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SUMMARY:The Galaxy and Beyond with the Arcminute Microkelvin Imager - Yvet
 te Perrott (Cavendish Astrophysics)
DTSTART:20130611T153000Z
DTEND:20130611T163000Z
UID:TALK44794@talks.cam.ac.uk
CONTACT:David Titterington
DESCRIPTION:Although AMI was designed specifically for studying galaxy clu
 sters via the SZ effect\, it has also been used extensively for studies of
  galactic objects such as spinning dust and compact HII regions.  I will p
 resent some of the first results from the AMI Galactic Plane Survey\, a la
 rge-area survey of the outer galactic plane providing arcminute resolution
  images at mJy sensitivity at 15 GHz.\n\nI will also provide an update on 
 AMI’s observing programme following up galaxy clusters detected by Planc
 k\, and the use of these observations to investigate the accuracy of commo
 nly used ‘universal’ pressure profiles.\n
LOCATION:Martin Ryle Seminar Room\, Kavli Institute
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