J
Jared R. Males
Researcher at University of Arizona
Publications - 312
Citations - 7798
Jared R. Males is an academic researcher from University of Arizona. The author has contributed to research in topics: Exoplanet & Adaptive optics. The author has an hindex of 45, co-authored 272 publications receiving 6837 citations. Previous affiliations of Jared R. Males include Steward Health Care System.
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Journal ArticleDOI
The Subaru Coronagraphic Extreme Adaptive Optics System: Enabling High-Contrast Imaging on Solar-System Scales
Nemanja Jovanovic,Nemanja Jovanovic,Frantz Martinache,Olivier Guyon,Olivier Guyon,Christophe Clergeon,Garima Singh,Garima Singh,Tomoyuki Kudo,Vincent Garrel,K. Newman,K. Newman,D. Doughty,D. Doughty,Julien Lozi,Jared R. Males,Yosuke Minowa,Yutaka Hayano,Naruhisa Takato,Jun-Ichi Morino,Jonas Kühn,Eugene Serabyn,Barnaby Norris,Peter G. Tuthill,Guillaume Schworer,Paul Stewart,Laird M. Close,Elsa Huby,Guy Perrin,Sylvestre Lacour,L. Gauchet,Sébastien Vievard,Naoshi Murakami,Fumika Oshiyama,Naoshi Baba,Taro Matsuo,Jun Nishikawa,Motohide Tamura,Motohide Tamura,Olivier Lai,Olivier Lai,Franck Marchis,Gaspard Duchêne,Gaspard Duchêne,Takayuki Kotani,Julien Woillez +45 more
TL;DR: The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument as discussed by the authors is a multiband instrument which makes use of light from 600 to 2500 nm, allowing for coronagraphic direct exoplanet imaging of the inner 3λ/D from the stellar host.
Journal ArticleDOI
Accreting protoplanets in the LkCa 15 transition disk
Steph Sallum,Katherine B. Follette,Josh A. Eisner,Laird M. Close,P. M. Hinz,Kaitlin M. Kratter,Jared R. Males,Andy Skemer,Bruce Macintosh,Peter G. Tuthill,Vanessa P. Bailey,Denis Defrere,Katie M. Morzinski,Timothy J. Rodigas,Eckhart Spalding,Amali Vaz,Alycia J. Weinberger +16 more
TL;DR: In this paper, adaptive optics observations of LkCa 15 that probe within the disk clearing are reported, with accurate source positions over multiple epochs spanning 2009-2015, infer the presence of multiple companions on Keplerian orbits.
Journal ArticleDOI
The gemini/nici planet-finding campaign: the frequency of planets around young moving group stars*
Beth Biller,Michael C. Liu,Zahed Wahhaj,Eric L. Nielsen,Thomas L. Hayward,Jared R. Males,Andrew J. Skemer,Laird M. Close,Mark Chun,Christ Ftaclas,Fraser Clarke,Niranjan Thatte,Evgenya L. Shkolnik,I. Neill Reid,Markus Hartung,Alan P. Boss,Douglas N. C. Lin,Silvia H. P. Alencar,Elisabete M. de Gouveia Dal Pino,Jane Gregorio-Hetem,Douglas W. Toomey +20 more
TL;DR: In this paper, the authors report results of a direct imaging survey for giant planets around 80 members of the? Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI Planet Finding Campaign.
Journal ArticleDOI
HD?106906?b: A Planetary-mass Companion Outside a Massive Debris Disk
Vanessa P. Bailey,Tiffany Meshkat,Megan Reiter,Katie M. Morzinski,Jared R. Males,Kate Y. L. Su,Philip M. Hinz,Matthew A. Kenworthy,Daniel P. Stark,Eric E. Mamajek,Runa Briguglio,Laird M. Close,Katherine B. Follette,Alfio Puglisi,Timothy J. Rodigas,Timothy J. Rodigas,Alycia J. Weinberger,Marco Xompero +17 more
TL;DR: In this paper, the Magellan Adaptive Optics (MAGAO) + Clio2 system was used to detect a planetary-mass companion, HD?106906 b, at a projected separation of 7''1 (650 AU).
Journal ArticleDOI
FIRST LIGHT LBT AO IMAGES OF HR 8799 bcde AT 1.6 AND 3.3 μm: NEW DISCREPANCIES BETWEEN YOUNG PLANETS AND OLD BROWN DWARFS*
Andrew J. Skemer,Philip M. Hinz,Simone Esposito,Adam Burrows,Jarron Leisenring,Michael F. Skrutskie,Silvano Desidera,Dino Mesa,Carmelo Arcidiacono,Filippo Mannucci,Timothy J. Rodigas,Laird M. Close,Donald W. McCarthy,Craig Kulesa,Guido Agapito,Daniel Apai,Javier Argomedo,Vanessa P. Bailey,K. Boutsia,Runa Briguglio,Guido Brusa,Lorenzo Busoni,Riccardo Claudi,Joshua Eisner,Luca Fini,Katherine B. Follette,Peter M. Garnavich,Raffaele Gratton,J. C. Guerra,John M. Hill,William F. Hoffmann,Terry J. Jones,M. Krejny,Jared R. Males,Elena Masciadri,Michael Meyer,Douglas L. Miller,Katie M. Morzinski,Matthew J. Nelson,Enrico Pinna,Alfio Puglisi,Sascha P. Quanz,Fernando Quiros-Pacheco,Armando Riccardi,P. Stefanini,Vidhya Vaitheeswaran,John C. Wilson,Marco Xompero +47 more
TL;DR: In this paper, the spectral energy distribution of the HR 8799 planets is modeled as a mixture of clouds of varying opacity, similar to the patchy cloud structures on Jupiter and L/T transition brown dwarfs.