Future Science Prospects for AMI
dc.contributor.author | Grainge, K | |
dc.contributor.author | Alexander, P | |
dc.contributor.author | Battye, R | |
dc.contributor.author | Birkinshaw, M | |
dc.contributor.author | Blain, A | |
dc.contributor.author | Bremer, M | |
dc.contributor.author | Bridle, S | |
dc.contributor.author | Brown, M | |
dc.contributor.author | Davis, R | |
dc.contributor.author | Dickinson, C | |
dc.contributor.author | Edge, A | |
dc.contributor.author | Efstathiou, G | |
dc.contributor.author | Fender, R | |
dc.contributor.author | Hardcastle, M | |
dc.contributor.author | Hatchell, J | |
dc.contributor.author | Hobson, M | |
dc.contributor.author | Jarvis, M | |
dc.contributor.author | Maughan, B | |
dc.contributor.author | McHardy, I | |
dc.contributor.author | Middleton, M | |
dc.contributor.author | Lasenby, A | |
dc.contributor.author | Saunders, R | |
dc.contributor.author | Savini, G | |
dc.contributor.author | Scaife, A | |
dc.contributor.author | Smith, G | |
dc.contributor.author | Thompson, M | |
dc.contributor.author | White, G | |
dc.contributor.author | Zarb-Adami, K | |
dc.contributor.author | Allison, J | |
dc.contributor.author | Buckle, J | |
dc.contributor.author | Castro-Tirado, A | |
dc.contributor.author | Chernyakova, M | |
dc.contributor.author | Deane, R | |
dc.contributor.author | Feroz, F | |
dc.contributor.author | Santos, RG | |
dc.contributor.author | Green, D | |
dc.contributor.author | Hannikainen, D | |
dc.contributor.author | Heywood, I | |
dc.contributor.author | Hurley-Walker, N | |
dc.contributor.author | Kneissl, R | |
dc.contributor.author | Koljonen, K | |
dc.contributor.author | Kulkarni, S | |
dc.contributor.author | Markoff, S | |
dc.contributor.author | MacTavish, C | |
dc.contributor.author | McCollough, M | |
dc.contributor.author | Migliari, S | |
dc.contributor.author | Miller, JM | |
dc.contributor.author | Miller-Jones, J | |
dc.contributor.author | Olamaie, M | |
dc.contributor.author | Paragi, Z | |
dc.contributor.author | Pearson, T | |
dc.contributor.author | Pooley, G | |
dc.contributor.author | Pottschmidt, K | |
dc.contributor.author | Rebolo, R | |
dc.contributor.author | Richer, J | |
dc.contributor.author | Riley, J | |
dc.contributor.author | Rodriguez, J | |
dc.contributor.author | Rodriguez-Gonzalvez, C | |
dc.contributor.author | Rushton, A | |
dc.contributor.author | Savolainen, P | |
dc.contributor.author | Scott, P | |
dc.contributor.author | Shimwell, T | |
dc.contributor.author | Tavani, M | |
dc.contributor.author | Tomsick, J | |
dc.contributor.author | Tudose, V | |
dc.contributor.author | Heyden, KVD | |
dc.contributor.author | Horst, AVD | |
dc.contributor.author | Varlotta, A | |
dc.contributor.author | Waldram, E | |
dc.contributor.author | Wilms, J | |
dc.contributor.author | Zdziarski, A | |
dc.contributor.author | Zwart, J | |
dc.contributor.author | Perrott, Y | |
dc.contributor.author | Rumsey, C | |
dc.contributor.author | Schammel, M | |
dc.date.accessioned | 2017-03-15T13:06:50Z | |
dc.date.issued | 2012-08-17 | |
dc.description.abstract | The Arcminute Microkelvin Imager (AMI) is a telescope specifically designed for high sensitivity measurements of low-surface-brightness features at cm-wavelength and has unique, important capabilities. It consists of two interferometer arrays operating over 13.5-18 GHz that image structures on scales of 0.5-10 arcmin with very low systematics. The Small Array (AMI-SA; ten 3.7-m antennas) couples very well to Sunyaev-Zel'dovich features from galaxy clusters and to many Galactic features. The Large Array (AMI-LA; eight 13-m antennas) has a collecting area ten times that of the AMI-SA and longer baselines, crucially allowing the removal of the effects of confusing radio point sources from regions of low surface-brightness, extended emission. Moreover AMI provides fast, deep object surveying and allows monitoring of large numbers of objects. In this White Paper we review the new science - both Galactic and extragalactic - already achieved with AMI and outline the prospects for much more. | en_GB |
dc.identifier.uri | http://hdl.handle.net/10871/26588 | |
dc.language.iso | en | en_GB |
dc.publisher | arXiv.org | en_GB |
dc.relation.url | http://arxiv.org/abs/1208.1966v2 | en_GB |
dc.title | Future Science Prospects for AMI | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2017-03-15T13:06:50Z | |
dc.identifier.journal | arXiv | en_GB |