The SPHERE infrared survey for exoplanets (SHINE) - Archive ouverte HAL
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2021

The SPHERE infrared survey for exoplanets (SHINE)

Arthur Vigan (1) , Clémence Fontanive (2, 3) , M. Meyer (4, 5) , Beth Biller (6, 7, 8) , Mariangela Bonavita (6) , Markus Feldt (8) , Silvano Desidera (3) , Gabriel-Dominique Marleau (9, 2, 8) , Alexandre Emsenhuber (10, 2) , Raphael Galicher (11) , Ken Rice (7, 12) , Duncan Forgan (12) , Christoph Mordasini (2, 8) , Raffaele Gratton (3) , Hervé Le Coroller (1) , Anne-Lise Maire (13, 8) , Faustine Cantalloube (8) , Gaël Chauvin (14, 15) , Anthony K. Cheetham (16) , Janis Hagelberg (16) , Anne-Marie Lagrange (14) , Maud Langlois (17, 1) , Mickaël Bonnefoy (14) , Jean-Luc Beuzit (1, 14) , Anthony Boccaletti (11) , Valentina D’orazi (3) , Philippe Delorme (14) , Carsten Dominik (18) , Thomas Henning (8) , Markus Janson (8, 19) , Éric Lagadec (20) , Cecilia Lazzoni (3) , Roxanne Ligi (21) , François Menard (14) , Dino Mesa (3) , Sergio Messina (22) , Claire Moutou (23, 1) , André Müller (8) , Clément Perrot (11, 24, 25) , Matthias Samland (8, 19) , Hans Martin Schmid (5) , T. Schmidt (11) , Elena Sissa (3) , Massimo Turatto (3) , Stéphane Udry (16) , Alice Zurlo (1, 26) , Lyu Abe (27) , Jacopo Antichi (3) , Ruben Asensio-Torres (8) , Andrea Baruffolo (3) , Pierre Baudoz (11) , Jacques Baudrand (11) , Andrea Bazzon (5) , Patrick Blanchard (1) , Alexander J. Bohn (28) , Samantha Brown-Sevilla (8) , Marcel Carbillet (20) , Michaël Carle (1) , Enrico Cascone (3) , Julien Charton (14) , R. Claudi (3) , Anne Costille (1) , Vincenzo de Caprio (28) , Alain Delboulbé (14) , Kjetil Dohlen (1) , Natalia Engler (5) , Daniela Fantinel (3) , Philippe Feautrier (14) , Thierry Fusco (1, 29) , Pierre Gigan (11) , Julien H. Girard (24, 30, 14) , Enrico Giro (3) , Daniel Gisler (5) , Laurence Gluck (14) , Cécile Gry (1) , Norbert Hubin (31) , Emmanuel Hugot (1) , Marc Jaquet (1) , Markus Kasper (31, 14) , David Le Mignant (1) , Marc Llored (1) , Fabrice Madec (1) , Yves Magnard (14) , Patrice Martinez (20) , Didier Maurel (14) , Ole Möller-Nilsson (8) , David Mouillet (14) , Thibaut Moulin (14) , Alain Origné (1) , Alexey Pavlov (8) , Denis Perret (11) , Cyril Petit (32) , Johan Pragt (14) , Pascal Puget (14) , Patrick Rabou (14) , J. Ramos (14) , Emily Rickman (16) , Florence Rigal (14) , Sylvain Rochat (14) , Ronald Roelfsema (33) , Gérard Rousset (11) , Alain Roux (14) , Bernardo Salasnich (3) , Jean-François Sauvage (32, 1) , Arnaud Sevin (11) , Christian Soenke (31) , Eric Stadler (14) , Marcos Suarez (31) , Zahed Wahhaj (34, 1) , Luc Weber (16) , François Wildi (16)
1 LAM - Laboratoire d'Astrophysique de Marseille
2 CSH - Center for Space and Habitability
3 OAPD - INAF - Osservatorio Astronomico di Padova
4 University of Michigan [Ann Arbor]
5 IPA - Institute for Particle Physics and Astrophysics [ETH Zürich]
6 IfA - Institute for Astronomy [Edinburgh]
7 SUPA - Scottish Universities Physics Alliance
8 MPIA - Max Planck Institute for Astronomy
9 Eberhard Karls Universität Tübingen = University of Tübingen
10 LPL - Lunar and Planetary Laboratory [Tucson]
11 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics
12 Centre for Exoplanet Science
13 STAR - Space Sciences, Technologies and Astrophysics Research Institute
14 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
15 LFCA - Laboratoire Franco-Chilien d'Astronomie
16 Geneva Observatory
17 CRAL - Centre de Recherche Astrophysique de Lyon
18 AI PANNEKOEK - Astronomical Institute Anton Pannekoek
19 Stockholm University
20 LAGRANGE - Joseph Louis LAGRANGE
21 OAB - INAF - Osservatorio Astronomico di Brera
22 Dipartimento di Fisica e Astronomia [Catania]
23 IRAP - Institut de recherche en astrophysique et planétologie
24 STSci - Space Telescope Science Institute
25 Instituto de Fisica y Astronomia [Valparaiso]
26 UDP - Universidad Diego Portales [Santiago - Chili]
27 OCA - Observatoire de la Côte d'Azur
28 Leiden Observatory [Leiden]
29 DOTA, ONERA, Université Paris Saclay [Palaiseau]
30 Universidad de Valparaiso [Chile]
31 ESO - European Southern Observatory
32 ONERA
33 NOVA - NOVA Optical Infrared Instrumentation Group
34 ESO - European Southern Observatory [Santiago]
Arthur Vigan
Faustine Cantalloube
Anthony K. Cheetham
Janis Hagelberg
Carsten Dominik
Thomas Henning
Éric Lagadec
Roxanne Ligi
Dino Mesa
Massimo Turatto
Stéphane Udry
Lyu Abe
Jacopo Antichi
  • Fonction : Auteur
  • PersonId : 897455
Alexander J. Bohn
Marcel Carbillet
R. Claudi
Anne Costille
  • Fonction : Auteur
  • PersonId : 866177
Vincenzo de Caprio
  • Fonction : Auteur
  • PersonId : 1342454
Kjetil Dohlen
Enrico Giro
  • Fonction : Auteur
  • PersonId : 1342425
Cécile Gry
Emmanuel Hugot
David Le Mignant
Fabrice Madec
Patrice Martinez
Cyril Petit
  • Fonction : Auteur
  • PersonId : 1105871
Emily Rickman
Luc Weber
  • Fonction : Auteur
François Wildi
  • Fonction : Auteur
  • PersonId : 1340948

Résumé

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.
Fichier principal
Vignette du fichier
aa38107-20.pdf (2.85 Mo) Télécharger le fichier
Origine Fichiers produits par l'(les) auteur(s)

Dates et versions

hal-04709662 , version 1 (25-09-2024)

Identifiants

Citer

Arthur Vigan, Clémence Fontanive, M. Meyer, Beth Biller, Mariangela Bonavita, et al.. The SPHERE infrared survey for exoplanets (SHINE). Astronomy and Astrophysics - A&A, 2021, 651, pp.A72. ⟨10.1051/0004-6361/202038107⟩. ⟨hal-04709662⟩
40 Consultations
6 Téléchargements

Altmetric

Partager

More