Beam-combining superconducting detector for submillimetre-wave astronomical interferometry
The feasibility of making single-chip, superconducting detectors for submillimetre-wave astronomical inteferometry is demonstrated. An experimental device based on back-to-back corrugated horns, and back-to-back finline transitions, was fabricated. The detector was illuminated at 350 GHz, using a co...
Main Authors: | , , , , , |
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Format: | Journal article |
Language: | English |
Published: |
2003
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_version_ | 1797077022900486144 |
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author | Withington, S Campbell, E Yassin, G Tham, C Wolfe, S Jacobs, K |
author_facet | Withington, S Campbell, E Yassin, G Tham, C Wolfe, S Jacobs, K |
author_sort | Withington, S |
collection | OXFORD |
description | The feasibility of making single-chip, superconducting detectors for submillimetre-wave astronomical inteferometry is demonstrated. An experimental device based on back-to-back corrugated horns, and back-to-back finline transitions, was fabricated. The detector was illuminated at 350 GHz, using a coherent laboratory source, and 0.6° fringes were measured. |
first_indexed | 2024-03-07T00:11:50Z |
format | Journal article |
id | oxford-uuid:797f6034-8397-4f92-8b6e-822c5ea45eb8 |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T00:11:50Z |
publishDate | 2003 |
record_format | dspace |
spelling | oxford-uuid:797f6034-8397-4f92-8b6e-822c5ea45eb82022-03-26T20:37:46ZBeam-combining superconducting detector for submillimetre-wave astronomical interferometryJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:797f6034-8397-4f92-8b6e-822c5ea45eb8EnglishSymplectic Elements at Oxford2003Withington, SCampbell, EYassin, GTham, CWolfe, SJacobs, KThe feasibility of making single-chip, superconducting detectors for submillimetre-wave astronomical inteferometry is demonstrated. An experimental device based on back-to-back corrugated horns, and back-to-back finline transitions, was fabricated. The detector was illuminated at 350 GHz, using a coherent laboratory source, and 0.6° fringes were measured. |
spellingShingle | Withington, S Campbell, E Yassin, G Tham, C Wolfe, S Jacobs, K Beam-combining superconducting detector for submillimetre-wave astronomical interferometry |
title | Beam-combining superconducting detector for submillimetre-wave astronomical interferometry |
title_full | Beam-combining superconducting detector for submillimetre-wave astronomical interferometry |
title_fullStr | Beam-combining superconducting detector for submillimetre-wave astronomical interferometry |
title_full_unstemmed | Beam-combining superconducting detector for submillimetre-wave astronomical interferometry |
title_short | Beam-combining superconducting detector for submillimetre-wave astronomical interferometry |
title_sort | beam combining superconducting detector for submillimetre wave astronomical interferometry |
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