iLocater: a diffraction-limited Doppler spectrometer for the Large Binocular Telescope
AuthorCrepp, Justin R.
Gaudi, B S.
Kratter, Kaitlin M.
AffiliationUniv Arizona, Steward Observ, Dept Astron
MetadataShow full item record
PublisherSPIE-INT SOC OPTICAL ENGINEERING
CitationJustin R. Crepp ; Jonathan Crass ; David King ; Andrew Bechter ; Eric Bechter ; Ryan Ketterer ; Robert Reynolds ; Philip Hinz ; Derek Kopon ; David Cavalieri ; Louis Fantano ; Corina Koca ; Eleanya Onuma ; Karl Stapelfeldt ; Joseph Thomes ; Sheila Wall ; Steven Macenka ; James McGuire ; Ronald Korniski ; Leonard Zugby ; Joshua Eisner ; B S. Gaudi ; Fred Hearty ; Kaitlin Kratter ; Marc Kuchner ; Giusi Micela ; Matthew Nelson ; Isabella Pagano ; Andreas Quirrenbach ; Christian Schwab ; Michael Skrutskie ; Alessandro Sozzetti ; Charles Woodward and Bo Zhao " iLocater: a diffraction-limited Doppler spectrometer for the Large Binocular Telescope ", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 990819 (August 4, 2016); doi:10.1117/12.2233135; http://dx.doi.org/10.1117/12.2233135
Rights© 2016 SPIE
Collection InformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at firstname.lastname@example.org.
AbstractWe are developing a stable and precise spectrograph for the Large Binocular Telescope (LBT) named "iLocater." The instrument comprises three principal components: a cross-dispersed echelle spectrograph that operates in the YJ-bands (0.97-1.30 mu m), a fiber-injection acquisition camera system, and a wavelength calibration unit. iLocater will deliver high spectral resolution (R similar to 150,000-240,000) measurements that permit novel studies of stellar and substellar objects in the solar neighborhood including extrasolar planets. Unlike previous planet-finding instruments, which are seeing-limited, iLocater operates at the diffraction limit and uses single mode fibers to eliminate the effects of modal noise entirely. By receiving starlight from two 8.4m diameter telescopes that each use "extreme" adaptive optics (AO), iLocater shows promise to overcome the limitations that prevent existing instruments from generating sub-meter-per-second radial velocity (RV) precision. Although optimized for the characterization of low-mass planets using the Doppler technique, iLocater will also advance areas of research that involve crowded fields, line-blanketing, and weak absorption lines.
VersionFinal published version