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Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2021

The SPHERE infrared survey for exoplanets (SHINE)

M. Langlois (1) , R. Gratton (2) , A.-M. Lagrange (3) , P. Delorme (3) , A. Boccaletti (4) , M. Bonnefoy (3) , A.-L. Maire (5) , D. Mesa (6) , G. Chauvin (3) , S. Desidera (2) , A. Vigan , A. Cheetham (7) , J. Hagelberg (7) , M. Feldt (8) , M. Meyer (9, 10) , P. Rubini (11) , H. Le Coroller , F. Cantalloube (12) , B. Biller , M. Bonavita (13) , T. Bhowmik , W. Brandner , S. Daemgen , V. D’orazi , O. Flasseur (1) , C. Fontanive (2, 14) , R. Galicher (4) , J. Girard (3) , P. Janin-Potiron (15, 16) , M. Janson (8) , M. Keppler , T. Kopytova (17) , E. Lagadec (18) , J. Lannier , C. Lazzoni (2) , R. Ligi (19) , N. Meunier (3) , A. Perreti , C. Perrot , L. Rodet , C. Romero (20) , D. Rouan , M. Samland (8) , G. Salter , E. Sissa (2) , T. Schmidt , A. Zurlo (16) , D. Mouillet (3) , L. Denis (21) , E. Thiébaut (1) , J. Milli (3) , Z. Wahhaj (16) , J.-L. Beuzit , C. Dominik , Th. Henning , F. Ménard (3) , A. Müller (22) , H. M. Schmid , M. Turatto (2) , S. Udry , L. Abe (18) , J. Antichi (2) , F. Allard (23) , A. Baruffolo (2) , P. Baudoz (24) , J. Baudrand (4) , A. Bazzon (10) , P. Blanchard (25, 25, 26) , M. Carbillet (27) , M. Carle (16) , E. Cascone (2) , J. Charton (3) , R. Claudi , A. Costille (16) , V. de Caprio (28) , A. Delboulbé (3) , K. Dohlen , D. Fantinel , P. Feautrier (3) , Thierry Fusco (16, 15) , P. Gigan (4) , E. Giro (2) , D. Gisler (29) , L. Gluck (3) , C. Gry (16) , N. Hubin (30) , E. Hugot (16) , M. Jaquet (16) , M. Kasper , D. Le Mignant , M. Llored , F. Madec (16) , Y. Magnard (3) , P. Martinez (31) , D. Maurel (3) , S. Messina (32) , O. Möller-Nilsson (8) , Laurent Mugnier (15) , T. Moulin (3) , A. Origné (16) , A. Pavlov (33) , D. Perret (4) , Cyril Petit (15) , J. Pragt , P. Puget (3) , P. Rabou (3) , J. Ramos , F. Rigal (3) , S. Rochat (3) , R. Roelfsema , G. Rousset , A. Roux (3) , B. Salasnich , J.-F. Sauvage (16, 15) , A. Sevin (4) , C. Soenke (30) , E. Stadler (3) , M. Suarez , L. Weber (34) , F. Wildi (7) , E. Rickman (7)
1 CRAL - Centre de Recherche Astrophysique de Lyon
2 OAPD - INAF - Osservatorio Astronomico di Padova
3 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
4 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics
5 Max-Planck-Institut
6 Department of Biochemistry and Molecular Biology
7 Geneva Observatory
8 Max Planck Institute for Radio Astronomy
9 University of Michigan [Ann Arbor]
10 IPA - Institute for Particle Physics and Astrophysics [ETH Zürich]
11 Pixyl Medical [Grenoble]
12 MPIA - Max Planck Institute for Astronomy
13 Edin. - University of Edinburgh
14 CSH - Center for Space and Habitability
15 DOTA, ONERA, Université Paris Saclay [Châtillon]
16 LAM - Laboratoire d'Astrophysique de Marseille
17 MPIA - Max-Planck-Institut für Astronomie
18 LAGRANGE - Joseph Louis LAGRANGE
19 OAB - INAF - Osservatorio Astronomico di Brera
20 CEDETE - Centre d'Etudes pour le Développement des Territoires et l'Environnement
21 LHC - Laboratoire Hubert Curien
22 LBMC UMR T9406 - Laboratoire de Biomécanique et Mécanique des Chocs
23 LaSIE - Laboratoire des Sciences de l'Ingénieur pour l'Environnement - UMR 7356
24 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
25 CHU Tenon [AP-HP]
26 CHU Pitié-Salpêtrière [AP-HP]
27 FIZEAU - Laboratoire Hippolyte Fizeau
28 OAC - INAF - Osservatorio Astronomico di Capodimonte
29 IMAPP - Institute for Mathematics, Astrophysics and Particle Physics
30 ESO - European Southern Observatory
31 EPOC - Environnements et Paléoenvironnements OCéaniques
32 OACT - INAF - Osservatorio Astrofisico di Catania
33 GSFC - NASA Goddard Space Flight Center
34 Centre Hospitalier Henri Duffaut (Avignon)
R. Gratton
A.-L. Maire
S. Desidera
A. Vigan
A. Cheetham
J. Hagelberg
P. Rubini
H. Le Coroller
  • Fonction : Auteur
F. Cantalloube
B. Biller
  • Fonction : Auteur
M. Bonavita
T. Bhowmik
  • Fonction : Auteur
W. Brandner
S. Daemgen
  • Fonction : Auteur
V. D’orazi
M. Janson
M. Keppler
  • Fonction : Auteur
E. Lagadec
J. Lannier
  • Fonction : Auteur
R. Ligi
A. Perreti
  • Fonction : Auteur
C. Perrot
L. Rodet
  • Fonction : Auteur
D. Rouan
  • Fonction : Auteur
M. Samland
G. Salter
  • Fonction : Auteur
T. Schmidt
  • Fonction : Auteur
A. Zurlo
Z. Wahhaj
J.-L. Beuzit
C. Dominik
Th. Henning
H. M. Schmid
  • Fonction : Auteur
M. Turatto
S. Udry
L. Abe
  • Fonction : Auteur
A. Baruffolo
M. Carbillet
E. Cascone
R. Claudi
K. Dohlen
D. Fantinel
E. Giro
C. Gry
M. Kasper
  • Fonction : Auteur
D. Le Mignant
  • Fonction : Auteur
M. Llored
  • Fonction : Auteur
F. Madec
S. Messina
J. Pragt
  • Fonction : Auteur
J. Ramos
  • Fonction : Auteur
R. Roelfsema
  • Fonction : Auteur
G. Rousset
  • Fonction : Auteur
B. Salasnich
M. Suarez
  • Fonction : Auteur
L. Weber
  • Fonction : Auteur
  • PersonId : 1000277
  • IdRef : 220196206
F. Wildi
  • Fonction : Auteur
E. Rickman
  • Fonction : Auteur

