Arthur Vigan
Aix-Marseille University
468 Papers
3.6K Citations
Arthur Vigan is an academic researcher from Aix-Marseille University. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 60, co-authored 416 publications. Previous affiliations of Arthur Vigan include University of Exeter & University of New South Wales.
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Papers
A narrow, edge-on disk resolved around HD 106906 with SPHERE
A-M. Lagrange,A-M. Lagrange,Maud Langlois,Maud Langlois,Raffaele Gratton,Anne-Lise Maire,Anne-Lise Maire,Julien Milli,Johan Olofsson,Johan Olofsson,Arthur Vigan,Arthur Vigan,Vanessa P. Bailey,Dino Mesa,Gael Chauvin,Gael Chauvin,Anthony Boccaletti,Raphael Galicher,Julien Girard,Mickael Bonnefoy,Mickael Bonnefoy,Matthias Samland,François Ménard,Thomas Henning,Matthew A. Kenworthy,Christian Thalmann,Hervé Beust,Hervé Beust,J. L. Beuzit,J. L. Beuzit,Wolfgang Brandner,Esther Buenzli,Esther Buenzli,Anthony Cheetham,Markus Janson,H. Le Coroller,H. Le Coroller,J. Lannier,J. Lannier,David Mouillet,David Mouillet,S. Peretti,Clément Perrot,Graeme Salter,E. Sissa,Zahed Wahhaj,Lyu Abe,Silvano Desidera,Markus Feldt,F. Madec,D. Perret,Cyril Petit,P. Rabou,P. Rabou,C. Soenke,L. Weber +55 more
TL;DR: In this article, the authors used the IRDIS imager and the Integral Field Spectrometer (IFS) to detect a highly inclined, ring-like disk at a distance of 65 au from the star.
Molecular line mapping of the giant molecular cloud associated with RCW 106 - II. Column density and dynamical state of the clumps
Tony Wong,Tony Wong,Tony Wong,E. F. Ladd,D. Brisbin,D. Brisbin,Michael G. Burton,Indra Bains,Indra Bains,Maria Cunningham,Nadia Lo,Nadia Lo,Paul A. Jones,K. L. Thomas,Steven N. Longmore,Steven N. Longmore,Steven N. Longmore,Arthur Vigan,Bhaswati Mookerjea,Bhaswati Mookerjea,Carsten Kramer,Yasuo Fukui,Akiko Kawamura +22 more
TL;DR: In this article, the authors present a fully sampled C 18 O (1-0) map towards the southern giant molecular cloud (GMC) associated with the H II region RCW 106, and use it to estimate the gas column density as a function of position and velocity.
Asteroid (16) Psyche’s primordial shape: A possible Jacobi ellipsoid
Marin Ferrais,Pierre Vernazza,Laurent Jorda,Nicolas Rambaux,Josef Hanus,Benoit Carry,F. Marchis,F. Marchis,Michael Marsset,Matti Viikinkoski,Miroslav Brož,Romain Fétick,Alexis Drouard,Thierry Fusco,M. Birlan,M. Birlan,E. Podlewska-Gaca,E. Podlewska-Gaca,Emmanuel Jehin,P. Bartczak,Jérôme Berthier,Julie Castillo-Rogez,Fabrice Cipriani,François Colas,Grzegorz Dudziński,Christophe Dumas,Josef Ďurech,Mikko Kaasalainen,Agnieszka Kryszczyńska,P. Lamy,H. Le Coroller,A. Marciniak,Tadeusz Michalowski,Patrick Michel,Toni Santana-Ros,Toni Santana-Ros,Paolo Tanga,F. Vachier,Arthur Vigan,Olivier Witasse,Bin Yang +40 more
TL;DR: In this article, the shape and bulk density of (16) Psyche were analyzed using two independent shape modeling algorithms (MPCD and ADAM) and a shape analysis was performed, including a comparison with equilibrium figures and the identification of mass deficit regions.
