New Results from the Multi-Object Keck Exoplanet Tracker

Details New Results from the Multi-Object Keck Exoplanet Tracker New Results from the Multi-Object Keck Exoplanet Tracker

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007rmxac..29..151v&link_type=abstract

First Light Science with the GTC (Eds. R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa, & S. Torres-Peimbert) Revista Mexicana d

Astronomy and Astrophysics

Astronomy

1

Instrumentation: Interferometers, Instrumentation: Spectrographs, Planetary Systems, Surveys, Techniques: Radial Velocities

Scientific paper

The W. M. Keck Exoplanet Tracker is a precision Doppler radial velocity instrument for extrasolar planet detection based on a new technique, dispersed fixed-delay interferometry (DFDI), which allows for multi-object surveying for the first time. Installed at the 2.5-m Sloan telescope at Apache Point Observatory, the combination of Michelson interferometer and medium resolution spectrograph (Erskine & Ge 2000; Ge 2002) allows design for simultaneous Doppler measurements of 60 targets (Ge et al. 2005).

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