Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Terry Pfister"'
Publikováno v:
SPIE Proceedings.
The Keck Cosmic Web Imager (KCWI) is a new facility instrument being developed for the W. M. Keck Observatory and funded for construction by the Telescope System Instrumentation Program (TSIP) of the National Science Foundation (NSF). KCWI is a bench
Autor:
Terry Pfister, Nobuhiko P. Kobayashi, Michael Bolte, Andrew C. Phillips, Christopher Ratliff, David Cowley, David M. Fryauf, Brian DuPraw
Publikováno v:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation.
We describe progress in the on-going effort at the University of California Observatories Advanced Coatings Lab to develop efficient, durable silver-based coatings for telescope mirrors. We have continued to improve previously identified recipes prod
Autor:
Jennifer Burt, Jeffrey Lewis, Steven S. Vogt, Eugenio J. Rivera, Sandra M. Faber, Maureen McLean, William Deich, Sandy Keiser, Brad Holden, Tony Misch, Myra Katsuki, John Wareham, Mingzhi Wei, Greg Laughlin, David F. Hilyard, Steve Allen, Lee Laiterman, Dick Kanto, Elinor L. Gates, Mike Saylor, Richard J. Stover, Mike Bolte, Wayne Earthman, Robert I. Kibrick, Kyle Lanclos, Jerry Cabak, Kostas Chloros, Chris Wright, Matthew Thompson, Debra A. Fischer, Michael Peck, Paul Lynam, Matthew Radovan, Geoffrey W. Marcy, Andrew L. Phillips, Joseph S. Miller, David Cowley, James Ward, Chris Lockwood, R. Paul Butler, Brian DuPraw, Barry Alcott, Bernie Walp, Pamela Arriagada, Ken Johnston, Terry Pfister, Dale Sandford, Harland W. Epps
The Automated Planet Finder (APF) is a facility purpose-built for the discovery and characterization of extrasolar planets through high-cadence Doppler velocimetry of the reflex barycentric accelerations of their host stars. Located atop Mt. Hamilton
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c62f58dc83463ac54890d7665514598
http://arxiv.org/abs/1402.6684
http://arxiv.org/abs/1402.6684
Autor:
Daren Dillon, David Cowley, Terry Pfister, William Deich, Elinor L. Gates, Jerry Cabak, Jim Ward, Christopher Ratliff, Renate Kupke, Donald Gavel, Mike Saylor
A Cassegrain mounted adaptive optics instrument presents unique challenges for opto-mechanical design. The flexure and temperature tolerances for stability are tighter than those of seeing limited instruments. This criteria requires particular attent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83e0d32c63b7a3d176fbf9a34b7d7d1b
Autor:
Renate Kupke, Terry Pfister, Jim Ward, Rosalie McGurk, William Deich, Srikar Srinath, C. M. Rockosi, Jerry Cabak, Chris Ratliff, Kyle Lanclos, Andrew L. Phillips, Andrew P. Norton, John Gates, Michael Saylor, Michael Peck, Donald Gavel, Daren Dillon
A new high-order adaptive optics system is now being commissioned at the Lick Observatory Shane 3-meter telescope in California. This system uses a high return efficiency sodium beacon and a combination of low and high-order deformable mirrors to ach
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d82a649a5b322490954d22e6af41f65f
Autor:
Constance M. Rockosi, Michael Peck, John Gates, Donald T. Gavel, Jason Weiss, Barry Alcott, Srikar Srinath, Renate Kupke, David Cowley, William Deich, Terry Pfister, Daren Dillon, Jim Ward, Dale Sandford, Mike Saylor, Kyle Lanclos, Rosalie C. McGurk, Andrew Norton, Elinor L. Gates
We describe the design and first-light early science performance of the Shane Adaptive optics infraRed Camera-Spectrograph (ShARCS) on Lick Observatory's 3-m Shane telescope. Designed to work with the new ShaneAO adaptive optics system, ShARCS is cap
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::487bc5606e5ea5783b43364dd21048c3
Autor:
David Kirk Gilmore, Robert I. Kibrick, Terry Pfister, Barry Alcott, Chris Wright, David Cowley
Publikováno v:
SPIE Proceedings.
The DEep Imaging Multi-Object Spectrograph (DEIMOS) images with an 8K x 8K science mosaic composed of eight 2K x 4K MIT/Lincoln Lab (MIT/LL) CCDs. It also incorporates two 1200 x 600 Orbit Semiconductor CCDs for active, close-loop flexure compensatio
Publikováno v:
SPIE Proceedings.
DEIMOS is a large multi-object spectrograph with an imaging mode that is being built for the W. M. Keck 2 Telescope. The detector is a 2 X 4 mosaic of eight 2048 X 4096 pixel CCDs. The mosaic assembly process must position the CCDs to be planar to wi
Autor:
Dean Tucker, David F. Hilyard, Michael J. Keane, Neal Jern, William E. Brown, E. Horn, M. Couture, Gerard H. Pardeilhan, T. Ricketts, Al Conrad, Robert I. Kibrick, Steven S. Vogt, Steven L. Allen, Richard J. Stover, Conor P. Delaney, Darrie Hilyard, James W. Lewis, Harland W. Epps, L. Bresee, Terry Pfister, Janice M. Ward, Bruce C. Bigelow, Jack Osborne, Dick Kanto, Lloyd B. Robinson, T. Cantrall, Mingzhi Wei
Publikováno v:
Instrumentation in Astronomy VIII.
We describe the high resolution echelle spectrometer (HIRES) now in operation on the Keck Telescope. HIRES, which is permanently located at a Nasmyth focus, is a standard in-plane echelle spectrometer with grating post dispersion. The collimated beam
Conference
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