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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

Year
2004
Citations
25

Abstract

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).

Keywords

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

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