Large format heterodyne arrays for observing far-infrared lines with SOFIA
C. K. Walker(University of Arizona), Christopher Martin, W. D. Langer, P. F. Goldsmith(Jet Propulsion Laboratory), David Lesser, Jonathan H. Kawamura(Jet Propulsion Laboratory), Michael L. Edgar(California Institute of Technology), J. Stützki(University of Cologne), Craig Kulesa(University of Arizona), S. J. E. Radford(California Institute of Technology), J. Žmuidzinas(California Institute of Technology), T. Cottam(University of Arizona), Imran Mehdi(Jet Propulsion Laboratory), J. R. Gao(Space Research Organisation Netherlands), H. Yorke(Jet Propulsion Laboratory), Chris Groppi(Arizona State University), H.-W. Huebers, D. J. Hollenbach(Ames Research Center), Jenna Kloosterman(University of Arizona)
Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE
July 1, 2010
Cited by 10
Related Papers
CHARACTERISTICS OF PLANETARY CANDIDATES OBSERVED BY<i>KEPLER</i>. II. ANALYSIS OF THE FIRST FOUR MONTHS OF DATA
|The Astrophysical Journal|2011|1.1k
C-12/C-13 isotope ratio across the Galaxy from observations of C-13/O-18 in molecular clouds
|The Astrophysical Journal|1990|339
(C-12)/(C-13) isotope ratio in the local interstellar medium from observations of (C-13)(O-18) in molecular clouds
|The Astrophysical Journal|1993|233
Terahertz Spectroscopy for Astronomy: From Comets to Cosmology
|IEEE Transactions on Terahertz Science and Technology|2011|217
The [ITAL]Submillimeter Wave Astronomy Satellite[/ITAL]: Science Objectives and Instrument Description
|The Astrophysical Journal|2000|191