Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Penn State Erie
New York, State University, Stony Brook, N.Y.
Visiting scientist at the W. M. Keck Observatory, which is operated as a scientific partnership between Caltech, the University of California, and NASA and was made possible by the generous support of the W. M. Keck Foundation; School of Science, Pennsylvania State University at Erie, Station Road, Erie, PA 16563
Max-Planck-Institut für Kernphysik, Heidelberg, Germany; New York, State University, Stony Brook, N.Y.
NASA, Ames Research Center, Moffett Field, Calif.
Division of Science, Penn State Erie, The Behrend College, Erie, Pennsylvania
Penn. State University, Erie, Penn., USA
The Behrend College, Erie, PA, US
Department of Earth and Space Sciences, State University of New York at Stony Brook, Stony Brook, New York 11790
State University of New York, Stony Brook.
School of Science, Penn State University at Erie
Penn State, Behrend College
New York, State University, Stony Brook
Kitt Peak National Observatory; Steward Observatory, Tucson, Ariz.
Penn Sate Erie
Penn State Erie, The Behrend College, School of Science, Erie, Pennsylvania
Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany
Kitt Peak National Observatory, Tucson, Ariz.
Hawaii Univ., Honolulu.
Penn State University, Erie, PA 16563, USA
New York, State University, Stony Brook, NY; Max-Planck-Institut für Kernphysik, Heidelberg, Germany
Penn State Erie, Behrend College
Pennsylvania State University, Erie
Behrend School of Science, Pennsylvania State University Erie, Station Road, Erie, PA 16563
United Kingdom Infrared Telescope Unit, Hilo, HI.
Penn. State University, Erie, PA, USA
New York State University, Stony Brook
Kitt Peak Natl. Obs.
Department of Physics, University of California, Berkeley, California.
NASA, Marshall Space Flight Center, Huntsville, AL
Pennsylvania State University at Erie
Pennsylvania State University, Erie, PA.
School of Science, Penn State Erie, The Behrend College, Erie,
17-25 micrometer spectra of Jupiter and Saturn
2--14 microns Spectroscopy of Vega-type Stars
A 2-25 Micron Fourier Spectrometer.
A Mid-Infrared Survey of Vega-Like Sources
A Possible Identification of Interstellar Silicate Absorption in the Infrared Spectrum of 119 Tauri
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