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The Carnegie Planet Finder Spectrograph (PFS) has been constructed for use with the Magellan telescopes at
Las Campanas Observatory in Chile. PFS has been optimized for high-precision measurement of stellar radial
velocities in order to support an ongoing search for extrasolar planets. PFS uses an R4 echelle grating and a
prism cross-disperser in a Littrow arrangement to provide complete wavelength coverage between 390 and 620
nm distributed across 58 orders. Spectral resolution is 38,000 when using a 1 arcsec slit. An iodine absorption
cell is included in the pre-slit module to allow the superimposition of well-defined absorption features on the
stellar spectra. To improve velocity stability, the echelle grating is enclosed in a small vacuum tank with the
cross-dispersing prism acting as the vacuum window. The spectrograph is mounted on an invar optical bench that
is surrounded by an insulated enclosure with circulating liquid temperature control. Fabrication and assembly
have been completed, and testing will soon be underway. Delivery to Las Campanas Observatory is scheduled
for late 2008.
Jeffrey D. Crane,Stephen A. Shectman,R. Paul Butler,Ian B. Thompson, andGregory S. Burley
"The Carnegie Planet Finder Spectrograph: a status report", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 701479 (9 July 2008); https://doi.org/10.1117/12.789637
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Jeffrey D. Crane, Stephen A. Shectman, R. Paul Butler, Ian B. Thompson, Gregory S. Burley, "The Carnegie Planet Finder Spectrograph: a status report," Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 701479 (9 July 2008); https://doi.org/10.1117/12.789637