Dust emission from the bulk of galaxies at the Epoch of Reionization

[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representative of the bulk of the sources at these redshifts. In this work, we aim at constraining the dust properties of galaxies...

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Veröffentlicht in:	arXiv.org 2024-12
Hauptverfasser:	Ciesla, L, Adscheid, S, Magnelli, B, Boquien, M, Laporte, N, Bethermin, M, Carvajal, C, Schinnerer, E, Liu, D
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Bulk sampling Constraint modelling Cosmic dust Dust Galactic evolution Galaxies Infrared analysis Ionization Optical properties Red shift Star & galaxy formation Star formation
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Zusammenfassung:	[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representative of the bulk of the sources at these redshifts. In this work, we aim at constraining the dust properties of galaxies at 6
ISSN:	2331-8422