A maximum-likelihood approach to removing radio sources from observations of the Sunyaev-Zel'dovich effect, with application to Abell 611

William F. Grainger, Rhiju Das, Keith Grainge, Michael E. Jones, Rüdiger Kneissl, G. G. Pooley, Richard D E Saunders

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We describe a maximum-likelihood technique for the removal of contaminating radio sources from interferometric observations of the Sunyaev-Zel'dovich (SZ) effect. This technique based on a simultaneous fit for the radio sources and extended SZ emission, is also compared to techniques previously applied to Ryle Telescope observations and is found to be robust. The technique is then applied to new observations of the cluster Abell 611, and a decrement of -540 ± 125 μJy beam-1 is found. This is combined with a ROSAT HRI image and a published ASCA temperature to give an H0 estimate of 52+24-16 km s-1 Mpc-1.
    Original languageEnglish
    Pages (from-to)1207-1214
    Number of pages7
    JournalMonthly Notices of the Royal Astronomical Society
    Volume337
    Issue number4
    DOIs
    Publication statusPublished - 21 Dec 2002

    Keywords

    • Cosmic microwave background
    • Cosmology: observations
    • Distance scale
    • Galaxies: clusters: individual: Abell 611
    • Methods: data analysis
    • X-rays: galaxies: clusters

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