Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Kenneth G. Magnone"'
Autor:
Nils-Erik Rundquist, Andrea Zonca, Arun Surya, Shelley A. Wright, Aaron Brown, Maren Cosens, Michael Fitzgerald, Chris Johnson, Marc Kassis, Renate Kupke, Kyle Lanclos, James E. Larkin, Kenneth G. Magnone, Rosalie C. McGurk, Ji Man Sohn, Gregory Walth, James H. Wiley, Sherry Yeh
Liger is a second generation near-infrared imager and integral field spectrograph (IFS) for the W. M. Keck Observatory that will utilize the capabilities of the Keck All-sky Precision Adaptive-optics (KAPA) system. Liger operates at a wavelength rang
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c05fc32a69c9b8b47f99dc2bf96eeb79
http://arxiv.org/abs/2208.07937
http://arxiv.org/abs/2208.07937
Autor:
Sylvain Cetre, Nick Suominen, Mark Chun, Randall Bartos, Benjamin Calvin, Tobias Schofield, Charlotte Z. Bond, Greg W. Doppmann, Nemanja Jovanovic, Daniel Echeverri, Michael P. Fitzgerald, Evan Morris, Peter Wizinowich, Sam Ragland, Jorge Llop Sayson, E. Wetherell, Chris Johnson, Jean-Baptiste Ruffio, Ronald Lopez, J. Kent Wallace, Scott Lilley, Dimitri Mawet, Jacklyn Pezzato, Ji M. Sohn, Andrew J. Skemer, Eric Wang, Kenneth G. Magnone, Emily C. Martin, Jacques-Robert Delorme, Jason J. Wang, Garreth Ruane
The Keck Planet Imager and Characterizer (KPIC) is a purpose-built instrument to demonstrate technological and instrumental concepts initially developed for the exoplanet direct imaging field. Located downstream of the current Keck II adaptive optic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c8fa266170efac3ba6bdab306c4b3f2
https://resolver.caltech.edu/CaltechAUTHORS:20211006-171113651
https://resolver.caltech.edu/CaltechAUTHORS:20211006-171113651
Autor:
Chris Johnson, Theodore Aliado, Sean M. Adkins, James E. Lyke, James E. Larkin, Michael P. Fitzgerald, Ji Man Sohn, Eric Wang, Anna Boehle, Kenneth G. Magnone, Jason Weiss
Publikováno v:
SPIE Proceedings.
We present the results of the upgrade of the spectrograph detector in the integral field spectrograph, OSIRIS. OSIRIS is a near-infrared (1 to 2.5 microns) integral field spectrograph on the Keck I telescope. This instrument produces up to 3,000 spec
Autor:
Ian S. McLean, Carlos Quiroz, Bruce Macintosh, Brian J. Bauman, James E. Larkin, Quinn Konopacky, Jérôme Maire, James R. Graham, Chris Johnson, Daren Dillon, Markus Hartung, Simon Thibault, George Brims, Marshall D. Perrin, John Canfield, Evan Kress, Naru Sadakuni, Pascale Hibon, Leslie Saddlemyer, David Palmer, Philippe Vallée, Jennifer Dunn, Andrew Cardwell, Michael P. Fitzgerald, Sandrine Thomas, René Doyon, Theodore Aliado, Andrew Serio, Fredrik T. Rantakyrö, Jeffrey Chilcote, Kenneth G. Magnone, Patrick Ingraham, Stephen J. Goodsell, Jason Weiss
The Gemini Planet Imager (GPI) is a complex optical system designed to directly detect the self-emission of young planets within two arcseconds of their host stars. After suppressing the starlight with an advanced AO system and apodized coronagraph,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2fe456f8bc19f2a36a31e448bb84078
http://arxiv.org/abs/1407.2314
http://arxiv.org/abs/1407.2314
Autor:
Eric E. Becklin, Evan Kress, Erin C. Smith, Kenneth G. Magnone, George Brims, A. Oldag, T. Silvers, Gunnar E. Skulason, John Milburn, Ralph Y. Shuping, Ian S. McLean, Theodore Aliado
Publikováno v:
SPIE Proceedings.
FLITECAM is a 1-5 micron infrared camera for NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA). A 1024 ×1024 InSb ALADDIN III detector and large refractive optics provide a field of view of almost 8 arc minutes in diameter with a scale