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Disambiguation of "Dubois, Yohan"

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Snap, Crackle, Pop: sub-grid supernova feedback in AMR simulations of disk galaxies

, , , , and . (2016)cite arxiv:1609.01296Comment: 22 pages, 15 figures. Submitted to MNRAS, comments welcome.

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Yohan Shim

Yohan Seo

Yohan Lejosne

Fekadu Yohannes

Indra Yohannes

 

Other publications of authors with the same name

The impact of AGN feedback on galaxy intrinsic alignments in the Horizon simulations, , , , , , , , , and . (2019)cite arxiv:1908.11665Comment: 16 pages, 12 figures, submitted to MNRAS.Dual AGN in the Horizon-AGN simulation and their link to galaxy and massive black hole mergers, with an excursus on multiple AGN, , , , , , , and . (2021)cite arxiv:2112.07193Comment: Submitted to MNRAS.The black hole population in low-mass galaxies in large-scale cosmological simulations, , , , , , , , , and 1 other author(s). (2022)cite arxiv:2201.09888Comment: Submitted to MNRAS, 21 pages, 11 figures, 1 table.Snap, Crackle, Pop: sub-grid supernova feedback in AMR simulations of disk galaxies, , , , and . (2016)cite arxiv:1609.01296Comment: 22 pages, 15 figures. Submitted to MNRAS, comments welcome.Black hole evolution: I. Supernova-regulated black hole growth, , , , , and . (2015)cite arxiv:1504.00018Comment: 18 pages, 13 figures, submitted to MNRAS, comments welcome.The impact of AGN feedback on the 1D power spectra from the Ly$\alpha$ forest using the Horizon-AGN suite of simulations, , , , , , and . (2020)cite arxiv:2002.02822Comment: Submitted to MNRAS.Predicting the Observability of Population III Stars with ELT-HARMONI via the Helium $1640\rm\AA$ emission line, , , , , , , and . (2021)cite arxiv:2101.01725Comment: 23 Pages, 17 Figures, Accepted for publication in Monthly Notices of the Royal Astronomical Society.DUSTiER (DUST in the Epoch of Reionization): dusty galaxies in cosmological radiation-hydrodynamical simulations of the Epoch of Reionization with RAMSES-CUDATON, , , , , , and . (2022)cite arxiv:2204.03949Comment: submitted to MNRAS, 1st report received: under revision Have partially addressed referee's concerns, namely that the model predicts high dust masses and redder bright galaxies than expected, by discussing this aspect around the relevant results. Work is being carried out to present a clearer parameter exploration of the dust model.Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST, , , , , , , , , and . (2022)cite arxiv:2201.09892Comment: published in MNRAS, 19 pages, 8 figures, key figures: Fig. 3, Fig.5, and Fig. 7.Dancing in the dark: galactic properties trace spin swings along the cosmic web, , , , , , , , , and 23 other author(s). (2014)cite arxiv:1402.1165Comment: 17 pages, 20 pages, submitted to MNRAS, comments are welcome, movies and pictures of the simulation can be found at this address http://horizon-AGN.projet-horizon.fr.