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Publications of the Astronomical Society of the Pacific
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arXiv.org e-Print Archive
Preprint . 2008
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Publications of the Astronomical Society of the Pacific
Article . 2008 . Peer-reviewed
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https://dx.doi.org/10.48550/ar...
Article . 2008
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https://dx.doi.org/10.1086/593...
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High Redshift Galaxies in the Hubble Ultra Deep Field

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Nov 2008Embargo end date: 01 Jan 2008 English Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 120, pages 1,255-1,257 (issn: 0004-6280, eissn: 1538-3873, Copyright policy )
Authors: Hathi, Nimish P.;

doi: 10.1086/593982 , 10.48550/arxiv.0810.0268

arXiv: 0810.0268

High Redshift Galaxies in the Hubble Ultra Deep Field

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.

Accepted for publication as Dissertation Summary in PASP (2 pages; emulateapj). My full dissertation in PDF format (132 pages) is available at http://web.me.com/hathi/asu_thesis_files/hathi_thesis.pdf

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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