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Related papers: Discovery of a warm, dusty giant planet around HIP…

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Owing to its sensitivity to wide-orbit giant exoplanets, direct imaging is uniquely positioned to shed light on the interplay between protoplanetary disks and stellar hosts. In addition to constraining formation models, new detections are…

Planetary systems hold the imprint of the formation and of the evolution of planets especially at young ages, and in particular at the stage when the gas has dissipated leaving mostly secondary dust grains. The dynamical perturbation of…

We present new radial velocity measurements of eight stars secured with the spectrograph SOPHIE at the 193-cm telescope of the Haute-Provence Observatory allowing the detection and characterization of new giant extrasolar planets. The host…

We present JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet, HIP 65426 b, with the Near-Infrared Camera (NIRCam) from 2-5 $\mu$m, and with the Mid-Infrared Instrument (MIRI) from 11-16 $\mu$m. At a…

Earth and Planetary Astrophysics · Physics 2023-07-12 Aarynn L. Carter , Sasha Hinkley , Jens Kammerer , Andrew Skemer , Beth A. Biller , Jarron M. Leisenring , Maxwell A. Millar-Blanchaer , Simon Petrus , Jordan M. Stone , Kimberly Ward-Duong , Jason J. Wang , Julien H. Girard , Dean C. Hines , Marshall D. Perrin , Laurent Pueyo , William O. Balmer , Mariangela Bonavita , Mickael Bonnefoy , Gael Chauvin , Elodie Choquet , Valentin Christiaens , Camilla Danielski , Grant M. Kennedy , Elisabeth C. Matthews , Brittany E. Miles , Polychronis Patapis , Shrishmoy Ray , Emily Rickman , Steph Sallum , Karl R. Stapelfeldt , Niall Whiteford , Yifan Zhou , Olivier Absil , Anthony Boccaletti , Mark Booth , Brendan P. Bowler , Christine H. Chen , Thayne Currie , Jonathan J. Fortney , Carol A. Grady , Alexandra Z. Greenbaum , Thomas Henning , Kielan K. W. Hoch , Markus Janson , Paul Kalas , Matthew A. Kenworthy , Pierre Kervella , Adam L. Kraus , Pierre-Olivier Lagage , Michael C. Liu , Bruce Macintosh , Sebastian Marino , Mark S. Marley , Christian Marois , Brenda C. Matthews , Dimitri Mawet , Michael W. McElwain , Stanimir Metchev , Michael R. Meyer , Paul Molliere , Sarah E. Moran , Caroline V. Morley , Sagnick Mukherjee , Eric Pantin , Andreas Quirrenbach , Isabel Rebollido , Bin B. Ren , Glenn Schneider , Malavika Vasist , Kadin Worthen , Mark C. Wyatt , Zackery W. Briesemeister , Marta L. Bryan , Per Calissendorff , Faustine Cantalloube , Gabriele Cugno , Matthew De Furio , Trent J. Dupuy , Samuel M. Factor , Jacqueline K. Faherty , Michael P. Fitzgerald , Kyle Franson , Eileen C. Gonzales , Callie E. Hood , Alex R. Howe , Masayuki Kuzuhara , Anne-Marie Lagrange , Kellen Lawson , Cecilia Lazzoni , Ben W. P. Lew , Pengyu Liu , Jorge Llop-Sayson , James P. Lloyd , Raquel A. Martinez , Johan Mazoyer , Paulina Palma-Bifani , Sascha P. Quanz , Jea Adams Redai , Matthias Samland , Joshua E. Schlieder , Motohide Tamura , Xianyu Tan , Taichi Uyama , Arthur Vigan , Johanna M. Vos , Kevin Wagner , Schuyler G. Wolff , Marie Ygouf , Xi Zhang , Keming Zhang , Zhoujian Zhang

Context. The SAO 206462 (HD 135344B) disk is one of the few known transitional disks showing asymmetric features in scattered light and thermal emission. Near-infrared scattered-light images revealed two bright outer spiral arms and an…

The new planet finder for the Very Large Telescope (VLT), the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE), just had its first light in Paranal. A dedicated instrument for the direct detection of planets, SPHERE, is…

AIMS: Using Wide-field Infrared Survey Explorer (WISE) data and previous optical and near-infrared sky surveys, we try to identify still missing stellar and substellar neighbours of the Sun. METHODS: When checking the brightest red WISE…

Solar and Stellar Astrophysics · Physics 2015-06-17 Ralf-Dieter Scholz

51 Eridani b is an exoplanet around a young (20 Myr) nearby (29.4 pc) F0-type star, recently discovered by direct imaging. Being only 0.5" away from its host star it is well suited for spectroscopic analysis using integral field…

We present observations with the planet finder SPHERE of a selected sample of the most promising radial velocity (RV) companions for high-contrast imaging. Using a Monte Carlo simulation to explore all the possible inclinations of the orbit…

T and Y-dwarfs are among the coolest and least luminous objects detected, and they can help to understand the properties of giant planets. Their multiplicity properties can shed light on the formation process. We observed a sample six T…

Solar and Stellar Astrophysics · Physics 2015-05-27 N. Huélamo , V. D. Ivanov , R. Kurtev , J. H. Girard , J. Borissova , D. Mawet , K. Muzic , C. Cáceres , C. H. F. Melo , M. F. Sterzik , D. Minniti

Transition disks correspond to a short stage between the young protoplanetary phase and older debris phase. Along this evolutionary sequence, the gas component disappears leaving room for a dust-dominated environment where already-formed…

The SIRTF Wide-area InfraRed Extragalactic survey (SWIRE), the largest SIRTF Legacy program, is a wide-area, imaging survey to trace the evolution of dusty, star-forming galaxies, evolved stellar populations, and AGN as a function of…

Atmospheric composition provides essential markers of the most fundamental properties of giant exoplanets, such as their formation mechanism or internal structure. New-generation exoplanet imagers, like VLT/SPHERE or Gemini/GPI, have been…

Instrumentation and Methods for Astrophysics · Physics 2018-06-29 A. Vigan , G. P. P. L. Otten , E. Muslimov , K. Dohlen , M. W. Phillips , U. Seemann , J. -L. Beuzit , R. Dorn , M. Kasper , D. Mouillet , I. Baraffe , A. Reiners

Young giant planets and brown dwarf companions emit near-infrared radiation that can be linearly polarized up to several percent. This polarization can reveal the presence of a circumsubstellar accretion disk, rotation-induced oblateness of…

Context. PDS 70 is a young (5.4 Myr), nearby (~113 pc) star hosting a known transition disk with a large gap. Recent observations with SPHERE and NACO in the near-infrared (NIR) allowed us to detect a planetary mass companion, PDS70b,…

We provide a detailed characterisation of the planetary system orbiting HD 85426 (TOI-1774). This bright G-type star ($M_{\ast}$: 0.99 $\text{M}_{\odot}$; $R_{\ast}$: 1.13 $\text{R}_{\odot}$; age: 7.4 Gyr; V mag: 8.25) hosts a transiting…

Only a small number of exoplanets has been identified in stellar cluster environments. We initiated a high angular resolution direct imaging search using the Hubble Space Telescope (HST) and its NICMOS instrument for self-luminous giant…

Earth and Planetary Astrophysics · Physics 2020-11-10 Wolfgang Brandner , Hans Zinnecker , Taisiya Kopytova