Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST
We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of galaxy populations at redshifts from z ≈ 0 to = 8 in a full cosmological framework. We achieve this by coupling, in post-processing, the cosmological IllustrisTNG simulations with new-generation nebular-emissi...
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| Main Authors: | , , , , , , , , , , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
Dezember 2023
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2023, Volume: 526, Issue: 3, Pages: 3610-3636 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stad2955 |
| Online Access: | Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stad2955
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| Author Notes: | Michaela Hirschmann, Stephane Charlot, Anna Feltre, Emma Curtis-Lake, Rachel S. Somerville, Jacopo Chevallard, Ena Choi, Dylan Nelson, Christophe Morisset, Adele Plat and Alba Vidal-Garcia |
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| 100 | 1 | |a Hirschmann, Michaela |d 1981- |e VerfasserIn |0 (DE-588)1013612558 |0 (DE-627)664623603 |0 (DE-576)347423434 |4 aut | |
| 245 | 1 | 0 | |a Emission-line properties of IllustrisTNG galaxies |b from local diagnostic diagrams to high-redshift predictions for JWST |c Michaela Hirschmann, Stephane Charlot, Anna Feltre, Emma Curtis-Lake, Rachel S. Somerville, Jacopo Chevallard, Ena Choi, Dylan Nelson, Christophe Morisset, Adele Plat and Alba Vidal-Garcia |
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| 520 | |a We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of galaxy populations at redshifts from z ≈ 0 to = 8 in a full cosmological framework. We achieve this by coupling, in post-processing, the cosmological IllustrisTNG simulations with new-generation nebular-emission models, accounting for line emission from young stars, post-asymptotic giant branch (PAGB) stars, accreting black holes (BHs) and, for the first time, fast radiative shocks. The optical emission-line properties of simulated galaxies dominated by different ionizing sources in our models are largely consistent with those expected from classical diagnostic diagrams and reflect the observed increase in [O iii]/Hβ at fixed [N ii]/Hα and the evolution of the Hα, [O iii]λ5007, and [O ii] λ3727 luminosity functions from z ≈ 0 to ∼ 2. At higher redshift, we find that the emission-line galaxy population is dominated by star-forming and active galaxies, with negligible fractions of shock- and PAGB-dominated galaxies. We highlight 10 UV-diagnostic diagrams able to robustly identify the dominant ionizing sources in high-redshift galaxies. We also compute the evolution of several optical- and UV-line-luminosity functions from z = 4 to 7, and the number of galaxies expected to be detectable per field of view in deep, medium-resolution spectroscopic observations with the NIRSpec instrument on board the JWST. We find that 2-h-long exposures are sufficient to achieve unbiased censuses of Hα and [O iii]λ5007 emitters, while at least 5 h are required for Hβ, and even 10 h will detect only progressively smaller fractions of [O ii] λ3727, O iii] λ1663, C iii] λ1908, C iv λ1550, [N ii]λ6584, Si iii] λ1888, and He ii λ1640 emitters, especially in the presence of dust. | ||
| 700 | 1 | |a Charlot, Stephane |e VerfasserIn |4 aut | |
| 700 | 1 | |a Feltre, Anna |e VerfasserIn |4 aut | |
| 700 | 1 | |a Curtis-Lake, Emma |e VerfasserIn |4 aut | |
| 700 | 1 | |a Somerville, Rachel S |e VerfasserIn |4 aut | |
| 700 | 1 | |a Chevallard, Jacopo |e VerfasserIn |4 aut | |
| 700 | 1 | |a Choi, Ena |e VerfasserIn |4 aut | |
| 700 | 1 | |a Nelson, Dylan |e VerfasserIn |0 (DE-588)115182805X |0 (DE-627)101233600X |0 (DE-576)42382581X |4 aut | |
| 700 | 1 | |a Morisset, Christophe |e VerfasserIn |4 aut | |
| 700 | 1 | |a Plat, Adele |e VerfasserIn |4 aut | |
| 700 | 1 | |a Vidal-Garcia, Alba |e VerfasserIn |4 aut | |
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