A high resolution echelle spectrograph for exoplanet searches with small aperture telescopes
Document Type
Conference Proceeding
Department or Administrative Unit
Physics
Publication Date
7-6-2018
Abstract
High precision Doppler observations of bright stars can be made efficiently with small aperture telescopes. We are constructing a high resolution echelle spectrograph for the new 0.6 m telescope at Central Washington University. The spectrograph is fed by a multimode fiber and operates in the visible wavelength range of 380-670 nm. The spectrograph uses a white pupil design with 100 mm beam diameter and a monolithic R4 echelle grating.
Recommended Citation
DuBois, L., Lentini, N., Schwab, C., Kuo Tiong, B. C., Feger, T., Coutts, D. W., & Fallscheer, C. (2018). A high resolution echelle spectrograph for exoplanet searches with small aperture telescopes. Ground-Based and Airborne Instrumentation for Astronomy VII. https://doi.org/10.1117/12.2313065
Journal
Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII
Rights
© 2018 COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).
Comments
This article was originally published in Ground-based and Airborne Instrumentation for Astronomy VII. The full-text article from the publisher can be found here.
Due to copyright restrictions, this article is not available for free download from ScholarWorks @ CWU.