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The far-infrared–radio correlation in MS0451-03

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dc.contributor.author Randriamampandry, SM
dc.contributor.author Crawford, SM
dc.contributor.author Cress, CM
dc.contributor.author Hess, KM
dc.contributor.author Vaccari, M
dc.contributor.author Wilcots, EM
dc.contributor.author Bershady, MA
dc.contributor.author Wirth, GD
dc.date.accessioned 2015-05-25T10:54:45Z
dc.date.available 2015-05-25T10:54:45Z
dc.date.issued 2014-12
dc.identifier.citation Randriamampandry, SM,Crawford, SM, Cress, CM, Hess, KM, Vaccari, M, Wilcots, EM, Bershady, MA and Wirth, GD. 2014. The far-infrared–radio correlation in MS0451-03. Monthly Notices of the Royal Astronomical Society, pp 168–177 en_US
dc.identifier.issn 0035-8711
dc.identifier.uri http://hdl.handle.net/10204/7982
dc.description Copyright: 2014 Oxford University Press en_US
dc.description.abstract We present a multi-wavelength analysis of star-forming galaxies in the massive cluster MS0451.6-0305 at z ~ 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 µm 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(subFIR) = 1.80±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(sup+23)(sub-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(subFIR) = 2.01±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 en_US
dc.language.iso en en_US
dc.publisher Oxford University Press en_US
dc.relation.ispartofseries Workflow 14570
dc.subject Cluster MS0451.6-0305 en_US
dc.subject Galaxies en_US
dc.subject Cosmic rays en_US
dc.subject Clusters en_US
dc.subject General galaxies en_US
dc.subject Photometry en_US
dc.subject Radio continuum galaxies en_US
dc.title The far-infrared–radio correlation in MS0451-03 en_US
dc.type Article


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