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ESI, a New Keck Observatory Echellette Spectrograph and Imager

2002; Institute of Physics; Volume: 114; Issue: 798 Linguagem: Inglês

10.1086/341706

1538-3873

Andrew Sheinis, M. Bolte, Harland W. Epps, Robert I. Kibrick, J. S. Miller, Matthew V. Radovan, Bruce C. Bigelow, Brian M. Sutin,

Astronomical Observations and Instrumentation

The Echellette Spectrograph and Imager (ESI) is a multipurpose instrument which has been delivered by the Instrument Development Laboratory of Lick Observatory for use at the Cassegrain focus of the Keck II telescope. ESI saw first light on August 29, 1999. ESI is a multi-mode instrument that enables the observer to seamlessly switch between three modes during an observation. The three modes of ESI are: An R=13,000-echellette mode; Low-dispersion prismatic mode; Direct imaging mode. ESI contains a unique flexure compensation system which reduces the small instrument flexure to negligible proportions. Long-exposure images on the sky show FWHM spot diameters of 34 microns (0.34") averaged over the entire field of view. These are the best non-AO images taken in the visible at Keck Observatory to date. Maximum efficiencies are measured to be 28% for the echellette mode and greater than 41% for low-dispersion prismatic mode including atmospheric, telescope and detector losses. In this paper we describe the instrument and its development. We also discuss the performance-testing and some observational results.