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The 6.5-m MMT's f/5 wide-field optics and instruments

Daniel G. Fabricant, Robert Fata, B. A. McLeod, Andrew Szentgyorgyi, Jack Barberis, Henry Bergner, Warren R. Brown, Nelson Caldwell, Maureen A. Conroy, Roger Eng, Harland W. Epps, Gábor Fürész, Tom M. Gauron, John C. Geary, Richard E. Goddard, Lee Hartmann, Edward Hertz, M. Honsa, Mark Mueller, Timothy Norton

发表年份
2004
引用次数
25

摘要

In 2003, the converted MMT’s wide-field f/5 focus was commissioned. A 1.7-m diameter secondary and a large refractive corrector offer a 1° diameter field of view for spectroscopy and a 0.5° diameter field of view for imaging. Stellar images during excellent seeing are smaller than 0.5" FWHM across the spectroscopic field of view, and smaller than 0.4" across the imaging field of view. Three wide-field f/5 instruments are now in routine operation: Hectospec (an R~1000 optical spectrograph fed by 300 robotically-positioned optical fibers), Hectochelle (an R~40,000 optical spectrograph fed by the same fibers), and Megacam (a 340 megapixel, 36 CCD optical imager covering a 25' by 25' format).

关键词

SpectrographOpticsDepth of fieldField (mathematics)Field of viewFocus (optics)PhysicsSpectroscopyOptical fiberMathematics

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