Abstract
CHIRON is a fiber-fed Echelle spectrograph with observing modes for resolutions from 28,000 to 120,000, built primarily for measuring precise radial velocities (RVs). We present the instrument performance as determined during integration and commissioning. We discuss the PSF, the effect of glass inhomogeneity on the cross-dispersion prism, temperature stabilization, stability of the spectrum on the CCD, and detector characteristics. The RV precision is characterized, with an iodine cell or a ThAr lamp as the wavelength reference. Including all losses from the sky to the detector, the overall efficiency is about 6%; the dominant limitation is coupling losses into the fiber due to poor guiding.
Original language | English |
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Title of host publication | Ground-Based and Airborne Instrumentation for Astronomy IV |
Editors | Ian S. McLean, Suzanne K. Ramsay, Hideki Takami |
Place of Publication | Bellingham, WA |
Publisher | SPIE |
Pages | 1-16 |
Number of pages | 16 |
Volume | 8446 |
ISBN (Print) | 9780819491473 |
DOIs | |
Publication status | Published - 2012 |
Externally published | Yes |
Event | Ground-Based and Airborne Instrumentation for Astronomy IV - Amsterdam, Netherlands Duration: 1 Jul 2012 → 6 Jul 2012 |
Other
Other | Ground-Based and Airborne Instrumentation for Astronomy IV |
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Country/Territory | Netherlands |
City | Amsterdam |
Period | 1/07/12 → 6/07/12 |
Keywords
- Doppler method
- Echelle
- Exoplanets
- Fiber-fed spectrograph
- Iodine cell
- Radial velocities
- Spectroscopy