Paper
24 September 2012 High-resolution Fourier transform spectrograph for characterization of echelle spectrograph wavelength calibrators
Alexander G. Glenday, David F. Phillips, Matthew Webber, Chih-Hao Li, Gabor Furesz, Guoqing Chang, Li-Jin Chen, Franz X. Kärtner, Dimitar D. Sasselov, Andrew H. Szentgyorgyi, Ronald L. Walsworth
Author Affiliations +
Abstract
Wavelength calibrators are a critical component of high precision and accuracy radial velocity measurements. An order of magnitude improvement of the state-of-the-art of calibration of echelle spectrographs is amongst the requirements needed to achieve detection of earth-mass planets around sun-like stars in the habitable zone. We present studies of calibrators using a custom Fourier Transform Spectrograph (FTS) optimized for characterizing broadband, high repetition-rate laser frequency combs ("astro-combs") as well as other calibration sources including Th:Ar lamps and white-light etalons.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alexander G. Glenday, David F. Phillips, Matthew Webber, Chih-Hao Li, Gabor Furesz, Guoqing Chang, Li-Jin Chen, Franz X. Kärtner, Dimitar D. Sasselov, Andrew H. Szentgyorgyi, and Ronald L. Walsworth "High-resolution Fourier transform spectrograph for characterization of echelle spectrograph wavelength calibrators", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 844696 (24 September 2012); https://doi.org/10.1117/12.926366
Lens.org Logo
CITATIONS
Cited by 5 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Fourier transforms

Calibration

Spectrographs

Signal to noise ratio

Interferometers

Fabry–Perot interferometers

Collimation

Back to Top