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HI Simulations for Cosmology with the SKA Observatory

T0 review · 1 major / 2 minor · reviewed 2026-06-25 · grok-4.3

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Pith's one-line read Semi-analytical and empirical models agree on cosmic HI density but differ systematically in the HI-halo mass relation and its redshift evolution.

desk verdict A useful but narrow inter-model comparison of HI predictions that flags differences in halo relations without new methods or broad validation. read the letter →

arxiv 2606.25969 v1 pith:2EVIXQNA submitted 2026-06-24 astro-ph.CO

Tommaso Ronconi , Gabriella De Lucia , Marta Spinelli , Pascal Hitz , Fabio Fontanot , Francesco Sinigaglia , Lizhi Xie , Robert M. Yates
show 10 more authors
José Luis Bernal Anna Bonaldi Stefano Camera Isabella P. Carucci Steven Cunnington Francisco-Shu Kitaura Joël Mayor Rajesh Mondal Giulia Piccirilli Digvijay Wadekar
This is my paper · ORCID
classification astro-ph.CO
keywords neutralhydrogenHImodelingsemi-analyticalmodelsempiricalhalomassrelationpost-reionizationcosmologySKAsurveys
open problems Dark Matter
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 compares methods for modeling neutral hydrogen in the post-reionization Universe ahead of large radio surveys. Semi-analytical approaches evolve baryonic components inside dark matter merger trees according to physical prescriptions, while empirical schemes rely on fast approximations tuned to observables. The side-by-side assessment finds agreement on the total cosmic HI density yet systematic differences in the shape, scatter, and redshift evolution of the HI-halo mass relation. This distinction matters because accurate models are required both to interpret new HI measurements and to plan survey strategies. The work notes that semi-analytical models rest on chosen prescriptions while empirical ones trade some robustness for speed in unexplored parameter regions.

What carries the argument

The direct comparison of semi-analytical models that self-consistently evolve baryonic components within dark matter merger trees against empirical schemes based on fast approximations for large ensemble studies.

What would settle it

New HI observations that either remove the reported systematic differences in the HI-halo mass relation across redshifts or produce substantially larger discrepancies than those identified in the comparison.

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Extended reading notes

Core claim

By comparing the predictions from the different methods considered, we find overall consistency in integrated quantities such as Ω_HI, yet systematic differences in the detailed shape and scatter of the HI--halo mass relation and its redshift evolution. Semi-analytical models offer physically grounded predictions but depend on assumed prescriptions, while empirical methods provide flexibility and computational efficiency at the expense of robustness in extrapolated regions of the parameter space.

Load-bearing premise

The collection of semi-analytical and empirical models examined is representative enough of plausible physical assumptions to support general statements about differences between the two classes.

Editorial extensions

If this is right

  • New HI measurements will supply critical observational constraints to refine and calibrate current simulation methodologies.
  • Increasingly realistic HI simulations will help interpret data and guide survey design and analysis strategies.
  • Integrated quantities such as the cosmic HI density remain robust across modeling approaches.
  • The detailed HI-halo mass relation and its evolution require further calibration because different methods produce systematic variations in shape and scatter.

Reading between the lines

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

  • If future data favor one class of models over the other in the scatter at fixed halo mass, that could guide which approach to prioritize for volume-limited forecasts.
  • Empirical models might be adjusted using semi-analytical outputs in well-constrained regimes to combine speed with physical insight for very large mock catalogs.
  • Differences in redshift evolution could alter predictions for how HI traces the growth of cosmic structure at higher redshifts.
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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

1 major / 2 minor

Summary. The manuscript provides a comparative overview of semi-analytical and empirical methods for modeling neutral hydrogen (HI) distribution in the post-reionization Universe in preparation for SKAO surveys. It assesses how different physical and empirical assumptions affect predictions for key observables including the cosmic HI density Ω_HI, the HI mass function, and the HI-halo mass relation. The central finding is overall consistency across methods in integrated quantities such as Ω_HI, accompanied by systematic differences in the detailed shape, scatter, and redshift evolution of the HI-halo mass relation.

Significance. If the reported class-level differences hold after addressing model selection, the work would help quantify modeling uncertainties relevant to interpreting SKA precursor data from MeerKAT, ASKAP, and FAST and to guiding SKAO survey design. The explicit contrast between physically motivated but prescription-dependent semi-analytical models and computationally efficient but less robust empirical schemes identifies where future observations can provide calibration.

major comments (1)
  1. [Model selection and comparison sections] The headline claim of systematic differences between the semi-analytical and empirical classes (abstract and concluding discussion) is load-bearing for the paper's utility, yet rests on the untested assumption that the finite set of examined models spans the dominant physical variations within each class. The manuscript does not demonstrate coverage of key variants such as alternative feedback implementations or HI assignment schemes, leaving open the possibility that reported differences are model-specific rather than class-wide.
minor comments (2)
  1. The abstract would be strengthened by stating the exact number of models in each category and the redshift range over which the comparisons are performed.
  2. Figure captions comparing the HI-halo mass relation should explicitly label which curves correspond to semi-analytical versus empirical approaches and note any shared parameter choices.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for the constructive report and the recommendation for major revision. We address the major comment point by point below, proposing targeted revisions to clarify the scope of our model comparison while preserving the paper's core findings on consistency in integrated quantities and differences in the HI-halo mass relation.

read point-by-point responses

  1. Referee: [Model selection and comparison sections] The headline claim of systematic differences between the semi-analytical and empirical classes (abstract and concluding discussion) is load-bearing for the paper's utility, yet rests on the untested assumption that the finite set of examined models spans the dominant physical variations within each class. The manuscript does not demonstrate coverage of key variants such as alternative feedback implementations or HI assignment schemes, leaving open the possibility that reported differences are model-specific rather than class-wide.

    Authors: We agree that the manuscript should more explicitly address the rationale and limitations of model selection. The models examined are the primary state-of-the-art examples used in the SKAO preparation literature, chosen because they represent the dominant semi-analytical frameworks (varying in merger-tree evolution and baryonic prescriptions) and empirical schemes (differing in observable-based HI assignments) available at the time of writing. Nevertheless, we acknowledge that the comparison does not exhaustively sample all possible variants. In revision, we will add a dedicated paragraph to the model selection section discussing the criteria for inclusion, noting unexamined alternatives such as different AGN feedback implementations or alternative HI partitioning schemes, and qualifying that the reported class-level trends are based on the models considered. We will also revise the abstract and concluding discussion to state that systematic differences are observed among the examined models, while the consistency in Ω_HI holds across them. These changes will be made without expanding the model set, as the work is a comparative overview rather than a comprehensive parameter survey. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: inter-model comparison without derivation chain

full rationale

The paper is a comparative overview of existing semi-analytical and empirical HI modeling methods, reporting consistency in integrated quantities like Ω_HI and differences in the HI-halo mass relation shape and evolution. No new derivation, prediction, or first-principles result is claimed that reduces by construction to fitted inputs, self-citations, or ansatzes defined inside the paper. The central claims rest on direct inter-model comparisons rather than any load-bearing step that equates output to input. This is self-contained against external benchmarks and matches the expected honest non-finding for such survey-style work.

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

The paper is an overview; it does not introduce new free parameters, axioms, or invented entities beyond those already present in the referenced semi-analytical and empirical HI models.

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Cite this review

Pith. "Pith review of HI Simulations for Cosmology with the SKA Observatory." pith.science (2026). https://pith.science/paper/2EVIXQNA

@misc{pith2026260625969,
  author       = {Pith},
  title        = {Pith review of: HI Simulations for Cosmology with the SKA Observatory},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/2EVIXQNA}},
  note         = {Machine review of arXiv:2606.25969}
}
abstract

We present a comparative overview of state-of-the-art methods for modelling the distribution of neutral hydrogen (HI) in the post-reionization Universe, developed in preparation for upcoming SKAO cosmological surveys. Our aim is to assess how different physical and empirical assumptions reflect into predictions for key observables such as the cosmic HI density, the HI mass function, and the HI-halo mass relation. We consider both: (i) semi-analytical approaches that self-consistently evolve baryonic components within dark matter merger trees through physically motivated prescriptions and (ii) empirical schemes tailored to different observables and based on fast approximations designed for large ensemble studies. By comparing the predictions from the different methods considered, we find overall consistency in integrated quantities such as $\Omega_{\mathrm{HI}}$, yet systematic differences in the detailed shape and scatter of the HI--halo mass relation and its redshift evolution. Semi-analytical models offer physically grounded predictions but depend on assumed prescriptions, while empirical methods provide flexibility and computational efficiency at the expense of robustness in extrapolated regions of the parameter space. The increasing number of HI measurements from SKA precursors and pathfinders (including surveys with MeerKAT, ASKAP, and FAST) will provide critical observational constraints to refine and calibrate current simulation methodologies. In turn, increasingly realistic HI simulations play a key role in interpreting these data, guiding survey design and analysis strategies, in preparation for the advent of SKAO data.

Figures

Figures reproduced from arXiv: 2606.25969 by the authors.

