Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Caltech Optical Observatoires, California Institute of Technology, USA
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125; W. M. Keck Observatory, 65-1120 Mamalahoa Highway, Kamuela, HI 96743.
Caltech Optical Observatoires, California Institute of Technology, Pasadena, CA 91125, USA
W.M. Keck Observatory, Waimea, HI 96743, USA; Caltech Optical Observatoires, California Institute of Technology, Pasadena, CA 91125, USA
Caltech Optical Observatoires, California Institute of Technology, Pasadena, California, USA
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA
Caltech Optical Observatoires, USA
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California.
W.M. Keck Observatory, USA
W. M. Keck Observatory, Kamuela, HI 96743, USA
Caltech Optical Observatoires, Mail Code 105-24, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125.
W. M. Keck Observatory
Caltech
W. M. Keck Observatory, 65-1120 Mamalahoa Highway, Kamuela, HI 96743 Keck Observatory
Div. of Geol. and Planetary Sci., Caltech
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California
W. M. Keck Observatory, 65-1120 Mamalahoa Highway, Kamuela, HI 96743; Caltech Optical Observatoires, Mail Code 105-24, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125.
A 5-Micron-Bright Spot on Titan: Evidence for Surface Diversity
A Close Companion Search around L Dwarfs using Aperture Masking Interferometry and Palomar Laser Guide Star Adaptive Optics
A high-Resolution Catalog of Cometary Emission Lines
A large cloud outburst at Titan's south pole
A low density of 0.8 g/cc for the Trojan binary asteroid 617 Patroclus
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