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REVIEW 2 major objections 1 minor 217 references

New constraints on stellar feedback through [O III] emission: interpreting ALMA and JWST observations with SPICE simulations

T0 review · 2 major / 1 minor · reviewed 2026-05-10 · grok-4.3

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Pith's one-line read Bursty supernova feedback produces fewer bright [OIII] emitters than smooth feedback by z=5.

desk verdict The paper shows clear differences in [OIII] luminosity functions and galaxy properties across three supernova feedback models in SPICE, but those differences rest on an unvalidated sub-grid emission prescription. read the letter →

arxiv 2604.18730 v1 submitted 2026-04-20 astro-ph.GA

Benedetta Casavecchia , Aniket Bhagwat , Benedetta Ciardi , Celine Peroux , Tiago Costa This is my paper · ORCID
classification astro-ph.GA
keywords stellarfeedback[OIII]emissionhigh-redshiftgalaxiessupernovaprescriptionsmetalenrichmentluminosityfunctionscosmologicalsimulationsEpochofReionization
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper introduces a post-processing pipeline to calculate [OIII] line emission from radiation-hydrodynamical simulations that test three different supernova feedback prescriptions. It finds that the bursty supernova model ionizes gas efficiently yet enriches galaxies with metals less effectively than the smooth model, yielding fewer luminous [OIII] sources at high redshift while both the bursty and hypernova models suppress the bright end of the luminosity function. Emission arises mainly from gas that is simultaneously shock-heated and radiatively ionized, with links to neutral gas content and the mass-metallicity relation. This matters for interpreting new ALMA and JWST detections of [OIII] at z greater than 6, because the line serves as a direct probe of how stellar feedback shapes early galaxy growth and metal distribution.

What carries the argument

Post-processing pipeline for [OIII] line emission that applies a sub-grid model of combined shock heating and radiative ionization to the output of SPICE simulations run with three distinct supernova feedback prescriptions.

What would settle it

Comparison of the predicted [OIII] luminosity functions at z approximately 5 to 7 from each feedback model against the number counts of bright emitters measured in JWST or ALMA surveys; mismatch at the bright end would falsify the differential effect of bursty versus smooth feedback.

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Extended reading notes

Core claim

We have developed a post-processing pipeline that implements a sub-grid model for [OIII] line emission within the SPICE radiation-hydrodynamical simulations exploring three supernova feedback prescriptions: bursty-sn, smooth-sn, and hyper-sn. [OIII] emission predominantly originates from gas that is both shock-heated and radiatively ionized. The bursty-sn model efficiently ionizes gas but enriches galaxies less effectively by z = 5, leading to fewer bright [OIII] emitters compared to the smooth-sn model, while both bursty-sn and hyper-sn produce suppressed luminosity functions. Spatially resolved maps show that smooth-sn tends to generate more compact galaxies and slightly higher V/σ values,

Load-bearing premise

The sub-grid model for [OIII] line emission accurately represents the combined effects of shock heating and radiative ionization across unresolved scales in the simulations.

Editorial extensions

If this is right

  • [OIII] emission acts as a sensitive tracer of stellar feedback at high redshift.
  • Bursty and hypernova models both suppress the bright end of the [OIII] luminosity function relative to smooth feedback.
  • Smooth feedback produces more compact galaxies with modestly higher V/σ ratios, though substantial overlap remains between models.
  • The correlation between neutral gas fraction and [OIII] luminosity differs across feedback prescriptions.
  • Observations must reach fainter luminosities to capture the strongest effects of feedback on [OIII] emission.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the models are correct, wide-field JWST [OIII] surveys at z greater than 6 could discriminate among supernova feedback implementations used in galaxy formation simulations.
  • The significant overlap in morphological and kinematic properties suggests that multi-line or spatially resolved data will be required to break degeneracies between feedback models.
  • The same post-processing approach could be applied to other rest-frame optical or far-infrared lines to test consistency of the inferred feedback effects.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

2 major / 1 minor

Summary. The manuscript introduces a post-processing pipeline implementing a sub-grid model for [O III] line emission applied to SPICE radiation-hydrodynamical simulations. These simulations compare three supernova feedback prescriptions: bursty-sn, smooth-sn, and hyper-sn. The analysis focuses on how these models influence metal enrichment, neutral gas fractions, ionized halo morphologies, and [O III] luminosity functions at high redshifts (z > 5). The paper concludes that [O III] emission primarily comes from gas that is both shock-heated and radiatively ionized, that the bursty-sn model ionizes gas efficiently but enriches less effectively leading to fewer bright [O III] emitters by z=5, and that both bursty-sn and hyper-sn produce suppressed luminosity functions compared to smooth-sn.

Significance. Should the sub-grid [O III] model prove reliable, the results offer significant implications for interpreting JWST and ALMA observations of high-redshift galaxies. By linking specific feedback implementations to observable [O III] properties, the work highlights [O III] as a useful tracer for stellar feedback effects during the Epoch of Reionization. The multi-model comparison and emphasis on faint luminosity regimes where feedback impacts are pronounced represent valuable contributions to the field.

major comments (2)
  1. [Post-processing pipeline description] All reported differences between the feedback models in terms of [O III] luminosity functions, ionization efficiency, and enrichment (e.g., bursty-sn producing fewer bright emitters) depend on the sub-grid prescription for [O III] emissivity. The manuscript should include explicit validation tests of this model, such as comparisons to higher-resolution simulations or analytic models of shock and photo-ionization, to confirm that the joint effects are accurately captured rather than being dominated by the approximation.
  2. [Results section on luminosity functions and correlations] The claims of suppressed luminosity functions for bursty-sn and hyper-sn lack accompanying quantitative measures of uncertainty, such as Poisson errors or cosmic variance estimates, and do not discuss how sensitive these suppressions are to the sub-grid parameters. This makes it challenging to evaluate the robustness of the conclusion that these models are distinguishable from smooth-sn.
minor comments (1)
  1. [Discussion of spatially resolved properties] The statement regarding significant overlap between models in V/σ values could be expanded with quantitative metrics or histograms to better illustrate the degree of overlap.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their constructive and insightful report. Their comments correctly identify areas where additional validation and quantitative robustness checks would strengthen the manuscript. We address each major comment below and describe the revisions we will implement.

read point-by-point responses

  1. Referee: [Post-processing pipeline description] All reported differences between the feedback models in terms of [O III] luminosity functions, ionization efficiency, and enrichment (e.g., bursty-sn producing fewer bright emitters) depend on the sub-grid prescription for [O III] emissivity. The manuscript should include explicit validation tests of this model, such as comparisons to higher-resolution simulations or analytic models of shock and photo-ionization, to confirm that the joint effects are accurately captured rather than being dominated by the approximation.

    Authors: We agree that the sub-grid [O III] model is foundational to all reported differences and that explicit validation strengthens the interpretation. The model combines standard treatments of collisional excitation in shock-heated gas with radiative ionization, calibrated to local benchmarks and theoretical expectations as outlined in the methods. However, the original manuscript did not present dedicated validation tests against higher-resolution simulations or analytic ionization models. In the revised version we will add a new subsection containing such tests, including direct comparisons to analytic shock and photo-ionization calculations and, where feasible, to results from higher-resolution zoom simulations. These additions will demonstrate that the model captures the joint effects without dominating the differences between feedback prescriptions. revision: yes

  2. Referee: [Results section on luminosity functions and correlations] The claims of suppressed luminosity functions for bursty-sn and hyper-sn lack accompanying quantitative measures of uncertainty, such as Poisson errors or cosmic variance estimates, and do not discuss how sensitive these suppressions are to the sub-grid parameters. This makes it challenging to evaluate the robustness of the conclusion that these models are distinguishable from smooth-sn.

    Authors: We accept that the luminosity-function figures would benefit from explicit uncertainty quantification. The simulations occupy large cosmological volumes, but Poisson errors and cosmic-variance estimates were not reported. In the revised manuscript we will add Poisson error bars to the luminosity-function panels and include a brief assessment of cosmic variance based on the box size and halo statistics. Regarding sensitivity to sub-grid parameters, we will expand the discussion with results from parameter-variation tests performed during model development; these tests show that the main trends (suppression in bursty-sn and hyper-sn relative to smooth-sn) persist across plausible ranges of the key parameters, and we will quantify this robustness explicitly. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: inter-model differences arise from distinct feedback prescriptions

full rationale

The paper executes SPICE radiation-hydrodynamical simulations under three separate supernova feedback prescriptions (bursty-sn, smooth-sn, hyper-sn) and applies the same sub-grid post-processing pipeline to derive [OIII] emissivities. Reported contrasts in metal enrichment, neutral gas fractions, ionized halo sizes, and luminosity functions are direct simulation outputs driven by the differing feedback implementations. No step reduces a claimed prediction to a fitted parameter by construction, invokes a self-citation as the sole justification for a uniqueness claim, or renames an input as an output. The sub-grid [OIII] model is a uniform modeling assumption rather than a definitional loop, leaving the derivation chain self-contained against the simulation inputs.

