AMI-LA observations of the SuperCLASS supercluster

C. J. Riseley*, K. J.B. Grainge, Y. C. Perrott, A. M.M. Scaife, R. A. Battye, R. J. Beswick, M. Birkinshaw, M. L. Brown, C. M. Casey, C. Demetroullas, C. A. Hales, I. Harrison, C. L. Hung, N. J. Jackson, T. Muxlow, B. Watson, T. M. Cantwell, S. H. Carey, P. J. Elwood, J. HickishT. Z. Jin, N. Razavi-Ghods, P. F. Scott, D. J. Titterington

*Corresponding author for this work

Research output: Contribution to journalArticle (Academic Journal)peer-review

2 Citations (Scopus)
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We present a deep survey of the Super-Cluster Assisted Shear Survey (SuperCLASS) supercluster - a region of sky known to contain five Abell clusters at redshift z ~ 0.2 - performed using the Arcminute Microkelvin Imager (AMI) Large Array (LA) at 15.5 GHz. Our survey covers an area of approximately 0.9 deg2.We achieve a nominal sensitivity of 32.0 μJy beam-1 towards the field centre, finding 80 sources above a 5s threshold. We derive the radio colour- colour distribution for sources common to three surveys that cover the field and identify three sources with strongly curved spectra - a high-frequency-peaked source and two GHz-peakedspectrum sources. The differential source count (i) agrees well with previous deep radio source counts, (ii) exhibits no evidence of an emerging population of star-forming galaxies, down to a limit of 0.24 mJy, and (iii) disagrees with some models of the 15 GHz source population. However, our source count is in agreement with recent work that provides an analytical correction to the source count from the Square Kilometre Array Design Study (SKADS) Simulated Sky, supporting the suggestion that this discrepancy is caused by an abundance of flat-spectrum galaxy cores as yet not included in source population models.

Original languageEnglish
Article numberstx3118
Pages (from-to)5598-5613
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Issue number4
Early online date1 Dec 2017
Publication statusPublished - 1 Mar 2018

Bibliographical note

17 pages, 14 figures, 3 tables. Accepted for publication in MNRAS


  • Galaxies: clusters: general
  • Radio continuum: general
  • Surveys


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