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W.M. Keck Observatory

W.M. Keck Observatory. A LGS system similar to the Lick Observatory design has been commissioned at the Keck Observatory (see Section 14.4.3.4). [Pg.229]

Important weather details are not only provided by the newest information from the Cassini orbiter the Very Large Telescope in the Atacama desert and the W. M. Keck Observatory on Hawaii are also involved. Near-IR spectra show increased cloudiness in the Titanian troposphere on the morning side, i.e., there are methane clouds at a height of about 30 km and methane drizzle at the surface (Adamkovics et al., 2007). [Pg.292]

K. MATTHEWS and B.T. SOIFER Palomar Observatory California Institute of Technology Based on observations obtained at the W.M.Keck Observatory, which is operated jointly by the California Institute of Technology and the University of California... [Pg.239]


See other pages where W.M. Keck Observatory is mentioned: [Pg.113]    [Pg.146]    [Pg.113]    [Pg.146]    [Pg.34]    [Pg.239]   
See also in sourсe #XX -- [ Pg.146 ]




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