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Thomas G. Phillips

Researcher at California Institute of Technology

Publications -  477
Citations -  21382

Thomas G. Phillips is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Caltech Submillimeter Observatory & Molecular cloud. The author has an hindex of 77, co-authored 477 publications receiving 20630 citations. Previous affiliations of Thomas G. Phillips include Bayer & ASTRON.

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Molecular abundances in OMC-1 - the chemical composition of interstellar molecular clouds and the influence of massive star formation

TL;DR: In this article, the chemical composition of the various regions in the core of the Orion molecular cloud (OMC-1) was investigated based on results from the Caltech Owens Valley Radio Observatory (OVRO) spectral line survey (Sutton et al., Blake et al.).
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The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI)

Th. de Graauw, +179 more
TL;DR: The Heterodyne Instrument for the Far-Infrared (HIFI) was launched onboard ESA's Herschel Space Observatory in May 2009 as mentioned in this paper, which is a set of 7 heterodyne receivers that are electronically tuneable, covering 480-1250 GHz with SIS mixers and the 1410-1910 GHz range with hot electron bolometer mixers.
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SHARC-2 350 μm Observations of Distant Submillimeter-selected Galaxies

TL;DR: In this paper, the authors verified the linear radio-far-infrared correlation at redshifts of z ~ 1-3 and luminosities of 10^(11)-10^(13) L_☉, with a power-law index of 102 ± 012 and rms scatter of 012 dex However, the correlation constant q or the dust emissivity index β is lower than measured locally.
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SHARC-2 350 Micron Observations of Distant Submillimeter Selected Galaxies

TL;DR: In this paper, the authors verified the linear radio-far-infrared correlation at redshifts of z ~ 1--3 and luminosities of 10^11--10^13 L_sun, with a power-law index of 1.02+-0.12 and rms scatter of 0.12 dex.
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In-orbit performance of Herschel-HIFI

Pieter R. Roelfsema, +111 more
TL;DR: In this paper, the calibration and in-orbit performance of the Heterodyne Instrument for the Far-Infrared (HIFI) is described based on a combination of ground and in flight tests.