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 μm
Aarynn L. Carter,Sasha Hinkley,C. Kammerer,Andrew J. Skemer,Beth Biller,Jarron Leisenring,Maxwell A. Millar-Blanchaer,S. Petrus,Jordan M. Stone,Kimberly Ward-Duong,Jason J. Wang,Julien Girard,Dean C. Hines,Marshall D. Perrin,Laurent Pueyo,W. Balmer,Mariangela Bonavita,Mickael Bonnefoy,Gael Chauvin,Elodie Choquet,Valentin Christiaens,Camilla Danielski,R. Kennedy,Elisabeth Matthews,Brittany E. Miles,Polychronis Patapis,S. Ray,E. L. Rickman,Steph Sallum,Karl R. Stapelfeldt,Niall Whiteford,Yifan Zhou,Olivier Absil,Anthony Boccaletti,Mark Booth,Brendan P. Bowler,Christine Chen,Thayne Currie,Jonathan J. Fortney,Carol A. Grady,Alexandra Z. Greenbaum,Th. 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 Meyer,Paul Mollière,Sarah E. Moran,Caroline V. Morley,Sagnick Mukherjee,Eric Pantin,Andreas Quirrenbach,I. Rebollido,Bin Ren,O. Schneider,Malavika Vasist,Kadin Worthen,Mark C. Wyatt,Zackery Briesemeister,Marta L. Bryan,Per Calissendorff,Faustine Cantalloube,G. Cugno,Matthew De Furio,Trent J. Dupuy,Samuel Factor,Jacqueline K. Faherty,Michael P. Fitzgerald,Kyle Franson,Eileen C. Gonzales,Callie Hood,Alex R. Howe,Masayuki Kuzuhara,Anne-Marie Lagrange,Kellen Lawson,C. Lazzoni,Ben W. P. Lew,Peng Li,Jorge Llop-Sayson James P. Lloyd,Raquel A. Martinez,Johan Mazoyer,Sascha P. Quanz,J. A. Redai,Matthias Samland,Joshua E. Schlieder,Motohide Tamura,Xianyu Tan,Taichi Uyama,Arthur Vigan,Johanna M. Vos,Kevin Wagner,Schuyler Wolff,Marie Ygouf,Xi Zhang,Keming Zhang,Zhoujian Zhang +108 more
TL;DR: In this article , the authors presented JWST Early Release Science coronagraphic observations of the super-Jupiter exoplanet HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 μm, and with the Mid Infrared Instrument (MIRI) from 11 to 16 μm.
Orbit and atmosphere of HIP 99770 b through the eyes of VLTI/GRAVITY
T. Winterhalder,S. Lacour,A. M'erand,M. Nowak,T. Stolker,G.-D. Marleau,A. Amorim,J. Berger,Hervé Beust,S. Blunt,Mickael Bonnefoy,H. Bonnet,M. S. Bordoni,G. Bourdarot,Faustine Cantalloube,Gael Chauvin,Valentin Christiaens,Y. Cl'enet,R. Davies,Roderick Dembet,J. Dexter,Antonia Drescher,A. Eckart,Frank Eisenhauer,N. M. Förster Schreiber,T. Gardner,E. Gendron,R. Genzel,Stefan Gillessen,S. Grant,Xavier Haubois,T. Henning,Sasha Hinkley,Stephen E Hippler,M. Houll'e,Z. Hubert,Laurent Jocou,Miriam Keppler,Pierre Kervella,Nicolás T. Kurtovic,D. Lutz,Anne-Lise Maire,C. Mordasini,David Mouillet,E. Nasedkin,G. Otten,Thibaut Paumard,Karine Perraut,G. Perrin,N. Pourr'e,D. C. Ribeiro,Zafar Rustamkulov,T. Shimizu,D. Sing,Julia Stadler,L.J. Tacconi,Ewine F. van Dishoeck,Arthur Vigan,F. H. Vincent,S. von Fellenberg,Felix Widmann,J. Woillez,Senol Yazici,the Gravity Collaboration +63 more
- 27 Jun 2025