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Proceedings Paper

A study on the use of the PACS bolometer arrays for submillimeter ground-based telescopes
Author(s): Vincent Reveret; Louis R. Rodriguez; Philippe André; Benoit Horeau; Jean Le Pennec; Patrick Agnèse
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Paper Abstract

A new kind of bolometric architecture has been successfully developed for the PACS photometer onboard the Herschel submillimeter observatory. These new generation CCD-like arrays are buttable and enable the conception of large fully sampled focal planes. We present a feasibility study of the adaptation of these bolometer arrays to ground-based submillimeter telescopes. We have developed an electro-thermal numerical model to simulate the performances of the bolometers under specific ground-based conditions (different wavelengths and background powers for example). This simulation permits to determine the optimal parameters for each condition and shows that the bolometers can be background limited in each transmission window between 200 and 450 microns. We also present a new optical system that enables to have a maximum absorption of the bolometer in each atmospheric windows. The description of this system and measurements are shown.

Paper Details

Date Published: 6 July 2006
PDF: 9 pages
Proc. SPIE 6275, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III, 627502 (6 July 2006); doi: 10.1117/12.670941
Show Author Affiliations
Vincent Reveret, European Southern Observatory (Chile)
CEA/DSM/DAPNIA Service d’Astrophysique (France)
Louis R. Rodriguez, CEA/DSM/DAPNIA Service d’Astrophysique (France)
Philippe André, CEA/DSM/DAPNIA Service d’Astrophysique (France)
Benoit Horeau, CEA/DSM/DAPNIA Service d’Astrophysique (France)
Jean Le Pennec, CEA/DSM/DAPNIA Service d’Astrophysique (France)
Patrick Agnèse, LETI/CEA Grenoble (France)


Published in SPIE Proceedings Vol. 6275:
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III
Jonas Zmuidzinas; Wayne S. Holland; Stafford Withington; William D. Duncan, Editor(s)

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