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Proceedings Paper

An ultra-broadband optical system for ALMA Band 2+3
Author(s): V. Tapia; R. Nesti; A. González; I. Barrueto; F. P. Mena; N. Reyes; F. Villa; F. Cuttaia; P. Yagoubov
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Paper Abstract

ALMA is the largest radio astronomical facility in the world providing high sensitivity between 35 and 950 GHz, divided in 10 bands with fractional bandwidths between 19 and 36%. Having a lifespan of at least 30 years, ALMA carries out a permanent upgrading plan which, for the receivers, is focused on achieving better sensitivity and larger bandwidths. As result, an international consortium works on demonstrating a prototype receiver covering currents Bands 2 and 3 (67 to 116 GHz) which corresponds to a fractional bandwidth of 54%. Here we present the preliminary design, implementation and characterization of suitable refractive optics. Results indicate an excellent performance in good agreement with simulations.

Paper Details

Date Published: 20 July 2016
PDF: 7 pages
Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 99142X (20 July 2016); doi: 10.1117/12.2233143
Show Author Affiliations
V. Tapia, Univ. de Chile (Chile)
R. Nesti, INAF - Osservatorio Astrofisico di Arcetri (Italy)
A. González, National Astronomical Observatory of Japan (Japan)
I. Barrueto, Univ. de Chile (Chile)
F. P. Mena, Univ. de Chile (Chile)
N. Reyes, Univ. de Chile (Chile)
F. Villa, INAF - IASF Bologna (Italy)
F. Cuttaia, INAF - IASF Bologna (Italy)
P. Yagoubov, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 9914:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

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