The ALMA Band 9 receiver - Design, construction, characterization, and first light
A.M. Baryshev, R. Hesper, F.P. Mena, T.M. Klapwijk, T.A. van Kempen,, M.R. Hogerheijde, B.D. Jackson, J. Adema, G.J. Gerlofsma, M.E. Bekema, J., Barkhof, L.H.R. de Haan-Stijkel, M. van den Bemt, A. Koops, K. Keizer, C., Pieters, J. Koops van het Jagt, H.H.A. Schaeffer

TL;DR
This paper details the design, construction, and testing of ALMA's Band 9 receivers (600-720 GHz), demonstrating their excellent laboratory and on-sky performance in detecting and down-converting polarized millimeter/submillimeter signals.
Contribution
It introduces the novel design and successful implementation of the ALMA Band 9 heterodyne receivers with detailed performance characterization.
Findings
Receivers meet all ALMA performance requirements.
Laboratory tests show high sensitivity and stability.
On-sky tests confirm effective polarization detection.
Abstract
We describe the design, construction, and characterization of the Band 9 heterodyne receivers (600-720 GHz) for the Atacama Large Millimeter / submillimeter Array (ALMA). The ALMA Band 9 receiver units ("cartridges"), which are installed in the telescope's front end, have been designed to detect and down-convert two orthogonal linear polarization components of the light collected by the ALMA antennas. The light entering the front end is refocused with a compact arrangement of mirrors, which is fully contained within the cartridge. The arrangement contains a grid to separate the polarizations and two beam splitters to combine each resulting beam with a local oscillator signal. The combined beams are fed into independent double-sideband mixers, each with a corrugated feedhorn coupling the radiation by way of a waveguide with backshort cavity into an impedance-tuned SIS junction that…
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Taxonomy
TopicsSuperconducting and THz Device Technology · Astrophysics and Star Formation Studies · Radio Astronomy Observations and Technology
