The SPHERE infrared survey for exoplanets (SHINE): I. Sample definition and target characterization

Planets and satellites: general; Stars: activity; Stars: fundamental parameters; Stars: kinematics and dynamics; Stars: pre-main sequence; Stars: rotation; Extrasolar planets; Spheres; Surveys; Detection limits; High contrast imaging; Original sample; Planet detection; Rotation period; Statistical constraints; Statistical samples; Target characterization; Stars

Abstract :

[en] Large surveys with new-generation high-contrast imaging instruments are needed to derive the frequency and properties of exoplanet populations with separations from ~5 to 300 au. A careful assessment of the stellar properties is crucial for a proper understanding of when, where, and how frequently planets form, and how they evolve. The sensitivity of detection limits to stellar age makes this a key parameter for direct imaging surveys. Aims. We describe the SpHere INfrared survey for Exoplanets (SHINE), the largest direct imaging planet-search campaign initiated at the VLT in 2015 in the context of the SPHERE Guaranteed Time Observations of the SPHERE consortium. In this first paper we present the selection and the properties of the complete sample of stars surveyed with SHINE, focusing on the targets observed during the first phase of the survey (from February 2015 to February 2017). This early sample composed of 150 stars is used to perform a preliminary statistical analysis of the SHINE data, deferred to two companion papers presenting the survey performance, main discoveries, and the preliminary statistical constraints set by SHINE. Methods. Based on a large database collecting the stellar properties of all young nearby stars in the solar vicinity (including kinematics, membership to moving groups, isochrones, lithium abundance, rotation, and activity), we selected the original sample of 800 stars that were ranked in order of priority according to their sensitivity for planet detection in direct imaging with SPHERE. The properties of the stars that are part of the early statistical sample wererevisited, including for instance measurements from the Gaia Data Release 2. Rotation periods were derived for the vast majority of the late-type objects exploiting TESS light curves and dedicated photometric observations. Results. The properties of individual targets and of the sample as a whole are presented. © ESO 2021.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Desidera, S.; Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy

Chauvin, G.; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France

Bonavita, M.; Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy, Supa, Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom, Centre for Exoplanet Science, University of Edinburgh, Edinburgh, EH9 3HJ, United Kingdom

Messina, S.; Inaf - Osservatorio Astrofisico di Catania, Via S. Sofia 78, Catania, 95123, Italy

Lecoroller, H.; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France

Schmidt, T.; Hamburger Sternwarte, Gojenbergsweg 112, Hamburg, 21029, Germany, Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France

Gratton, R.; Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy

Lazzoni, C.; Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy, Dipartimento di Fisica e Astronomia Galileo Galilei, Universitá di Padova, Vicolo dell'Osservatorio 3, Padova, 35122, Italy

Meyer, M.; Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, United States, Institute for Particle Physics and Astrophysics, Eth Zurich, Wolfgang-Pauli-Strasse 27, Zurich, 8093, Switzerland

Schlieder, J.; Exoplanets and Stellar Astrophysics Laboratory, Code 667, Nasa Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, United States, Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany

More authors (99 more)

Language :

English

Title :

The SPHERE infrared survey for exoplanets (SHINE): I. Sample definition and target characterization

Publication date :

July 2021

Journal title :

Astronomy and Astrophysics

ISSN :

0004-6361

eISSN :

1432-0746

Publisher :

EDP Sciences, Les Ulis, France

Volume :

651

Pages :

A71

Peer reviewed :

Peer Reviewed verified by ORBi

Available on ORBi :

since 05 February 2022

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