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Further Sunyaev-Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager

We present follow-up observations of two galaxy clusters detected blindly via the Sunyaev-Zel'dovich (SZ) effect and released in the Planck Early Release Compact Source Catalogue. We use the Arcminute Microkelvin Imager, a dual-array 14-18 GHz radio interferometer. After radio source subtraction, we find a SZ decrement of integrated flux density -1.08+/-0.10 mJy toward PLCKESZ G121.11+57.01, and improve the position measurement of the cluster, finding the centre to be RA 12 59 36.4, Dec +60 04 46.8, to an accuracy of 20 arcseconds. The region of PLCKESZ G115.71+17.52 contains strong extended emission, so we are unable to confirm the presence of this cluster via the SZ effect.

preprint2011arXivOpen access
The AMI Consortium:Natasha Hurley-WalkerMichael L. BrownMatthew L. DaviesFarhan FerozThomas M. O. FranzenKeith GraingeMichael P. HobsonAnthony LasenbyMalak OlamaieGuy PooleyCarmen Rodriguez-GonzalvezRichard D. E. SaundersMichel P. SchammelAnna M. M. ScaifePaul F. ScottTimothy ShimwellDavid TitteringtonElizabeth Waldram
astro-ph.CO
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The AMI Consortium:Natasha Hurley-WalkerMichael L. BrownMatthew L. DaviesFarhan FerozThomas M. O. FranzenKeith GraingeMichael P. HobsonAnthony LasenbyMalak OlamaieGuy PooleyCarmen Rodriguez-GonzalvezRichard D. E. SaundersMichel P. SchammelAnna M. M. ScaifePaul F. ScottTimothy ShimwellDavid TitteringtonElizabeth Waldram

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