High Redshift Galaxies in the Hubble Ultra Deep Field
Nimish P. Hathi
TL;DR
This dissertation analyzes high redshift galaxies in the Hubble Ultra Deep Field to understand their structure and physical properties through three recent investigations.
Contribution
It provides new insights into high redshift galaxy properties based on three recent studies in the HUDF, advancing understanding of early universe galaxy formation.
Findings
Characterization of high redshift galaxy structures
Physical property measurements of early galaxies
Insights into galaxy evolution at high redshift
Abstract
My dissertation presents results from three recent investigations in the Hubble Ultra Deep Field (HUDF) focusing on understanding structural and physical properties of high redshift galaxies. Here I summarize results from these studies. This thesis work was conducted at Arizona State University under the guidance of Prof. Rogier Windhorst and Prof. Sangeeta Malhotra.
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Radio Astronomy Observations and Technology