Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
Scientist
Louisiana State University
Planetary Science Institute, Tucson, AZ, USA; State University; Space Science Institute
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA Propulsion Lab, Caltech, 4800 Oak Grove Drive, Pasadeba, CA 91109, USA Science Institute, Tucson, AZ 85719, USA; Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA of Physics and Astronomy, Louisiana State University
Louisiana State University; Space Science Inst.
NASA Jet Propulsion Laboratory California Inst. Technology, 4800 Oak Grove Dr. 183-501, Pasadena, CA 91109, USA Propulsion Laboratory, California Institute of Technology, Pasadena, CA State University, Department of Physics and Astronomy, Baton Rouge, LA 70803, USA; Space Science Institute, 4750 Walnut St., Suite 205, Boulder, CO 80301, USA
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Space Science Institute, Boulder, Colorado, USA
Planetary Science Institute
NASA Jet Propulsion Laboratory, California Institute of Technology
Planetary Science Institute, 1700 East Fort Lowell Road, Suite 106, Tucson, AZ 85719-2395, USA; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803 State University and Agricultural & Mechanical College, Louisiana, USA
A Mid-latitude Cloud Eruption on Titan Observed by the Cassini Visual Infrared Mapping Spectrometer (VIMS) in July 2007
A New Method For Obtaining Optical Constants In The Near-IR To UV From Single-crystal Absorption Spectra: SiC And Silicates As Examples
Application of modern radiative transfer tools to model laboratory quartz emissivity
Bolometric Bond Albedos For Saturnian Satellites From Cassini VIMS: Leading and Trailing Hemispheres
Challenging the identification of nitride dust in extreme carbon star spectra
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