Figure 1
Figure 1. Measurements of ΩHI at different redshifts from 3 methods out of the 4 listed in the Chapter. For comparison, we also mark the empirical relation found in Crighton et al. (2015) that represents a fit to observational data. slice considered and is thus not present for sam1 and sam2 whose boxes are associated to discrete redshift values. The ΩHI-dimension error was computed by bootstrap resampling both the boxes and t… view at source ↗
Figure 2
Figure 2. HI mass functions at redshift 𝑧 = 0 (left panel) and 𝑧 = 0.5 (right panel). Measurements from sam1 (green diamonds), sam2 (light-blue plus symbols), emp1.1 (lavender triangles) and emp1.2 (empty golden squares) are shown along with analytical models fitted to data. The models shown in the upper left panel represent fit to different survey data: HIPASS (bronze dashed-dotted line, Zwaan et al., 2005), ALFALFA-40% (gra… view at source ↗
Figure 3
Figure 3. Comparison of the Hi –halo mass (HIHM) relation at 𝑧 = 0.25 obtained from all the models considered in this work. The upper panels and lower left panel show the percent abundance of haloes in the (𝑀halo, 𝑀HI) plane for sam2 (upper left), emp1 (upper right) and emp3 (lower left). Blue shaded regions indicate the density of simulated haloes, while empty black squares with error bars mark the mean and standard deviatio… view at source ↗
Figures from the paper (2 more)
Figure 4
Figure 4. Figure 4: Same as [PITH_FULL_IMAGE:figures/full_fig_p019_4.png]
Figure 5
Figure 5. Figure 5: Marked power spectrum measured on the redshift 𝑧 = 1 boxes of sam1 (green diamonds connected by a green solid line), emp2 (blue downward triangles connected by blue solid line) and emp3 (orange crosses connected by the orange solid line). As a term of comparison, we ov…

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Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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    astro-ph.CO 2026-07 accept novelty 5.0 of 10

    meer21cm is a publicly available Python toolkit for post-calibration analysis of single-dish HI intensity mapping surveys, achieving percent-level accuracy on simulated MeerKAT data in the k range 0.02-0.2 h/Mpc.

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Works this paper leans on

298 extracted references · 263 canonical work pages · cited by 1 Pith paper

  1. [1]

    2026 ,publisher =

    Priyamvad Tripathi and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  2. [2]

    2026 ,publisher =

    Marco Regis and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  3. [3]

    2026 ,publisher =

    Jacobo Asorey&Hale and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  4. [4]

    2026 ,publisher =

    Manisha Caleb and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  5. [5]

    2026 ,publisher =

    Aishrila Mazumder and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  6. [6]

    2026 ,publisher =

    Steven Cunnington&Wang and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  7. [7]

    2026 ,publisher =

    José Fonseca and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  8. [8]

    2026 ,publisher =

    Stefano Camera and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

Show all 298 references
  1. [9]

    2026 ,publisher =

    Khandakar Md Asif Elahi and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  2. [10]

    2026 ,publisher =

    Ian Harrison and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  3. [11]

    2026 ,publisher =

    Tommaso Ronconi and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  4. [12]

    2026 ,publisher =

    Suman Majumdar and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  5. [13]

    2026 ,publisher =

    Daniele Bertacca and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  6. [14]

    2026 ,publisher =

    Joël Mayor and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  7. [15]

    2026 ,publisher =

    Ainulnabilah Nasirudin and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  8. [16]

    2026 ,publisher =

    Debanjan Sarkar and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  9. [17]

    2026 ,publisher =

    Marta Spinelli and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  10. [18]

    2026 ,publisher =

    Suman Chatterjee and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  11. [19]

    2026 ,publisher =

    Tessa Baker and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  12. [20]

    2026 ,publisher =

    Laura Wolz and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  13. [21]

    2026 ,publisher =

    Mamta Pandey-Pommier and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  14. [22]

    Lagos and author2 and author3 and author4 and author5 ,title =

    Claudia D.P. Lagos and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  15. [23]

    , keywords =

    Damped Ly absorbers and atomic hydrogen in galaxies: the view of the GAEA model. , keywords =. doi:10.1093/mnras/staa2067 , archivePrefix =. 2007.05040 , primaryClass =

    2007 doi

  16. [24]

    A multitracer empirically driven approach to line-intensity mapping light cones

    Sato-Polito, Gabriela and Kokron, Nickolas and Bernal, Jos \'e Luis. A multitracer empirically driven approach to line-intensity mapping light cones. Mon. Not. Roy. Astron. Soc. 2023. doi:10.1093/mnras/stad2498. arXiv:2212.08056

    2023 doi

  17. [25]

    and Hearin, Andrew P

    Behroozi, Peter and Wechsler, Risa H. and Hearin, Andrew P. and Conroy, Charlie. UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0 - 10. Mon. Not. Roy. Astron. Soc. 2019. doi:10.1093/mnras/stz1182. arXiv:1806.07893

    2019 doi arXiv

  18. [26]

    SIMPLE: Simple Intensity Map Producer for Line Emission

    Lujan Niemeyer, Maja and Bernal, Jos \'e Luis and Komatsu, Eiichiro. SIMPLE: Simple Intensity Map Producer for Line Emission. Astrophys. J. 2023. doi:10.3847/1538-4357/acfef4. arXiv:2307.08475

    2023 doi

  19. [27]

    , keywords =

    Constraining the shape of dark matter haloes with globular clusters and diffuse stellar light in the E-MOSAICS simulations. , keywords =. doi:10.1093/mnras/stad920 , adsurl =

    doi

  20. [28]

    , keywords =

    FIREbox: simulating galaxies at high dynamic range in a cosmological volume. , keywords =. doi:10.1093/mnras/stad1205 , archivePrefix =. 2205.15325 , primaryClass =

    doi

  21. [29]

    arXiv e-prints , keywords =

    The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution. arXiv e-prints , keywords =. doi:10.48550/arXiv.2508.21126 , archivePrefix =. 2508.21126 , primaryClass =

    doi arXiv

  22. [30]

    , keywords =

    Generating dark matter halo merger trees. , keywords =. doi:10.1111/j.1365-2966.2007.12517.x , archivePrefix =. 0708.1382 , primaryClass =

    2007 doi

  23. [31]

    Towards improving galaxy formation models using subhaloes

    Building merger trees from cosmological N-body simulations. Towards improving galaxy formation models using subhaloes. , keywords =. doi:10.1051/0004-6361/200911787 , archivePrefix =. 0902.0679 , primaryClass =

    doi arXiv

  24. [32]

    Results at z=0

    Populating a cluster of galaxies - I. Results at z=0. , keywords =. doi:10.1046/j.1365-8711.2001.04912.x , archivePrefix =. astro-ph/0012055 , primaryClass =

    2001 doi

  25. [33]

    , keywords =

    Chemical enrichment of the intracluster and intergalactic medium in a hierarchical galaxy formation model. , keywords =. doi:10.1111/j.1365-2966.2004.07584.x , archivePrefix =. astro-ph/0310268 , primaryClass =

    2004 doi

  26. [34]

    , keywords =

    The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. , keywords =. doi:10.1111/j.1365-2966.2005.09675.x , archivePrefix =. astro-ph/0508046 , primaryClass =

    2005 doi

  27. [35]

    Galaxies , keywords =

    Approximate Methods for the Generation of Dark Matter Halo Catalogs in the Age of Precision Cosmology. Galaxies , keywords =. doi:10.3390/galaxies4040053 , archivePrefix =. 1605.07752 , primaryClass =

    doi arXiv

  28. [36]

    , keywords =

    The atomic hydrogen content of the post-reionization Universe. , keywords =. doi:10.1093/mnras/staa604 , archivePrefix =. 1909.02242 , primaryClass =

    1909 doi

  29. [37]

    2019 , eprint=

    Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1) , author=. 2019 , eprint=

    2019

  30. [38]

    The foreground transfer function for H\,i intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications

    Cunnington, Steven and others. The foreground transfer function for H\,i intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications. Mon. Not. Roy. Astron. Soc. 2023. doi:10.1093/mnras/stad1567. arXiv:2302.07034

    2023 doi

  31. [39]

    and Chang, Tzu-Ching and Masui, Kiyoshi W

    Switzer, Eric R. and Chang, Tzu-Ching and Masui, Kiyoshi W. and Pen, Ue-Li and Voytek, Tabitha C. Interpreting the unresolved intensity of cosmologically redshifted line radiation. Astrophys. J. 2015. doi:10.1088/0004-637X/815/1/51. arXiv:1504.07527

    2015 doi arXiv

  32. [40]

    Murray , title =

    Steven G. Murray , title =. 2018 , publisher =. doi:10.21105/joss.00850 , url =

    2018 doi

  33. [41]

    Generating Log-normal Mock Catalog of Galaxies in Redshift Space

    Agrawal, Aniket and Makiya, Ryu and Chiang, Chi-Ting and Jeong, Donghui and Saito, Shun and Komatsu, Eiichiro. Generating Log-normal Mock Catalog of Galaxies in Redshift Space. JCAP. 2017. doi:10.1088/1475-7516/2017/10/003. arXiv:1706.09195

    2017 doi arXiv

  34. [42]

    MeerKLASS L-band deep-field intensity maps: entering the H\,i dominated regime

    MeerKLASS Collaboration and others. MeerKLASS L-band deep-field intensity maps: entering the H\,i dominated regime. Mon. Not. Roy. Astron. Soc. 2025. doi:10.1093/mnras/staf195. arXiv:2407.21626

    2025 doi

  35. [43]

    New Fitting Formula for Cosmic Nonlinear Density Distribution

    Shin, Jihye and Kim, Juhan and Pichon, Christophe and Jeong, Donghui and Park, Changbom. New Fitting Formula for Cosmic Nonlinear Density Distribution. Astrophys. J. 2017. doi:10.3847/1538-4357/aa74b9. arXiv:1705.06863

    2017 doi arXiv

  36. [44]

    2015 , publisher=

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , author=. 2015 , publisher=

    2015

  37. [45]

    Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission. arXiv e-prints , keywords =. doi:10.48550/arXiv.2405.13495 , archivePrefix =. 2405.13495 , primaryClass =

    doi

  38. [46]

    and Tinker, Jeremy L

    Wechsler, Risa H. and Tinker, Jeremy L. The Connection Between Galaxies and Their Dark Matter Halos. Annual Review of Astronomy and Astrophysics. 2018. doi:https://doi.org/10.1146/annurev-astro-081817-051756

