{
  "id": "1411.3677",
  "version": "v1",
  "published": "2014-11-13T19:37:26.000Z",
  "updated": "2014-11-13T19:37:26.000Z",
  "title": "The Far-Infrared-Radio Correlation in MS0451-03",
  "authors": [
    "S. M. Randriamampandry",
    "S. M. Crawford",
    "C. M. Cress",
    "K. M. Hess",
    "M. Vaccari",
    "E. M. Wilcots",
    "M. A. Bershady",
    "G. D. Wirth"
  ],
  "comment": "14 pages, 4 figures, accepted for publication in MNRAS",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "We present a multi-wavelength analysis of star-forming galaxies in the massive cluster MS0451.6-0305 at z $\\sim$ 0.54 to shed new light on the evolution of the far-infrared-radio relationship in distant rich clusters. We have derived total infrared luminosities for a spectroscopically confirmed sample of cluster and field galaxies through an empirical relation based on $Spitzer$ MIPS 24 $\\mu$m photometry. The radio flux densities were measured from deep Very Large Array 1.4 GHz radio continuum observations. We find the ratio of far-infrared to radio luminosity for galaxies in an intermediate redshift cluster to be $q_{\\rm FIR}$ = 1.80$\\pm$0.15 with a dispersion of 0.53. Due to the large intrinsic dispersion, we do not find any observable change in this value with either redshift or environment. However, a higher percentage of galaxies in this cluster show an excess in their radio fluxes when compared to low redshift clusters ($27^{+23}_{-13}\\%$ to $11\\%$), suggestive of a cluster enhancement of radio-excess sources at this earlier epoch. In addition, the far-infrared-radio relationship for blue galaxies, where $q_{\\rm FIR}$ = 2.01$\\pm$0.14 with a dispersion of 0.35, is consistent with the predicted value from the field relationship, although these results are based on a sample from a single cluster.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-11-13T19:37:26.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "far-infrared-radio correlation",
      "ghz radio continuum observations",
      "far-infrared-radio relationship",
      "distant rich clusters",
      "low redshift clusters"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1093/mnras/stu2411",
      "journal": "Monthly Notices of the Royal Astronomical Society",
      "year": 2015,
      "month": "Feb",
      "volume": 447,
      "number": 1,
      "pages": 168
    },
    "note": {
      "typesetting": "TeX",
      "pages": 14,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1327796,
      "adsabs": "2015MNRAS.447..168R"
    }
  }
}