Assumptions & free parameters 0 free parameters · 0 assumptions · 0 invented entities

Abstract-only review provides no explicit list of free parameters, axioms, or invented entities. The work relies on standard assumptions in radiation-hydrodynamical simulations (e.g., sub-grid physics for star formation and feedback) and the validity of the new [OIII] post-processing model.

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Cite this review

Pith. "Pith review of New constraints on stellar feedback through [O III] emission: interpreting ALMA and JWST observations with SPICE simulations." pith.science (2026). https://pith.science/paper/2604.18730

@misc{pith2026260418730,
  author       = {Pith},
  title        = {Pith review of: New constraints on stellar feedback through [O III] emission: interpreting ALMA and JWST observations with SPICE simulations},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/2604.18730}},
  note         = {Machine review of arXiv:2604.18730}
}
read the original abstract

ALMA and JWST have recently detected emission lines from the interstellar medium of star-forming galaxies during the Epoch of Reionization, reaching redshifts up to z = 14. Among these, [OIII] lines provide a powerful diagnostic of metal enrichment, gas ionization, and the impact of stellar feedback in galaxies at z > 6. Modeling this emission in cosmological simulations is challenging due to the wide range of spatial scales and physical processes involved. To address this, we have developed a post-processing pipeline that implements a sub-grid model for [OIII] line emission within the SPICE radiation-hydrodynamical simulations. These simulations explore three supernova feedback prescriptions: bursty-sn, smooth-sn, and the hypernova-based hyper-sn. We investigate how these feedback models affect metal enrichment, the neutral gas fraction, and the size and morphology of ionized halos traced by [OIII] emission in both the optical and far-infrared. We find that [OIII] emission predominantly originates from gas that is both shock-heated and radiatively ionized. We also examine the mass-metallicity relation and the correlation between neutral gas fraction and [OIII] luminosity. Our results show that the bursty-sn model efficiently ionizes gas but enriches galaxies less effectively by z = 5, leading to fewer bright [OIII] emitters compared to the smooth-sn model. Both bursty-sn and hyper-sn produce suppressed luminosity functions. Spatially resolved [OIII] emission further indicates that smooth-sn tends to generate more compact galaxies and slightly higher V/{\sigma} values, although there is significant overlap between models. Overall, our findings demonstrate that [OIII] emission is a sensitive tracer of stellar feedback at high redshift and highlight the importance of observations probing fainter luminosities, where feedback effects are strongest.

Figures

Figures reproduced from arXiv: 2604.18730 by the authors.

Figure 1
Figure 1. Maps of surface brightness in [O iii] integrated along the line of sight at 5008 Å (top row) and 88 𝜇m (bottom row) for the most massive galaxy at 𝑧 = 7. The first column shows the map for the bursty-sn model, the second for hyper-sn, and the third for smooth-sn. In each panel, the insets in the bottom-right corner display the velocity field maps derived from the luminosities at 5008 Å (top) and 88 𝜇m (bottom). Addi… view at source ↗
Figure 2
Figure 2. Temperature–density diagram of gas cells in the most massive galaxy at 𝑧 = 5, for the bursty-sn (top panel) and smooth-sn (bottom panel) models. The 2D distribution is color-coded by the sum of intrinsic optical [O iii] luminosities in each density–temperature bin. The plot reveals a multiphase interstellar medium, structured as follows: diffuse, hot gas pro￾duced by stellar feedback (a); shocked gas (b); warm gas i… view at source ↗
Figure 3
Figure 3. Contribution from each gas phase to the total intrinsic optical [O iii] luminosity, at redshifts 𝑧 = 10, 7, and 5. Red, green, and blue bars represent results from the bursty-sn, hyper-sn, and smooth-sn feedback models, respectively. Following the notation introduced in [PITH_FULL_IMAGE:figures/full_fig_p006_3.png] view at source ↗
Figures from the paper (7 more)
Figure 4
Figure 4. Figure 4: The left y-axis shows the gas metallicities (dots), while the right y-axis indicates metallicities expressed in terms of [O/H] (crosses). Solid lines show the optical [O iii] luminosity-weighted mean relations in bins of stellar mass. Red, green, and blue points corres…
Figure 5
Figure 5. Figure 5: Dust-corrected luminosity functions of [O iii] at 𝑧 = 10, 7, and 5 for the bursty-sn (red), hyper-sn (green), and smooth-sn (blue) feedback models. Solid and dashed lines show median values for the emission at 5008 Å, and 88 𝜇m, respectively. Black points represent JWS…
Figure 6
Figure 6. Figure 6: Dust-corrected 𝐿[O iii] at 5008 Å (top) and 88 𝜇m (bottom) as a function of the neutral gas fraction within the virial radius for galaxies at 𝑧 = 10 (left) and 𝑧 = 5 (right) in the bursty-sn (red), hyper-sn (green), and smooth-sn (blue) models. Contours enclose 50% and…
Figure 8
Figure 8. Figure 8: Redshift evolution of the 𝐿[O III],5008 Å half-light radius, for the bursty-sn (red), hyper-sn (green) and smooth-sn (blue) stellar feedback models. Each point corresponds to the luminosity-weighted median value, and the error bars represent the 16th and 84th percentil…
Figure 7
Figure 7. Figure 7: Dust-corrected 𝐿[O iii] as a function of gas metallicity at 𝑧 = 10 (top), 𝑧 = 7 (middle) and 𝑧 = 5 (bottom) for the bursty-sn (red), hyper-sn (green), and smooth-sn (blue) models. Lines indicate the median luminosi￾ties for the 5008 Å (solid) and the 88 𝜇m (dashed) tra…
Figure 9
Figure 9. Figure 9: Half light radius 𝑅1/2 as a function of [O iii] luminosity at 5008 Å. The solid lines represent the median values for bursty-sn (red), hyper-sn (green) and smooth-sn (blue), the shaded areas are the 16th and 84th per￾centiles, while the stars refers to individual galax…
Figure 10
Figure 10. Figure 10: Redshift evolution of luminosity weighted 𝑉/𝜎 for galaxies with 106 M⊙ ≤ 𝑀★ ≤ 108 M⊙ (top panel) and 𝑀★ > 108 M⊙ (bottom). Solid lines displays the median values for the bursty-sn (red), hyper-sn (green) and smooth-sn (blue) supernova feedback models, while the shaded…

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Works this paper leans on

217 extracted references · 217 canonical work pages

  1. [1]

    Physics of the Interstellar and Intergalactic Medium

    work page

  2. [2]

    , keywords =

    RAMSES-RTZ: non-equilibrium metal chemistry and cooling coupled to on-the-fly radiation hydrodynamics. , keywords =. doi:10.1093/mnras/stac423 , archivePrefix =. 2202.04083 , primaryClass =

    work page doi:10.1093/mnras/stac423

  3. [3]

    , keywords =

    Non-equilibrium ionization and cooling of metal-enriched gas in the presence of a photoionization background. , keywords =. doi:10.1093/mnras/stt1043 , archivePrefix =. 1302.5710 , primaryClass =

    work page doi:10.1093/mnras/stt1043

  4. [4]

    Atomic Data and Nuclear Data Tables , year = 1997, month = jan, volume =

    A Practical Fit Formula for Ionization Rate Coefficients of Atoms and Ions by Electron Impact: Z = 1-28. Atomic Data and Nuclear Data Tables , year = 1997, month = jan, volume =. doi:10.1006/adnd.1997.0732 , adsurl =

    work page doi:10.1006/adnd.1997.0732 1997

  5. [5]

    R., 2006, @doi [The Astrophysical Journal Supplement Series] 10.1086/508465 , 167, 334–342

    Radiative Recombination Data for Modeling Dynamic Finite-Density Plasmas. , keywords =. doi:10.1086/508465 , archivePrefix =. astro-ph/0604144 , primaryClass =

    work page doi:10.1086/508465

  6. [6]

    Atomic Data for Astrophysics. II. New Analytic Fits for Photoionization Cross Sections of Atoms and Ions. , keywords =. doi:10.1086/177435 , archivePrefix =. astro-ph/9601009 , primaryClass =

    work page Pith review doi:10.1086/177435

  7. [7]

