Heterodyn receiver for the Origins Space Telescope concept 2
| Autor: | Belitsky, Victor, Desmaris, Vincent, Di Giorgio, Anna Maria, Goldstein, Christophe, Ellison, Brian, Gallego, Juan-Daniel, Herpin, Fabrice, Huet, Jean-Michel, Krieg, Jean-Michel, Laporte, Philippe, Quertier-Dagorn, Benjamin, Plume, René, Risacher, Christophe, De Beck, Elvire, Goldsmith, Paul, Hogerheijde, Michiel, Hunt, Leslie, Lis, Darek, Aalto, Susanne, Viti, Serena, Wyrowski, Friedrich, Neufeld, David, Melnick, Gary, Bergin, Edwin, Battersby, Cara, Milam, Stefanie, Borgo, Bruno, Carter, Ruth, Cooray, Asantha, Corsetti, James, Delorme, Yan, Dipirro, Michael, Eggens, Martin, Hills, Richard, Keizer, Geert, Kroes, Gabby, Leisawitz, David, Meixner, Margaret, Nguyen Tuong, Napoléon, Pontoppidan, Klaus, Staguhn, Johannes, Martins, Gregory, Wiedner, Martina, Baryshev, Andrey, Laurens, André, Gerin, Maryvonne, Helmich, Frank, Jellema, Willem, Mehdi, Imran, Amatucci, Edward, MacEwen, Howard, Lystrup, Makenzie, Fazio, Giovanni, Batalha, Natalie, Tong, Edward, Siegler, Nicholas |
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| Přispěvatelé: | FORMATION STELLAIRE 2018, Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Calgary], University of Calgary, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Max-Planck-Institut für Radioastronomie (MPIFR), Harvard-Smithsonian Center for Astrophysics (CfA), Smithsonian Institution-Harvard University [Cambridge], Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), California Institute of Technology (CALTECH), Observatoire de Paris, Université Paris sciences et lettres (PSL), Astronomy |
| Jazyk: | angličtina |
| Rok vydání: | 2018 |
| Předmět: |
Heterodyne
Pixel Computer science Astronomy 7. Clean energy 01 natural sciences Focal Plane Arrays Spitzer Space Telescope Planet 0103 physical sciences HERO Satellite [SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] 010306 general physics 010303 astronomy & astrophysics ComputingMilieux_MISCELLANEOUS |
| Zdroj: | Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, Jun 2018, Austin, France. ⟨10.1117/12.2313384⟩ Proceedings of SPIE, 10698. SPIE |
| ISSN: | 0361-0748 |
| Popis: | 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. |
| Databáze: | OpenAIRE |
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