    2018 doi

  39. [47]

    arXiv e-prints , keywords =

    Painting a full radio sky -- Empirical mock catalogues with multiple source populations for future radio surveys. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.25650 , archivePrefix =. 2603.25650 , primaryClass =

    doi

  40. [48]

    2016 , month =

    Carbone, Carmelita and Petkova, Margarita and Dolag, Klaus , title =. 2016 , month =. doi:10.1088/1475-7516/2016/07/034 , url =

    2016 doi

  41. [49]

    and Carbone, C

    Parimbelli, G. and Carbone, C. and Bel, J. and Bose, B. and Calabrese, M. and Carella, E. and Zennaro, M. , title =. 2022 , month =. doi:10.1088/1475-7516/2022/11/041 , url =

    2022 doi

  42. [50]

    2024 , month =

    Hernández-Molinero, Beatriz and Carbone, Carmelita and Jimenez, Raul and Garay, Carlos Peña , title =. 2024 , month =. doi:10.1088/1475-7516/2024/01/006 , url =

    2024 doi

  43. [51]

    Monthly Notices of the Royal Astronomical Society , volume =

    Bonaldi, Anna and Bonato, Matteo and Galluzzi, Vincenzo and Harrison, Ian and Massardi, Marcella and Kay, Scott and DeZotti, Gianfranco and Brown, Michael L , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2018 , month =. doi:10.1093/mnras/sty2603 , url =

    2018 doi

  44. [52]

    Monthly Notices of the Royal Astronomical Society , volume =

    Bonaldi, Anna and Hartley, Philippa and Ronconi, Tommaso and DeZotti, Gianfranco and Bonato, Matteo , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2023 , month =. doi:10.1093/mnras/stad1913 , url =

    2023 doi

  45. [53]

    and Zehavi, Idit and Chuang, Chia-Hsun and Comparat, Johan and Favole, Ginevra and Gottloeber, Stefan and Klypin, Anatoly and Prada, Francisco and Rodríguez-Torres, Sergio A

    Guo, Hong and Zheng, Zheng and Behroozi, Peter S. and Zehavi, Idit and Chuang, Chia-Hsun and Comparat, Johan and Favole, Ginevra and Gottloeber, Stefan and Klypin, Anatoly and Prada, Francisco and Rodríguez-Torres, Sergio A. and Weinberg, David H. and Yepes, Gustavo , title =....

    2016 doi

  46. [54]

    Monthly Notices of the Royal Astronomical Society , volume =

    Ronconi, Tommaso and Lapi, Andrea and Viel, Matteo and Sartori, Alberto , title = ". Monthly Notices of the Royal Astronomical Society , volume =. 2020 , month =. doi:10.1093/mnras/staa2201 , url =

    2020 doi

  47. [55]

    Monthly Notices of the Royal Astronomical Society , volume =

    Hale, C L and Jarvis, M J and Delvecchio, I and Hatfield, P W and Novak, M and Smolčić, V and Zamorani, G , title = ". Monthly Notices of the Royal Astronomical Society , volume =. 2017 , month =. doi:10.1093/mnras/stx2954 , url =

    2017 doi

  48. [56]

    and Giovanelli, Riccardo and Haynes, Martha P

    Martin, Ann M. and Giovanelli, Riccardo and Haynes, Martha P. and Guzzo, Luigi , title =. 2012 , month =. doi:10.1088/0004-637X/750/1/38 , url =

    2012 doi

  49. [57]

    Monthly Notices of the Royal Astronomical Society: Letters , volume =

    Mondal, Rajesh and Bharadwaj, Somnath and Majumdar, Suman and Bera, Apurba and Acharyya, Ayan , title =. Monthly Notices of the Royal Astronomical Society: Letters , volume =. 2015 , month =. doi:10.1093/mnrasl/slv015 , url =

    2015 doi

  50. [58]

    Monthly Notices of the Royal Astronomical Society , volume =

    Mondal, Rajesh and Bharadwaj, Somnath and Majumdar, Suman , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2015 , month =. doi:10.1093/mnras/stv2772 , url =

    2015 doi

  51. [59]

    and Gawiser, Eric and Prochaska, Jason X

    Cooke, Jeff and Wolfe, Arthur M. and Gawiser, Eric and Prochaska, Jason X. , title =. 2006 , month =. doi:10.1086/507476 , url =

    2006 doi

  52. [60]

    Kim, Han-Seek and Wyithe, J. Stuart. B. and Baugh, C. M. and Lagos, C. d. P. and Power, C. and Park, Jaehong , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2016 , month =. doi:10.1093/mnras/stw2779 , url =

    2016 doi

  53. [61]

    and Tormen, Giuseppe , title =

    Sheth, Ravi K. and Tormen, Giuseppe , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2002 , month =. doi:10.1046/j.1365-8711.2002.04950.x , url =

    2002 doi

  54. [62]

    and Frenk, C

    Jenkins, A. and Frenk, C. S. and White, S. D. M. and Colberg, J. M. and Cole, S. and Evrard, A. E. and Couchman, H. M. P. and Yoshida, N. , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2001 , month =. doi:10.1046/j.1365-8711.2001.04029.x , url =

    2001 doi

  55. [63]

    Bagla, J. S. and Khandai, Nishikanta and Datta, Kanan K. , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2010 , month =. doi:10.1111/j.1365-2966.2010.16933.x , url =

    2010 doi

  56. [64]

    , title =

    Mondal, Rajesh and Bharadwaj, Somnath and Datta, Kanan K. , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2017 , month =. doi:10.1093/mnras/stx2888 , url =

    2017 doi

  57. [65]

    2025 , month =

    Hitz, Pascal and Berner, Pascale and Crichton, Devin and Hennig, John and Refregier, Alexandre , title =. 2025 , month =. doi:10.1088/1475-7516/2025/04/003 , url =

    2025 doi

  58. [67]

    , year = 1991, month = oct, volume =

    Excursion Set Mass Functions for Hierarchical Gaussian Fluctuations. , year = 1991, month = oct, volume =. doi:10.1086/170520 , adsurl =

    1991 doi

  59. [68]

    , year = 1995, month = jul, volume =

    The Mass Function of Cosmic Structures with Nonspherical Collapse. , year = 1995, month = jul, volume =. doi:10.1086/175853 , archivePrefix =. astro-ph/9406029 , primaryClass =

    1995 doi arXiv

  60. [69]

    Monthly Notices of the Royal Astronomical Society , volume =

    Monaco, Pierluigi , title =. Monthly Notices of the Royal Astronomical Society , volume =. 1997 , month =. doi:10.1093/mnras/290.3.439 , url =

    1997 doi

  61. [70]

    L. B. Newburgh and K. Bandura and M. A. Bucher, et al. , title =. Ground-based and Airborne Telescopes VI , editor =. 2016 , doi =

    2016

  62. [71]

    , title =

    Devin Crichton and Moumita Aich and Adam Amara, et al. , title =. Journal of Astronomical Telescopes, Instruments, and Systems , number =. 2022 , doi =

    2022

  63. [72]

    Monthly Notices of the Royal Astronomical Society , volume =

    Padmanabhan, Hamsa and Refregier, Alexandre and Amara, Adam , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2017 , month =. doi:10.1093/mnras/stx979 , url =

    2017 doi

  64. [73]

    and Haehnelt, Martin G

    Barnes, Luke A. and Haehnelt, Martin G. , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2014 , month =. doi:10.1093/mnras/stu445 , url =

    2014 doi

  65. [74]

    and Patel, Prina and Santos, Mário G

    Bull, Philip and Ferreira, Pedro G. and Patel, Prina and Santos, Mário G. , title =. 2015 , month =. doi:10.1088/0004-637X/803/1/21 , url =

    2015 doi

  66. [75]

    2018 , issn =

    PyCosmo: An integrated cosmological Boltzmann solver , journal =. 2018 , issn =. doi:https://doi.org/10.1016/j.ascom.2018.08.001 , url =

    2018 doi

  67. [76]

    2021 , issn =

    Predicting cosmological observables with PyCosmo , journal =. 2021 , issn =. doi:https://doi.org/10.1016/j.ascom.2021.100484 , url =

    2021 doi

  68. [77]

    2022 , issn =

    Symbolic implementation of extensions of the PyCosmo Boltzmann solver , journal =. 2022 , issn =. doi:https://doi.org/10.1016/j.ascom.2022.100603 , url =

    2022 doi

  69. [78]

    , keywords =

    HInet: Generating Neutral Hydrogen from Dark Matter with Neural Networks. , keywords =. doi:10.3847/1538-4357/ac033a , archivePrefix =. 2007.10340 , primaryClass =

    2007 doi

  70. [79]

    arXiv e-prints , keywords =

    Modeling assembly bias with machine learning and symbolic regression. arXiv e-prints , keywords =. doi:10.48550/arXiv.2012.00111 , archivePrefix =. 2012.00111 , primaryClass =

    2012 doi

  71. [80]

    , keywords =

    Simulations of the formation, evolution and clustering of galaxies and quasars. , keywords =. doi:10.1038/nature03597 , archivePrefix =. astro-ph/0504097 , primaryClass =

    doi arXiv

  72. [81]

    , keywords =

    Resolving cosmic structure formation with the Millennium-II Simulation. , keywords =. doi:10.1111/j.1365-2966.2009.15191.x , archivePrefix =. 0903.3041 , primaryClass =

    2009 doi

  73. [82]

    , keywords =

    Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter haloes. , keywords =. doi:10.1093/mnras/sty3427 , archivePrefix =. 1808.08276 , primaryClass =

    doi arXiv

  74. [83]

    , keywords =

    Tracing the quenching journey across cosmic time. , keywords =. doi:10.1051/0004-6361/202349045 , archivePrefix =. 2401.06211 , primaryClass =

    doi

  75. [84]

