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THE UNIVERSITY OF CALIFORNIA TEN METER TELESCOPE
PROJECTTHE SEGMENTED DESIGN
THE KITT PEAK NGT PROJECT
17 other sections not shown
accuracy achieved Airy Disc allow angular resolution aperture arc second arcsec aspheric astronomers atmospheric axial axis baseline beam Cassegrain CERGA coherence collecting area Cooke triplet correction corrector cost coude detection diameter diffraction limited discussed dome effects efficiency elements fiber field of view flexure focal ratio focus frequency fringe galaxies heterodyne hour angle infrared instruments interferometer Kitt Peak Labeyrie large telescopes limiting magnitudes MAMA detector measurements meter telescope metre microns mount noise objects observations Observatory obtained operation Optical Telescopes paraboloid performance phase photon pixel polar axle possible primary mirror prism problems QSOs radial radio refraction region relatively scale sensor shown in Figure Singles Array sources Space Telescope spatial speckle imaging speckle interferometry spectral spectrograph spectrum spherical stars stellar structure surface Table technique telescope array thermal tion tube visible wavelengths weight