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Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties

, , , , , , , , , , , , , , , and . (2014)cite arxiv:1405.0492Comment: 18 pages, 16 figures, Accepted by A&A.

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Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z $\sim$ 3, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1906.05469.CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths, , , , , , , , , and 30 other author(s). (2022)cite arxiv:2206.15146Comment: 9 pages, 7 figures, to appear in the Proceedings of SPIE Astronomical Telescopes + Instrumentation 2022.A deep search for molecular gas in two massive Lyman break galaxies at z=3 and 4: vanishing CO-emission due to low metallicity?, , , , , , , , , and 7 other author(s). (2013)cite arxiv:1309.5448Comment: 9 pages, 3 figures, accepted for publication in Astrophysical Journal Letters.The early early type: discovery of a passive galaxy at z=3, , , , , , , , and . (2012)cite arxiv:1210.4299Comment: 6 pages, 4 figures, 1 table. Accepted for publication in The Astrophysical Journal Letters.ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using CI and CO, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1703.05764Comment: Accepted for publication in A&A.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.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.Tomography of the Cosmic Dawn and Reionization Eras with Multiple Tracers, , , , , , , , , and 34 other author(s). (2019)cite arxiv:1903.11744Comment: Astro2020 Science White Paper; 5 pages, 1 figure.Imaging the Molecular Interstellar Medium in a Gravitationally Lensed Star-forming Galaxy at z=5.7, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1905.12738Comment: 13 pages, 10 figures, accepted for publication in Astronomy and Astrophysics.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.