K
Katie M. Morzinski
Researcher at University of Arizona
Publications - 227
Citations - 10232
Katie M. Morzinski 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 55, co-authored 215 publications receiving 9280 citations. Previous affiliations of Katie M. Morzinski include National Science Foundation & Lawrence Livermore National Laboratory.
Papers
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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
The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU
Eric L. Nielsen,Robert J. De Rosa,Bruce Macintosh,Jason J. Wang,Jean-Baptiste Ruffio,Eugene Chiang,Mark S. Marley,Didier Saumon,Dmitry Savransky,S. Mark Ammons,Vanessa P. Bailey,Travis Barman,Celia Blain,Joanna Bulger,Jeffrey Chilcote,Tara Cotten,Ian Czekala,René Doyon,Gaspard Duchene,Thomas M. Esposito,Daniel C. Fabrycky,Michael P. Fitzgerald,Katherine B. Follette,Jonathan J. Fortney,Benjamin L. Gerard,Stephen J. Goodsell,James R. Graham,Alexandra Z. Greenbaum,Pascale Hibon,Sasha Hinkley,Lea A. Hirsch,Justin Hom,Li-Wei Hung,Rebekah I. Dawson,Patrick Ingraham,Paul Kalas,Quinn Konopacky,James E. Larkin,Eve J. Lee,Jonathan W. Lin,Jérôme Maire,Franck Marchis,Christian Marois,Stanimir Metchev,Maxwell A. Millar-Blanchaer,Katie M. Morzinski,Rebecca Oppenheimer,D. M. Palmer,Jennifer Patience,Marshall D. Perrin,Lisa Poyneer,Laurent Pueyo,Roman R. Rafikov,Abhijith Rajan,Julien Rameau,Fredrik T. Rantakyrö,Bin Ren,Adam C. Schneider,Anand Sivaramakrishnan,Inseok Song,Rémi Soummer,Melisa Tallis,Sandrine Thomas,Kimberly Ward-Duong,Schuyler Wolff +64 more
TL;DR: In this paper, a statistical analysis of the first 300 stars observed by the Gemini Planet Imager Exoplanet Survey (GPIES) includes six detected planets and three brown dwarfs; from these detections and their contrast curves, infer the underlying distributions of substellar companions with respect to their mass, semi-major axis, and host stellar mass.
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.
Journal ArticleDOI
First Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: 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,Juan Carlos Guerra,John M. Hill,William F. Hoffmann,Terry Jones,Megan 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 authors used the LBT adaptive optics system, PISCES, and LBTI/LMIRCam to image all four of the HR 8799 planets at H-band and 3.3 microns.
Proceedings ArticleDOI
The Gemini Planet Imager
Bruce Macintosh,James R. Graham,David Palmer,René Doyon,Donald T. Gavel,James E. Larkin,Ben R. Oppenheimer,L. Saddlemyer,J. Kent Wallace,Brian J. Bauman,Julia W. Evans,Darren Erikson,Katie M. Morzinski,Donald W. Phillion,Lisa Poyneer,Anand Sivaramakrishnan,Rémi Soummer,Simon Thibault,Jean-Pierre Véran +18 more
TL;DR: The Gemini Planet Imager (GPI) as discussed by the authors is a system for direct imaging of the planets themselves, which can achieve contrast levels of 10-7 to 10-8, sufficient to detect warm self-luminous Jovian planets.