eprintid: 22194 rev_number: 12 eprint_status: archive userid: 2842 dir: disk0/00/02/21/94 datestamp: 2016-11-25 12:23:09 lastmod: 2016-12-01 12:27:33 status_changed: 2016-11-25 12:23:09 type: doctoralThesis metadata_visibility: show creators_name: Brady, Emer title: Radio Sources in the COSMOS Field: Star Forming Properties of High Luminosity Radio Sources subjects: 520 divisions: 130001 adv_faculty: af-13 abstract: Radio wavelengths offer a dust-unobscured window to the early universe. The aim of this thesis has been to characterize the star-forming properties of the high redshift radio galaxy population. We present a preliminary catalogue of the first 610MHz map of the COSMOS feld and find that the sample properties are consistent with predictions for the low frequency radio population. Furthermore, we compare radio and IR star formation rate (SFR) tracers on a large sample of starburst galaxies and find that locally calibrated infrared (IR) and 1.4 GHz radio continuum SFR tracers produce inconsistent results for the most active starbursts. These starbursts are rare locally, but become increasingly common in the early universe. The high redshift starburst population may to be more diffuse, and hence cooler, than local counterparts. In addition, the infrared-radio correlation, observed thus far to be linear and constant for a wide range of galaxies, may exhibit redshift or luminosity evolution. We conclude that a dedicated effort to better model the IR and radio spectral energy distributions of starbursts will be essential to accurately characterize the SFR density at higher redhifts than those considered by studies to date. date: 2016 id_scheme: DOI id_number: 10.11588/heidok.00022194 ppn_swb: 1654362379 own_urn: urn:nbn:de:bsz:16-heidok-221945 date_accepted: 2016-11-10 advisor: HASH(0x564e1c76f0d0) language: eng bibsort: BRADYEMERRADIOSOURC2016 full_text_status: public place_of_pub: Heidelberg, Germany citation: Brady, Emer (2016) Radio Sources in the COSMOS Field: Star Forming Properties of High Luminosity Radio Sources. [Dissertation] document_url: https://archiv.ub.uni-heidelberg.de/volltextserver/22194/1/Thesis.pdf