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KPF: Keck Planet Finder

Gibson, Steven R. and Howard, Andrew W. and Marcy, Geoffrey W. and Edelstein, Jerry and Wishnow, Edward H. and Poppett, Claire L. (2016) KPF: Keck Planet Finder. In: Ground-based and Airborne Instrumentation for Astronomy VI. Proceedings of SPIE. No.9908. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 990870. ISBN 978-1-5106-0196-3. http://resolver.caltech.edu/CaltechAUTHORS:20170629-115638990

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Abstract

KPF is a fiber-fed, high-resolution, high-stability spectrometer in development at the UC Berkeley Space Sciences Laboratory for the W.M. Keck Observatory. The instrument is designed to characterize exoplanets via Doppler spectroscopy with a single measurement precision of 0.5ms_(-1) or better, however its resolution and stability will enable a wide variety of astrophysical pursuits. KPF will have a 200mm collimated beam diameter and a resolving power of >80,000. The design includes a green channel (440nm to 590 nm) and red channel (590nm to 850 nm). A novel design aspect of KPF is the use of a Zerodur optical bench, and Zerodur optics with integral mounts, to provide stability against thermal expansion and contraction effects.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1117/12.2233334DOIArticle
http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=2544281PublisherArticle
ORCID:
AuthorORCID
Howard, Andrew W.0000-0001-8638-0320
Marcy, Geoffrey W.0000-0002-2909-0113
Additional Information:© 2016 Society of Photo-Optical Instrumentation Engineers. The authors thank the W.M. Keck Foundation, the Heising-Simons Foundation, the University of California, Berkeley, and the University of Hawai'i for financial support of KPF. The authors also wish to thank the technical and engineering staff at the W.M. Keck Observatory (in particular Sean Adkins), as well as Connie Rockosi, David Cowley, and Dale Sandford of the University of California Observatories detector group. The contributions of Daniel Finstad, Yuzo Ishikawa, Tim Miller, Jeremy McCauley and Christopher Smith of the Space Sciences Laboratory are also noted, along with Trish Dobson and the Lab's administrative support team.
Funders:
Funding AgencyGrant Number
W. M. Keck FoundationUNSPECIFIED
Heising-Simons FoundationUNSPECIFIED
University of California, BerkeleyUNSPECIFIED
University of HawaiiUNSPECIFIED
Subject Keywords:Spectrometer, exoplanets, Doppler spectroscopy, Zerodur
Record Number:CaltechAUTHORS:20170629-115638990
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170629-115638990
Official Citation:Steven R. Gibson ; Andrew W. Howard ; Geoffrey W. Marcy ; Jerry Edelstein ; Edward H. Wishnow ; Claire L. Poppett; KPF: Keck Planet Finder . Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 990870 (August 9, 2016); doi:10.1117/12.2233334.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:78693
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:30 Jun 2017 17:40
Last Modified:21 Aug 2017 20:22

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