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dc.contributor.authorGrainge, K
dc.contributor.authorAlexander, P
dc.contributor.authorBattye, R
dc.contributor.authorBirkinshaw, M
dc.contributor.authorBlain, A
dc.contributor.authorBremer, M
dc.contributor.authorBridle, S
dc.contributor.authorBrown, M
dc.contributor.authorDavis, R
dc.contributor.authorDickinson, C
dc.contributor.authorEdge, A
dc.contributor.authorEfstathiou, G
dc.contributor.authorFender, R
dc.contributor.authorHardcastle, M
dc.contributor.authorHatchell, J
dc.contributor.authorHobson, M
dc.contributor.authorJarvis, M
dc.contributor.authorMaughan, B
dc.contributor.authorMcHardy, I
dc.contributor.authorMiddleton, M
dc.contributor.authorLasenby, A
dc.contributor.authorSaunders, R
dc.contributor.authorSavini, G
dc.contributor.authorScaife, A
dc.contributor.authorSmith, G
dc.contributor.authorThompson, M
dc.contributor.authorWhite, G
dc.contributor.authorZarb-Adami, K
dc.contributor.authorAllison, J
dc.contributor.authorBuckle, J
dc.contributor.authorCastro-Tirado, A
dc.contributor.authorChernyakova, M
dc.contributor.authorDeane, R
dc.contributor.authorFeroz, F
dc.contributor.authorSantos, RG
dc.contributor.authorGreen, D
dc.contributor.authorHannikainen, D
dc.contributor.authorHeywood, I
dc.contributor.authorHurley-Walker, N
dc.contributor.authorKneissl, R
dc.contributor.authorKoljonen, K
dc.contributor.authorKulkarni, S
dc.contributor.authorMarkoff, S
dc.contributor.authorMacTavish, C
dc.contributor.authorMcCollough, M
dc.contributor.authorMigliari, S
dc.contributor.authorMiller, JM
dc.contributor.authorMiller-Jones, J
dc.contributor.authorOlamaie, M
dc.contributor.authorParagi, Z
dc.contributor.authorPearson, T
dc.contributor.authorPooley, G
dc.contributor.authorPottschmidt, K
dc.contributor.authorRebolo, R
dc.contributor.authorRicher, J
dc.contributor.authorRiley, J
dc.contributor.authorRodriguez, J
dc.contributor.authorRodriguez-Gonzalvez, C
dc.contributor.authorRushton, A
dc.contributor.authorSavolainen, P
dc.contributor.authorScott, P
dc.contributor.authorShimwell, T
dc.contributor.authorTavani, M
dc.contributor.authorTomsick, J
dc.contributor.authorTudose, V
dc.contributor.authorHeyden, KVD
dc.contributor.authorHorst, AVD
dc.contributor.authorVarlotta, A
dc.contributor.authorWaldram, E
dc.contributor.authorWilms, J
dc.contributor.authorZdziarski, A
dc.contributor.authorZwart, J
dc.contributor.authorPerrott, Y
dc.contributor.authorRumsey, C
dc.contributor.authorSchammel, M
dc.date.accessioned2017-03-15T13:06:50Z
dc.date.issued2012-08-17
dc.description.abstractThe 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.urihttp://hdl.handle.net/10871/26588
dc.language.isoenen_GB
dc.publisherarXiv.orgen_GB
dc.relation.urlhttp://arxiv.org/abs/1208.1966v2en_GB
dc.titleFuture Science Prospects for AMIen_GB
dc.typeArticleen_GB
dc.date.available2017-03-15T13:06:50Z
dc.identifier.journalarXiven_GB


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