    , keywords =

    Analytical strong line diagnostics and their redshift evolution. , keywords =. doi:10.1093/mnras/stae2337 , archivePrefix =. 2312.09213 , primaryClass =

    work page doi:10.1093/mnras/stae2337

  8. [8]

    arXiv e-prints , keywords =

    A New Framework for ISM Emission Line Models: Connecting Multi-Scale Simulations Across Cosmological Volumes. arXiv e-prints , keywords =. doi:10.48550/arXiv.2409.03997 , archivePrefix =. 2409.03997 , primaryClass =

    work page doi:10.48550/arxiv.2409.03997

Show all 217 references
  1. [9]

    CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST. , keywords =. doi:10.3847/2041-8213/acade4 , archivePrefix =. 2211.05792 , primaryClass =

    doi

  2. [10]

    , keywords =

    A Comprehensive Study of Galaxies at z 9-16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch. , keywords =. doi:10.3847/1538-4365/acaaa9 , archivePrefix =. 2208.01612 , primaryClass =

    doi

  3. [11]

    , keywords =

    Two Remarkably Luminous Galaxy Candidates at z 10-12 Revealed by JWST. , keywords =. doi:10.3847/2041-8213/ac9b22 , archivePrefix =. 2207.09434 , primaryClass =

    doi

  4. [12]

    , keywords =

    UV luminosity density results at z > 8 from the first JWST/NIRCam fields: limitations of early data sets and the need for spectroscopy. , keywords =. doi:10.1093/mnras/stad1014 , archivePrefix =. 2212.06683 , primaryClass =

    doi

  5. [13]

    , keywords =

    Evolution of the UV LF from z 15 to z 8 using new JWST NIRCam medium-band observations over the HUDF/XDF. , keywords =. doi:10.1093/mnras/stad1145 , archivePrefix =. 2211.02607 , primaryClass =

    doi

  6. [14]

    Nature Astronomy , keywords =

    Spectroscopic confirmation of four metal-poor galaxies at z = 10.3-13.2. Nature Astronomy , keywords =. doi:10.1038/s41550-023-01918-w , archivePrefix =. 2212.04568 , primaryClass =

    doi

  7. [15]

    Nature Astronomy , keywords =

    Identification and properties of intense star-forming galaxies at redshifts z > 10. Nature Astronomy , keywords =. doi:10.1038/s41550-023-01921-1 , archivePrefix =. 2212.04480 , primaryClass =

    doi

  8. [16]

    , keywords =

    ALMA Detection of [O III] 88 m at z = 12.33: Exploring the Nature and Evolution of GHZ2 as a Massive Compact Stellar System. , keywords =. doi:10.3847/2041-8213/ad8f38 , archivePrefix =. 2411.03593 , primaryClass =

    doi

  9. [17]

    , keywords =

    The onset of star formation 250 million years after the Big Bang. , keywords =. doi:10.1038/s41586-018-0117-z , archivePrefix =. 1805.05966 , primaryClass =

    doi

  10. [18]

    , keywords =

    Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O III] 88 m, [C II] 158 m, and dust continuum with ALMA. , keywords =. doi:10.1093/pasj/psz049 , archivePrefix =. 1806.00486 , primaryClass =

    doi

  11. [19]

    Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6

    The ALPINE-ALMA [CII] survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6. , keywords =. doi:10.1051/0004-6361/201936965 , archivePrefix =. 1910.09517 , primaryClass =

    1910 doi

  12. [20]

    , keywords =

    A Long Time Ago in a Galaxy Far, Far Away: A Candidate z 12 Galaxy in Early JWST CEERS Imaging. , keywords =. doi:10.3847/2041-8213/ac966e , archivePrefix =. 2207.12474 , primaryClass =

    doi

  13. [21]

    , keywords =

    JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34. , keywords =. doi:10.3847/1538-4357/ad5f88 , archivePrefix =. 2403.10238 , primaryClass =

    doi

  14. [22]

    , keywords =

    Spectroscopic confirmation of two luminous galaxies at a redshift of 14. , keywords =. doi:10.1038/s41586-024-07860-9 , archivePrefix =. 2405.18485 , primaryClass =

    doi

  15. [23]

    , keywords =

    The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?. , keywords =. doi:10.1051/0004-6361/202452451 , archivePrefix =. 2409.20533 , primaryClass =

    doi

  16. [24]

    arXiv e-prints , keywords =

    The dual nature of GHZ9: coexisting AGN and star formation activity in a remote X-ray source at z=10.145. arXiv e-prints , keywords =. doi:10.48550/arXiv.2410.18763 , archivePrefix =. 2410.18763 , primaryClass =

    doi

  17. [25]

    , keywords =

    The abundance of z 10 galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging. , keywords =. doi:10.1093/mnras/stad471 , archivePrefix =. 2212.10126 , primaryClass =

    doi

  18. [26]

    , keywords =

    The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 - 15 from deep JWST and ground-based near-infrared imaging. , keywords =. doi:10.1093/mnras/stac3472 , archivePrefix =. 2207.12356 , primaryClass =

    doi

  19. [27]

    arXiv e-prints , keywords =

    The z rsim 9 galaxy UV luminosity function from the JWST Advanced Deep Extragalactic Survey: insights into early galaxy evolution and reionization. arXiv e-prints , keywords =. doi:10.48550/arXiv.2501.00984 , archivePrefix =. 2501.00984 , primaryClass =

    doi

  20. [28]

    , keywords =

    Exploring the nature of UV-bright z 10 galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?. , keywords =. doi:10.1093/mnras/stae651 , archivePrefix =. 2305.04944 , primaryClass =

    doi

  21. [29]

    , keywords =

    Seven wonders of Cosmic Dawn: JWST confirms a high abundance of galaxies and AGN at z ≃ 9 11 in the GLASS field. , keywords =. doi:10.1051/0004-6361/202452090 , archivePrefix =. 2410.10967 , primaryClass =

    doi

  22. [30]

    , keywords =

    On the stunning abundance of super-early, luminous galaxies revealed by JWST. , keywords =. doi:10.1093/mnras/stad1095 , archivePrefix =. 2208.00720 , primaryClass =

    doi

  23. [31]

    , keywords =

    The eventful life of GS-z14-0, the most distant galaxy at redshift z = 14.32. , keywords =. doi:10.1051/0004-6361/202450944 , archivePrefix =. 2405.20370 , primaryClass =

    doi

  24. [32]

    , keywords =

    The brightest galaxies at cosmic dawn. , keywords =. doi:10.1093/mnras/stad035 , archivePrefix =. 2207.14808 , primaryClass =

    doi

  25. [33]

    , keywords =

    Balancing the efficiency and stochasticity of star formation with dust extinction in z 10 galaxies observed by JWST. , keywords =. doi:10.1093/mnras/stac3578 , archivePrefix =. 2208.12826 , primaryClass =

    doi

  26. [34]

    , keywords =

    The impact of UV variability on the abundance of bright galaxies at z 9. , keywords =. doi:10.1093/mnras/stad2508 , archivePrefix =. 2305.05679 , primaryClass =

    doi

  27. [35]

    , keywords =

    A Lower Bound of Star Formation Activity in Ultra-high-redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources. , keywords =. doi:10.3847/2041-8213/ac9310 , archivePrefix =. 2208.06872 , primaryClass =

    doi

  28. [36]

    , keywords =

    Efficient formation of massive galaxies at cosmic dawn by feedback-free starbursts. , keywords =. doi:10.1093/mnras/stad1557 , archivePrefix =. 2303.04827 , primaryClass =

    doi

  29. [37]

    , keywords =

    Feedback-free starbursts at cosmic dawn: Observable predictions for JWST. , keywords =. doi:10.1051/0004-6361/202348727 , archivePrefix =. 2311.14662 , primaryClass =

    doi

  30. [38]

    , keywords =

    Redshift-dependent galaxy formation efficiency at z = 5 ‑ 13 in the FirstLight Simulations. , keywords =. doi:10.1051/0004-6361/202450224 , archivePrefix =. 2404.02537 , primaryClass =

    doi

  31. [39]

    , keywords =

    Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency. , keywords =. doi:10.1093/mnras/stae2633 , archivePrefix =. 2407.02674 , primaryClass =

    doi

  32. [40]

    arXiv e-prints , keywords =

    Detection of [OIII]88 m in JADES-GS-z14-0 at z=14.1793. arXiv e-prints , keywords =. doi:10.48550/arXiv.2409.20549 , archivePrefix =. 2409.20549 , primaryClass =

    doi

  33. [41]

    , keywords =

    Cold dust and low [O III]/[C II] ratios: an evolved star-forming population at redshift 7. , keywords =. doi:10.1093/mnras/stad3111 , archivePrefix =. 2301.09659 , primaryClass =

    doi

  34. [42]

