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Author de Graauw, T.; Caux, E.; Guesten, R.; Helmich, F.; Pearson, J.; Phillips, T. G.; Schieder, R.; Tielens, X.; Saraceno, P.; Stutzki, J.; Wafelbakker, C. K.; Whyborn, N. D.
Title The Herschel-heterodyne instrument for the far-infrared (HIFI) Type Conference Article
Year 2005 Publication Bulletin of the American Astronomical Society Abbreviated Journal
Volume Issue Pages 1219
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Language Summary Language Original Title
Series Editor Series Title Bulletin of the American Astronomical Society Abbreviated Series Title
Series Volume 37 Series Issue Edition
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Area Expedition Conference
Notes Approved no
Call Number ref2005AAS...207.3503D Serial 420
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Author Phillips, T. G.; Keene, J.
Title Submillimeter astronomy [heterodyne spectroscopy] Type Conference Article
Year 1992 Publication Proc. IEEE Abbreviated Journal
Volume 80 Issue Pages 1662-1678
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Notes To approve: number, series, pages Approved no
Call Number Serial 250
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Author Gordon, N. T.; Lees, D. J.; Bowen, G.; Phillips, T. S.; Haigh, M.; Jones, C. L.; Maxey, C. D.; Hipwood, L.; Catchpole, R. A.
Title HgCdTe detectors operating above 200 K Type Journal Article
Year 2006 Publication J. Electron. Mater. Abbreviated Journal
Volume 35 Issue 6 Pages 1140-1144
Keywords HgCdTe detector
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ISSN 0361-5235 ISBN Medium
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Notes Approved no
Call Number Serial 467
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Author Joblin, C.; Pilleri, P.; Montillaud, J.; Fuente, A.; Gerin, M.; Berné, O.; Ossenkopf, V.; Le Bourlot, J.; Teyssier, D.; Goicoechea, J. R.; Le Petit, F.; Röllig, M.; Akyilmaz, M.; Benz, A. O.; Boulanger, F.; Bruderer, S.; Dedes, C.; France, K.; Güsten, R.; Harris, A.; Klein, T.; Kramer, C.; Lord, S. D.; Martin, P. G.; Martin-Pintado, J.; Mookerjea, B.; Okada, Y.; Phillips, T. G.; Rizzo, J. R.; Simon, R.; Stutzki, J.; van der Tak, F.; Yorke, H. W.; Steinmetz, E.; Jarchow, C.; Hartogh, P.; Honingh, C. E.; Siebertz, O.; Caux, E.; Colin, B.
Title Gas morphology and energetics at the surface of PDRs: New insights with Herschel observations of NGC 7023 Type Journal Article
Year 2010 Publication Astron. Astrophys. Abbreviated Journal
Volume 521 Issue Pages L25
Keywords HEB mixer applications, HIFI, Herschel, ISM: structure / ISM: kinematics and dynamics / ISM: molecules / submillimeter: ISM
Abstract (up) Context. We investigate the physics and chemistry of the gas and dust in dense photon-dominated regions (PDRs), along with their dependence on the illuminating UV field.

Aims. Using Herschel/HIFI observations, we study the gas energetics in NGC 7023 in relation to the morphology of this nebula. NGC 7023 is the prototype of a PDR illuminated by a B2V star and is one of the key targets of Herschel.

Methods. Our approach consists in determining the energetics of the region by combining the information carried by the mid-IR spectrum (extinction by classical grains, emission from very small dust particles) with that of the main gas coolant lines. In this letter, we discuss more specifically the intensity and line profile of the 158 μm (1901 GHz) [C ii] line measured by HIFI and provide information on the emitting gas.

Results. We show that both the [C ii] emission and the mid-IR emission from polycyclic aromatic hydrocarbons (PAHs) arise from the regions located in the transition zone between atomic and molecular gas. Using the Meudon PDR code and a simple transfer model, we find good agreement between the calculated and observed [C ii] intensities.

Conclusions. HIFI observations of NGC 7023 provide the opportunity to constrain the energetics at the surface of PDRs. Future work will include analysis of the main coolant line [O i] and use of a new PDR model that includes PAH-related species.
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Notes Approved no
Call Number Serial 1095
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Author Phillips, T. G.; Jefferts, K. B.
Title A low temperature bolometer heterodyne receiver for Millimeter wave astronomy Type Journal Article
Year 1973 Publication Rev. Sci. Instrum. Abbreviated Journal Rev. Sci. Instrum.
Volume 44 Issue 8 Pages 1009-1014
Keywords InSb HEB mixer
Abstract (up) Liquid helium cooled InSb hot electronbolometers are used in a balanced mixer configuration as detectors for an imagelessmicrowave receiver. The system is designed for mounting at the prime focus of the National Radio Astronomy Observatory (NRAO) 11 m antenna at Kitt Peak, Arizona, and is suitable for the study of rotational line spectra of interstellar gas molecules. Currently the operating frequency is in the 90–140 GHz band where the double sideband system noise temperature is 250 K.
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Notes Recommended by Klapwijk Approved no
Call Number Serial 927
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