Literature DB >> 20940813

Visible wavelength astro-comb.

Andrew J Benedick1, Guoqing Chang, Jonathan R Birge, Li-Jin Chen, Alexander G Glenday, Chih-Hao Li, David F Phillips, Andrew Szentgyorgyi, Sylvain Korzennik, Gabor Furesz, Ronald L Walsworth, Franz X Kärtner.   

Abstract

We demonstrate a tunable laser frequency comb operating near 420 nm with mode spacing of 20-50 GHz, usable bandwidth of 15 nm and output power per line of ~20 nW. Using the TRES spectrograph at the Fred Lawrence Whipple Observatory, we characterize this system to an accuracy below 1m/s, suitable for calibrating high-resolution astrophysical spectrographs used, e.g., in exoplanet studies.

Year:  2010        PMID: 20940813     DOI: 10.1364/OE.18.019175

Source DB:  PubMed          Journal:  Opt Express        ISSN: 1094-4087            Impact factor:   3.894


  1 in total

1.  A spectrograph for exoplanet observations calibrated at the centimetre-per-second level.

Authors:  Tobias Wilken; Gaspare Lo Curto; Rafael A Probst; Tilo Steinmetz; Antonio Manescau; Luca Pasquini; Jonay I González Hernández; Rafael Rebolo; Theodor W Hänsch; Thomas Udem; Ronald Holzwarth
Journal:  Nature       Date:  2012-05-30       Impact factor: 49.962

  1 in total

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