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Disambiguation of "Charlot, Stéphane"

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Spectroscopy of an extreme OIII emitting active galactic nucleus at $z=3.212$: implications for the reionisation era

, , , , , , and . (2021)cite arxiv:2109.04493Comment: 11 pages, 7 figures, submitted to MNRAS.

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Stéphane Müller

Stéphane Haussler

Stéphane Klein

Stéphane Aubry

Stéphane Audière

 

Other publications of authors with the same name

Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey, , , , , , , , , and 12 other author(s). Monthly Notices of the Royal Astronomical Society, 341 (1): 33--53 (2003)Timing the starburst–AGN connection, , and . Monthly Notices of the Royal Astronomical Society, 405 (2): 933--947 (2010)Bursty stellar populations and obscured active galactic nuclei in galaxy bulges, , , , , , , and . Monthly Notices of the Royal Astronomical Society, 381 (2): 543--572 (2007)Modelling and interpreting spectral energy distributions of galaxies with BEAGLE, and . (2016)cite arxiv:1603.03037Comment: 28 pages, 14 figures, 8 tables, submitted to MNRAS.MMT Spectroscopy of Lyman-alpha at z$\simeq$7: Evidence for Accelerated Reionization Around Massive Galaxies, , , , , , and . (2020)cite arxiv:2010.03566Comment: 19 pages, 9 figures. Submitted to MNRAS.Strong Gravitational Lensing and the Stellar IMF of Early-type Galaxies, , , , , and . (2015)cite arxiv:1512.00462Comment: submitted to MNRAS, 17 pages, 12 figures, 3 tables.Ultraviolet spectra of extreme nearby star-forming regions --- approaching a local reference sample for JWST, , , , , , , , , and . (2017)cite arxiv:1706.00881Comment: 26 pages, 13 figures, 11 tables, submitted to MNRAS.The ionization properties of extreme nearby star-forming regions, , , , , , , , , and . (2017)cite arxiv:1709.03503Comment: 6 pages, 5 figures, submitted to MNRAS Letters, comments welcome.A Critical Look at the Mass-Metallicity-SFR Relation in the Local Universe: Non-parametric Analysis Framework and Confounding Systematics, , , , , , , and . (2014)cite arxiv:1411.7391Comment: ApJ. Part 1 of 2. Comments are welcome.How robustly can we constrain the low-mass end of the $z\sim6-7$ stellar mass function? -- The limits of lensing models and stellar population assumptions in the Hubble Frontier Fields, , , , and . (2020)cite arxiv:2011.13991Comment: Accepted for publication in MNRAS. 24 pages, 21 figures.