The IRX-β relation of high-redshift galaxies

Lichen Liang*, Robert Feldmann, Christopher C. Hayward, Desika Narayanan, Onur Çatmabacak, Dušan Kereš, Claude André Faucher-Giguère, Philip F. Hopkins

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

The relation between infrared excess (IRX) and UV spectral slope (βUV) is an empirical probe of dust properties of galaxies. The shape, scatter, and redshift evolution of this relation are not well understood, however, leading to uncertainties in estimating the dust content and star formation rates (SFRs) of galaxies at high redshift. In this study, we explore the nature and properties of the IRX-βUV relation with a sample of z = 2-6 galaxies (M∗ 109-1012, M⊙) extracted from high-resolution cosmological simulations (MassiveFIRE) of the Feedback in Realistic Environments (FIRE) project. The galaxies in our sample show an IRX-βUV relation that is in good agreement with the observed relation in nearby galaxies. IRX is tightly coupled to the UV optical depth, and is mainly determined by the dust-to-star geometry instead of total dust mass, while βUV is set both by stellar properties, UV optical depth, and the dust extinction law. Overall, much of the scatter in the IRX-βUV relation of our sample is found to be driven by variations of the intrinsic UV spectral slope. We further assess how the IRX-βUV relation depends on viewing direction, dust-to-metal ratio, birth-cloud structures, and the dust extinction law and we present a simple model that encapsulates most of the found dependencies. Consequently, we argue that the reported 'deficit' of the infrared/sub-millimetre bright objects at z 5 does not necessarily imply a non-standard dust extinction law at those epochs.

Original languageEnglish (US)
Pages (from-to)3210-3241
Number of pages32
JournalMonthly Notices of the Royal Astronomical Society
Volume502
Issue number3
DOIs
StatePublished - Apr 1 2021

Keywords

  • Dust
  • extinction
  • galaxies: ISM
  • galaxies: evolution
  • galaxies: high-redshift
  • infrared: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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