Utente:Vale maio/Sandbox3: differenze tra le versioni

Versione delle 21:06, 13 mar 2009

Versione delle 16:37, 17 mar 2009

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# Top row

[[Image:Mrao ami lba ryle.jpg|thumb|250px|The AMI Large Array, utilizing antennas from the [[Ryle Telescope]]. The telescopes have been re-positioned since this photo was taken.]]

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The '''Arcminute Microkelvin Imager''' (AMI) is an interferometer [[radio telescope]] designed principally to image secondary [[anisotropy|anisotropies]] in the [[cosmic microwave background]] (CMB) at higher angular resolution than the [[Very Small Array]]. It consists of two [[interferometry|interferometric]] arrays, the Small Array and the Large Array, sited at the [[Mullard Radio Astronomy Observatory]] in Cambridge (UK), both operating in the frequency range 12-18 GHz. The (short-baseline) Small Array consists of 10 3.7-m parabolic antennas while the long-baseline Large Array is composed of eight 13-m antennas. The two arrays have essentially identical receivers and back-end electronics.

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The main goal of the project is to carry out a survey of clusters of galaxies via the [[Sunyaev-Zel'dovich effect]] (the scattering of the CMB off the hot gas in the cluster). AMI will also make very high-resolution observations of the primary CMB power spectrum.

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==See also==

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* [[South Pole Telescope]]

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* [[Sunyaev-Zel'dovich Array]]

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* [[Atacama_Cosmology_Telescope|Atacama Cosmology Telescope]]

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== References ==

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* {{cite journal | first= | last=AMI Consortium: Zwart et al. | coauthors= | doi= | id={{arxiv | id=0807.2469}} | title=The Arcminute Microkelvin Imager | year=2008}}

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* {{cite journal | first= | last=AMI Consortium | coauthors= | doi=10.1111/j.1745-3933.2006.00151.x | id={{arxiv | archive=astro-ph | id=0509215}} | title=High-significance Sunyaev-Zel'dovich measurement: Abell 1914 seen with the Arcminute Microkelvin Imager | journal=Monthly Notices of the Royal Astronomical Society: Letters | volume=369 | pages=L1 | year=2006}}

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* {{cite web | url=http://www.mrao.cam.ac.uk/telescopes/ami/ | title=Arcminute MicroKelvin Imager official page | accessdate=2006-10-18}}

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== Further reading ==

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* {{cite journal | first=Michael | last=Jones | title = SZ surveys with the Arcminute MicroKelvin Imager | year=2001 | id={{arxiv|archive=astro-ph|id=0109351}} }}

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* {{cite journal | url=http://ukads.nottingham.ac.uk/cgi-bin/nph-bib_query?bibcode=2001MNRAS.328..783 | last=Kneissl | first=Rüdiger | coauthors = et al. | title=Surveying the sky with the Arcminute MicroKelvin Imager: expected constraints on galaxy cluster evolution and cosmology | journal=MNRAS | year=2001 | volume=328 | pages=783 | id={{arxiv|archive=astro-ph|id=0103042}} | doi=10.1046/j.1365-8711.2001.04815.x }}

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{{Radiazione cosmica di fondo}}

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[[:Category:Cosmic Microwave Background Experiments]]

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[[:Category:Cavendish Laboratory]]

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[[:Category:Interferometric telescopes]]

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[[en:Arcminute Microkelvin Imager]]

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