Back to Search Start Over

A 3mm multipixel SIS receiver for IRAM 30-m Pico Veleta Telescope

Authors :
Patrice Serres
Catherine Boucher
Olivier Garnier
Irvin Stil
Dave John
Bastien Lefranc
S. Navarro
Gilles Butin
Francois Mattiocco
Karl F. Schuster
Florence Cope
Anne-Laure Fontana
Alessandro Navarrini
Yves Bortolotti
Source :
SPIE Proceedings.
Publication Year :
2012
Publisher :
SPIE, 2012.

Abstract

A 3mm band focal plane array heterodyne receiver is being developed for Nasmyth focus of the IRAM 30-m Pico Veleta Radio Telescope located in the Sierra Nevada Mountains, south of Spain. This receiver will comprise 25 dual linear polarization pixels operating across the 80-116GHz nominal band. Design efforts are being made to enlarge the band to cover the full 3mm atmospheric transmission window available at Pico Veleta, i.e. 72-116GHz. The instrument will be coupled to the Pico Veleta Telescope via a purely reflective low-loss optical system that includes a de-rotator. The receiver will be based on 5 x 5 cryogenically cooled dual-linear polarized feed horns cascaded with Ortho Mode Transducers (OMT) and side band separating SIS mixers, a technology which offers state-of-the-art performances for millimeter and sub-millimeter receivers.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
SPIE Proceedings
Accession number :
edsair.doi...........98f63743c38d35b59fa4334952289f96