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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

, , , , , , , , , , , , , , , , , , , и . (2014)cite arxiv:1409.5796Comment: 17 pages, 14 figures, 2 tables, submitted to A&A.

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Véronique Trappe

Véronique Porra

Véronique Buschmann

Véronique Mersseman

Véronique Henn

 

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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, , , , , , , , , и 10 other автор(ы). (2014)cite arxiv:1409.5796Comment: 17 pages, 14 figures, 2 tables, submitted to A&A.Fitting AGN/galaxy X-ray-to-radio SEDs with CIGALE and improvement of the code, , , , , , , , , и 4 other автор(ы). (2022)cite arxiv:2201.03718Comment: ApJ accepted. The code is available at https://cigale.lam.fr/news/.The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, , , , , , , , , и 54 other автор(ы). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.The Herschel view of the dominant mode of galaxy growth from z=4 to the present day, , , , , , , , , и 13 other автор(ы). (2014)cite arxiv:1409.5433Comment: 28 pages, 25 figures, submitted to A&A.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , и 49 other автор(ы). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.Impact of star formation history on the measurement of star formation rates, , и . (2014)cite arxiv:1409.5792Comment: 10 pages, 10 figures, 1 table. Accepted for publication in A&A.A hyperluminous obscured quasar at a redshift of z ~ 4.3, , , , , , , , , и 2 other автор(ы). (2021)cite arxiv:2103.08032Comment: Accepted for publication in Monthly Notices of the Royal Astronomical Society Letters. Models used in this work are available at http://ahpc.euc.ac.cy/.CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST, , , , , , , , , и 57 other автор(ы). (2022)cite arxiv:2211.05792Comment: 41 pages, 20 figures, 6 tables, submitted to ApJL. Key results in Figures 13-15, discussed in Sections 7 and 8.Getting ready for the LSST data -- estimating the physical properties of $z<2.5$ main sequence galaxies, , , , , , , , , и 1 other автор(ы). (2021)cite arxiv:2106.12573Comment: Accepted to A&A.