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Physical Properties of Sub-galactic Clumps at 0.5 $z łeq$ 1.5 in the UVUDF

, , , , , , , , , , and . (2017)cite arxiv:1702.03038Comment: Accepted for publication in ApJ. 18 pages, 18 figures.

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A Thirty Kiloparsec Chain of "Beads on a String" Star Formation Between Two Merging Early Type Galaxies in the Core of a Strong-Lensing Galaxy Cluster, , , , , , , , , and 3 other author(s). (2014)cite arxiv:1407.2251Comment: 7 pages, 4 figures, accepted for publication in ApJ Letters. High resolution images of the cluster can be found at http://hubblesite.org/news/2014/26.UVUDF: Ultraviolet Imaging of the Hubble Ultradeep Field with Wide-field Camera 3, , , , , , , , , and 16 other author(s). (2013)cite arxiv:1305.1357Comment: Submitted AJ.Physical Properties of Sub-galactic Clumps at 0.5 $z łeq$ 1.5 in the UVUDF, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1702.03038Comment: Accepted for publication in ApJ. 18 pages, 18 figures.