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Disambiguation of "Gruppioni, C."

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On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density

, , , , , , , , , , , , , , , , , , , , , and . (2013)cite arxiv:1304.7000Comment: Submitted to A&A.

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Guido C C Clinckspoor

Thomas C C Knöbig

Ullrich C C Jagstaidt

Guido C C Clinckspoor

Thomas C C Gartenmann

 

Other publications of authors with the same name

SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust, , , , , , , , , and 26 other author(s). (2017)cite arxiv:1710.02150Comment: In press. This paper belongs to the "SPICA Special Issue" on PASA.The lesser role of starbursts for star formation at z=2, , , , , , , , , and 24 other author(s). (2011)cite arxiv:1108.0933Comment: Accepted for publication in ApJ Letters.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.The dust mass function from z~0 to z~2, , , , , and . (2019)cite arxiv:1909.11333Comment: MNRAS in press, 12 pages, 6 pages.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.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.A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time, , , , , , , and . (2019)cite arxiv:1902.09172Comment: 21 pages, 10 figures, 8 table, accepted for publication in A&A.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.