    , keywords =

    The hierarchical formation of the brightest cluster galaxies. , keywords =. doi:10.1111/j.1365-2966.2006.11287.x , archivePrefix =. astro-ph/0606519 , primaryClass =

    2006 doi

  76. [85]

    , keywords =

    Elemental abundances in Milky Way-like galaxies from a hierarchical galaxy formation model. , keywords =. doi:10.1093/mnras/stu1752 , archivePrefix =. 1407.7867 , primaryClass =

    doi arXiv

  77. [86]

    , keywords =

    H I-selected galaxies in hierarchical models of galaxy formation and evolution. , keywords =. doi:10.1093/mnras/stw2901 , archivePrefix =. 1610.02042 , primaryClass =

    doi arXiv

  78. [87]

    , keywords =

    H _ 2 -based star formation laws in hierarchical models of galaxy formation. , keywords =. doi:10.1093/mnras/stx889 , archivePrefix =. 1611.09372 , primaryClass =

    doi arXiv

  79. [88]

    , keywords =

    The rise of active galactic nuclei in the galaxy evolution and assembly semi-analytic model. , keywords =. doi:10.1093/mnras/staa1716 , archivePrefix =. 2002.10576 , primaryClass =

    2002 doi

  80. [89]

    , keywords =

    The influence of environment on satellite galaxies in the GAEA semi-analytic model. , keywords =. doi:10.1093/mnras/staa2370 , archivePrefix =. 2003.12757 , primaryClass =

    2003 doi

  81. [90]

    , keywords =

    Galaxy assembly, stellar feedback and metal enrichment: the view from the GAEA model. , keywords =. doi:10.1093/mnras/stw1318 , archivePrefix =. 1512.04531 , primaryClass =

    doi arXiv

  82. [91]

    , keywords =

    Galaxy assembly and evolution in the P-Millennium simulation: Galaxy clustering. , keywords =. doi:10.1051/0004-6361/202452029 , archivePrefix =. 2409.02194 , primaryClass =

    doi

  83. [92]

    , keywords =

    The Role of Pressure in GMC Formation II: The H _ 2 -Pressure Relation. , keywords =. doi:10.1086/505417 , archivePrefix =. astro-ph/0605035 , primaryClass =

    doi arXiv

  84. [93]

    , keywords =

    The pinocchio algorithm: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field. , keywords =. doi:10.1046/j.1365-8711.2002.05162.x , archivePrefix =. astro-ph/0109323 , primaryClass =

    2002 doi

  85. [94]

    The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling. , keywords =. doi:10.1093/mnras/stae2663 , archivePrefix =. 2407.09949 , primaryClass =

    doi

  86. [95]

    arXiv e-prints , keywords =

    Spectral Hierarchy of the Cosmic Web. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.15834 , archivePrefix =. 2603.15834 , primaryClass =

    doi

  87. [96]

    arXiv e-prints , keywords =

    Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis. arXiv e-prints , keywords =. doi:10.48550/arXiv.2606.04830 , archivePrefix =. 2606.04830 , primaryClass =

    doi arXiv

  88. [97]

    , keywords =

    One simulation to fit them all - changing the background parameters of a cosmological N-body simulation. , keywords =. doi:10.1111/j.1365-2966.2010.16459.x , archivePrefix =. 0912.4277 , primaryClass =

    2010 doi

  89. [98]

    , keywords =

    Bayesian cosmic density field inference from redshift space dark matter maps. , keywords =. doi:10.1093/mnras/stz1864 , archivePrefix =. 1810.05189 , primaryClass =

    doi arXiv

  90. [99]

    arXiv e-prints , keywords =

    The Hierarchical Cosmic Web and Assembly Bias. arXiv e-prints , keywords =. doi:10.48550/arXiv.2403.19337 , archivePrefix =. 2403.19337 , primaryClass =

    doi

  91. [100]

    , keywords =

    CosmoMIA: cosmic web-based redshift space halo distribution. , keywords =. doi:10.1088/1475-7516/2024/07/001 , archivePrefix =. 2402.17581 , primaryClass =

    2024 doi

  92. [101]

    , keywords =

    A high-fidelity realization of the Euclid code comparison N-body simulation with ABACUS. , keywords =. doi:10.1093/mnras/stz634 , archivePrefix =. 1810.02916 , primaryClass =

    doi arXiv

  93. [102]

    , keywords =

    The ABACUS cosmological N-body code. , keywords =. doi:10.1093/mnras/stab2482 , archivePrefix =. 2110.11392 , primaryClass =

    doi

  94. [103]

    Monthly Notices of the Royal Astronomical Society , volume =

    Heavens, Alan and Peacock, John , title = ". Monthly Notices of the Royal Astronomical Society , volume =. 1988 , month =. doi:10.1093/mnras/232.2.339 , url =

    1988 doi

  95. [104]

    Hahn and C

    O. Hahn and C. Porciani and C. M. Carollo and A. Dekel , title =. doi:10.1111/j.1365-2966.2006.11318.x , url =

    2006 doi

  96. [105]

    , keywords =

    Simulating structure formation of the Local Universe. , keywords =. doi:10.1093/mnras/stt1428 , archivePrefix =. 1304.6565 , primaryClass =

    doi arXiv

  97. [106]

    , keywords =

    Clustering in real space and in redshift space. , keywords =. doi:10.1093/mnras/227.1.1 , adsurl =

    doi

  98. [107]

    , keywords =

    Multiscale inference of matter fields and baryon acoustic oscillations from the Ly forest. , keywords =. doi:10.1111/j.1365-2966.2011.19997.x , archivePrefix =. 1011.6233 , primaryClass =

    2011 doi

  99. [108]

    , keywords =

    Cosmic structure and dynamics of the local Universe. , keywords =. doi:10.1111/j.1745-3933.2012.01340.x , archivePrefix =. 1205.5560 , primaryClass =

    2012 doi

  100. [109]

    , keywords =

    Cosmological structure formation with augmented lagrangian perturbation theory. , keywords =. doi:10.1093/mnrasl/slt101 , archivePrefix =. 1212.3514 , primaryClass =

    doi arXiv

  101. [110]

    , keywords =

    Modelling baryon acoustic oscillations with perturbation theory and stochastic halo biasing. , keywords =. doi:10.1093/mnrasl/slt172 , archivePrefix =. 1307.3285 , primaryClass =

    doi arXiv

  102. [111]

    , keywords =

    Bayesian redshift-space distortions correction from galaxy redshift surveys. , keywords =. doi:10.1093/mnrasl/slw009 , archivePrefix =. 1507.08724 , primaryClass =

    doi arXiv

  103. [112]

    , keywords =

    The cosmic web connection to the dark matter halo distribution through gravity. , keywords =. doi:10.1093/mnras/stac671 , archivePrefix =. 2005.11598 , primaryClass =

    2005 doi

  104. [113]

    , keywords =

    ABACUSSUMMIT: a massive set of high-accuracy, high-resolution N-body simulations. , keywords =. doi:10.1093/mnras/stab2484 , archivePrefix =. 2110.11398 , primaryClass =

    doi

  105. [114]

    doi:10.1088/1475-7516/2009/08/020 , url =

    Patrick McDonald and Arabindo Roy , title =. doi:10.1088/1475-7516/2009/08/020 , url =

    2009 doi

  106. [115]

    Planck 2018 results. VI. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201833910 , archivePrefix =. 1807.06209 , primaryClass =

    2018 doi arXiv

  107. [116]

    , keywords =

    SKAO H I intensity mapping: blind foreground subtraction challenge. , keywords =. doi:10.1093/mnras/stab3064 , archivePrefix =. 2107.10814 , primaryClass =

    doi

  108. [117]

    , keywords =

    An accurate tool for the fast generation of dark matter halo catalogues. , keywords =. doi:10.1093/mnras/stt907 , archivePrefix =. 1305.1505 , primaryClass =

    doi arXiv

  109. [118]

    , keywords =

    Improving fast generation of halo catalogues with higher order Lagrangian perturbation theory. , keywords =. doi:10.1093/mnras/stw3085 , archivePrefix =. 1605.04788 , primaryClass =

    doi arXiv

  110. [119]

    , keywords =

    PINOCCHIO and the hierarchical build-up of dark matter haloes. , keywords =. doi:10.1046/j.1365-8711.2002.05441.x , archivePrefix =. astro-ph/0109324 , primaryClass =

    2002 doi

  111. [120]

    , archivePrefix = "arXiv", eprint =

    MULTINEST: an efficient and robust Bayesian inference tool for cosmology and particle physics. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2009.14548.x , adsurl =

    2009 doi

  112. [121]

    , keywords =

    The Structure of Cold Dark Matter Halos. , keywords =. doi:10.1086/177173 , archivePrefix =. astro-ph/9508025 , primaryClass =

    doi arXiv

  113. [122]

    HIBAYES: Global 21-cm Bayesian Monte-Carlo Model Fitting

  114. [123]

    , keywords =

    Mapping the Three-dimensional Ly Forest Large-scale Structure in Real and Redshift Space. , keywords =. doi:10.3847/1538-4357/ac5112 , archivePrefix =. 2107.07917 , primaryClass =

    doi

  115. [124]

    Balaguera-Antolínez and Kentaro Nagamine and Metin Ata and Ikkoh Shimizu and M

    Francesco Sinigaglia and Francisco-Shu Kitaura and A. Balaguera-Antolínez and Kentaro Nagamine and Metin Ata and Ikkoh Shimizu and M. Sánchez-Benavente , title =. 2021 , month =. doi:10.3847/1538-4357/ac158b , url =

    2021 doi

  116. [125]

    , keywords =

    Field-level Lyman- forest modeling in redshift space via augmented nonlocal Fluctuating Gunn-Peterson Approximation. , keywords =. doi:10.1051/0004-6361/202346931 , archivePrefix =. 2305.10428 , primaryClass =

    doi

  117. [126]

    arXiv e-prints , keywords =

    The negative BAO shift in the Ly forest from cosmological simulations. arXiv e-prints , keywords =. doi:10.48550/arXiv.2407.03918 , archivePrefix =. 2407.03918 , primaryClass =

    doi

  118. [127]

    , keywords =

    Ingredients for 21 cm Intensity Mapping. , keywords =. doi:10.3847/1538-4357/aadba0 , archivePrefix =. 1804.09180 , primaryClass =

    doi arXiv

  119. [128]

    , keywords =

    Halo mass distribution reconstruction across the cosmic web. , keywords =. doi:10.1093/mnras/stv1262 , archivePrefix =. 1501.05520 , primaryClass =

    doi arXiv

  120. [129]

    Crighton, Neil H. M. and Murphy, Michael T. and Prochaska, J. Xavier and Worseck, Gábor and Rafelski, Marc and Becker, George D. and Ellison, Sara L. and Fumagalli, Michele and Lopez, Sebastian and Meiksin, Avery and O'Meara, John M. , title =. Monthly Notices of the Royal Ast...