Résumé

Context. In recent decades, direct imaging has confirmed the existence of substellar companions (exoplanets or brown dwarfs) on wide orbits (>10 au) around their host stars. In striving to understand their formation and evolution mechanisms, in 2015 we initiated the SPHERE infrared survey for exoplanets (SHINE), a systematic direct imaging survey of young, nearby stars that is targeted at exploring their demographics.Aims. We aim to detect and characterize the population of giant planets and brown dwarfs beyond the snow line around young, nearby stars. Combined with the survey completeness, our observations offer the opportunity to constrain the statistical properties (occurrence, mass and orbital distributions, dependency on the stellar mass) of these young giant planets.Methods. In this study, we present the observing and data analysis strategy, the ranking process of the detected candidates, and the survey performances for a subsample of 150 stars that are representative of the full SHINE sample. Observations were conducted in a homogeneous way between February 2015 and February 2017 with the dedicated ground-based VLT/SPHERE instrument equipped with the IFS integral field spectrograph and the IRDIS dual-band imager, covering a spectral range between 0.9 and 2.3 μm. We used coronographic, angular, and spectral differential imaging techniques to achieve the best detection performances for this study, down to the planetary mass regime.Results. We processed, in a uniform manner, more than 300 SHINE observations and datasets to assess the survey typical sensitivity as a function of the host star and of the observing conditions. The median detection performance reached 5σ-contrasts of 13 mag at 200 mas and 14.2 mag at 800 mas with the IFS (YJ and YJH bands), and of 11.8 mag at 200 mas, 13.1 mag at 800 mas, and 15.8 mag at 3 as with IRDIS in H band, delivering one of the deepest sensitivity surveys thus far for young, nearby stars. A total of sixteen substellar companions were imaged in this first part of SHINE: seven brown dwarf companions and ten planetary-mass companions.These include two new discoveries, HIP 65426 b and HIP 64892 B, but not the planets around PDS70 that had not been originally selected for the SHINE core sample. A total of 1483 candidates were detected, mainly in the large field of view that characterizes IRDIS. The color-magnitude diagrams, low-resolution spectrum (when available with IFS), and follow-up observations enabled us to identify the nature (background contaminant or comoving companion) of about 86% of our subsample. The remaining cases are often connected to crowded-field follow-up observations that were missing. Finally, even though SHINE was not initially designed for disk searches, we imaged twelve circumstellar disks, including three new detections around the HIP 73145, HIP 86598, and HD 106906 systems.Conclusions. Nowadays, direct imaging provides a unique opportunity to probe the outer part of exoplanetary systems beyond 10 au to explore planetary architectures, as highlighted by the discoveries of: one new exoplanet, one new brown dwarf companion, and three new debris disks during this early phase of SHINE. It also offers the opportunity to explore and revisit the physical and orbital properties of these young, giant planets and brown dwarf companions (relative position, photometry, and low-resolution spectrum in near-infrared, predicted masses, and contrast in order to search for additional companions). Finally, these results highlight the importance of finalizing the SHINE systematic observation of about 500 young, nearby stars for a full exploration of their outer part to explore the demographics of young giant planets beyond 10 au and to identify the most interesting systems for the next generation of high-contrast imagers on very large and extremely large telescopes.
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Dates et versions

hal-03286624 , version 1 (14-07-2021)

Identifiants

Citer

M. Langlois, R. Gratton, A.-M. Lagrange, P. Delorme, A. Boccaletti, et al.. The SPHERE infrared survey for exoplanets (SHINE): II. Observations, data reduction and analysis, detection performances, and initial results. Astronomy and Astrophysics - A&A, 2021, 651, pp.A71. ⟨10.1051/0004-6361/202039753⟩. ⟨hal-03286624⟩
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