    , keywords =

    JWST and ALMA Multiple-line Study in and around a Galaxy at z = 8.496: Optical to Far-Infrared Line Ratios and the Onset of an Outflow Promoting Ionizing Photon Escape. , keywords =. doi:10.3847/1538-4357/ad235c , archivePrefix =. 2212.06863 , primaryClass =

    doi

  35. [43]

    , keywords =

    The nature of high [O III] _ 88 m /[C II] _ 158 m galaxies in the epoch of reionization: Low carbon abundance and a top-heavy IMF?. , keywords =. doi:10.1093/mnras/stac028 , archivePrefix =. 2108.01074 , primaryClass =

    doi

  36. [44]

    arXiv e-prints , keywords =

    A theoretical investigation of far-infrared fine structure lines at z>6 and of the origin of the [OIII]88/[CII]158 enhancement. arXiv e-prints , keywords =. doi:10.48550/arXiv.2410.18471 , archivePrefix =. 2410.18471 , primaryClass =

    doi

  37. [45]

    arXiv e-prints , keywords =

    Deep Constraints on [CII]158 m in JADES-GS-z14-0: Further Evidence for a Galaxy with Low Gas Content at z=14.2. arXiv e-prints , keywords =. doi:10.48550/arXiv.2502.01610 , archivePrefix =. 2502.01610 , primaryClass =

    doi

  38. [46]

    , keywords =

    First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O III]/H Emitter at z = 6.11. , keywords =. doi:10.3847/2041-8213/ac8938 , archivePrefix =. 2207.11259 , primaryClass =

    doi

  39. [47]

    , keywords =

    ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 - 6. , keywords =. doi:10.3847/1538-4357/ac6e3f , archivePrefix =. 2204.07187 , primaryClass =

    doi

  40. [48]

    , keywords =

    The Science Performance of JWST as Characterized in Commissioning. , keywords =. doi:10.1088/1538-3873/acb293 , archivePrefix =. 2207.05632 , primaryClass =

    doi

  41. [49]

    , keywords =

    High-z galaxies with JWST and local analogues - it is not only star formation. , keywords =. doi:10.1093/mnras/stad1704 , archivePrefix =. 2208.07467 , primaryClass =

    doi

  42. [50]

    , keywords =

    A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses, and star-formation histories. , keywords =. doi:10.1093/mnrasl/slac136 , archivePrefix =. 2207.08778 , primaryClass =

    doi

  43. [51]

    , keywords =

    Direct T _ e -based Metallicities of z = 2─9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon. , keywords =. doi:10.3847/1538-4357/ad15fc , archivePrefix =. 2303.08149 , primaryClass =

    doi

  44. [52]

    , keywords =

    JADES: Detecting [OIII] 4363 emitters and testing strong line calibrations in the high-z Universe with ultra-deep JWST/NIRSpec spectroscopy up to z 9.5. , keywords =. doi:10.1051/0004-6361/202347133 , archivePrefix =. 2306.03120 , primaryClass =

    doi

  45. [53]

    , keywords =

    The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z 8. , keywords =. doi:10.1093/mnras/stac2737 , archivePrefix =. 2207.12375 , primaryClass =

    doi

  46. [54]

    , keywords =

    First insights into the ISM at z > 8 with JWST: possible physical implications of a high [O III] 4363/[O III] 5007. , keywords =. doi:10.1093/mnras/stac2657 , archivePrefix =. 2207.13693 , primaryClass =

    doi

  47. [55]

    , keywords =

    Finding Peas in the Early Universe with JWST. , keywords =. doi:10.3847/2041-8213/acaaaf , archivePrefix =. 2207.13020 , primaryClass =

    doi

  48. [56]

    , keywords =

    First look with JWST spectroscopy: Resemblance among z 8 galaxies and local analogs. , keywords =. doi:10.1051/0004-6361/202244556 , archivePrefix =. 2207.10034 , primaryClass =

    doi

  49. [57]

    , keywords =

    On the Stellar Populations of Galaxies at z = 9-11: The Growth of Metals and Stellar Mass at Early Times. , keywords =. doi:10.3847/1538-4357/ac4cad , archivePrefix =. 2111.05351 , primaryClass =

    doi

  50. [58]

    , keywords =

    Metallicities of Five z > 5 Emission-line Galaxies in SMACS 0723 Revealed by JWST. , keywords =. doi:10.3847/2041-8213/ac959d , archivePrefix =. 2208.06418 , primaryClass =

    doi

  51. [59]

    , keywords =

    The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations. , keywords =. doi:10.3847/1538-4357/acba8a , archivePrefix =. 2207.12388 , primaryClass =

    doi

  52. [60]

    , keywords =

    Spatially resolved Kennicutt-Schmidt relation at z 7 and its connection with the interstellar medium properties. , keywords =. doi:10.1093/mnras/stad3150 , archivePrefix =. 2309.07957 , primaryClass =

    doi

  53. [61]

    , keywords =

    Gas-phase metallicity gradients in galaxies at z 6 8. , keywords =. doi:10.1051/0004-6361/202449855 , archivePrefix =. 2403.03977 , primaryClass =

    doi

  54. [62]

    , keywords =

    The 2017 Release Cloudy. , keywords =. doi:10.48550/arXiv.1705.10877 , archivePrefix =. 1705.10877 , primaryClass =

    2017 doi

  55. [63]

    Radiative shock-wave theory. II. High-velocity shocks and thermal instabilities. , keywords =. doi:10.1086/163544 , adsurl =

    doi

  56. [64]

    , keywords =

    Cooling Functions for Low-Density Astrophysical Plasmas. , keywords =. doi:10.1086/191823 , adsurl =

    doi

  57. [65]

    MAPPINGS V: Astrophysical plasma modeling code

  58. [66]

    , keywords =

    The THESAN project: Lyman- emission and transmission during the Epoch of Reionization. , keywords =. doi:10.1093/mnras/stac713 , archivePrefix =. 2110.02966 , primaryClass =

    doi

  59. [67]

    , keywords =

    Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization. , keywords =. doi:10.1093/mnras/stab3710 , archivePrefix =. 2110.00584 , primaryClass =

    doi

  60. [68]

    , keywords =

    H emission in local galaxies: star formation, time variability, and the diffuse ionized gas. , keywords =. doi:10.1093/mnras/stac818 , archivePrefix =. 2112.00027 , primaryClass =

    doi

  61. [69]

    arXiv e-prints , keywords =

    Ly with SPICE: Interpreting Ly emission at z>5. arXiv e-prints , keywords =. doi:10.48550/arXiv.2408.16063 , archivePrefix =. 2408.16063 , primaryClass =

    doi

  62. [70]

    , keywords =

    SPICE: the connection between cosmic reionization and stellar feedback in the first galaxies. , keywords =. doi:10.1093/mnras/stae1125 , archivePrefix =. 2310.16895 , primaryClass =

    doi

  63. [71]

    arXiv e-prints , keywords =

    Variability of the UV luminosity function with SPICE. arXiv e-prints , keywords =. doi:10.48550/arXiv.2501.18559 , archivePrefix =. 2501.18559 , primaryClass =

    doi

  64. [72]

    , keywords =

    Suppression of star formation in dwarf galaxies by photoelectric grain heating feedback. , keywords =. doi:10.1038/nature18292 , archivePrefix =. 1605.00650 , primaryClass =

    doi

  65. [73]

    , keywords =

    Variable interstellar radiation fields in simulated dwarf galaxies: supernovae versus photoelectric heating. , keywords =. doi:10.1093/mnras/stx1773 , archivePrefix =. 1701.08779 , primaryClass =

    doi

  66. [74]

    , keywords =

    Stellar Radiation Is Critical for Regulating Star Formation and Driving Outflows in Low-mass Dwarf Galaxies. , keywords =. doi:10.3847/2041-8213/aae315 , archivePrefix =. 1808.00468 , primaryClass =

    doi

  67. [75]

    , keywords =

    The Formation of Low-metallicity Globular Clusters in Dwarf Galaxy Mergers. , keywords =. doi:10.3847/2041-8213/ab2a13 , archivePrefix =. 1905.09840 , primaryClass =

    doi

  68. [76]

    , keywords =

    EDGE: the mass-metallicity relation as a critical test of galaxy formation physics. , keywords =. doi:10.1093/mnras/stz3053 , archivePrefix =. 1904.02723 , primaryClass =

    1904 doi

  69. [77]

    , keywords =

    Simulations of the star-forming molecular gas in an interacting M51-like galaxy. , keywords =. doi:10.1093/mnras/stz3600 , archivePrefix =. 1909.10520 , primaryClass =

    1909 doi

  70. [78]

    , keywords =

    Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency. , keywords =. doi:10.1051/0004-6361/202347792 , archivePrefix =. 2308.12363 , primaryClass =

    doi

  71. [79]

