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Heterodyn receiver for the Origins Space Telescope concept 2
Author(s): M. C. Wiedner; Susanne Aalto; Edward G. Amatucci; Andrey Baryshev; Cara Battersby; Victor Belitsky; Edwin A. Bergin; Bruno Borgo; Ruth C. Carter; Asantha Cooray; James A. Corsetti; Elvire De Beck; Yan Delorme; Michael J. Dipirro; Vincent Desmaris; Brian Ellison; Juan-Daniel Gallego; Anna Maria Di Giorgio; Martin Eggens; Maryvonne Gerin; Paul F. Goldsmith; Christophe Goldstein; Frank Helmich; Fabrice Herpin; Richard E. Hills; Michiel R. Hogerheijde; Jean-Michel Huet; Leslie K. Hunt; Willem Jellema; Geert Keizer; Jean-Michel Krieg; Gabby Kroes; Philippe Laporte; André Laurens; David T. Leisawitz; Darek Lis; Gregory E. Martins; Imran Mehdi; Margaret Meixner; Gary Melnick; Stefanie N. Milam; David A. Neufeld; Napoléon Nguyen Tuong; René Plume; Klaus M. Pontoppidan; Benjamin Quertier-Dagorn; Christophe Risacher; Johannes G. Staguhn; Serena Viti; Friedrich Wyrowski
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Paper Abstract

The Origins Space Telescope (OST) is a NASA study for a large satellite mission to be submitted to the 2020 Decadal Review. The proposed satellite has a fleet of instruments including the HEterodyne Receivers for OST (HERO). HERO is designed around the quest to follow the trail of water from the ISM to disks around protostars and planets. HERO will perform high-spectral resolution measurements with 2x9 pixel focal plane arrays at any frequency between 468GHz to 2,700GHz (617 to 111 μm). HERO builds on the successful Herschel/HIFI heritage, as well as recent technological innovations, allowing it to surpass any prior heterodyne instrument in terms of sensitivity and spectral coverage.

Paper Details

Date Published: 30 July 2018
PDF: 10 pages
Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 106981B (30 July 2018); doi: 10.1117/12.2313384
Show Author Affiliations
M. C. Wiedner, Sorbonne Univ., Observatoire de Paris, Univ. PSL, CNRS, LERMA (France)
Susanne Aalto, Chalmers Univ. of Technology (Sweden)
Edward G. Amatucci, NASA Goddard Space Flight Ctr. (United States)
Andrey Baryshev, Kapteyn Astronomical Institute, Univ. of Groningen (Netherlands)
Cara Battersby, Univ. of Connecticut (United States)
Victor Belitsky, Chalmers Univ. of Technology (Sweden)
Edwin A. Bergin, Univ. of Michigan (United States)
Bruno Borgo, LESIA, Observatoire de Paris, CNRS (France)
Ruth C. Carter, NASA Goddard Space Flight Ctr. (United States)
Asantha Cooray, Univ. of California, Irvine (United States)
James A. Corsetti, NASA Goddard Space Flight Ctr. (United States)
Elvire De Beck, Chalmers Univ. of Technology (Sweden)
Yan Delorme, Sorbonne Univ., Observatoire de Paris, Univ. PSL, CNRS, LERMA (France)
Michael J. Dipirro, NASA Goddard Space Flight Ctr. (United States)
Vincent Desmaris, Chalmers Univ. of Technology (Sweden)
Brian Ellison, STFC Rutherford Appleton Lab. (United Kingdom)
Juan-Daniel Gallego, Ctr. Astronómico de Yebes (Spain)
Anna Maria Di Giorgio, Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali (Italy)
Martin Eggens, SRON Netherlands Institute for Space Research (Netherlands)
Maryvonne Gerin, Sorbonne Univ., Observatoire de Paris, Univ. PSL, CNRS, LERMA (France)
Paul F. Goldsmith, Jet Propulsion Lab. (United States)
Christophe Goldstein, Ctr. National d'Études Spatiales (France)
Frank Helmich, SRON Netherlands Institute for Space Research (Netherlands)
Fabrice Herpin, Lab. d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS (France)
Richard E. Hills, Cavendish Lab., Cambridge Univ. (United Kingdom)
Michiel R. Hogerheijde, Leiden Univ. (Netherlands)
Jean-Michel Huet, GEPI, Observatoire de Paris, CNRS (France)
Leslie K. Hunt, INAF - Osservatorio Astrofisico di Arcetri (Italy)
Willem Jellema, SRON Netherlands Institute for Space Research (Netherlands)
Geert Keizer, SRON Netherlands Institute for Space Research (Netherlands)
Jean-Michel Krieg, Sorbonne Univ. Observatoire de Paris, Univ. PSL, CNRS, LERMA (France)
Gabby Kroes, NOVA-ASTRON (Netherlands)
Philippe Laporte, GEPI, Observatoire de Paris, CNRS (France)
André Laurens, Ctr. National d'Études Spatiales (France)
David T. Leisawitz, NASA Goddard Space Flight Ctr. (United States)
Darek Lis, Sorbonne Univ., Observatoire de Paris, Univ. PSL, CNRS, LERMA (France)
Gregory E. Martins, NASA Goddard Space Flight Ctr. (United States)
Imran Mehdi, Jet Propulsion Lab. (United States)
Margaret Meixner, NASA Goddard Space Flight Ctr. (United States)
Space Science Telescope Institute (United States)
Johns Hopkins Univ. (United States)
Gary Melnick, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Stefanie N. Milam, NASA Goddard Space Flight Ctr. (United States)
David A. Neufeld, Johns Hopkins Univ. (United States)
Napoléon Nguyen Tuong, LESIA, Observatoire de Pairs, CNRS (France)
René Plume, Univ. of Calgary (Canada)
Klaus M. Pontoppidan, Space Telescope Science Institute (United States)
Benjamin Quertier-Dagorn, Lab. d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS (France)
Christophe Risacher, Max-Planck-Institut für Radioastronomie (Germany)
IRAM (France)
Johannes G. Staguhn, NASA Goddard Space Flight Ctr. (United States)
Johns Hopkins Univ. (United States)
Serena Viti, Sorbonne Univ. Observatoire de Paris, Univ. PSL, CNRS, LERMA (France)
Chalmers Univ. of Technology (Sweden)
Friedrich Wyrowski, Max-Planck-Institut für Radioastronomie (Germany)


Published in SPIE Proceedings Vol. 10698:
Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
Makenzie Lystrup; Howard A. MacEwen; Giovanni G. Fazio; Natalie Batalha; Nicholas Siegler; Edward C. Tong, Editor(s)

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