Telescopes IV, 84440X (17 September 2012); https://doi.org/10.1117/12.926998
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KEYWORDS
Telescopes

Mirrors

Space telescopes

Astronomical telescopes

Optical instrument design

Adaptive optics

Manufacturing

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