    , keywords =

    The masses, structure, and lifetimes of cold clouds in a high-resolution simulation of a low-metallicity starburst. , keywords =. doi:10.1093/mnras/stae2072 , archivePrefix =. 2408.16887 , primaryClass =

    doi

  72. [80]

    arXiv e-prints , keywords =

    SILCC -- VIII: The impact of far-ultraviolet radiation on star formation and the interstellar medium. arXiv e-prints , keywords =. doi:10.48550/arXiv.2410.00124 , archivePrefix =. 2410.00124 , primaryClass =

    doi

  73. [81]

    , keywords =

    Deep into the structure of the first galaxies: SERRA views. , keywords =. doi:10.1093/mnras/stz1383 , archivePrefix =. 1905.08254 , primaryClass =

    1905 doi

  74. [82]

    , keywords =

    High [O III]/[C II] surface brightness ratios trace early starburst galaxies. , keywords =. doi:10.1093/mnras/stab1674 , archivePrefix =. 2106.05279 , primaryClass =

    doi

  75. [83]

    , keywords =

    Constraining the physical properties of gas in high-z galaxies with far-infrared and submillimetre line ratios. , keywords =. doi:10.1051/0004-6361/202449903 , archivePrefix =. 2406.11559 , primaryClass =

    doi

  76. [84]

    , keywords =

    High resolution modelling of [CII], [CI], [OIII], and CO line emission from the interstellar medium and circumgalactic medium of a star-forming galaxy at z 6.5. , keywords =. doi:10.1051/0004-6361/202346945 , archivePrefix =. 2306.00583 , primaryClass =

    doi

  77. [85]

    , keywords =

    The THESAN project: public data release of radiation-hydrodynamic simulations matching reionization-era JWST observations. , keywords =. doi:10.1093/mnras/stae839 , archivePrefix =. 2309.06475 , primaryClass =

    doi

  78. [86]

    , keywords =

    The THESAN project: predictions for multitracer line intensity mapping in the epoch of reionization. , keywords =. doi:10.1093/mnras/stac1557 , archivePrefix =. 2111.02411 , primaryClass =

    doi

  79. [87]

    Cosmic Reionization on Computers. II. Reionization History and Its Back-reaction on Early Galaxies. , keywords =. doi:10.1088/0004-637X/793/1/30 , archivePrefix =. 1403.4251 , primaryClass =

    doi

  80. [88]

    , keywords =

    Cosmic Dawn (CoDa): the First Radiation-Hydrodynamics Simulation of Reionization and Galaxy Formation in the Local Universe. , keywords =. doi:10.1093/mnras/stw2036 , archivePrefix =. 1511.00011 , primaryClass =

    doi

  81. [89]

    , keywords =

    Cosmic Dawn II (CoDa II): a new radiation-hydrodynamics simulation of the self-consistent coupling of galaxy formation and reionization. , keywords =. doi:10.1093/mnras/staa1266 , archivePrefix =. 1811.11192 , primaryClass =

    doi

  82. [90]

    , keywords =

    The short ionizing photon mean free path at z = 6 in Cosmic Dawn III, a new fully coupled radiation-hydrodynamical simulation of the Epoch of Reionization. , keywords =. doi:10.1093/mnras/stac2383 , archivePrefix =. 2202.05869 , primaryClass =

    doi

  83. [91]

    , keywords =

    The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results. , keywords =. doi:10.1093/mnras/stw2869 , archivePrefix =. 1603.00034 , primaryClass =

    doi

  84. [92]

    , keywords =

    The OBELISK simulation: Galaxies contribute more than AGN to H I reionization of protoclusters. , keywords =. doi:10.1051/0004-6361/202037698 , archivePrefix =. 2002.04045 , primaryClass =

    2002 doi

  85. [93]

    , keywords =

    The SPHINX cosmological simulations of the first billion years: the impact of binary stars on reionization. , keywords =. doi:10.1093/mnras/sty1655 , archivePrefix =. 1801.07259 , primaryClass =

    doi

  86. [94]

    , keywords =

    LyC escape from SPHINX galaxies in the Epoch of Reionization. , keywords =. doi:10.1093/mnras/stac1942 , archivePrefix =. 2207.03232 , primaryClass =

    doi

  87. [95]

    , keywords =

    Galactic Stellar and Substellar Initial Mass Function. , keywords =. doi:10.1086/376392 , archivePrefix =. astro-ph/0304382 , primaryClass =

    doi arXiv

  88. [96]

    , keywords =

    JWST Census for the Mass-Metallicity Star Formation Relations at z = 4-10 with Self-consistent Flux Calibration and Proper Metallicity Calibrators. , keywords =. doi:10.3847/1538-4365/acd556 , archivePrefix =. 2301.12825 , primaryClass =

    doi

  89. [97]

    , keywords =

    The Extreme Low-mass End of the Mass Metallicity Relation at z 7. , keywords =. doi:10.3847/2041-8213/ad8dc910.1134/S1063772908080040 , archivePrefix =. 2407.17110 , primaryClass =

    doi

  90. [98]

    EIGER. II. First Spectroscopic Characterization of the Young Stars and Ionized Gas Associated with Strong H and [O III] Line Emission in Galaxies at z = 5-7 with JWST. , keywords =. doi:10.3847/1538-4357/acc846 , archivePrefix =. 2211.08255 , primaryClass =

    doi

  91. [99]

    , keywords =

    JADES: Discovery of extremely high equivalent width Lyman- emission from a faint galaxy within an ionized bubble at z = 7.3. , keywords =. doi:10.1051/0004-6361/202346245 , archivePrefix =. 2302.12805 , primaryClass =

    doi

  92. [100]

    , keywords =

    First Sample of H +[O III] 5007 Line Emitters at z > 6 Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line-luminosity Functions. , keywords =. doi:10.3847/1538-4357/acd53c , archivePrefix =. 2209.03374 , primaryClass =

    doi

  93. [101]

    , keywords =

    JWST FRESCO: a comprehensive census of H + [O III] emitters at 6.8 < z < 9.0 in the GOODS fields. , keywords =. doi:10.1093/mnras/stae2353 , archivePrefix =. 2405.05111 , primaryClass =

    doi

  94. [102]

    , keywords =

    UNCOVERing the Faint End of the z 7 [O III] Luminosity Function with JWST's F410M Medium Bandpass Filter. , keywords =. doi:10.3847/1538-4357/ada8a6 , archivePrefix =. 2407.19023 , primaryClass =

    doi

  95. [103]

    arXiv e-prints , keywords =

    EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations. arXiv e-prints , keywords =. doi:10.48550/arXiv.2503.03813 , archivePrefix =. 2503.03813 , primaryClass =

    doi

  96. [104]

    , keywords =

    Simulating the interstellar medium and stellar feedback on a moving mesh: implementation and isolated galaxies. , keywords =. doi:10.1093/mnras/stz2391 , archivePrefix =. 1905.08806 , primaryClass =

    1905 doi

  97. [105]

    , keywords =

    The Evolution of the Intergalactic Medium. , keywords =. doi:10.1146/annurev-astro-082214-122355 , archivePrefix =. 1512.00086 , primaryClass =

    doi

  98. [106]

    , keywords =

    GRACKLE: a chemistry and cooling library for astrophysics. , keywords =. doi:10.1093/mnras/stw3291 , archivePrefix =. 1610.09591 , primaryClass =

    doi

  99. [107]

    , keywords =

    First light and reionization epoch simulations (FLARES) V: the redshift frontier. , keywords =. doi:10.1093/mnras/stac3280 , archivePrefix =. 2204.09431 , primaryClass =

    doi

  100. [108]

    , keywords =

    EPOCHS VI: the size and shape evolution of galaxies since z 8 with JWST Observations. , keywords =. doi:10.1093/mnras/stad3597 , archivePrefix =. 2309.04377 , primaryClass =

    doi

  101. [109]

    , keywords =

    Size Growth on Short Timescales of Star-forming Galaxies: Insights from Size Variation with Rest-frame Wavelength with JADES. , keywords =. doi:10.3847/1538-4357/ad919a , archivePrefix =. 2411.07458 , primaryClass =

    doi

  102. [110]

    , keywords =

    Size Evolution of the Most Massive Galaxies at 1.7 < z < 3 from GOODS NICMOS Survey Imaging. , keywords =. doi:10.1086/592836 , archivePrefix =. 0807.4141 , primaryClass =

    doi

  103. [111]

    , keywords =

    The Growth of Massive Galaxies Since z = 2. , keywords =. doi:10.1088/0004-637X/709/2/1018 , archivePrefix =. 0912.0514 , primaryClass =

    doi

  104. [112]

