A Proposed Heterodyne Receiver for the Origins Space Telescope
Journal article, 2018
The HEterodyne Receiver for the Origins Space Telescope (HERO) is a proposed design for a heterodyne focal plane array for a large space mission. The Origins Space Telescope (OST) is one of the four missions selected to be studied by NASA for the 2020 Astronomy and Astrophysics Decadal survey. HERO is designed to observe the trail of water from the interstellar medium (ISM) to disks around protostars. In Concept 1, HERO provides continuous frequency coverage from 468 to 2700 GHz in five bands and a sixth band to cover 4700 GHz. Most bands include 2 × 64 pixels providing at least an order of magnitude higher mapping speeds than available with today's instruments. Receiver sensitivities are expected to be close to the quantum limit. HERO Concept 2, highly constrained by cost and denoted Little-HERO, includes four bands with continuous coverage from 486 to 2700 GHz and with focal plane arrays having only 2 × 9 pixels per band. Both of these THz receiver concepts will be described and the designs will be motivated by the science drivers, the space craft constraints and the latest technological developments. The HERO design builds on the highly successful Herschel/Heterodyne Instrument for the Far-Infrared, on Stratospheric Observatory for Far-Infrared Astronomy/upGREAT and many other heterodyne receivers, but surpasses these in terms of frequency coverage, array size and sensitivity, thanks to the latest technical advances. HERO can be considered an example of a new generation of heterodyne focal plane arrays for future space missions.
heterodyne receivers
heterodyne instruments
THz astronomy
Array receivers
far-infrared (far-IR) space instruments
THz detectors
Author
M.C. Wiedner
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
Imran Mehdi
Jet Propulsion Laboratory, California Institute of Technology
A. M. Baryshev
University of Groningen
Victor Belitsky
Chalmers, Space, Earth and Environment, Onsala Space Observatory, GARD Technology
Vincent Desmaris
Chalmers, Space, Earth and Environment, Onsala Space Observatory, GARD Technology
Anna Maria Digiorgio
Istituto nazionale di astrofisica (INAF)
J. D. Gallego
Yebes Observatory
M. Gerin
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
P. F. Goldsmith
Jet Propulsion Laboratory, California Institute of Technology
F. Helmich
University of Groningen
Netherlands Institute for Space Research (SRON)
W. Jellema
Netherlands Institute for Space Research (SRON)
University of Groningen
Andre Laurens
CNES Centre National d'Etudes Spatiales
Christophe Risacher
Max Planck Society
Institut de RadioAstronomie Millimetrique (IRAM)
A. Cooray
University of California at Irvine (UCI)
Margaret Meixner
Johns Hopkins University
Space Telescope Science Institute (STScI)
NASA Goddard Space Flight Center
IEEE Transactions on Terahertz Science and Technology
2156-342X (ISSN)
Vol. 8 6 558-571 8491320Subject Categories
Aerospace Engineering
Infrastructure
Onsala Space Observatory
DOI
10.1109/TTHZ.2018.2876093