Paul F. Goldsmith
California Institute of Technology
429 Papers
3.5K Citations
Paul F. Goldsmith is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Molecular cloud & Star formation. The author has an hindex of 78, co-authored 403 publications. Previous affiliations of Paul F. Goldsmith include Cornell University & ASTRON.
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Papers
CALISTO: the Cryogenic Aperture Large Infrared Space Telescope Observatory
Paul F. Goldsmith,M. Bradford,Mark Dragovan,Chris Paine,C. Satter,Bill Langer,Harold W. Yorke,Kevin M. Huffenberger,Dominic J. Benford,Dan F. Lester +9 more
TL;DR: The Cryogenic Aperture Large Infrared Space Telescope Observatory (CALISTO) as mentioned in this paper was designed to provide high-resolution spectroscopic observations at wavelengths between those accessible by JWST and future ground based facilities.
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A Continuous Comparison at 97 GHz Radiometer
TL;DR: In this article, a continuous comparison radiometer has been implemented at 97 GHz using quasi-optical techniques for local oscillator injection and realization of a 90° hybrid with Schottky-diode mixers and FET amplifiers.
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Detection of a dense clump in a filament interacting with W51e2
Bhaswati Mookerjea,Charlotte Vastel,Charlotte Vastel,George E. Hassel,Maryvonne Gerin,Jérôme Pety,Paul F. Goldsmith,John H. Black,Thomas F. Giesen,T. Harrison,Carina M. Persson,Juergen Stutzki +11 more
TL;DR: In this paper, the authors used a gas-grain warm-up based chemical model with physical parameters derived from the NH3 data to explain the observed abundances of different chemical species.
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•Posted Content
The Uptake of Interstellar Gaseous CO into Icy Grain Mantles in a Quiescent Dark Cloud
TL;DR: In this paper, the authors combined data from the Five College Radio Astronomy Observatory CO Mapping Survey of the Taurus molecular cloud with extinction data for a sample of 292 background field stars to investigate the uptake of CO from the gas to icy grain mantles on dust within the cloud.
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Detection of a dense clump in a filament interacting with W51e2
Bhaswati Mookerjea,Charlotte Vastel,Charlotte Vastel,George E. Hassel,Maryvonne Gerin,Jérôme Pety,Paul F. Goldsmith,John H. Black,Thomas F. Giesen,T. Harrison,Carina M. Persson,Juergen Stutzki +11 more
TL;DR: In this article, the authors used a gas-grain warm-up based chemical model with physical parameters derived from the NH3 data to explain the observed abundances of different chemical species, and proposed that the 70 km s-1 narrow feature arises in a dense and cold clump that probably undergoes collapse to form a low-mass protostar formed on the trailing side of the high-velocity filament, which is thought to be interacting with the W51 main cloud.