{"paper":{"title":"AMI-LA Observations of the SuperCLASS Super-cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. M. M. Scaife, B. Watson, C. A. Hales, C. Demetroullas, C. J. Riseley, C.-L. Hung, C. M. Casey, D. J. Titterington, I. Harrison, J. Hickish, K. J. B. Grainge, M. Birkinshaw, M. L. Brown, N. J. Jackson, N. Razavi-Ghods, P. F. Scott, P. J. Elwood, R. A. Battye, R. J. Beswick, S. H. Carey, T. M. Cantwell, T. Muxlow, T. Z. Jin, Y. C. Perrott","submitted_at":"2017-11-30T03:06:17Z","abstract_excerpt":"We present a deep survey of the SuperCLASS super-cluster - a region of sky known to contain five Abell clusters at redshift $z\\sim0.2$ - performed using the Arcminute Microkelvin Imager (AMI) Large Array (LA) at 15.5$~$GHz. Our survey covers an area of approximately 0.9 square degrees. We achieve a nominal sensitivity of $32.0~\\mu$Jy beam$^{-1}$ toward the field centre, finding 80 sources above a $5\\sigma$ 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-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.11199","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}