2002/03/31 by P. N. Best · 1 citation
Physics and Astronomy · #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2002.05896.x
published as Mon.Not.Roy.Astron.Soc. 336 (2002) 1293 · MNRAS, in consideration. 11 pages, including 6 figures. Minor typos corrected
arxiv created 2002/04/03 · openalex publication_date 2002/11/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Deep submillimetre (submm) observations using SCUBA are presented of the central regions of four high-redshift clusters which have been extensively studied optically: CL0023 + 0423 (z= 0.84), J0848 + 4453 (z= 1.27), CL1604 + 4304 (z= 0.90) and CL1604 + 4321 (z= 0.92). 10 submm sources are securely detected towards these four clusters at 850 μm, with two further tenuous detections; the raw 850-μm source counts exceed those determined from blank-field surveys by a factor ∼3–4. In particular, towards CL1604 + 4304, six sources are detected with S850μm > 4 mJy making this the richest submm field discovered to date. Corrections for gravitational lensing by these high-redshift clusters reduce these excess sources counts, but are unlikely to account for more than about half of the excess, with the remainder presumably directly associated with cluster galaxies. The 450- to 850-μm flux density ratios of the detected sources are systematically higher (at a significance level >98 per cent) than those determined for blank-field selected sources, consistent with them being at the cluster redshifts. If subsequent identifications confirm cluster membership, these results will demonstrate that the optical Butcher–Oemler effect is also observed at submm wavelengths.