120 lines
5.5 KiB
BibTeX
120 lines
5.5 KiB
BibTeX
@article{10.1093,
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author = {Mirocha, Jordan and Furlanetto, Steven R},
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title = {Balancing the efficiency and stochasticity of star formation with dust extinction in z ≳ 10 galaxies observed by JWST},
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journal = {Monthly Notices of the Royal Astronomical Society},
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volume = {519},
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number = {1},
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pages = {843-853},
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year = {2022},
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month = {12},
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abstract = {Early observations with JWST indicate an overabundance of bright galaxies at redshifts z ≳ 10 relative to Hubble-calibrated model predictions. More puzzling still is the apparent lack of evolution in the abundance of such objects between z ∼ 9 and the highest redshifts yet probed, z ∼ 13–17. In this study, we first show that, despite a poor match with JWST luminosity functions (LFs), semi-empirical models calibrated to rest-ultraviolet LFs and colours at 4 ≲ z ≲ 8 are largely consistent with constraints on the properties of individual JWST galaxies, including their stellar masses, ages, and spectral slopes. We then show that order-of-magnitude scatter in the star formation rate of galaxies (at fixed halo mass) can indeed boost the abundance of bright galaxies, provided that star formation is more efficient than expected in low-mass haloes. However, this solution to the abundance problem introduces tension elsewhere: because it relies on the upscattering of low-mass haloes into bright magnitude bins, one expects typical ages, masses, and spectral slopes to be much lower than constraints from galaxies observed thus far. This tension can be alleviated by non-negligible reddening, suggesting that – if the first batch of photometrically selected candidates are confirmed – star formation and dust production could be more efficient than expected in galaxies at z ≳ 10.},
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issn = {0035-8711},
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doi = {10.1093/mnras/stac3578},
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url = {https://doi.org/10.1093/mnras/stac3578},
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eprint = {https://academic.oup.com/mnras/article-pdf/519/1/843/48343456/stac3578.pdf},
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}
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### The three main THESAN papers
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@article{Kannan_2021,
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title={Introducing the <scp>thesan</scp> project: radiation-magnetohydrodynamic simulations of the epoch of reionization},
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volume={511},
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ISSN={1365-2966},
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url={http://dx.doi.org/10.1093/mnras/stab3710},
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DOI={10.1093/mnras/stab3710},
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number={3},
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journal={Monthly Notices of the Royal Astronomical Society},
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publisher={Oxford University Press (OUP)},
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author={Kannan, R and Garaldi, E and Smith, A and Pakmor, R and Springel, V and Vogelsberger, M and Hernquist, L},
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year={2021},
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month=dec, pages={4005–4030}
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}
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@article{Garaldi_2022,
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title={The<scp>thesan</scp>project: properties of the intergalactic medium and its connection to reionization-era galaxies},
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volume={512},
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ISSN={1365-2966},
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url={http://dx.doi.org/10.1093/mnras/stac257},
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DOI={10.1093/mnras/stac257},
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number={4},
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journal={Monthly Notices of the Royal Astronomical Society},
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publisher={Oxford University Press (OUP)},
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author={Garaldi, E and Kannan, R and Smith, A and Springel, V and Pakmor, R and Vogelsberger, M and Hernquist, L},
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year={2022},
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month=feb, pages={4909–4933}
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}
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@article{Smith_2022,
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title={The<scp>thesan</scp>project: Lyman-α emission and transmission during the Epoch of Reionization},
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volume={512},
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ISSN={1365-2966},
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url={http://dx.doi.org/10.1093/mnras/stac713},
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DOI={10.1093/mnras/stac713},
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number={3},
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journal={Monthly Notices of the Royal Astronomical Society},
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publisher={Oxford University Press (OUP)},
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author={Smith, A and Kannan, R and Garaldi, E and Vogelsberger, M and Pakmor, R and Springel, V and Hernquist, L},
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year={2022},
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month=mar, pages={3243–3265}
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}
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### Beorn specific
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# original beorn paper
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@article{Schaeffer_2023,
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title={<scp>beorn</scp>: a fast and flexible framework to simulate the epoch of reionization and cosmic dawn},
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volume={526},
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ISSN={1365-2966},
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url={http://dx.doi.org/10.1093/mnras/stad2937},
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DOI={10.1093/mnras/stad2937},
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number={2},
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journal={Monthly Notices of the Royal Astronomical Society},
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publisher={Oxford University Press (OUP)},
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author={Schaeffer, Timothée and Giri, Sambit K and Schneider, Aurel},
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year={2023},
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month=sep, pages={2942–2959} }
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# theoretical foundation - halo model of reionization
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@misc{schneider2023cosmologicalforecast21cmpower,
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title={Cosmological forecast of the 21-cm power spectrum using the halo model of reionization},
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author={Aurel Schneider and Timothée Schaeffer and Sambit K. Giri},
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year={2023},
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eprint={2302.06626},
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archivePrefix={arXiv},
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primaryClass={astro-ph.CO},
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url={https://arxiv.org/abs/2302.06626},
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}
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# Wouthuysen-Field effect
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@ARTICLE{Wouthuysen,
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author = {{Wouthuysen}, S.~A.},
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title = "{On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line.}",
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journal = {\aj},
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year = 1952,
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month = jan,
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volume = {57},
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pages = {31-32},
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doi = {10.1086/106661},
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adsurl = {https://ui.adsabs.harvard.edu/abs/1952AJ.....57R..31W},
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adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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}
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@ARTICLE{Field,
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author={Field, George B.},
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journal={Proceedings of the IRE},
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title={Excitation of the Hydrogen 21-CM Line},
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year={1958},
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volume={46},
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number={1},
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pages={240-250},
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keywords={Hydrogen;Clouds;Electromagnetic wave absorption;Kinetic theory;Equations;Deuterium;Temperature distribution;Observatories;Electrons;Atomic measurements},
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doi={10.1109/JRPROC.1958.286741}}
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