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Disambiguation of "Amorín, R."

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No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $3.1 z 3.5$

, , , , , , , , , , , , , , , , , and . (2021)cite arxiv:2109.03662Comment: 18 pages, 11 figures, 1 appendix, submitted to Monthly Notices of the Royal Astronomical Society.

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R Riordan

R Manzke

R Schneider

R Ringseis

R Schäfer

 

Other publications of authors with the same name

Size evolution of star-forming galaxies with $2<z<4.5$ in the VIMOS Ultra-Deep Survey, , , , , , , , , and 8 other author(s). (2016)cite arxiv:1602.01840Comment: 22 pages, 20 figures (+3 in appendix), submitted to A&A.The VIMOS Ultra Deep Survey: Ly$\alpha$ Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5, , , , , , , , , and 38 other author(s). (2015)cite arxiv:1503.01753Comment: 17 pages, 10 figures, 1 table, submitted to A&A.A major merger origin for the high fraction of galaxies at 2<z<6 with 2 bright clumps in the VIMOS Ultra-Deep Survey, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1611.05869Comment: 17 pages, 11 figures, submitted to A&A.The Kennicutt-Schmidt Relation in Extremely Metal-Poor Dwarf Galaxies, , , , , and . (2016)cite arxiv:1602.04772Comment: Accepted for publication in ApJ.The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1703.10170Comment: 26 pages, 14 figures, 1 table, submitted to A&A.The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$, , , , , , , , , and 13 other author(s). (2020)cite arxiv:2007.01322Comment: 18 pages, 13 figures, submitted to A&A.A Virtual Observatory Census to Address Dwarfs Origins. AVOCADO - I. Science goals, sample selection and analysis tools, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1301.5320Comment: 13 pages, 12 figures (a few with degraded resolution). Accepted to A&A.No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $3.1 z 3.5$, , , , , , , , , and 8 other author(s). (2021)cite arxiv:2109.03662Comment: 18 pages, 11 figures, 1 appendix, submitted to Monthly Notices of the Royal Astronomical Society.An extreme OIII emitter at $z=3.2$: a low metallicity Lyman continuum source, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1507.06648Comment: 13 pages, 10 figures, submitted to A&A. Comments welcome.The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1911.09999Comment: 19 pages, 10 figures (including appendix), submitted to A&A. Comments welcome!.