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

ABSTRACT 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 subtra...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society. Letters 2011-06, Vol.414 (1), p.L75-L79
Hauptverfasser: Hurley-Walker, Natasha, Brown, Michael L., Davies, Matthew L., Feroz, Farhan, Franzen, Thomas M. O., Grainge, Keith, Hobson, Michael P., Lasenby, Anthony, Olamaie, Malak, Pooley, Guy, Rodríguez-Gonzálvez, Carmen, Saunders, Richard D. E., Schammel, Michel P., Scaife, Anna M. M., Scott, Paul F., Shimwell, Timothy, Titterington, David, Waldram, Elizabeth
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Sprache:eng
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Zusammenfassung:ABSTRACT 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 towards PLCKESZ G121.11+57.01, and improve the position measurement of the cluster, finding the centre to be RA , to an accuracy of 20 arcsec. 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.
ISSN:1745-3925
1745-3933
DOI:10.1111/j.1745-3933.2011.01059.x