    2015 doi

  121. [130]

    and Bagla, Jasjeet S

    Bera, Apurba and Kanekar, Nissim and Chengalur, Jayaram N. and Bagla, Jasjeet S. , title =. 2022 , month =. doi:10.3847/2041-8213/ac9d32 , url =

    2022 doi

  122. [131]

    arXiv e-prints , keywords =

    A first detection of neutral hydrogen intensity mapping on Mpc scales at z 0.32 and z 0.44. arXiv e-prints , keywords =. doi:10.48550/arXiv.2301.11943 , archivePrefix =. 2301.11943 , primaryClass =

    doi arXiv

  123. [132]

    and Haynes, Martha P

    Guo, Hong and Jones, Michael G. and Haynes, Martha P. and Fu, Jian , title =. 2020 , month =. doi:10.3847/1538-4357/ab886f , url =

    2020 doi

  124. [133]

    Monthly Notices of the Royal Astronomical Society , volume =

    Rhee, Jonghwan and Meyer, Martin and Popping, Attila and Bellstedt, Sabine and Driver, Simon P and Robotham, Aaron S G and Whiting, Matthew and Baldry, Ivan K and Brough, Sarah and Brown, Michael J I and Bunton, John D and Dodson, Richard and Holwerda, Benne W and Hopkins, And...

    2022

  125. [134]

    Monthly Notices of the Royal Astronomical Society , volume =

    Chauhan, Garima and Lagos, Claudia del P and Stevens, Adam R H and Bravo, Matías and Rhee, Jonghwan and Power, Chris and Obreschkow, Danail and Meyer, Martin , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2021 , month =. doi:10.1093/mnras/stab1925 , url =

    2021 doi

  126. [135]

    , keywords =

    WALLABY an SKA Pathfinder H I survey. , keywords =. doi:10.1007/s10509-020-03831-4 , archivePrefix =. 2002.07311 , primaryClass =

    2002 doi

  127. [136]

    10.1051/0004-6361/202039655

    MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey⋆ , DOI= "10.1051/0004-6361/202039655", url= "https://doi.org/10.1051/0004-6361/202039655", journal =

    doi

  128. [137]

    MeerKAT Science: On the Pathway to the SKA , year = 2016, month = jan, eid =

    LADUMA: Looking at the Distant Universe with the MeerKAT Array. MeerKAT Science: On the Pathway to the SKA , year = 2016, month = jan, eid =. doi:10.22323/1.277.0004 , adsurl =

    2016 doi

  129. [138]

    Monthly Notices of the Royal Astronomical Society , volume =

    Hartley, P and Bonaldi, A and Braun, R and Aditya, J N H S and Aicardi, S and Alegre, L and Chakraborty, A and Chen, X and Choudhuri, S and Clarke, A O and Coles, J and Collinson, J S and Cornu, D and Darriba, L and Veneri, M Delli and Forbrich, J and Fraga, B and Galan, A and...

    2023 doi

  130. [139]

    2602.21058 , archivePrefix=

    2026 , title =. 2602.21058 , archivePrefix=

    2026

  131. [140]

    and Mellema, Garrelt and Iliev, Ilian T

    Mao, Yi and Shapiro, Paul R. and Mellema, Garrelt and Iliev, Ilian T. and Koda, Jun and Ahn, Kyungjin , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2012 , month =. doi:10.1111/j.1365-2966.2012.20471.x , url =

    2012 doi

  132. [141]

    Furlanetto and S

    Steven R. Furlanetto and S. Cosmology at low frequencies: The 21cm transition and the high-redshift Universe , journal =. 2006 , issn =. doi:https://doi.org/10.1016/j.physrep.2006.08.002 , url =

    2006 doi

  133. [142]

    Christopher

    Péroux, Céline and Howk, J. Christopher. The Cosmic Baryon and Metal Cycles. Annual Review of Astronomy and Astrophysics. 2020. doi:https://doi.org/10.1146/annurev-astro-021820-120014

    2020 doi

  134. [143]

    , keywords =

    The halo-model description of marked statistics. , keywords =. doi:10.1111/j.1365-2966.2005.09609.x , archivePrefix =. astro-ph/0511772 , primaryClass =

    2005 doi

  135. [144]

    , keywords =

    A marked correlation function for constraining modified gravity models. , keywords =. doi:10.1088/1475-7516/2016/11/057 , archivePrefix =. 1609.08632 , primaryClass =

    2016 doi arXiv

  136. [145]

    , keywords =

    Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12. , keywords =. doi:10.1093/mnras/stz009 , archivePrefix =. 1901.01447 , primaryClass =

    1901 doi arXiv

  137. [146]

    , keywords =

    Using the Marked Power Spectrum to Detect the Signature of Neutrinos in Large-Scale Structure. , keywords =. doi:10.1103/PhysRevLett.126.011301 , archivePrefix =. 2001.11024 , primaryClass =

    2001 doi

  138. [147]

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year = 2015, month = apr, eid =

    Exploring Neutral Hydrogen and Galaxy Evolution with the SKA. Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year = 2015, month = apr, eid =. doi:10.22323/1.215.0128 , archivePrefix =. 1501.01295 , primaryClass =

    2015 doi arXiv

  139. [148]

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year = 2015, month = apr, eid =

    Cosmology from a SKA HI intensity mapping survey. Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year = 2015, month = apr, eid =. doi:10.22323/1.215.0019 , archivePrefix =. 1501.03989 , primaryClass =

    2015 doi arXiv

  140. [149]

    , year = 2010, month = dec, volume =

    Cosmology: Hydrogen was not ionized abruptly. , year = 2010, month = dec, volume =. doi:10.1038/468772b , adsurl =

    2010 doi

  141. [150]

    , keywords =

    Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys. , keywords =. doi:10.1093/mnras/sty3451 , archivePrefix =. 1810.12158 , primaryClass =

    doi

  142. [151]

    , keywords =

    On the spatial distribution of neutral hydrogen in the Universe: bias and shot-noise of the H I power spectrum. , keywords =. doi:10.1093/mnras/stx1599 , archivePrefix =. 1609.05157 , primaryClass =

    doi arXiv

  143. [152]

    , keywords =

    Modeling HI at the field level. , keywords =. doi:10.1103/PhysRevD.108.083528 , archivePrefix =. 2207.12398 , primaryClass =

    doi

  144. [153]

    , keywords =

    Atomic and molecular gas in IllustrisTNG galaxies at low redshift. , keywords =. doi:10.1093/mnras/stz1323 , archivePrefix =. 1902.10714 , primaryClass =

    1902 doi arXiv

  145. [154]

    , keywords =

    Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies. , keywords =. doi:10.1093/mnras/stac1934 , archivePrefix =. 2202.06961 , primaryClass =

    doi

  146. [155]

    , year = 2010, month = jul, volume =

    An intensity map of hydrogen 21-cm emission at redshift z -0.5ex 0.8. , year = 2010, month = jul, volume =. doi:10.1038/nature09187 , adsurl =

    2010 doi

  147. [156]

    Advancing precision cosmology with 21 cm intensity mapping

  148. [157]

    , keywords =

    Theoretical and observational constraints on the H I intensity power spectrum. , keywords =. doi:10.1093/mnras/stu2702 , archivePrefix =. 1407.6366 , primaryClass =

    doi arXiv

  149. [159]

    GLASS: Generator for Large Scale Structure

    Tessore, Nicolas and Loureiro, Arthur and Joachimi, Benjamin and von Wietersheim-Kramsta, Maximilian and Jeffrey, Niall. GLASS: Generator for Large Scale Structure. 2023. doi:10.21105/astro.2302.01942. arXiv:2302.01942

    2023 doi

  150. [160]

    Monthly Notices of the Royal Astronomical Society , volume =

    Mesinger, Andrei and Furlanetto, Steven and Cen, Renyue , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2011 , month =. doi:10.1111/j.1365-2966.2010.17731.x , url =

    2011 doi

  151. [161]

    and Greig, Bradley and Mesinger, Andrei and Muñoz, Julian B

    Murray, Steven G. and Greig, Bradley and Mesinger, Andrei and Muñoz, Julian B. and Qin, Yuxiang and Park, Jaehong and Watkinson, Catherine A. , title =. 2020 , publisher =. doi:10.21105/joss.02582 , url =

    2020 doi

  152. [162]

    doi:10.1017/pasa.2019.51 , journal=

    Cosmology with Phase 1 of the Square Kilometre Array Red Book 2018: Technical specifications and performance forecasts , volume=. doi:10.1017/pasa.2019.51 , journal=

    2018 doi

  153. [163]

    arXiv e-prints , keywords =

    Predicted number counts and clustering of Hi galaxies from future radio surveys. arXiv e-prints , keywords =. doi:10.48550/arXiv.2604.26886 , archivePrefix =. 2604.26886 , primaryClass =

    doi arXiv

  154. [164]

