R
Remi A. Cabanac
Researcher at University of Toulouse
Publications - 101
Citations - 4244
Remi A. Cabanac is an academic researcher from University of Toulouse. The author has contributed to research in topics: Galaxy & Weak gravitational lensing. The author has an hindex of 30, co-authored 100 publications receiving 3695 citations. Previous affiliations of Remi A. Cabanac include Los Angeles Trade–Technical College & Centre national de la recherche scientifique.
Papers
More filters
Journal ArticleDOI
Large-scale magnetic topologies of early M dwarfs
Jean-François Donati,Julien Morin,Pascal Petit,X. Delfosse,T. Forveille,Michel Aurière,Remi A. Cabanac,B. Dintrans,Rim Fares,Thomas Gastine,Moira Jardine,François Lignières,Frédéric Paletou,J. C. Ramirez Velez,S. Théado +14 more
TL;DR: In this article, a small sample of stars ranging from spectral type M0 to M8 was used to investigate how dynamo processes operate in stars on both sides of the full convection threshold (spectral type M4).
Journal ArticleDOI
Large-scale magnetic topologies of early M dwarfs
Julien Morin,Jean-François Donati,Pascal Petit,Xavier Delfosse,Thierry Forveille,Loic Albert,Michel Aurière,Remi A. Cabanac,B. Dintrans,Rim Fares,Thomas Gastine,Moira Jardine,François Lignières,Frédéric Paletou,J. C. Ramirez Velez,S. Théado +15 more
TL;DR: In this paper, the authors used tomographic imaging techniques to determine the rotation period and reconstruct the large-scale magnetic topologies of six early M dwarfs, and they found that early-M stars preferentially host large scale fields with dominantly toroidal and non-axisymmetric poloidal configurations, along with significant differential rotation.
Journal Article
The UVES Paranal Observatory Project: A Library of High- Resolution Spectra of Stars across the Hertzsprung-Russell Diagram
Journal ArticleDOI
The CFHTLS strong lensing legacy survey - I. Survey overview and T0002 release sample
Remi A. Cabanac,C. Alard,M. Dantel-Fort,Bernard Fort,Raphael Gavazzi,P. Gomez,Jean-Paul Kneib,O. Le Fevre,Yannick Mellier,Yannick Mellier,R. Pello,Genevieve Soucail,J.-F. Sygnet,D. Valls-Gabaud,D. Valls-Gabaud +14 more
TL;DR: In this paper, the authors presented a preliminary sample of about 40 strong lensing candidates discovered in the CFHTLS T0002 release, covering an effective field of view of 28 deg$^2$, consisting mainly of gravitational arc systems with splitting angles between 2 and 15 arcsec.
Journal ArticleDOI
Deep Impact: Observations from a worldwide Earth-based campaign
