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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.
Original language | English |
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Title of host publication | Ground-based and Airborne Instrumentation for Astronomy VII |
Editors | Christopher J. Evans, Luc Simard, Hideki Takami |
Place of Publication | Bellingham, Washington |
Publisher | SPIE |
Pages | 1-6 |
Number of pages | 6 |
ISBN (Electronic) | 9781510619586 |
ISBN (Print) | 9781510619579 |
DOIs | |
Publication status | Published - 6 Jul 2018 |
Event | Ground-based and Airborne Instrumentation for Astronomy VII 2018 - Austin, United States Duration: 10 Jun 2018 → 14 Jun 2018 |
Publication series
Name | Proceedings of SPIE |
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Volume | 10702 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Conference
Conference | Ground-based and Airborne Instrumentation for Astronomy VII 2018 |
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Country/Territory | United States |
City | Austin |
Period | 10/06/18 → 14/06/18 |
Keywords
- Doppler spectroscopy
- echelle spectrographs
- exoplanet
- multi-mode fiber
- radial velocity
- thermal and pressure control
- ultra-stable
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Dive into the research topics of 'A high resolution echelle spectrograph for exoplanet searches with small aperture telescopes'. Together they form a unique fingerprint.Projects
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Harnessing Astrophotonics and Adaptive Optics to Discover Habitable Planets
Schwab, C., Coutts, D. W. & MQRES, M.
1/01/16 → …
Project: Research