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  • 2108.10455v2

    Rights statement: This is an author-created, un-copyedited version of an article accepted for publication/published in Astronomical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-3881/ac20d6

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    Embargo ends: 18/10/22

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Towards precise galaxy evolution: a comparison between spectral indices of $z\sim1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey

Research output: Contribution to journalJournal articlepeer-review

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  • Po-Feng Wu
  • Dylan Nelson
  • Arjen van der Wel
  • Annalisa Pillepich
  • Stefano Zibetti
  • Rachel Bezanson
  • Francesco D'Eugenio
  • Anna Gallazzi
  • Camilla Pacifici
  • Caroline M. S. Straatman
  • Ivana Barišić
  • Eric F. Bell
  • Michael V. Maseda
  • Adam Muzzin
  • David Sobral
  • Katherine E. Whitaker
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Article number201
<mark>Journal publication date</mark>18/10/2021
<mark>Journal</mark>The Astronomical Journal
Issue number5
Volume162
Number of pages14
Publication StatusPublished
<mark>Original language</mark>English

Abstract

We present the first comparison of observed stellar continuum spectra of high-redshift galaxies and mock galaxy spectra generated from hydrodynamical simulations. The mock spectra are produced from the IllustrisTNG TNG100 simulation combined with stellar population models and take into account dust attenuation and realistic observational effects (aperture effects and noise). We compare the simulated $D_n4000$ and EW(H$\delta$) of galaxies with $10.5 \leq \log(M_\ast/M_\odot) \leq 11.5$ at $0.6 \leq z \leq 1.0$ to the observed distributions from the LEGA-C survey. TNG100 globally reproduces the observed distributions of spectral indices, implying that the age distribution of galaxies in TNG100 is generally realistic. Yet there are small but significant differences. For old galaxies, TNG100 shows small $D_n4000$ when compared to LEGA-C, while LEGA-C galaxies have larger EW(H$\delta$) at fixed $D_n4000$. There are several possible explanations: 1) LEGA-C galaxies have overall older ages combined with small contributions (a few percent in mass) from younger ($

Bibliographic note

This is an author-created, un-copyedited version of an article accepted for publication/published in Astronomical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-3881/ac20d6