T
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.
Papers
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Proceedings ArticleDOI
Terahertz-frequency receiver instrumentation for Herschel's heterodyne instrument for far infrared (HIFI)
John C. Pearson,Imran Mehdi,Erich Schlecht,Frank Maiwald,Alain Maestrini,John Gill,S.C. Martin,Dave Pukala,John Ward,J. Kawamura,William R. McGrath,W. A. Hatch,Dennis G. Harding,Henry G. LeDuc,J. A. Stern,Bruce Bumble,Lorene Samoska,Todd Gaier,Robert Ferber,David P. Miller,Alexandre Karpov,Jonas Zmuidzinas,Thomas G. Phillips,Neal R. Erickson,Jerry Swift,Yun Chung,Richard Lai,Huei Wang +27 more
TL;DR: In this paper, the Heterodyne Instrument for Far Infrared (HIFI) on ESA's Herschel Space Observatory is comprised of five SIS receiver channels covering 480-1250 GHz and two HEB channel covering 1410-1910 GHz.
Journal ArticleDOI
The development of an 850 GHz waveguide receiver using tuned sis junctions on 1µm Si 3 N 4 membranes
Jacob Kooi,M. Chan,M. Bin,Bruce Bumble,Henry G. LeDuc,Christopher K. Walker,Thomas G. Phillips +6 more
TL;DR: In this paper, the authors report preliminary development work on a 850 GHz SIS heterodyne receiver employing a tuned niobium tunnel junction on a 1 µm Si3N4 supporting membrane.
Journal ArticleDOI
The 60-μm extragalactic background radiation intensity, dust-enshrouded active galactic nuclei and the assembly of groups and clusters of galaxies
TL;DR: In this article, the authors investigate possible sources of this excess CBR emission, assuming that it has a genuine extragalactic origin, and propose and test three explanations, each involving additional populations of luminous, evolving galaxies not readily detected in existing submm-wave surveys.
Journal ArticleDOI
Evidence for optically thin CO emission from the Kleinmann-Low Nebula.
Journal ArticleDOI
Magnetic Field in the Isolated Massive Dense Clump IRAS 20126+4104
Hiroko Shinnaga,Giles Novak,John E. Vaillancourt,Masahiro N. Machida,Akimasa Kataoka,Kohji Tomisaka,Jacqueline A. Davidson,Thomas G. Phillips,C. Darren Dowell,Lerothodi Leonard Leeuw,Lerothodi Leonard Leeuw,Martin Houde,Martin Houde +12 more
TL;DR: In this paper, the authors measured polarized dust emission at 350µm towards the high-mass star forming massive dense clump IRAS 20126+4104 using the SHARC II Polarimeter, SHARP, at the Caltech Submillimeter Observatory.