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The SPHERE infrared survey for exoplanets (SHINE) ; The SPHERE infrared survey for exoplanets (SHINE): III. The demographics of young giant exoplanets below 300 au with SPHERE

Title: The SPHERE infrared survey for exoplanets (SHINE) ; The SPHERE infrared survey for exoplanets (SHINE): III. The demographics of young giant exoplanets below 300 au with SPHERE
Authors: Vigan, Arthur; Fontanive, Clémence; Meyer, M.; Biller, Beth; Bonavita, Mariangela; Feldt, Markus; Desidera, Silvano; Marleau, Gabriel-Dominique; Emsenhuber, Alexandre; Galicher, Raphael; Rice, Ken; Forgan, Duncan; Mordasini, Christoph; Gratton, Raffaele; Le Coroller, Hervé; Maire, Anne-Lise; Cantalloube, Faustine; Chauvin, Gaël; Cheetham, Anthony K.; Hagelberg, Janis; Lagrange, Anne-Marie; Langlois, Maud; Bonnefoy, Mickaël; Beuzit, Jean-Luc; Boccaletti, Anthony; D’orazi, Valentina; Delorme, Philippe; Dominik, Carsten; Henning, Thomas; Janson, Markus; Lagadec, Éric; Lazzoni, Cecilia; Ligi, Roxanne; Menard, François; Mesa, Dino; Messina, Sergio; Moutou, Claire; Müller, André; Perrot, Clément; Samland, Matthias; Schmid, Hans Martin; Schmidt, T.; Sissa, Elena; Turatto, Massimo; Udry, Stéphane; Zurlo, Alice; Abe, Lyu; Antichi, Jacopo; Asensio-Torres, Ruben; Baruffolo, Andrea; Baudoz, Pierre; Baudrand, Jacques; Bazzon, Andrea; Blanchard, Patrick; Bohn, Alexander, J.; Brown-Sevilla, Samantha; Carbillet, Marcel; Carle, Michaël; Cascone, Enrico; Charton, Julien; Claudi, R.; Costille, Anne; de Caprio, Vincenzo; Delboulbé, Alain; Dohlen, Kjetil; Engler, Natalia; Fantinel, Daniela; Feautrier, Philippe; Fusco, Thierry; Gigan, Pierre; H. Girard, Julien; Giro, Enrico; Gisler, Daniel; Gluck, Laurence; Gry, Cécile; Hubin, Norbert; Hugot, Emmanuel; Jaquet, Marc; Kasper, Markus; Le Mignant, David; Llored, Marc; Madec, Fabrice; Magnard, Yves; Martinez, Patrice; Maurel, Didier; Möller-Nilsson, Ole; Mouillet, David; Moulin, Thibaut; Origné, Alain; Pavlov, Alexey; Perret, Denis; Petit, Cyril; Pragt, Johan; Puget, Pascal; Rabou, Patrick; Ramos, J.; Rickman, Emily; Rigal, Florence; Rochat, Sylvain; Roelfsema, Ronald; Rousset, Gérard; Roux, Alain; Salasnich, Bernardo; Sauvage, Jean-François; Sevin, Arnaud; Soenke, Christian; Stadler, Eric; Suarez, Marcos; Wahhaj, Zahed; Weber, Luc; Wildi, François
Contributors: Laboratoire d'Astrophysique de Marseille (LAM); Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS); Center for Space and Habitability (CSH); Universität Bern = University of Bern = Université de Berne (UNIBE); INAF - Osservatorio Astronomico di Padova (OAPD); Istituto Nazionale di Astrofisica Rome (INAF); Université du Michigan = University of Michigan Ann Arbor (UMich); Institute for Particle Physics and Astrophysics ETH Zürich (IPA); Department of Physics = Departement Physik ETH Zürich (D-PHYS); Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich)-Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich); Institute for Astronomy Edinburgh (IfA); The University of Edinburgh; Scottish Universities Physics Alliance (SUPA); Max-Planck-Institut für Astronomie = Max Planck Institute for Astronomy (MPIA); Max-Planck-Gesellschaft; Eberhard Karls Universität Tübingen = University of Tübingen; Lunar and Planetary Laboratory Tucson (LPL); University of Arizona; Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA); Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris; Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité); Centre for Exoplanet Science; Space Sciences, Technologies and Astrophysics Research Institute (STAR); Université de Liège = University of Liège = Universiteit van Luik = Universität Lüttich (ULiège); Institut de Planétologie et d'Astrophysique de Grenoble (IPAG); Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (Fédération OSUG)-Université Grenoble Alpes (UGA); Laboratoire Franco-Chilien d'Astronomie (LFCA); Universidad de Chile = University of Chile Santiago (UCHILE)-Pontificia Universidad Católica de Chile = Pontifical Catholic University of Chile Santiago (PUC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Universidad de Concepción = University of Concepción Chile (UdeC); Geneva Observatory; Université de Genève = University of Geneva (UNIGE); Centre de Recherche Astrophysique de Lyon (CRAL); École normale supérieure de Lyon (ENS de Lyon); Université de Lyon-Université de Lyon-Université Claude Bernard Lyon 1 (UCBL); Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Astronomical Institute Anton Pannekoek (AI PANNEKOEK); Universiteit van Amsterdam = University of Amsterdam (UvA); Stockholm University; Joseph Louis LAGRANGE (LAGRANGE); Université Nice Sophia Antipolis (1965 - 2019) (UNS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur; Université Côte d'Azur (UniCA)-Université Côte d'Azur (UniCA)-Centre National de la Recherche Scientifique (CNRS); INAF - Osservatorio Astronomico di Brera (OAB); Dipartimento di Fisica e Astronomia Catania; Università degli studi di Catania = University of Catania (Unict); Institut de recherche en astrophysique et planétologie (IRAP); Université Toulouse III - Paul Sabatier (UT3); Communauté d'universités et établissements de Toulouse (Comue de Toulouse)-Communauté d'universités et établissements de Toulouse (Comue de Toulouse)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Space Telescope Science Institute (STSci); Instituto de Fisica y Astronomia Valparaiso; Universidad de Valparaiso = Valparaiso University; Universidad Diego Portales Santiago - Chili (UDP); Observatoire de la Côte d'Azur; Université Côte d'Azur (UniCA); Leiden Observatory Leiden; Universiteit Leiden = Leiden University; DOTA, ONERA, Université Paris Saclay Palaiseau; ONERA-Université Paris-Saclay; European Southern Observatory (ESO); ONERA; NOVA Optical Infrared Instrumentation Group (NOVA); European Southern Observatory Santiago (ESO); C.P. acknowledge financial support from Fondecyt (grant 3190691) and financial support from the ICM (Iniciativa Científica Milenio) via the Núcleo Milenio de Formación Planetaria grant, from the Universidad de Valparaíso. G.-D.M. acknowledges the support of the DFG priority program SPP 1992 “Exploring the Diversity of Extrasolar Planets” (KU 2849/7-1). C.M., A.E., and G.-D.M. acknowledge the support from the Swiss National Science Foundation under grant BSSGI0_155816 “PlanetsInTime”.; SPHERE also received funding from the European Commission Sixth and Seventh Framework Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6 (2004–2008), grant number 226604 for FP7 (2009–2012) and grant number 312430 for FP7 (2013–2016).; ANR-10-LABX-0056,OSUG@2020,Innovative strategies for observing and modelling natural systems(2010); ANR-16-CE31-0013,PLANET-FORMING-DISKS,De meilleurs modèles pour de meilleures données(2016); ANR-14-CE33-0018,GIPSE,Exploration des planetes géantes extrasolaires(2014); European Project: 757561,ERC-2017-STG,ERC-2017-STG,HiRISE(2017); European Project: 832428,ERC-2018-ADG,ERC-2018-ADG,Origins(2019)
Source: ISSN: 0004-6361.
Publisher Information: CCSD; EDP Sciences
Publication Year: 2021
Collection: Université Toulouse III - Paul Sabatier: HAL-UPS
Subject Terms: Planets and satellites formation; Infrared planetary systems; Statistical methods; High angular resolution; [SDU]Sciences of the Universe [physics]
Description: International audience ; The SpHere INfrared Exoplanet (SHINE) project is a 500-star survey performed with SPHERE on the Very Large Telescope for the purpose of directly detecting new substellar companions and understanding their formation and early evolution. Here we present an initial statistical analysis for a subsample of 150 stars spanning spectral types from B to M that are representative of the full SHINE sample. Our goal is to constrain the frequency of substellar companions with masses between 1 and 75 M Jup and semimajor axes between 5 and 300 au. For this purpose, we adopt detection limits as a function of angular separation from the survey data for all stars converted into mass and projected orbital separation using the BEX-COND-hot evolutionary tracks and known distance to each system. Based on the results obtained for each star and on the 13 detections in the sample, we use a Markov chain Monte Carlo tool to compare our observations to two different types of models. The first is a parametric model based on observational constraints, and the second type are numerical models that combine advanced core accretion and gravitational instability planet population synthesis. Using the parametric model, we show that the frequencies of systems with at least one substellar companion are 23.0 +13.5 -9.7 , 5.8 +4.7 -2.8 , and 12.6 +12.9 -7.1 % for BA, FGK, and M stars, respectively. We also demonstrate that a planet-like formation pathway probably dominates the mass range from 1-75 M Jup for companions around BA stars, while for M dwarfs, brown dwarf binaries dominate detections. In contrast, a combination of binary star-like and planet-like formation is required to best fit the observations for FGK stars. Using our population model and restricting our sample to FGK stars, we derive a frequency of 5.7 +3.8 -2.8 %, consistent with predictions from the parametric model. More generally, the frequency values that we derive are in excellent agreement with values obtained in previous studies.
Document Type: article in journal/newspaper
Language: English
Relation: info:eu-repo/grantAgreement//757561/EU/High-Resolution Imaging and Spectroscopy of Exoplanets/HiRISE; info:eu-repo/grantAgreement//832428/EU/From Planet-Forming Disks to Giant Planets/Origins
DOI: 10.1051/0004-6361/202038107
Availability: https://hal.science/hal-04709662; https://hal.science/hal-04709662v1/document; https://hal.science/hal-04709662v1/file/aa38107-20.pdf; https://doi.org/10.1051/0004-6361/202038107
Rights: https://about.hal.science/hal-authorisation-v1/ ; info:eu-repo/semantics/OpenAccess
Accession Number: edsbas.2B883DDA
Database: BASE