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Disambiguation of "Pozzi, F."

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The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&A.

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Daniel Pozzi

Franz Pozzi

Riccardo Edmondo Pozzi

Carlo Pozzi

Angelo Pozzi

 

Other publications of authors with the same name

On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1304.7000Comment: Submitted to A&A.The evolution of the dust and gas content in galaxies, , , , , , , , , and 29 other author(s). (2013)cite arxiv:1311.3670Comment: Accepted for publication in A&A.The ALPINE-ALMA C II Survey: C II158micron Emission Line Luminosity Functions at $z 4-6$, , , , , , , , , and 21 other author(s). (2020)cite arxiv:2006.04835Comment: 17 pages, 9 Figures, submitted to ApJ. This paper is related to the two other ALPINE papers submitted today by Loiacono and Gruppioni.Non-linearity and environmental dependence of the star forming galaxies Main Sequence, , , , , , , , , and 23 other author(s). (2015)cite arxiv:1511.01899Comment: 14 pages, 14 figures, accepted for publication in MNRAS.Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1308.2199Comment: 23 pages, 11 figures. Accepted for publication in A&A.The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel, , , , , , , , , and 33 other author(s). (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&amp;A.Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6?, , , , , , , , , and 20 other author(s). (2013)cite arxiv:1310.1398Comment: Accepted for publication in MNRAS.The dust mass function from z~0 to z~2, , , , , and . (2019)cite arxiv:1909.11333Comment: MNRAS in press, 12 pages, 6 pages.The ALPINE-ALMA CII Survey: nature, luminosity function and star formation history of continuum non-target galaxies up to z~6, , , , , , , , , and 23 other author(s). (2020)cite arxiv:2006.04974Comment: 23 pages, 14 figures. Submitted to A&A. This paper is related to the two other ALPINE papers submitted today by Loiacono and Yan.Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1403.3615Comment: 24 pages, 23 figures, accepted for publication in MNRAS.