Paper
22 July 2016 An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus
David F. Phillips, Alex G. Glenday, Xavier Dumusque, Nicolas Buchschacher, Andrew Collier Cameron, Massimo Cecconi, David Charbonneau, Rosario Cosentino, Adriano Ghedina, Raphäelle Haywood, David W. Latham, Chih-Hao Li, Marcello Lodi, Christophe Lovis, Emilio Molinari, Francesco Pepe, Dimitar Sasselov, Andrew Szentgyorgyi, Stephane Udry, Ronald L. Walsworth
Author Affiliations +
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.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David F. Phillips, Alex G. Glenday, Xavier Dumusque, Nicolas Buchschacher, Andrew Collier Cameron, Massimo Cecconi, David Charbonneau, Rosario Cosentino, Adriano Ghedina, Raphäelle Haywood, David W. Latham, Chih-Hao Li, Marcello Lodi, Christophe Lovis, Emilio Molinari, Francesco Pepe, Dimitar Sasselov, Andrew Szentgyorgyi, Stephane Udry, and Ronald L. Walsworth "An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus", Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99126Z (22 July 2016); https://doi.org/10.1117/12.2232452
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Cited by 13 scholarly publications.
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KEYWORDS
Solar telescopes

Calibration

Sun

Spectrographs

Telescopes

Venus

Integrating spheres

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