    , keywords =

    The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at 7 < z < 8. , keywords =. doi:10.3847/1538-4357/ab3213 , archivePrefix =. 1907.05512 , primaryClass =

    1907 doi

  105. [113]

    , keywords =

    UNIVERSEMACHINE: The correlation between galaxy growth and dark matter halo assembly from z = 0-10. , keywords =. doi:10.1093/mnras/stz1182 , archivePrefix =. 1806.07893 , primaryClass =

    doi

  106. [114]

    , keywords =

    Expectations of the Size Evolution of Massive Galaxies at 3 z 6 from the TNG50 Simulation: The CEERS/JWST View. , keywords =. doi:10.3847/1538-4357/acb926 , archivePrefix =. 2208.00007 , primaryClass =

    doi

  107. [115]

    , keywords =

    GA-NIFS: The core of an extremely massive protocluster at the epoch of reionisation probed with JWST/NIRSpec. , keywords =. doi:10.1051/0004-6361/202348824 , archivePrefix =. 2312.00899 , primaryClass =

    doi

  108. [116]

    arXiv e-prints , keywords =

    The dawn of disks: unveiling the turbulent ionised gas kinematics of the galaxy population at z 4-6 with JWST/NIRCam grism spectroscopy. arXiv e-prints , keywords =. doi:10.48550/arXiv.2503.21863 , archivePrefix =. 2503.21863 , primaryClass =

    doi

  109. [117]

    , keywords =

    Ionised gas kinematics and dynamical masses of z 6 galaxies from JADES/NIRSpec high-resolution spectroscopy. , keywords =. doi:10.1051/0004-6361/202347755 , archivePrefix =. 2308.09742 , primaryClass =

    doi

  110. [118]

    , keywords =

    ALMA hints at the presence of turbulent disk galaxies at z > 5. , keywords =. doi:10.1051/0004-6361/202245603 , archivePrefix =. 2304.00036 , primaryClass =

    doi

  111. [119]

    Science , keywords =

    A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang. Science , keywords =. doi:10.1126/science.abc1893 , archivePrefix =. 2102.05957 , primaryClass =

    doi

  112. [120]

    , keywords =

    A dynamically cold disk galaxy in the early Universe. , keywords =. doi:10.1038/s41586-020-2572-6 , archivePrefix =. 2009.01251 , primaryClass =

    2009 doi

  113. [121]

    , keywords =

    REBELS-25: discovery of a dynamically cold disc galaxy at z = 7.31. , keywords =. doi:10.1093/mnras/stae2217 , archivePrefix =. 2405.06025 , primaryClass =

    doi

  114. [122]

    , keywords =

    GA-NIFS: NIRSpec reveals evidence for non-circular motions and AGN feedback in GN20. , keywords =. doi:10.1093/mnras/stae1993 , archivePrefix =. 2403.03192 , primaryClass =

    doi

  115. [123]

    , keywords =

    The KMOS ^ 3D Survey: Design, First Results, and the Evolution of Galaxy Kinematics from 0.7 <= z <= 2.7. , keywords =. doi:10.1088/0004-637X/799/2/209 , archivePrefix =. 1409.6791 , primaryClass =

    doi

  116. [124]

    , keywords =

    The SINS Survey: SINFONI Integral Field Spectroscopy of z -0.5ex 2 Star-forming Galaxies. , keywords =. doi:10.1088/0004-637X/706/2/1364 , archivePrefix =. 0903.1872 , primaryClass =

    doi

  117. [125]

    , keywords =

    Rotation Curves in z 1-2 Star-forming Disks: Evidence for Cored Dark Matter Distributions. , keywords =. doi:10.3847/1538-4357/abb0ea , archivePrefix =. 2006.03046 , primaryClass =

    2006 doi

  118. [126]

    , keywords =

    The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z 1 star-forming galaxies. , keywords =. doi:10.1093/mnras/stw129 , archivePrefix =. 1601.03400 , primaryClass =

    doi

  119. [127]

    , keywords =

    The Evolution and Origin of Ionized Gas Velocity Dispersion from z 2.6 to z 0.6 with KMOS ^ 3D. , keywords =. doi:10.3847/1538-4357/ab27cc , archivePrefix =. 1906.02737 , primaryClass =

    1906 doi

  120. [128]

    , keywords =

    First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time. , keywords =. doi:10.1093/mnras/stz2338 , archivePrefix =. 1902.05553 , primaryClass =

    1902 doi

  121. [129]

    , keywords =

    Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence. , keywords =. doi:10.1088/2041-8205/804/2/L40 , archivePrefix =. 1503.01117 , primaryClass =

    doi

  122. [130]

    arXiv e-prints , keywords =

    A Cosmic Miracle: A Remarkably Luminous Galaxy at z_ spec =14.44 Confirmed with JWST. arXiv e-prints , keywords =

  123. [131]

    , keywords =

    Dual constraints with ALMA: new [O III] 88- m and dust-continuum observations reveal the ISM conditions of luminous LBGs at z 7. , keywords =. doi:10.1093/mnras/stac1905 , archivePrefix =. 2207.00022 , primaryClass =

    doi

  124. [132]

    , keywords =

    The ALPINE-ALMA [C II] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements. , keywords =. doi:10.3847/1538-4365/ab7ccd , archivePrefix =. 1912.01621 , primaryClass =

    1912 doi

  125. [133]

    , keywords =

    Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe. , keywords =. doi:10.3847/1538-4357/ac5a4a , archivePrefix =. 2106.13719 , primaryClass =

    doi

  126. [134]

    Survey overview and case studies

    The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was -0.5ex 1 Gyr old I. Survey overview and case studies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2505.06340 , archivePrefix =. 2505.06340 , primaryClass =

    doi

  127. [135]

    Dust attenuation properties and obscured star formation at z 4.4-5.8

    The ALPINE-ALMA [CII] survey. Dust attenuation properties and obscured star formation at z 4.4-5.8. , keywords =. doi:10.1051/0004-6361/202038163 , archivePrefix =. 2004.10760 , primaryClass =

    2004 doi

  128. [136]

    , keywords =

    The ALMA REBELS Survey: dust continuum detections at z > 6.5. , keywords =. doi:10.1093/mnras/stac1779 , archivePrefix =. 2203.15136 , primaryClass =

    doi

  129. [137]

    , keywords =

    COLDSIM predictions of [C II] emission in primordial galaxies. , keywords =. doi:10.1051/0004-6361/202450332 , archivePrefix =. 2406.01277 , primaryClass =

    doi

  130. [138]

    arXiv e-prints , keywords =

    Temporarily quiescent galaxies at cosmic dawn: probing bursty star formation. arXiv e-prints , keywords =. doi:10.48550/arXiv.2501.16418 , archivePrefix =. 2501.16418 , primaryClass =

    doi

  131. [139]

    , keywords =

    The Impact of Mass-dependent Stochasticity at Cosmic Dawn. , keywords =. doi:10.3847/1538-4357/ad7b36 , archivePrefix =. 2405.13108 , primaryClass =

    doi

  132. [140]

    arXiv e-prints , keywords =

    Cosmology with the SPHEREX All-Sky Spectral Survey. arXiv e-prints , keywords =. doi:10.48550/arXiv.1412.4872 , archivePrefix =. 1412.4872 , primaryClass =

    doi

  133. [141]

    , keywords =

    Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions. , keywords =. doi:10.1093/mnras/sty1024 , archivePrefix =. 1706.06605 , primaryClass =

    doi

  134. [142]

    , keywords =

    Dust attenuation, dust emission, and dust temperature in galaxies at z 5: a view from the FIRE-2 simulations. , keywords =. doi:10.1093/mnras/stz1324 , archivePrefix =. 1902.10152 , primaryClass =

    1902 doi

  135. [143]

    arXiv e-prints , keywords =

    Introducing the THESAN-ZOOM project: radiation-hydrodynamic simulations of high-redshift galaxies with a multi-phase interstellar medium. arXiv e-prints , keywords =. doi:10.48550/arXiv.2502.20437 , archivePrefix =. 2502.20437 , primaryClass =

    doi

  136. [144]

    arXiv e-prints , keywords =

    The Impact of Star Formation and Feedback Recipes on the Stellar Mass and Interstellar Medium of High-Redshift Galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2411.07282 , archivePrefix =. 2411.07282 , primaryClass =

    doi

  137. [145]

    Ground-based and Airborne Telescopes VIII , year = 2020, editor =

    The Atacama Large Aperture Submillimeter Telescope (AtLAST). Ground-based and Airborne Telescopes VIII , year = 2020, editor =. doi:10.1117/12.2561315 , archivePrefix =. 2011.07974 , primaryClass =

    2020 doi

  138. [146]