    Monthly Notices of the Royal Astronomical Society , volume =

    Chen, Zhaoting and Wolz, Laura and Spinelli, Marta and Murray, Steven G , title =. Monthly Notices of the Royal Astronomical Society , volume =. 2021 , month =. doi:10.1093/mnras/stab386 , url =

    2021 doi

  155. [165]

    Metal Abundances of KISS Galaxies. III. Nebular Abundances for Fourteen Galaxies and the Luminosity-Metallicity Relationship for H II Galaxies. , eprint =. doi:10.1086/425156 , adsurl =

    doi

  156. [166]

    , archivePrefix = "arXiv", eprint =

    Green Pea Galaxies and Cohorts: Luminous Compact Emission-line Galaxies in the Sloan Digital Sky Survey. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/728/2/161 , adsurl =

    doi

  157. [167]

    , archivePrefix = "arXiv", eprint =

    ''Direct'' Gas-phase Metallicities, Stellar Properties, and Local Environments of Emission-line Galaxies at Redshifts below 0.90. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/780/2/122 , adsurl =

    doi

  158. [168]

    , eprint =

    Star Formation in Galaxies Along the Hubble Sequence. , eprint =. doi:10.1146/annurev.astro.36.1.189 , adsurl =

    doi

  159. [169]

    , archivePrefix = "arXiv", eprint =

    An H Imaging Survey of Galaxies in the Local 11 Mpc Volume. , archivePrefix = "arXiv", eprint =. doi:10.1086/590058 , adsurl =

    doi

  160. [170]

    , archivePrefix = "arXiv", eprint =

    An investigation of the luminosity-metallicity relation for a large sample of low-metallicity emission-line galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/200912414 , adsurl =

    doi

  161. [171]

    , archivePrefix = "arXiv", eprint =

    The relation between metallicity, stellar mass and star formation in galaxies: an analysis of observational and model data. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2012.20595.x , adsurl =

    2012 doi

  162. [172]

    , archivePrefix = "arXiv", eprint =

    Direct Oxygen Abundances for Low-luminosity LVL Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/754/2/98 , adsurl =

    doi

  163. [173]

    , eprint =

    The physical properties of star-forming galaxies in the low-redshift Universe. , eprint =. doi:10.1111/j.1365-2966.2004.07881.x , adsurl =

    2004 doi

  164. [174]

    , archivePrefix = "arXiv", eprint =

    UV Star Formation Rates in the Local Universe. , archivePrefix = "arXiv", eprint =. doi:10.1086/519218 , adsurl =

    doi

  165. [175]

    , eprint =

    The reversal of the star formation-density relation in the distant universe. , eprint =. doi:10.1051/0004-6361:20077525 , adsurl =

    doi

  166. [176]

    , archivePrefix = "arXiv", eprint =

    Superluminous supernova progenitors have a half-solar metallicity threshold. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stx1428 , adsurl =

    doi

  167. [177]

    , eprint =

    Metallicity and Nuclear Star Formation in Nearby Galaxy Pairs: Evidence for Tidally Induced Gas Flows. , eprint =. doi:10.1086/500295 , adsurl =

    doi

  168. [178]

    Galaxy Pairs in the Sloan Digital Sky Survey. I. Star Formation, Active Galactic Nucleus Fraction, and the Mass-Metallicity Relation. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/135/5/1877 , adsurl =

    doi

  169. [179]

    , archivePrefix = "arXiv", eprint =

    The mass-metallicity relation of interacting galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1745-3933.2008.00466.x , adsurl =

    2008 doi

  170. [180]

    Outliers from the Mass-Metallicity Relation. II. A Sample of Massive Metal-Poor Galaxies from SDSS. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/695/1/259 , adsurl =

    doi

  171. [181]

    , archivePrefix = "arXiv", eprint =

    The H I content of extremely metal-deficient blue compact dwarf galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stw2259 , adsurl =

    doi

  172. [182]

    , archivePrefix = "arXiv", eprint =

    Measuring Nebular Temperatures: The Effect of New Collision Strengths with Equilibrium and -distributed Electron Energies. , archivePrefix = "arXiv", eprint =. doi:10.1088/0067-0049/207/2/21 , adsurl =

    doi

  173. [183]

    Metal-poor Dwarf Galaxies in the SIGRID Galaxy Sample. I. H II Region Observations and Chemical Abundances. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/786/2/155 , adsurl =

    doi

  174. [184]

    Metal-poor Dwarf Galaxies in the SIGRID Galaxy Sample. II. The Electron Temperature-Abundance Calibration and the Parameters that Affect it. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/790/1/75 , adsurl =

    doi

  175. [185]

    , eprint =

    The chemical composition of metal-poor emission-line galaxies in the Data Release 3 of the Sloan Digital Sky Survey. , eprint =. doi:10.1051/0004-6361:20053763 , adsurl =

    doi

  176. [186]

    , archivePrefix = "arXiv", eprint =

    New Strong-line Abundance Diagnostics for H II Regions: Effects of -distributed Electron Energies and New Atomic Data. , archivePrefix = "arXiv", eprint =. doi:10.1088/0067-0049/208/1/10 , adsurl =

    doi

  177. [187]

    Studies of NGC 6720 with Calibrated HST/WFC3 Emission-line Filter Images. II. Physical Conditions. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/145/4/93 , adsurl =

    doi

  178. [188]

    Astrophysics of gaseous nebulae and active galactic nuclei, 2nd

    Astrophysics of gaseous nebulae and active galactic nuclei. Astrophysics of gaseous nebulae and active galactic nuclei, 2nd. ed. by D.E. Osterbrock and G.J. Ferland. Sausalito, CA: University Science Books, 2006 , year = 2006, adsurl =

    2006

  179. [189]

    , archivePrefix = "arXiv", eprint =

    Resolving the Electron Temperature Discrepancies in H II Regions and Planetary Nebulae: -distributed Electrons. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/752/2/148 , adsurl =

    doi

  180. [190]

    EAS Publications Series , year = 2012, series =

    Oxygen in the Universe. EAS Publications Series , year = 2012, series =

    2012

  181. [191]

    I - High signal-to-noise optical spectroscopy

    The stellar populations and evolution of H II galaxies. I - High signal-to-noise optical spectroscopy. , keywords =. doi:10.1093/mnras/223.4.811 , adsurl =

    doi

  182. [192]

    , keywords =

    The primordial helium abundance from observations of extragalactic H II regions. , keywords =. doi:10.1093/mnras/255.2.325 , adsurl =

    doi

  183. [193]

    , archivePrefix = "arXiv", eprint =

    Eliminating error in the chemical abundance scale for extragalactic H II regions. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2012.21145.x , adsurl =

    2012 doi

  184. [194]

    Metal Abundances of KISS Galaxies. V. Nebular Abundances of 15 Intermediate Luminosity Star-forming Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/150/3/71 , adsurl =

    doi

  185. [195]

    , archivePrefix = "arXiv", eprint =

    Hunting for extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey: MMT and 3.5 m APO observations. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201219733 , adsurl =

    doi

  186. [196]

    , year = 1958, month = may, volume = 63, pages =

    The law of interstellar reddening. , year = 1958, month = may, volume = 63, pages =. doi:10.1086/107725 , adsurl =

    1958 doi

  187. [197]

    , keywords =

    Gradients in the physical conditions of M101 and the pregalactic helium abundance. , keywords =. doi:10.1086/159796 , adsurl =

    doi

  188. [198]

    , keywords =

    The relationship between infrared, optical, and ultraviolet extinction. , keywords =. doi:10.1086/167900 , adsurl =

    doi

  189. [199]

    , archivePrefix = "arXiv", eprint =

    Measuring Reddening with Sloan Digital Sky Survey Stellar Spectra and Recalibrating SFD. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/737/2/103 , adsurl =

    doi

  190. [200]

    Metal Abundances of KISS Galaxies. I. Coarse Metal Abundances and the Metallicity-Luminosity Relation. , eprint =. doi:10.1086/339834 , adsurl =

    doi

  191. [201]

    , eprint =

    Galactic Stellar and Substellar Initial Mass Function. , eprint =. doi:10.1086/376392 , adsurl =

    doi

  192. [202]

    Planck 2013 results. XVI. Cosmological parameters. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201321591 , adsurl =

    2013 doi

  193. [203]

    , keywords =

    The primordial helium abundance from a new sample of metal-deficient blue compact galaxies. , keywords =. doi:10.1086/174843 , adsurl =

    doi

  194. [204]

    , archivePrefix = "arXiv", eprint =

    The Small Isolated Gas-rich Irregular Dwarf (SIGRID) Galaxy Sample: Description and First Results. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/142/3/83 , adsurl =

    doi

  195. [205]

    Metal Abundances of KISS Galaxies. IV. Galaxian Luminosity-Metallicity Relations in the Optical and Near-Infrared. , eprint =. doi:10.1086/429386 , adsurl =

    doi

  196. [206]

    , archivePrefix = "arXiv", eprint =

    Overview of the SDSS-IV MaNGA Survey: Mapping nearby Galaxies at Apache Point Observatory. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/798/1/7 , adsurl =

    doi

  197. [207]

    , archivePrefix = "arXiv", eprint =

    A Stellar Mass Threshold for Quenching of Field Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/757/1/85 , adsurl =

    doi

  198. [208]

    , eprint =

    Stellar population synthesis at the resolution of 2003. , eprint =. doi:10.1046/j.1365-8711.2003.06897.x , adsurl =

    2003 doi

  199. [209]

    , eprint =

    On the variation of the initial mass function. , eprint =. doi:10.1046/j.1365-8711.2001.04022.x , adsurl =

    2001 doi

  200. [210]

