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Mount Hopkins and the MMT
Multiple Mirror Telescopes of the Future
The MMT Program
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achieve active optics Aden Meinel alignment angle angular resolution aperture Aperture Synthesis arc sec arc seconds array aspheric astronomical Astrophysical Observatory axis beam combiner building camera collecting area collimator configuration construction corrector cost cross dispersed detector diameter edge field flat focal length focal plane focal ratio focus fused silica future galaxies grating Hopkins in-line mode individual telescopes infrared instrument interstellar Kitt Peak large telescopes laser lens light Meinel meters mount Mount Hopkins Multiple Mirror Telescope objects observing operation optical elements optical support structure optical system optical telescope optimization performance phasing photons pixels plate polishing position primary mirror prism problems Reticon rotation secondary mirror segments shown in figure six telescopes slit Smithsonian space speckle interferometry spectral spectrograph stellar Steward Observatory surface techniques tilt tion Tucson University of Arizona vignetting wavelengths