The ESI instrument is a versatile, multi-mode spectrograph and
imager. There are two distinct spectroscopic modes: a
medium-resolution echellette mode with prism cross dispersion;
and a high-throughput mode using prism dispersion only. The
spectrograph modes will cover the full wavelength range of the
Keck II silvered mirrors (3900 to 11000 A) in a single exposure.
The low-resolution, prism-only mode provides the same spectral
range, multi-object capability, and very high throughput. ESI
also provides an imaging mode with a field of view of 2 arcmin x
8 arcmin. An Epps refracting camera and a single 2K x 4K detector
are used for all three modes.
View some construction
images or engineering
drawings.
Project Principal Investigator: Joe Miller (Director -
UCO/Lick)
Co-Principal Investigators: Michael Bolte, Raja
Guhathakurta, Dennis Zaritsky
Optical Designers: Brian Sutin, Harland Epps
Project Manager: David Cowley
Project Engineers: Matthew Radovan, Andrew Sheinis
ESI has seen first light at Keck Observatory! (August 29, 1999) First light engineering run went very well. Some issues remain to be dealt with, such as the stray light from the Renishaw encoders on the slit/aperture/filter wheels, but work is in progress and a fix will be tested in the September observing run. See the Keck ESI page for the latest details.
Get more information on the new ESI logo jacket