Presentation + Paper
13 December 2020 Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets
Author Affiliations +
Abstract
The space missions TESS and PLATO plan to double the number of 4000 exoplanets already discovered and will measure the size of thousands of exoplanets around the brightest stars in the sky, allowing ground-based radial velocity spectroscopy follow-up to determine the orbit and mass of the detected planets. The new facility we are developing, MARVEL (Raskin et al. this conference1 ), will enable the ground-based follow-up of large numbers of exoplanet detections expected from TESS and PLATO, which cannot be carried out only by the current facilities that achieve the necessary radial velocity accuracy of 1 ms-1 or less. This paper presents the MARVEL observation strategy and performance analysis based on predicted PLATO transit detection yield simulations. The resulting observation scenario baseline will help in the instrument design choices and demonstrate the effectiveness of MARVEL as a TESS and PLATO science enabling facility.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Cyprien Lanthermann, Joris De Ridder, Hugues Sana, Pierre Royer, Denis Defrère, Gert Raskin, Bart Vandenbussche, Andrew Tkachenko, Christian Schwab, and Hans Van Winckel "Optimizing MARVEL for the radial velocity follow up of TESS and PLATO transiting exoplanets", Proc. SPIE 11449, Observatory Operations: Strategies, Processes, and Systems VIII, 1144913 (13 December 2020); https://doi.org/10.1117/12.2562486
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KEYWORDS
Exoplanets

Telescopes

Exoplanetary science

Planets

Space operations

Spectrographs

Spectroscopes

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