Karen J. Meech,N. Ageorges,Michael F. A'Hearn,Claude Arpigny,A. Ates,J. Aycock,Stefano Bagnulo,Jeremy Bailey,Rosemary Barber,L. Barrera,R. Barrena,James M. Bauer,M. J. S. Belton,F. Bensch,Bidushi Bhattacharya,N. Biver,Geoffrey A. Blake,Dominique Bockelée-Morvan,Hermann Boehnhardt,Boncho P. Bonev,Tanyu Bonev,Marc W. Buie,Michael G. Burton,Harold M. Butner,Remi A. Cabanac,Randy D. Campbell,Humberto Campins,Maria Teresa Capria,T. Carroll,F. Chaffee,Steven B. Charnley,R. Cleis,Andrew J. Coates,Anita L. Cochran,P. Colom,Al Conrad,Iain Coulson,Jacques Crovisier,J. Debuizer,Richard Dekany,J. de León,N. Dello Russo,A. Delsanti,Michael A. DiSanti,Jack D. Drummond,L. Dundon,P.B. Etzel,Tony L. Farnham,Paul D. Feldman,Yanga R. Fernandez,Miroslav Filipovic,S. Fisher,Alan Fitzsimmons,D. Fong,R. Fugate,Haruhiko Fujiwara,Takuya Fujiyoshi,R. Furusho,Tetsuharu Fuse,Erika L. Gibb,Olivier Groussin,Samuel Gulkis,Mark Gurwell,Edith Hadamcik,Olivier Hainaut,David E. Harker,D. Harrington,Martin Harwit,Sunao Hasegawa,Carl Hergenrother,Paul Hirst,Klaus-Werner Hodapp,Mitsuhiko Honda,Ellen S. Howell,Damien Hutsemekers,Daisuke Iono,Wing-Huen Ip,William M. Jackson,Emmanuel Jehin,Z.J. Jiang,Geraint H. Jones,Paul A. Jones,Toshihiko Kadono,U.W. Kamath,H. U. Kaufl,Toshihiro Kasuga,Hideyo Kawakita,Michael S. P. Kelley,Florian Kerber,M. Kidger,Daisuke Kinoshita,Matthew M. Knight,Luisa Lara,S. M. Larson,Susan M. Lederer,Choogon Lee,Anny Chantal Levasseur-Regourd,Jianguo Li,Qiang Li,Javier Licandro,Zhong-Yi Lin,Carey M. Lisse,G. LoCurto,Amy J. Lovell,Stephen C. Lowry,James E. Lyke,David K. Lynch,J. Ma,Karen Magee-Sauer,G. Maheswar,Jean Manfroid,O. Marco,Pierre Martin,Gary J. Melnick,Steve Miller,Takaki Miyata,Gerald Moriarty-Schieven,N. Moskovitz,B. E. A. Mueller,Michael J. Mumma,S. Muneer,David A. Neufeld,Takafumi Ootsubo,David J. Osip,S.K. Pandea,Eric Pantin,Rachel Paterno-Mahler,Brian M. Patten,Bryan E. Penprase,Alison B. Peck,G. Petitas,Noemi Pinilla-Alonso,J. Pittichova,Emanuela Pompei,Tushar P. Prabhu,Chunhua Qi,Ramprasad Rao,Heike Rauer,Harold J. Reitsema,S.D. Rodgers,P. Rodriguez,R. Ruane,G. Ruch,Wiphu Rujopakarn,D. K. Sahu,Shigeyuki Sako,Itsuki Sakon,Nalin H. Samarasinha,John Sarkissian,Ivo Saviane,M. Schirmer,Peter H. Schultz,Rita Schulz,Patrick Seitzer,Tomohiko Sekiguchi,Fernando Selman,Miquel Serra-Ricart,R. G. Sharp,Ronald L. Snell,Colin Snodgrass,Tom Stallard,G. R. Stecklein,Christiaan Sterken,J. A. Stüwe,Seiji Sugita,M. Sumner,Nicholas B. Suntzeff,R. Swaters,Shigehisa Takakuwa,Naruhisa Takato,J. E. Thomas-Osip,E. Thompson,Alan T. Tokunaga,G. P. Tozzi,H. Tran,Mitchell Troy,Chadwick A. Trujillo,J. van Cleve,R. Vasundhara,Roberto Vázquez,Faith Vilas,Geronimo L. Villanueva,K. von Braun,Patrick M. Vora,Richard J. Wainscoat,Kevin J. Walsh,J. Watanabe,Harold A. Weaver,W. Weaver,M. Weiler,Paul R. Weissman,William F. Welsh,David J. Wilner,Scott J. Wolk,Maria Womack,Diane H. Wooden,L. M. Woodney,Chick E Woodward,Z.-Y. Wu,J.-H. Wu,T. Yamashita,Bin Yang,Y.-B. Yang,S. Yokogawa,A. C. Zook,A. Zauderer,X. Zhao,Xin Zhou,J.-M. Zucconi +208 more
TL;DR: Data show that there was new material after impact that was compositionally different from that seen before impact, and the ratio of dust mass to gas mass in the ejecta was much larger than before impact.