Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
NASA Ames Research Center, MS 245-6, Moffett Field, CA, 94035, USA Research Center, MS 245-6, Moffett Field, CA 94035; SETI Institute, 515 North Whisman Road, Mountain View, CA 94043.
NASA-Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035-1000 Ames Research Center, MS 245-6, Moffett Field, CA 94035-1000 Ames Research Center, MS 245-6, Moffett Field, CA 94035, USA
NASA Ames Research Center, Moffett Field, CA
NASA Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035-1000 ; SETI Institute, 515 North Whisman Road, Mountain View, CA 94043. Ames Research Center, Moffett Field, CA 94035-1000; SETI Institute, 515 North Whisman Road, Mountain View, CA 94043.
NASA-Ames Research Center, Space Science Division, Mail Stop 245-6, Moffett Field, CA 94035, USA
NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035, USA; SETI Institute, 515 N. Whisman Road, Mountain View, CA 94043, USA
NASA Ames Research Center, Moffett Field, CA 94035-1000, USA
NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035, USA ; SETI Institute, 515 N. Whisman Road, Mountain View, CA 94043, USA
NASA Ames Research Center, Moffett Field, CA 94035-1000 ; Carl Sagan Center, SETI Institute, 515 North Whisman Road, Mountain View, CA 94043.
NASA Ames Research Center, Moffett Field, CA 9403; SETI Institute, 515 North Whisman Road, Mountain View, CA 94043; Astrophysics Branch, MS 245-6.
Space Science Division, Mail Stop 245-6, NASA Ames Research Center, Moffett Field, CA 94035, USA
Electronic and Vibrational Spectroscopy of Diamondoids and the Interstellar Infrared Bands between 3.35 and 3.55 μm
Erratum: "The 5.25 and 5.7 μm Astronomical Polycyclic Aromatic Hydrocarbon Emission Features" (2009, ApJ, 690, 1208)
Experimental Near-Infrared Spectroscopy of Polycyclic Aromatic Hydrocarbons between 0.7 and 2.5 μm
Far-Infrared Spectroscopy of Neutral Coronene, Ovalene, and Dicoronylene
Far-ir Pah Spectroscopy And The Identification Of An Individual Astronomical Pah Molecule
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