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Shape Evolution of Massive Early-Type Galaxies: Confirmation of Increased Disk Prevalence at z>1

, , , , , , and . (2012)cite arxiv:1211.2113Comment: accepted for publication in ApJ; 11 pages; 10 figures; 4 tables.

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Measures of Galaxy Environment I - What is "Environment"?, , , , , , , , , and 12 other author(s). (2011)cite arxiv:1109.6328 Comment: 14 pages, 9 figures, 1 table, accepted to MNRAS.Variations of the initial mass function in semi-analytical models: implications for the chemical enrichment of galaxies in the GAEA model, , , , , and . (2016)cite arxiv:1606.01908Comment: 13 pages, 8 figures, 2 tables, submitted to MNRAS.The Seventh Data Release of the Sloan Digital Sky Survey, , , , , , , , , and 194 other author(s). The Astrophysical Journal Supplement Series, 182 (2): 543 (2009)X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim2$, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1912.01619Comment: 30 pages, 10 figures, accepted in ApJ.Shape Evolution of Massive Early-Type Galaxies: Confirmation of Increased Disk Prevalence at z>1, , , , , , and . (2012)cite arxiv:1211.2113Comment: accepted for publication in ApJ; 11 pages; 10 figures; 4 tables.The Herschel Virgo Cluster Survey. XI. Environmental effects on molecular gas and dust in spiral disks, , , , , , , , , and 12 other author(s). (2012)cite arxiv:1207.5051Comment: 17pp, 14 fig., accepted for publications in Astronomy and Astrophysics.