Bibcode
DOI
Szentgyorgyi, Andrew; Furesz, Gabor; Cheimets, Peter; Conroy, Maureen; Eng, Roger; Fabricant, Daniel; Fata, Robert; Gauron, Thomas; Geary, John; McLeod, Brian; Zajac, Joseph; Amato, Stephen; Bergner, Henry; Caldwell, Nelson; Dupree, Andrea; Goddard, Richard; Johnston, Everett; Meibom, Soeren; Mink, Douglas; Pieri, Mario; Roll, John; Tokarz, Susan; Wyatt, William; Epps, Harland; Hartmann, Lee; Meszaros, Szabolcz
Referencia bibliográfica
Publications of the Astronomical Society of the Pacific, Volume 123, issue 908, pp.1188-1209
Fecha de publicación:
10
2011
Número de citas
54
Número de citas referidas
49
Descripción
The Hectochelle is an optical band, fiber-fed, multiobject echelle
spectrograph deployed at the MMT Observatory on Mount Hopkins, Arizona.
The optical fibers that feed the Hectochelle are positioned by the
Hectospec robot positioner on the MMT f/5 focal surface, and the
Hectochelle shares an optical fiber feed system with the Hectospec, a
moderate-dispersion spectrograph that is collocated with the
Hectochelle. Hectochelle can record up to 240 spectra simultaneously at
a resolution of 38,000. Spectra cover a single diffractive order that is
approximately 150 Å wide. The total potential operating passband
of the Hectochelle extends from 3800 Å to 9000 Å. Operated
in conjunction with the MMT f/5 secondary, the MMT wide-field corrector,
and the atmospheric dispersion compensator, the patrol field is 1°
in diameter and the individual fiber slits are 1.5' in diameter. The
throughput of the combined telescope, fiber feed, and spectrograph is
measured to be 6.1% at 5275 Å, exclusive of atmospheric
extinction. A 20 minute observation of a V=15 F-type star yields a
signal-to-noise ratio of 35 per resolution element. Hectochelle had
first light 2003 December 4 and continues to be operated at the MMT
today.