    , keywords =

    The ALMA Reionization Era Bright Emission Line Survey: The molecular gas content of galaxies at z 7. , keywords =. doi:10.1051/0004-6361/202347281 , archivePrefix =. 2309.15948 , primaryClass =

    doi

  139. [147]

    Molecular gas budget in the early Universe as traced by [C II]

    The ALPINE-ALMA [C II] survey. Molecular gas budget in the early Universe as traced by [C II]. , keywords =. doi:10.1051/0004-6361/202038231 , archivePrefix =. 2004.10771 , primaryClass =

    2004 doi

  140. [148]

    , keywords =

    Atomic and molecular gas as traced by [C II] emission. , keywords =. doi:10.1051/0004-6361/202452282 , archivePrefix =. 2410.14284 , primaryClass =

    doi

  141. [149]

    , keywords =

    Atomic and molecular gas from the epoch of reionisation down to redshift 2. , keywords =. doi:10.1051/0004-6361/202142264 , archivePrefix =. 2111.13701 , primaryClass =

    doi

  142. [150]

    , keywords =

    JWST high-redshift galaxy constraints on warm and cold dark matter models. , keywords =. doi:10.1051/0004-6361/202345851 , archivePrefix =. 2211.03620 , primaryClass =

    doi

  143. [151]

    , keywords =

    Molecular gas and dust properties in z > 7 quasar hosts. , keywords =. doi:10.1051/0004-6361/202453226 , archivePrefix =. 2412.02688 , primaryClass =

    doi

  144. [152]

    arXiv e-prints , keywords =

    Unveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation. arXiv e-prints , keywords =. doi:10.48550/arXiv.2505.12397 , archivePrefix =. 2505.12397 , primaryClass =

    doi

  145. [153]

    , keywords =

    RAMSES-RT: radiation hydrodynamics in the cosmological context. , keywords =. doi:10.1093/mnras/stt1722 , archivePrefix =. 1304.7126 , primaryClass =

    doi

  146. [154]

    , keywords =

    A scheme for radiation pressure and photon diffusion with the M1 closure in RAMSES-RT. , keywords =. doi:10.1093/mnras/stv567 , archivePrefix =. 1411.6440 , primaryClass =

    doi

  147. [155]

    A new high resolution code called RAMSES

    Cosmological hydrodynamics with adaptive mesh refinement. A new high resolution code called RAMSES. , keywords =. doi:10.1051/0004-6361:20011817 , archivePrefix =. astro-ph/0111367 , primaryClass =

    doi

  148. [156]

    , keywords =

    Higher order initial conditions for mixed baryon-CDM simulations. , keywords =. doi:10.1093/mnras/staa3773 , archivePrefix =. 2008.09124 , primaryClass =

    2008 doi

  149. [157]

    , keywords =

    Accurate initial conditions for cosmological N-body simulations: minimizing truncation and discreteness errors. , keywords =. doi:10.1093/mnras/staa3149 , archivePrefix =. 2008.09588 , primaryClass =

    2008 doi

  150. [158]

    Planck 2015 results. XIII. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201525830 , archivePrefix =. 1502.01589 , primaryClass =

    2015 doi

  151. [159]

    , year = 1998, month = jul, volume =

    CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra. , year = 1998, month = jul, volume =. doi:10.1086/316190 , adsurl =

    1998 doi

  152. [160]

    , keywords =

    Global Models of the Interstellar Medium in Disk Galaxies. , keywords =. doi:10.1086/175303 , adsurl =

    doi

  153. [161]

    , keywords =

    The Birth of a Galaxy: Primordial Metal Enrichment and Stellar Populations. , keywords =. doi:10.1088/0004-637X/745/1/50 , archivePrefix =. 1011.2632 , primaryClass =

    doi

  154. [162]

    Radiative Transfer in a Clumpy Universe. II. The Ultraviolet Extragalactic Background. , keywords =. doi:10.1086/177035 , archivePrefix =. astro-ph/9509093 , primaryClass =

    doi

  155. [163]

    , keywords =

    Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation. , keywords =. doi:10.1093/mnras/stz3495 , archivePrefix =. 1906.11836 , primaryClass =

    1906 doi

  156. [164]

    , keywords =

    Binary Population and Spectral Synthesis Version 2.1: Construction, Observational Verification, and New Results. , keywords =. doi:10.1017/pasa.2017.51 , archivePrefix =. 1710.02154 , primaryClass =

    2017 doi

  157. [165]

    , keywords =

    Re-evaluating old stellar populations. , keywords =. doi:10.1093/mnras/sty1353 , archivePrefix =. 1805.08784 , primaryClass =

    doi

  158. [166]

    , keywords =

    A simple model for molecular hydrogen chemistry coupled to radiation hydrodynamics. , keywords =. doi:10.1093/mnras/sty1556 , archivePrefix =. 1802.00445 , primaryClass =

    doi

  159. [167]

    European Southern Observatory Conference and Workshop Proceedings , year = 1989, editor =

    The OIII Temperature Problem for Extended Nebulosities. European Southern Observatory Conference and Workshop Proceedings , year = 1989, editor =

    1989

  160. [168]

    , keywords =

    Discrepancies between the [O iii] and [S iii] temperatures in H ii regions. , keywords =. doi:10.1051/0004-6361/201219515 , archivePrefix =. 1209.0808 , primaryClass =

    doi

  161. [169]

    Astrophysics of gaseous nebulae and active galactic nuclei

  162. [170]

    , keywords =

    Modern yields per stellar generation: the effect of the IMF. , keywords =. doi:10.1093/mnras/stv2598 , archivePrefix =. 1503.08300 , primaryClass =

    doi

  163. [171]

    Trading oxygen for iron. I. The [O/Fe]-specific star formation rate relation of galaxies. , keywords =. doi:10.1051/0004-6361/202347602 , archivePrefix =. 2308.00023 , primaryClass =

    doi

  164. [172]

    , keywords =

    Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations. , keywords =. doi:10.1111/j.1365-2966.2009.15331.x , archivePrefix =. 0902.1535 , primaryClass =

    2009 doi

  165. [173]

    , keywords =

    Galactic chemical enrichment with new metallicity dependent stellar yields. , keywords =. doi:10.48550/arXiv.astro-ph/9711337 , archivePrefix =. astro-ph/9711337 , primaryClass =

    doi

  166. [174]

    The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis. , keywords =. doi:10.1086/192237 , adsurl =

    doi

  167. [175]

    , keywords =

    Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback. , keywords =. doi:10.1093/mnras/stv2126 , archivePrefix =. 1501.03155 , primaryClass =

    doi

  168. [176]

    A model for chemical enrichment

    Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations - I. A model for chemical enrichment. , keywords =. doi:10.1111/j.1365-2966.2005.09574.x , archivePrefix =. astro-ph/0505440 , primaryClass =

    2005 doi

  169. [177]

    A multiphase model with supernova energy feedback

    Feedback and metal enrichment in cosmological SPH simulations - II. A multiphase model with supernova energy feedback. , keywords =. doi:10.1111/j.1365-2966.2006.10785.x , archivePrefix =. astro-ph/0604524 , primaryClass =

    2006 doi

  170. [178]

    Metal cooling and metal diffusion

    The enrichment of the intergalactic medium with adiabatic feedback - I. Metal cooling and metal diffusion. , keywords =. doi:10.1111/j.1365-2966.2010.17047.x , archivePrefix =. 0910.5956 , primaryClass =

    2010 doi

  171. [179]

    , keywords =

    The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations. , keywords =. doi:10.1093/mnras/stt1770 , archivePrefix =. 1309.2946 , primaryClass =

    doi

  172. [180]

    , keywords =

    Synthetic nebular emission from massive galaxies - I: origin of the cosmic evolution of optical emission-line ratios. , keywords =. doi:10.1093/mnras/stx2180 , archivePrefix =. 1706.00010 , primaryClass =

    doi

  173. [181]

    , keywords =

    S \'I GAME Simulations of the [CII], [OI], and [OIII] Line Emission from Star-forming Galaxies at z≃ 6. , keywords =. doi:10.3847/1538-4357/aa86b4 , archivePrefix =. 1708.04936 , primaryClass =

    doi

  174. [182]

    , keywords =

    The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. , keywords =. doi:10.1051/0004-6361/201322489 , archivePrefix =. 1402.4075 , primaryClass =

    doi

  175. [183]

    , keywords =

    Simulations of High-redshift [O III] Emitters: Chemical Evolution and Multiline Diagnostics. , keywords =. doi:10.3847/1538-4357/ace25a , archivePrefix =. 2301.02416 , primaryClass =

    doi

  176. [184]

