A comparison between the opto-thermo-mechanical model and lab measurements for CHEOPS

Date Issued
2018
Author(s)
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Beck, Thomas
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Bruno, Giordano
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Baroni, Marco
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Turella, Andrea
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Marinai, Massimo
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Rieder, Martin
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Busch, Martin Diego
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Piazza, Daniele
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Bandy, Timothy
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Broeg, Christopher
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Fortier, Andrea
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Hernandez, Eduardo
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Cessa, Virginie
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Benz, Willy
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Piotto, Giampaolo
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Giannuzzo, Ester
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Dami, Michele
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Battistelli, Enrico
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Salatti, Mario
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Tommasi, Elisabetta
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De Angelis, Luigi
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Deep, Atul
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Ngan, Ivan
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Ratti, Francesco
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Gambicorti, Lisa
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Rando, Nicola
DOI
Abstract
CHEOPS is the first small class mission adopted by ESA in the framework of the Cosmic Vision 2015-2025. Its launch is foreseen in early 2019. CHEOPS aims to get transits follow-up measurements of already known exo-planets, hosted by near bright stars (V<12). Thanks to its ultra-high precision photometry, CHEOPS science goal is accurately measure the radii of planets in the super-Earth to Neptune mass range (1
Coverage
Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
All editors
Lystrup, Makenzie; MacEwen, Howard A.; Fazio, Giovanni G.; Batalha, Natalie; Siegler, Nicholas; Tong, Edward C.
Series
Volume
10698
Start page
106983B
Conferenece
Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
Conferenece place
Austin, Texas, United States
Conferenece date
10-15 June, 2018
Uri
Url
Issn Identifier
0277-786X
Ads BibCode
2018SPIE10698E..3BM
Rights
open.access
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