P. Delorme
Max Planck Society
4 Papers
43 Citations
P. Delorme is an academic researcher from Max Planck Society. The author has contributed to research in topics: Planet & Planetary system. The author has an hindex of 3, co-authored 4 publications.
Chat about Author
Papers
Post-conjunction detection of β Pictoris b with VLT/SPHERE
A. M. Lagrange,Anthony Boccaletti,Maud Langlois,Maud Langlois,Gael Chauvin,Gael Chauvin,Raffaele Gratton,H. Beust,Silvano Desidera,Julien Milli,Mickael Bonnefoy,Anthony Cheetham,M. Feldt,Michael Meyer,Michael Meyer,Arthur Vigan,Beth Biller,Beth Biller,Mariangela Bonavita,Mariangela Bonavita,J.-L. Baudino,Faustine Cantalloube,M. Cudel,S. Daemgen,P. Delorme,Valentina D'Orazi,Julien Girard,C. Fontanive,C. Fontanive,Janis Hagelberg,Markus Janson,Markus Janson,Miriam Keppler,T. Koypitova,Raphaël Galicher,J. Lannier,H. Le Coroller,R. Ligi,R. Ligi,Anne-Lise Maire,Dino Mesa,S. Messina,A. Mueller,S. Peretti,C. Perrot,Daniel Rouan,Graeme Salter,Matthias Samland,T. Schmidt,E. Sissa,Alice Zurlo,Alice Zurlo,Jean-Luc Beuzit,D. Mouillet,Carsten Dominik,Th. Henning,Eric Lagadec,François Ménard,H. M. Schmid,Massimo Turatto,Stéphane Udry,Alexander J. Bohn,Benjamin Charnay,C. A. Gomez Gonzales,Cecile Gry,Matthew A. Kenworthy,Quentin Kral,Christoph Mordasini,C. Moutou,G. van der Plas,Joshua E. Schlieder,Joshua E. Schlieder,L. Abe,J. Antichi,Andrea Baruffolo,Pierre Baudoz,J. Baudrand,P. Blanchard,Andreas Bazzon,Tristan Buey,M. Carbillet,M. Carle,J. Charton,Enrico Cascone,Riccardo Claudi,Anne Costille,A. Deboulbe,V. De Caprio,Kjetil Dohlen,Daniela Fantinel,P. Feautrier,Thierry Fusco,P. Gigan,Enrico Giro,D. Gisler,L. Gluck,Norbert Hubin,Emmanuel Hugot,M. Jaquet,M. Kasper,F. Madec,Yves Magnard,P. Martinez,D. Maurel,D. Le Mignant,O. Möller-Nilsson,M. Llored,Thibaut Moulin,Alain Origne,A. Pavlov,D. Perret,Cyril Petit,J. Pragt,Judit Szulágyi,Francois Wildi +114 more
TL;DR: In this article, the authors used SPHERE at the VLT to precisely monitor the orbital motion of beta Pictoris b since first light of the instrument in 2014, and were able to monitor the planet until November 2016, when its angular separation became too small (125 mas, i.e., 1.6 au) and prevented further detection.
First direct detection of a polarized companion outside a resolved circumbinary disk around CS Chamaeleonis
Christian Ginski,Myriam Benisty,R. G. van Holstein,Attila Juhasz,T. Schmidt,G. Chauvin,J. de Boer,M. Wilby,Carlo F. Manara,P. Delorme,François Ménard,P. Pinilla,T. Birnstiel,Mario Flock,Christoph U. Keller,Matthew A. Kenworthy,Julien Milli,Johan Olofsson,Laura M. Pérez,Frans Snik,N. Vogt +20 more
TL;DR: In this article, the authors investigated the circumstellar environment of the spectroscopic binary T T Tauri star CS Cha and found a smooth, low inclination disk with an outer radius of similar to 55 au (at 165 pc).
Determining mass limits around HD 163296 through SPHERE direct imaging data
Dino Mesa,Dino Mesa,Maud Langlois,Maud Langlois,Antonio Garufi,R. G. Gratton,Silvano Desidera,Valentina D'Orazi,O. Flasseur,M. Barbieri,Myriam Benisty,Myriam Benisty,Th. Henning,R. Ligi,E. Sissa,Arthur Vigan,Alice Zurlo,Alice Zurlo,Anthony Boccaletti,M. Bonnefoy,Faustine Cantalloube,G. Chauvin,Anthony Cheetham,V. De Caprio,P. Delorme,M. Feldt,Thierry Fusco,Thierry Fusco,L. Gluck,Janis Hagelberg,A. M. Lagrange,C. Lazzoni,F. Madec,Anne-Lise Maire,Anne-Lise Maire,François Ménard,Michael Meyer,Michael Meyer,Joany Andreina Manjarres Ramos,E. L. Rickman,Daniel Rouan,T. Schmidt,G. van der Plas +42 more
TL;DR: In this paper, the authors have observed HD163296 with the near-infrared (NIR) branch of SPHERE composed by IRDIS and IFS with the aim to put tight constraints on the presence of substellar companions around this star.
Statistical analysis and lessons learned of SPHERE adaptive optics performance
D. Mouillet,Julien Milli,J. F. Sauvage,T. Fusco,Jean-Luc Beuzit,Arthur Vigan,D. Albert,A. Boccaletti,Faustine Cantalloube,Gael Chauvin,Carlos Correia,P. Delorme,Kjetil Dohlen,Markus Kasper,A. M. Lagrange,N. Meunier,Cyril Pannetier +16 more
- 10 Jul 2018
TL;DR: This work revisits the most important AO specifications for future high contrast imagers as a function of the primary science goals, the targets and the turbulence properties, and quantifies the dependency of the actual performance on the most relevant environmental parameters.