From the far-ultraviolet to the far-infrared – galaxy emission at 0≤z≤10 in theSHARKsemi-analytic model

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  • stz2427

    Final published version, 4.54 MB, PDF document

  • Claudia del P. Lagos
  • Aaron S. G. Robotham
  • James W. Trayford
  • Rodrigo Tobar
  • Matias Bravo
  • Sabine Bellstedt
  • Luke J. M. Davies
  • Simon P. Driver
  • Pascal J. Elahi
  • Danail Obreschkow
  • Chris Power

We combine the SHARK semi-analytic model of galaxy formation with the PROSPECT software tool for spectral energy distribution (SED) generation to study the multiwavelength emission of galaxies from the far-ultraviolet (FUV) to the far-infrared (FIR) at 0

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume489
Issue number3
Pages (from-to)4196-4216
Number of pages21
ISSN0035-8711
DOIs
Publication statusPublished - 1 Nov 2019

    Research areas

  • ISM: dust, extinction, galaxies: evolution, galaxies: formation, galaxies: luminosity function, SPECTRAL ENERGY-DISTRIBUTION, STELLAR POPULATION SYNTHESIS, STAR-FORMING GALAXIES, MASS ASSEMBLY GAMA, LUMINOSITY FUNCTION, LOCAL UNIVERSE, DUST CONTENT, MU-M, EVOLUTION, STABILITY

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ID: 244955411