    Diagnosing the interstellar medium of galaxies with far-infrared emission lines. II. [C II], [O I], [O III], [N II], and [N III] up to z = 6. , keywords =. doi:10.1051/0004-6361/202243358 , archivePrefix =. 2205.11955 , primaryClass =

    doi

  177. [185]

    arXiv e-prints , keywords =

    The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6. arXiv e-prints , keywords =. doi:10.48550/arXiv.2507.11600 , archivePrefix =. 2507.11600 , primaryClass =

    doi

  178. [186]

    arXiv e-prints , keywords =

    Exploring Spatially-Resolved Metallicities, Dynamics and Outflows in Low-Mass Galaxies at z 7.6. arXiv e-prints , keywords =. doi:10.48550/arXiv.2507.14936 , archivePrefix =. 2507.14936 , primaryClass =

    doi

  179. [187]

    arXiv e-prints , keywords =

    On the origins of oxygen: ALMA and JWST characterise the multi-phase, metal-enriched, star-bursting medium within a 'normal' z > 11 galaxy. arXiv e-prints , keywords =. doi:10.48550/arXiv.2507.22888 , archivePrefix =. 2507.22888 , primaryClass =

    doi

  180. [188]

    Science , keywords =

    Detection of an oxygen emission line from a high-redshift galaxy in the reionization epoch. Science , keywords =. doi:10.1126/science.aaf0714 , archivePrefix =. 1606.04989 , primaryClass =

    doi

  181. [189]

    , keywords =

    Extended ionised and clumpy gas in a normal galaxy at z = 7.1 revealed by ALMA. , keywords =. doi:10.1051/0004-6361/201630366 , archivePrefix =. 1701.03468 , primaryClass =

    doi

  182. [190]

    , keywords =

    Large Population of ALMA Galaxies at z > 6 with Very High [O III] 88 m to [C II] 158 m Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?. , keywords =. doi:10.3847/1538-4357/ab94bd , archivePrefix =. 1910.10927 , primaryClass =

    1910 doi

  183. [191]

    The Herschel Dwarf Galaxy Survey. I. Properties of the low-metallicity ISM from PACS spectroscopy. , keywords =. doi:10.1051/0004-6361/201425207 , archivePrefix =. 1502.03131 , primaryClass =

    doi

  184. [192]

    , keywords =

    ALMA uncovers the [C II] emission and warm dust continuum in a z = 8.31 Lyman break galaxy. , keywords =. doi:10.1093/mnras/staa509 , archivePrefix =. 2001.02812 , primaryClass =

    2001 doi

  185. [193]

    , keywords =

    The Mass-Metallicity Relation at z ≃ 8: Direct-method Metallicity Constraints and Near-future Prospects. , keywords =. doi:10.3847/1538-4357/abb943 , archivePrefix =. 2006.02447 , primaryClass =

    2006 doi

  186. [194]

    , keywords =

    Missing [C II] emission from early galaxies. , keywords =. doi:10.1093/mnras/staa3178 , archivePrefix =. 2006.09402 , primaryClass =

    2006 doi

  187. [195]

    , keywords =

    Ionization state of inter-stellar medium in galaxies: evolution, SFR-M _ * -Z dependence, and ionizing photon escape. , keywords =. doi:10.1093/mnras/stu902 , archivePrefix =. 1309.0207 , primaryClass =

    doi

  188. [196]

    , keywords =

    JADES: Probing interstellar medium conditions at z 5.5-9.5 with ultra-deep JWST/NIRSpec spectroscopy. , keywords =. doi:10.1051/0004-6361/202346107 , archivePrefix =. 2302.04298 , primaryClass =

    doi

  189. [197]

    arXiv e-prints , keywords =

    The Multi-Scale Multi-Phase Circumgalactic Medium: Observed and Simulated. arXiv e-prints , keywords =. doi:10.48550/arXiv.2411.07988 , archivePrefix =. 2411.07988 , primaryClass =

    doi

  190. [198]

    , keywords =

    Efficient simulations of ionized ISM emission lines: a detailed comparison between the FIRE high-redshift suite and observations. , keywords =. doi:10.1093/mnras/stad2571 , archivePrefix =. 2304.09261 , primaryClass =

    doi

  191. [199]

    , keywords =

    Standard Solar Composition. , keywords =. doi:10.1023/A:1005161325181 , adsurl =

    doi

  192. [200]

    , keywords =

    Fitting spectral energy distributions of FMOS-COSMOS emission-line galaxies at z 1.6: Star formation rates, dust attenuation, and [OIII] 5007 emission-line luminosities. , keywords =. doi:10.1051/0004-6361/202140890 , archivePrefix =. 2108.13321 , primaryClass =

    doi

  193. [201]

    arXiv e-prints , keywords =

    REBELS-IFU: on the origin of the elevated [OIII]/[CII] ratios in the early Universe. arXiv e-prints , keywords =. doi:10.48550/arXiv.2509.16071 , archivePrefix =. 2509.16071 , primaryClass =

    doi

  194. [202]

    , keywords =

    Galaxy growth in a massive halo in the first billion years of cosmic history. , keywords =. doi:10.1038/nature24629 , archivePrefix =. 1712.03020 , primaryClass =

    doi

  195. [203]

    , keywords =

    No Evidence for Enhanced [O III] 88 m Emission in a z 6 Quasar Compared to Its Companion Starbursting Galaxy. , keywords =. doi:10.3847/2041-8213/aaf4fa , archivePrefix =. 1811.12836 , primaryClass =

    doi

  196. [204]

    , keywords =

    Detection of the Far-infrared [O III] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era. , keywords =. doi:10.3847/1538-4357/ab0374 , archivePrefix =. 1806.04132 , primaryClass =

    doi

  197. [205]

    , keywords =

    ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13. , keywords =. doi:10.3847/1538-4357/ac795b , archivePrefix =. 2206.06939 , primaryClass =

    doi

  198. [206]

    , keywords =

    Detection of nitrogen and oxygen in a galaxy at the end of reionization. , keywords =. doi:10.1093/pasj/psac018 , archivePrefix =. 2202.09945 , primaryClass =

    doi

  199. [207]

    , keywords =

    ALMA Detections of [O III] and [C II] Emission Lines From A1689-zD1 at z = 7.13. , keywords =. doi:10.3847/1538-4357/ac5cc7 , adsurl =

    doi

  200. [208]

    , keywords =

    Gas conditions of a star-formation selected sample in the first billion years. , keywords =. doi:10.1093/mnras/stae1613 , archivePrefix =. 2406.19439 , primaryClass =

    doi

  201. [209]

    , keywords =

    The ALMA REBELS survey: [O III] _ 88 m line scans of UV-bright z 7.6 galaxies. , keywords =. doi:10.1093/mnras/staf1287 , archivePrefix =. 2508.02390 , primaryClass =

    doi

  202. [210]

    , keywords =

    RASCAS: RAdiation SCattering in Astrophysical Simulations. , keywords =. doi:10.1051/0004-6361/201834961 , archivePrefix =. 2001.11252 , primaryClass =

    2001 doi

  203. [211]

    , keywords =

    The origin and implications of dark matter anisotropic cosmic infall on -0.5ex _ * haloes. , keywords =. doi:10.1111/j.1365-2966.2004.07883.x , archivePrefix =. astro-ph/0402405 , primaryClass =

    2004 doi

  204. [212]

    , keywords =

    AGN-driven outflows and the formation of Ly nebulae around high-z quasars. , keywords =. doi:10.1093/mnras/stac2432 , archivePrefix =. 2203.11232 , primaryClass =

    doi

  205. [213]

    , keywords =

    Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era. , keywords =. doi:10.1093/mnras/staa2809 , archivePrefix =. 2001.01853 , primaryClass =

    2001 doi

  206. [214]

    , keywords =

    A survey of high-z galaxies: SERRA simulations. , keywords =. doi:10.1093/mnras/stac1281 , archivePrefix =. 2201.02636 , primaryClass =

    doi

  207. [215]

    arXiv e-prints , keywords =

    MEGATRON: Reproducing the Diversity of High-Redshift Galaxy Spectra with Cosmological Radiation Hydrodynamics Simulations. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.05201 , archivePrefix =. 2510.05201 , primaryClass =

    doi

  208. [216]

    , keywords =

    REBELS-IFU: evidence for metal-rich massive galaxies at z 6 - 8. , keywords =. doi:10.1093/mnras/staf2023 , archivePrefix =. 2501.10559 , primaryClass =

    doi

  209. [217]

    arXiv e-prints , keywords =

    MEGATRON: Disentangling Physical Processes and Observational Bias in the Multi-Phase ISM of High-Redshift Galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.06347 , archivePrefix =. 2510.06347 , primaryClass =

    doi

Pith tools

Reviewed May 10, 2026 · model on record in the stance chip above.