Proceedings Paper
An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus| Format | Member Price | Non-Member Price |
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Paper Abstract
We recently demonstrated sub-m/s sensitivity in measuring the radial velocity (RV) between the Earth and Sun using a simple solar telescope feeding the HARPS-N spectrograph at the Italian National Telescope, which is calibrated with a green astro-comb. We are using the solar telescope to characterize the effects of stellar (solar) RV jitter due to activity on the solar surface with the goal of detecting the solar RV signal from Venus, thereby demonstrating the sensitivity of these instruments to detect true Earth-twin exoplanets.
Paper Details
Date Published: 22 July 2016
PDF: 8 pages
Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99126Z (22 July 2016);
Published in SPIE Proceedings Vol. 9912:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II
Ramón Navarro; James H. Burge, Editor(s)
PDF: 8 pages
Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99126Z (22 July 2016);
Show Author Affiliations
David F. Phillips, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Alex G. Glenday, Komodo Health Inc. (United States)
Xavier Dumusque, Observatoire de Genève (Switzerland)
Nicolas Buchschacher, Observatoire de Genève (Switzerland)
Andrew Collier Cameron, Univ. of St. Andrews (United Kingdom)
Massimo Cecconi, Fundación Galileo Galilei - INAF (Spain)
David Charbonneau, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Rosario Cosentino, Fundación Galileo Galilei - INAF (Spain)
Adriano Ghedina, Fundación Galileo Galilei - INAF (Spain)
Raphäelle Haywood, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Alex G. Glenday, Komodo Health Inc. (United States)
Xavier Dumusque, Observatoire de Genève (Switzerland)
Nicolas Buchschacher, Observatoire de Genève (Switzerland)
Andrew Collier Cameron, Univ. of St. Andrews (United Kingdom)
Massimo Cecconi, Fundación Galileo Galilei - INAF (Spain)
David Charbonneau, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Rosario Cosentino, Fundación Galileo Galilei - INAF (Spain)
Adriano Ghedina, Fundación Galileo Galilei - INAF (Spain)
Raphäelle Haywood, Harvard-Smithsonian Ctr. for Astrophysics (United States)
David W. Latham, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Chih-Hao Li, AOSense, Inc. (United States)
Marcello Lodi, Fundación Galileo Galilei - INAF (Spain)
Christophe Lovis, Observatoire de Genève (Switzerland)
Emilio Molinari, Fundación Galileo Galilei - INAF (Spain)
INAF - IASF Milano (Italy)
Francesco Pepe, Observatoire de Genève (Switzerland)
Dimitar Sasselov, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Andrew Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Stephane Udry, Observatoire de Genève (Switzerland)
Ronald L. Walsworth, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Chih-Hao Li, AOSense, Inc. (United States)
Marcello Lodi, Fundación Galileo Galilei - INAF (Spain)
Christophe Lovis, Observatoire de Genève (Switzerland)
Emilio Molinari, Fundación Galileo Galilei - INAF (Spain)
INAF - IASF Milano (Italy)
Francesco Pepe, Observatoire de Genève (Switzerland)
Dimitar Sasselov, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Andrew Szentgyorgyi, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Stephane Udry, Observatoire de Genève (Switzerland)
Ronald L. Walsworth, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Published in SPIE Proceedings Vol. 9912:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II
Ramón Navarro; James H. Burge, Editor(s)
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