The Arcminute Microkelvin Imager
The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope is aimed principally at Sunyaev-Zel'dovich imaging of clusters of galaxies. We di...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2008
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| _version_ | 1797101712173957120 |
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| author | Consortium, AMI Zwart, J Barker, R Biddulph, P Bly, D Boysen, R Brown, A Clementson, C Crofts, M Culverhouse, T Czeres, J Dace, R Davies, M D'Alessandro, R Doherty, P Duggan, K Ely, J Felvus, M Feroz, F Flynn, W Franzen, T Geisbüsch, J Génova-Santos, R Grainge, K Grainger, W |
| author_facet | Consortium, AMI Zwart, J Barker, R Biddulph, P Bly, D Boysen, R Brown, A Clementson, C Crofts, M Culverhouse, T Czeres, J Dace, R Davies, M D'Alessandro, R Doherty, P Duggan, K Ely, J Felvus, M Feroz, F Flynn, W Franzen, T Geisbüsch, J Génova-Santos, R Grainge, K Grainger, W |
| author_sort | Consortium, AMI |
| collection | OXFORD |
| description | The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope is aimed principally at Sunyaev-Zel'dovich imaging of clusters of galaxies. We discuss the design of the telescope and describe and explain its electronic and mechanical systems. |
| first_indexed | 2024-03-07T05:55:43Z |
| format | Journal article |
| id | oxford-uuid:ea6ae415-3f83-4b3d-aa4f-b10100fd51f8 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T05:55:43Z |
| publishDate | 2008 |
| record_format | dspace |
| spelling | oxford-uuid:ea6ae415-3f83-4b3d-aa4f-b10100fd51f82022-03-27T11:02:18ZThe Arcminute Microkelvin ImagerJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:ea6ae415-3f83-4b3d-aa4f-b10100fd51f8EnglishSymplectic Elements at Oxford2008Consortium, AMIZwart, JBarker, RBiddulph, PBly, DBoysen, RBrown, AClementson, CCrofts, MCulverhouse, TCzeres, JDace, RDavies, MD'Alessandro, RDoherty, PDuggan, KEly, JFelvus, MFeroz, FFlynn, WFranzen, TGeisbüsch, JGénova-Santos, RGrainge, KGrainger, WThe Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope is aimed principally at Sunyaev-Zel'dovich imaging of clusters of galaxies. We discuss the design of the telescope and describe and explain its electronic and mechanical systems. |
| spellingShingle | Consortium, AMI Zwart, J Barker, R Biddulph, P Bly, D Boysen, R Brown, A Clementson, C Crofts, M Culverhouse, T Czeres, J Dace, R Davies, M D'Alessandro, R Doherty, P Duggan, K Ely, J Felvus, M Feroz, F Flynn, W Franzen, T Geisbüsch, J Génova-Santos, R Grainge, K Grainger, W The Arcminute Microkelvin Imager |
| title | The Arcminute Microkelvin Imager |
| title_full | The Arcminute Microkelvin Imager |
| title_fullStr | The Arcminute Microkelvin Imager |
| title_full_unstemmed | The Arcminute Microkelvin Imager |
| title_short | The Arcminute Microkelvin Imager |
| title_sort | arcminute microkelvin imager |
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