    , eprint =

    Stellar masses and star formation histories for 10 ^ 5 galaxies from the Sloan Digital Sky Survey. , eprint =. doi:10.1046/j.1365-8711.2003.06291.x , adsurl =

    2003 doi

  201. [211]

    , eprint =

    The Dust Content and Opacity of Actively Star-forming Galaxies. , eprint =. doi:10.1086/308692 , adsurl =

    doi

  202. [212]

    Research supported by the University of California, John Simon Guggenheim Memorial Foundation, University of Minnesota, et al

    Astrophysics of gaseous nebulae and active galactic nuclei. Research supported by the University of California, John Simon Guggenheim Memorial Foundation, University of Minnesota, et al. Mill Valley, CA, University Science Books, 1989, 422 p. , year = 1989, adsurl =

    1989

  203. [213]

    American Institute of Physics Conference Series , year = 1997, series =

    UV opacity in nearby galaxies and application to distant galaxies. American Institute of Physics Conference Series , year = 1997, series =. doi:10.1063/1.53764 , adsurl =. astro-ph/9706121 , editor =

    1997 doi arXiv

  204. [214]

    The Metal Abundances across Cosmic Time (MACT) Survey. I. Optical Spectroscopy in the Subaru Deep Field. , archivePrefix = "arXiv", eprint =. doi:10.3847/0067-0049/226/1/5 , adsurl =

    doi

  205. [215]

    The Metal Abundances across Cosmic Time (MACT) Survey. II. Evolution of the Mass-metallicity Relation over 8 Billion Years, Using [OIII]4363AA-based Metallicities. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/828/2/67 , adsurl =

    doi

  206. [216]

    , year = 1913, month = mar, volume = 73, pages =

    On a formula for correcting statistics for the effects of a known error of observation. , year = 1913, month = mar, volume = 73, pages =. doi:10.1093/mnras/73.5.359 , adsurl =

    1913 doi

  207. [217]

    , archivePrefix = "arXiv", eprint =

    Metallicity Calibrations and the Mass-Metallicity Relation for Star-forming Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1086/587500 , adsurl =

    doi

  208. [218]

    , archivePrefix = "arXiv", eprint =

    The Mass-Metallicity Relation with the Direct Method on Stacked Spectra of SDSS Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/765/2/140 , adsurl =

    doi

  209. [219]

    , eprint =

    On Extending the Mass-Metallicity Relation of Galaxies by 2.5 Decades in Stellar Mass. , eprint =. doi:10.1086/505573 , adsurl =

    doi

  210. [220]

    , archivePrefix = "arXiv", eprint =

    A Spectroscopic Study of Blue Supergiant Stars in the Sculptor Galaxy NGC 55: Chemical Evolution and Distance. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/829/2/70 , adsurl =

    doi

  211. [221]

    Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2002, series =

    The Electron Temperature in Ionized Nebulae. Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2002, series =. astro-ph/0102403 , editor =

    2002 arXiv

  212. [222]

    , eprint =

    Biases in abundance derivations for metal-rich nebulae. , eprint =. doi:10.1051/0004-6361:20042216 , adsurl =

    doi

  213. [223]

    , archivePrefix = "arXiv", eprint =

    On the universality of luminosity-metallicity and mass-metallicity relations for compact star-forming galaxies at redshifts 0 z 3. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stv1115 , adsurl =

    doi

  214. [224]

    , keywords =

    Empirical methods for determining elemental abundances tested on model H II regions. , keywords =

  215. [225]

    , archivePrefix = "arXiv", eprint =

    The Chemical Composition of the Sun. , archivePrefix = "arXiv", eprint =. doi:10.1146/annurev.astro.46.060407.145222 , adsurl =

    doi

  216. [226]

    , archivePrefix = "arXiv", eprint =

    An Objective Definition for the Main Sequence of Star-forming Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.1088/2041-8205/801/2/L29 , adsurl =

    doi

  217. [227]

    Extreme emission-line galaxies out to z \ 1 in zCOSMOS. I. Sample and characterization of global properties. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201322786 , adsurl =

    doi

  218. [228]

    , archivePrefix = "arXiv", eprint =

    Characterization of star-forming dwarf galaxies at 0.1 z 0.9 in VUDS: probing the low-mass end of the mass-metallicity relation. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201629762 , adsurl =

    doi

  219. [229]

    , archivePrefix = "arXiv", eprint =

    The Universal Relation of Galactic Chemical Evolution: The Origin of the Mass-Metallicity Relation. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/791/2/130 , adsurl =

    doi

  220. [230]

    , eprint =

    Metallicities of 0.3 z 1.0 Galaxies in the GOODS-North Field. , eprint =. doi:10.1086/425299 , adsurl =

    doi

  221. [231]

    , eprint =

    [OIII]/[NII] as an abundance indicator at high redshift. , eprint =. doi:10.1111/j.1365-2966.2004.07591.x , adsurl =

    2004 doi

  222. [232]

    , archivePrefix = "arXiv", eprint =

    The Relationship between Stellar Mass, Gas Metallicity, and Star Formation Rate for H -Selected Galaxies at z 0.8 from the NewH Survey. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/149/2/79 , adsurl =

    doi

  223. [233]

    , keywords =

    The zCOSMOS 10k-Bright Spectroscopic Sample. , keywords =. doi:10.1088/0067-0049/184/2/218 , adsurl =

    doi

  224. [234]

    , archivePrefix = "arXiv", eprint =

    Tracking the impact of environment on the galaxy stellar mass function up to z \ 1 in the 10 k zCOSMOS sample. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/200912801 , adsurl =

    doi

  225. [235]

    , archivePrefix = "arXiv", eprint =

    The VIMOS Ultra-Deep Survey: \ 10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 z 6. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201423829 , adsurl =

    doi

  226. [236]

    Astronomical Data Analysis Software and Systems XIV , year = 2005, series =

    TOPCAT STIL: Starlink Table/VOTable Processing Software. Astronomical Data Analysis Software and Systems XIV , year = 2005, series =

    2005

  227. [237]

    Instrument Design and Performance for Optical/Infrared Ground-based Telescopes , year = 2003, series =

    The DEIMOS spectrograph for the Keck II Telescope: integration and testing. Instrument Design and Performance for Optical/Infrared Ground-based Telescopes , year = 2003, series =. doi:10.1117/12.460346 , adsurl =

    2003 doi

  228. [238]

    , eprint =

    Hectospec, the MMT's 300 Optical Fiber-Fed Spectrograph. , eprint =. doi:10.1086/497385 , adsurl =

    doi

  229. [239]

    Planetary Nebulae in our Galaxy and Beyond , year = 2006, series =

    ELSA: An integrated, semi-automated nebular abundance package. Planetary Nebulae in our Galaxy and Beyond , year = 2006, series =. doi:10.1017/S1743921306003632 , adsurl =. astro-ph/0605099 , editor =

    2006 doi arXiv

  230. [240]

    , archivePrefix = "arXiv", eprint =

    Constraining the Low-mass Slope of the Star Formation Sequence at 0.5 z 2.5. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/795/2/104 , adsurl =

    doi

  231. [241]

    , keywords =

    Classification parameters for the emission-line spectra of extragalactic objects. , keywords =. doi:10.1086/130766 , adsurl =

    doi

  232. [242]

    , keywords =

    Spectral classification of emission-line galaxies. , keywords =. doi:10.1086/191166 , adsurl =

    doi

  233. [243]

    , archivePrefix = "arXiv", eprint =

    Active Galactic Nuclei Emission Line Diagnostics and the Mass-Metallicity Relation up to Redshift z \ 2: The Impact of Selection Effects and Evolution. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/788/1/88 , adsurl =

    doi

  234. [244]

    , eprint =

    Theoretical Modeling of Starburst Galaxies. , eprint =. doi:10.1086/321545 , adsurl =

    doi

  235. [245]

    , archivePrefix = "arXiv", eprint =

    The rate and luminosity function of long gamma ray bursts. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201526760 , adsurl =

    doi

  236. [246]

    , eprint =

    Beaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir. , eprint =. doi:10.1086/338119 , adsurl =

    doi

  237. [247]

    , archivePrefix = "arXiv", eprint =

    The Metal Aversion of Long-duration Gamma-Ray Bursts. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/774/2/119 , adsurl =

    doi

  238. [248]

    , eprint =

    The Supernova Gamma-Ray Burst Connection. , eprint =. doi:10.1146/annurev.astro.43.072103.150558 , adsurl =

    doi

  239. [249]

    , archivePrefix = "arXiv", eprint =

    A -ray burst at a redshift of z\ 8.2. , archivePrefix = "arXiv", eprint =. doi:10.1038/nature08459 , adsurl =

    doi

  240. [250]

    , archivePrefix = "arXiv", eprint =

    Reconciling the Metallicity Distributions of Gamma-Ray Burst, Damped Ly , and Lyman Break Galaxies at z 3. , archivePrefix = "arXiv", eprint =. doi:10.1086/589555 , adsurl =

    doi

  241. [251]

    , archivePrefix = "arXiv", eprint =

    Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201629228 , adsurl =

    doi

  242. [252]

    , eprint =

    Optical and Long-Wavelength Afterglow from Gamma-Ray Bursts. , eprint =. doi:10.1086/303625 , adsurl =

    doi

  243. [253]

    , archivePrefix = "arXiv", eprint =

    A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/700/2/1299 , adsurl =

    doi

  244. [254]

    A unified picture from low-metallicity systems to the Galaxy

    Dust-depletion sequences in damped Lyman- absorbers. A unified picture from low-metallicity systems to the Galaxy. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201527895 , adsurl =

    doi

  245. [255]

    , archivePrefix = "arXiv", eprint =

    The First Positive Detection of Molecular Gas in a GRB Host Galaxy. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/691/1/L27 , adsurl =

    doi

  246. [256]

