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Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation, , , , , , , , , and 10 other author(s). (2014)cite arxiv:1409.5796Comment: 17 pages, 14 figures, 2 tables, submitted to A&A.CO(1-0) line imaging of massive star-forming disk galaxies at z=1.5-2.2, , , , , , , , , and . (2014)cite arxiv:1404.7393Comment: Accepted for publication in MNRAS; 8 pages, 5 figures.Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1405.0492Comment: 18 pages, 16 figures, Accepted by A&A.Hierarchical fragmentation in high redshift galaxies revealed by hydrodynamical simulations, , , , , , and . (2021)cite arxiv:2101.11013Comment: 19 pages, 20 figures, 3 tables and 2 appendices. Accepted for publication in MNRAS.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, , , , , , , , , and 96 other author(s). (2011)cite arxiv:1105.3753.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics, , , , , , , , , and 112 other author(s). (2011)cite arxiv:1105.3754 Comment: 36 pages, 22 figures.On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3, , , , , , , , , and 16 other author(s). (2011)cite arxiv:1106.5502Comment: Accepted for publication in The Astrophysical Journal, 19 pages, 15 figures.ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass, , , , , , , , , and 18 other author(s). (2016)cite arxiv:1606.05280Comment: 31 pages, 16 figures, 13 tables, incorporating the first feedback from the referee on our submitted ApJ manuscript, paper VI of the ASPECS (ALMA Spectroscopic Survey in the Hubble Ultra Deep Field) series.ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas, , , , , , , , , and 30 other author(s). (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.The Herschel view of the dominant mode of galaxy growth from z=4 to the present day, , , , , , , , , and 13 other author(s). (2014)cite arxiv:1409.5433Comment: 28 pages, 25 figures, submitted to A&A.