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.
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Journal ArticleDOI
The HOSTS Survey for Exozodiacal Dust: Observational Results from the Complete Survey
Steve Ertel,Denis Defrere,Philip M. Hinz,B. Mennesson,Grant M. Kennedy,William C. Danchi,Christopher R. Gelino,John M. Hill,William F. Hoffmann,Johan Mazoyer,George H. Rieke,Andrew Shannon,K. R. Stapelfeldt,Eckhart Spalding,Jordan M. Stone,Amali Vaz,Alycia J. Weinberger,Phil Willems,Olivier Absil,P. Arbo,Vanessa P. Bailey,C. A. Beichman,G. Bryden,E. Downey,Olivier Durney,Simone Esposito,Andras Gaspar,P. Grenz,Christopher A. Haniff,Jarron Leisenring,Lindsay Marion,T. J. McMahon,Rafael Millan-Gabet,Manny Montoya,Katie M. Morzinski,S. Perera,Enrico Pinna,J.-U. Pott,Jennifer Power,Alfio Puglisi,Aki Roberge,Eugene Serabyn,A. Skemer,Kate Y. L. Su,Vidhya Vaitheeswaran,Mark C. Wyatt +45 more
TL;DR: In this article, the results from the LBTI/Hunt for Observable Signatures of Terrestrial Systems survey for exozodiacal dust were analyzed and a 1σ median sensitivity of 23 zodis times the solar system dust surface density in its habitable zone (HZ) was estimated.
Journal ArticleDOI
THE LEECH EXOPLANET IMAGING SURVEY: CHARACTERIZATION OF THE COLDEST DIRECTLY IMAGED EXOPLANET, GJ 504 b, AND EVIDENCE FOR SUPERSTELLAR METALLICITY *
Andrew J. Skemer,Caroline V. Morley,Neil T. Zimmerman,Michael F. Skrutskie,Jarron Leisenring,Esther Buenzli,Mickael Bonnefoy,Vanessa P. Bailey,Philip M. Hinz,Denis Defrere,Simone Esposito,Daniel Apai,Beth Biller,Wolfgang Brandner,Laird M. Close,Justin R. Crepp,Robert J. De Rosa,Silvano Desidera,Josh A. Eisner,Jonathan J. Fortney,Richard S. Freedman,Thomas Henning,Karl Heinz Hofmann,T. Kopytova,Roxana Lupu,Anne-Lise Maire,Jared R. Males,Mark S. Marley,Katie M. Morzinski,Apurva Oza,Jennifer Patience,Abhijith Rajan,George H. Rieke,Dieter Schertl,Joshua E. Schlieder,Jordan M. Stone,Kate Y. L. Su,Amali Vaz,Channon Visscher,Kimberly Ward-Duong,Gerd Weigelt,Charles E. Woodward +41 more
TL;DR: In this article, Kuzuhara et al. observed GJ 504 b in three narrow L-band filters (3.71, 3.88, and 4.00 μm), spanning the red end of the broad methane fundamental absorption feature.
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1 to 2.4 micron Near-IR spectrum of the Giant Planet $\beta$ Pictoris b obtained with the Gemini Planet Imager
Jeffrey Chilcote,Laurent Pueyo,Robert J. De Rosa,Jeffrey Vargas,Bruce Macintosh,Vanessa P. Bailey,Travis Barman,Brian J. Bauman,Sebastian Bruzzone,Joanna Bulger,Adam Burrows,Andrew Cardwell,Christine Chen,Tara Cotten,Daren Dillon,René Doyon,Zachary H. Draper,Gaspard Duchene,Jennifer Dunn,Darren Erikson,Michael P. Fitzgerald,Katherine B. Follette,Donald T. Gavel,Stephen J. Goodsell,James R. Graham,Alexandra Z. Greenbaum,Markus Hartung,Pascale Hibon,Li-Wei Hung,Patrick Ingraham,Paul Kalas,Quinn Konopacky,James E. Larkin,Jérôme Maire,Franck Marchis,Mark S. Marley,Christian Marois,Stanimir Metchev,Maxwell A. Millar-Blanchaer,Katie M. Morzinski,Eric L. Nielsen,Andrew Norton,Rebecca Oppenheimer,David Palmer,Jennifer Patience,Marshall D. Perrin,Lisa Poyneer,Abhijith Rajan,Julien Rameau,Fredrik T. Rantakyrö,Naru Sadakuni,Leslie Saddlemyer,Dmitry Savransky,Adam C. Schneider,Andrew Serio,Anand Sivaramakrishnan,Inseok Song,Rémi Soummer,Sandrine Thomas,J. Kent Wallace,Jason J. Wang,Kimberly Ward-Duong,Sloane Wiktorowicz,Schuyler Wolff +63 more
TL;DR: In this paper, the Gemini Planet Imager (GPI) was used to measure the near-infrared (1.0-2.4 micron) spectrum of the planetary companion to the nearby, young star Pictoris.
Journal ArticleDOI
On the morphology and chemical composition of the hr 4796a debris disk
Timothy J. Rodigas,Christopher C. Stark,Alycia J. Weinberger,John H. Debes,Philip M. Hinz,Laird M. Close,Christine Chen,Paul S. Smith,Jared R. Males,Andrew J. Skemer,Alfio Puglisi,Katherine B. Follette,Katie M. Morzinski,Ya-Lin Wu,Runa Briguglio,Simone Esposito,Enrico Pinna,Armando Riccardi,Glenn Schneider,Marco Xompero +19 more
TL;DR: In this article, the Magellan adaptive optics system paired with Clio-2 and VisAO was used to detect the HR-4796A debris disk and found that the average width of the ring is 14 (11.1) AU.
Journal ArticleDOI
The HOSTS survey - Exozodiacal dust measurements for 30 stars
Steve Ertel,Denis Defrere,Philip M. Hinz,Bertrand Mennesson,Grant M. Kennedy,Grant M. Kennedy,William C. Danchi,Christopher R. Gelino,John M. Hill,W. F. Hoffmann,George H. Rieke,Andrew Shannon,Eckhart Spalding,Jordan M. Stone,A. Vaz,Alycia J. Weinberger,Phil Willems,Olivier Absil,P. Arbo,Vanessa P. Bailey,Chas Beichman,Geoffrey Bryden,E. Downey,O. Durney,Simone Esposito,Andras Gaspar,P. Grenz,Christopher A. Haniff,Jarron Leisenring,Lindsay Marion,T. J. McMahon,Rafael Millan-Gabet,M. Montoya,Katie M. Morzinski,Enrico Pinna,Jennifer Power,Alfio Puglisi,Aki Roberge,Eugene Serabyn,A. J. Skemer,K. Stapelfeldt,Kate Y. L. Su,Vidhya Vaitheeswaran,Mark C. Wyatt +43 more
TL;DR: In this article, the authors used nulling interferometry in the N band to suppress the bright stellar light and to probe for low levels of HZ dust around the 30 stars observed so far.