    , archivePrefix = "arXiv", eprint =

    Unveiling the Secrets of Metallicity and Massive Star Formation Using DLAs along Gamma-Ray Bursts. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/804/1/51 , adsurl =

    doi

  247. [257]

    , eprint =

    Low-resolution VLT spectroscopy of GRBs 991216, 011211 and 021211. , eprint =. doi:10.1051/0004-6361:20053795 , adsurl =

    doi

  248. [258]

    , archivePrefix = "arXiv", eprint =

    GROND a 7-Channel Imager. , archivePrefix = "arXiv", eprint =. doi:10.1086/587032 , adsurl =

    doi

  249. [259]

    , archivePrefix = "arXiv", eprint =

    The SEDs and host galaxies of the dustiest GRB afterglows. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201117428 , adsurl =

    doi

  250. [260]

    The Swift GRB Host Galaxy Legacy Survey. II. Rest-frame Near-IR Luminosity Distribution and Evidence for a Near-solar Metallicity Threshold. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/817/1/8 , adsurl =

    doi

  251. [261]

    , archivePrefix = "arXiv", eprint =

    A Population of Massive, Luminous Galaxies Hosting Heavily Dust-obscured Gamma-Ray Bursts: Implications for the Use of GRBs as Tracers of Cosmic Star Formation. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/778/2/128 , adsurl =

    doi

  252. [262]

    The Composition Gradient in M101 Revisited. II. Electron Temperatures and Implications for the Nebular Abundance Scale. , eprint =. doi:10.1086/375398 , adsurl =

    doi

  253. [263]

    , eprint =

    On the electron temperature determination in high-metallicity HII regions. , eprint =. doi:10.1111/j.1365-2966.2006.11333.x , adsurl =

    2006 doi

  254. [264]

    , keywords =

    Electron temperature variations and the measurement of nebular abundances. , keywords =. doi:10.1086/116146 , adsurl =

    doi

  255. [265]

    , archivePrefix = "arXiv", eprint =

    On the electron temperatures in high-metallicity HII regions. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2009.15182.x , adsurl =

    2009 doi

  256. [266]

    , archivePrefix = "arXiv", eprint =

    The electron temperatures of SDSS high-metallicity giant extragalactic H ii regions. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2009.16166.x , adsurl =

    2009 doi

  257. [267]

    , archivePrefix = "arXiv", eprint =

    Biases in Metallicity Measurements from Global Galaxy Spectra: The Effects of Flux Weighting and Diffuse Ionized Gas Contamination. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/aa93e4 , adsurl =

    doi

  258. [268]

    , archivePrefix = "arXiv", eprint =

    A GALEX Ultraviolet Imaging Survey of Galaxies in the Local Volume. , archivePrefix = "arXiv", eprint =. doi:10.1088/0067-0049/192/1/6 , adsurl =

    doi

  259. [269]

    , archivePrefix = "arXiv", eprint =

    Improved Background Subtraction for the Sloan Digital Sky Survey Images. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/142/1/31 , adsurl =

    doi

  260. [270]

    , archivePrefix = "arXiv", eprint =

    The Seventh Data Release of the Sloan Digital Sky Survey. , archivePrefix = "arXiv", eprint =. doi:10.1088/0067-0049/182/2/543 , adsurl =

    doi

  261. [271]

    , eprint =

    The Oxygen Abundance in the Inner H II Regions of M101: Implications for the Calibration of Strong-Line Metallicity Indicators. , eprint =. doi:10.1086/510380 , adsurl =

    doi

  262. [272]

    , archivePrefix = "arXiv", eprint =

    Unresolved versus resolved: testing the validity of young simple stellar population models with VLT/MUSE observations of NGC 3603. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201628813 , adsurl =

    doi

  263. [273]

    Spectral synthesis method

    Semi-empirical analysis of Sloan Digital Sky Survey galaxies - I. Spectral synthesis method. , eprint =. doi:10.1111/j.1365-2966.2005.08752.x , adsurl =

    2005 doi

  264. [274]

    Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2009, series =

    The Star Formation Histories of Galaxies: A tour through the STARLIGHT-SDSS database. Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2009, series =. arXiv:0802.0849 , month = may, pages =

    2009

  265. [275]

    VLT/X-Shooter emission-line spectroscopy of 96 -ray-burst-selected galaxies at 0.1 z 3.6

    GRB hosts through cosmic time. VLT/X-Shooter emission-line spectroscopy of 96 -ray-burst-selected galaxies at 0.1 z 3.6. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201425561 , adsurl =

    doi

  266. [276]

    The Optically Unbiased Gamma-Ray Burst Host (TOUGH) Survey. I. Survey Design and Catalogs. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/756/2/187 , adsurl =

    doi

  267. [277]

    , archivePrefix = "arXiv", eprint =

    The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-6256/152/4/83 , adsurl =

    doi

  268. [278]

    , archivePrefix = "arXiv", eprint =

    Keck HIRES Spectroscopy of Extragalactic H II Regions: C and O Abundances from Recombination Lines. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/700/1/654 , adsurl =

    doi

  269. [279]

    , archivePrefix = "arXiv", eprint =

    Stars were Born in Significantly Denser Regions in the Early Universe. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/787/2/120 , adsurl =

    doi

  270. [280]

    , archivePrefix = "arXiv", eprint =

    Strong Nebular Line Ratios in the Spectra of z \ 2-3 Star Forming Galaxies: First Results from KBSS-MOSFIRE. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/795/2/165 , adsurl =

    doi

  271. [281]

    , archivePrefix = "arXiv", eprint =

    New insights into the stellar content and physical conditions of star-forming galaxies at z = 2-3 from spectral modelling. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2008.12914.x , adsurl =

    2008 doi

  272. [282]

    , archivePrefix = "arXiv", eprint =

    The Cosmic BPT Diagram: Confronting Theory with Observations. , archivePrefix = "arXiv", eprint =. doi:10.1088/2041-8205/774/1/L10 , adsurl =

    doi

  273. [283]

    , archivePrefix = "arXiv", eprint =

    Nebular Emission Line Ratios in z 2-3 Star-forming Galaxies with KBSS-MOSFIRE: Exploring the Impact of Ionization, Excitation, and Nitrogen-to-Oxygen Ratio. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/836/2/164 , adsurl =

    doi

  274. [284]

    , eprint =

    Using Strong Lines to Estimate Abundances in Extragalactic H II Regions and Starburst Galaxies. , eprint =. doi:10.1086/341326 , adsurl =

    doi

  275. [285]

    , eprint =

    The Mass-Metallicity Relation at z \ 2. , eprint =. doi:10.1086/503623 , adsurl =

    doi

  276. [286]

    Stellar Populations - Planning for the Next Decade , year = 2010, series =

    Nebular abundances in galaxies: Beware of biases. Stellar Populations - Planning for the Next Decade , year = 2010, series =. doi:10.1017/S1743921310002590 , adsurl =. arXiv:0910.0175 , editor =

    2010 doi arXiv

  277. [287]

    , archivePrefix = "arXiv", eprint =

    The mass-metallicity-star formation rate relation at z 2 with 3D Hubble Space Telescope. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stu443 , adsurl =

    doi

  278. [288]

    , archivePrefix = "arXiv", eprint =

    Chemical abundances in high-redshift galaxies: a powerful new emission line diagnostic. , archivePrefix = "arXiv", eprint =. doi:10.1007/s10509-016-2657-8 , adsurl =

    doi

  279. [289]

    , archivePrefix = "arXiv", eprint =

    Hot gas around SN 1998bw: Inferring the progenitor from its environment. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201630268 , adsurl =

    doi

  280. [290]

    Implications for chemical evolution

    Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolution. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stu1177 , adsurl =

    doi

  281. [291]

    , archivePrefix = "arXiv", eprint =

    Extragalactic Chemical Abundances: Do H II Regions and Young Stars Tell the Same Story? The Case of the Spiral Galaxy NGC 300. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/700/1/309 , adsurl =

    doi

  282. [292]

    , archivePrefix = "arXiv", eprint =

    Local Analogs for High-redshift Galaxies: Resembling the Physical Conditions of the Interstellar Medium in High-redshift Galaxies. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/822/2/62 , adsurl =

    doi

  283. [293]

    , eprint =

    A Flash in the Dark: UVES Very Large Telescope High-Resolution Spectroscopy of Gamma-Ray Burst Afterglows. , eprint =. doi:10.1086/429385 , adsurl =

    doi

  284. [294]

    , eprint =

    The line-of-sight towards GRB 030429 at z =2.66: Probing the matter at stellar, galactic and intergalactic scales. , eprint =. doi:10.1051/0004-6361:20041233 , adsurl =

    doi

  285. [295]

    The Metal-Rich Universe , year = 2008, eprint =

    Measuring chemical abundances in extragalactic metal-rich H II regions. The Metal-Rich Universe , year = 2008, eprint =

    2008

  286. [296]

    Philosophical Transactions of the Royal Society of London Series A , year = 1902, volume = 199, pages =

    The Stability of a Spherical Nebula. Philosophical Transactions of the Royal Society of London Series A , year = 1902, volume = 199, pages =. doi:10.1098/rsta.1902.0012 , adsurl =

    1902 doi

  287. [297]

    , archivePrefix = "arXiv", eprint =

    Regulation of Star Formation Rates in Multiphase Galactic Disks: A Thermal/Dynamical Equilibrium Model. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/721/2/975 , adsurl =

    doi

  288. [298]

    Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence. , eprint =. doi:10.1086/308891 , adsurl =

    doi

  289. [299]

    , keywords =

    The radial distribution of H II regions in spiral galaxies. , keywords =. doi:10.1086/160893 , adsurl =

    doi

  290. [300]

    I - The first-ranked H II regions

    Properties of H II region populations in galaxies. I - The first-ranked H II regions. , keywords =. doi:10.1086/166825 , adsurl =

    doi

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Reviewed June 25, 2026 · model on record in the stance chip above.