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doi: 10.5281/zenodo.836741 , 10.25916/sut.26279002.v1 , 10.25916/sut.26279002 , 10.5281/zenodo.836740 , 10.48550/arxiv.1707.01511
arXiv: 1707.01511
handle: 1959.3/440074
doi: 10.5281/zenodo.836741 , 10.25916/sut.26279002.v1 , 10.25916/sut.26279002 , 10.5281/zenodo.836740 , 10.48550/arxiv.1707.01511
arXiv: 1707.01511
handle: 1959.3/440074
The recent development of sensitive, multiplexed near infra-red instruments has presented astronomers the unique opportunity to survey mass/magnitude complete samples of galaxies at \emph{Cosmic Noon}, a time period where $\sim80\%$ of the observed baryonic mass is generated and galaxies are actively star-forming and evolving rapidly. This thesis takes advantage of the recently commissioned MOSFIRE spectrograph on Keck, to conduct a survey (ZFIRE) of galaxies at $1.5
PhD Thesis, 262 pages
spectroscopy, surveys, Astrophysics of Galaxies (astro-ph.GA), galaxies, FOS: Physical sciences, dust, clusters, infra-red, Astrophysics - Astrophysics of Galaxies, IMF, ISM, star formation
spectroscopy, surveys, Astrophysics of Galaxies (astro-ph.GA), galaxies, FOS: Physical sciences, dust, clusters, infra-red, Astrophysics - Astrophysics of Galaxies, IMF, ISM, star formation
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