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

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  • stz2427

    Forlagets udgivne version, 4,54 MB, PDF-dokument

  • 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

OriginalsprogEngelsk
TidsskriftMonthly Notices of the Royal Astronomical Society
Vol/bind489
Udgave nummer3
Sider (fra-til)4196-4216
Antal sider21
ISSN0035-8711
DOI
StatusUdgivet - 1 nov. 2019

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