Paper Citation Record · LEDGER

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation

As of 11 August 2026, this Paper Citation Record lists 32 of 32 outbound references and 4 inbound Pith citation observations for arXiv:2507.21409.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2507.21409 v1

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Outbound references

Observation 45ce620c-4d4a-4835-ba15-df1eefb483da · outbound

This paper cites J., 1990, @doi [ ] 10.1086/168721 , https://ui.adsabs.harvard.edu/abs/1990ApJ...354..644B 354, 644.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation J., 1990, @doi [ ] 10.1086/168721 , https://ui.adsabs.harvard.edu/abs/1990ApJ...354..644B 354, 644

Reference 1

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Observation 7179f10f-037d-4336-aedc-63df347462e1 · outbound

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 2

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This paper cites M., et al., 2024, @doi [ ] 10.3847/1538-4357/ad2075 , https://ui.adsabs.harvard.edu/abs/2024ApJ...965...98C 965, 98.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation M., et al., 2024, @doi [ ] 10.3847/1538-4357/ad2075 , https://ui.adsabs.harvard.edu/abs/2024ApJ...965...98C 965, 98

Reference 3

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Observation 5c6b2b1d-541c-407a-b26b-038d74b58437 · outbound

This paper cites Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at $z=4$ to $8$ from CEERS.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at $z=4$ to $8$ from CEERS

Reference 4

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Observation 49de0100-83fa-401b-9568-0775a532b1e7 · outbound

This paper cites R., Hutter A., Dayal P., Gottlöber S., Heintz K.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation R., Hutter A., Dayal P., Gottlöber S., Heintz K

Reference 5

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 6

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 7

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This paper cites Springer, @doi 10.1007/978-3-642-3034-3.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Springer, @doi 10.1007/978-3-642-3034-3

Reference 8

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 9

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Observation 2a32a152-8846-4ad2-b909-c9b81fcc1dde · outbound

This paper cites Constraining the Initial Mass function in the Epoch of Reionization from Astrophysical and Cosmological data.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Constraining the Initial Mass function in the Epoch of Reionization from Astrophysical and Cosmological data

Reference 10

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This paper cites A comparison of pre-existing $\Lambda$CDM predictions with the abundance of {\it JWST} galaxies at high redshift.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation A comparison of pre-existing $\Lambda$CDM predictions with the abundance of {\it JWST} galaxies at high redshift

Reference 11

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This paper cites SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Reference 12

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This paper cites The Interplay between the IMF and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation The Interplay between the IMF and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities

Reference 13

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Observation 458617f8-c44d-4cdb-b517-9dab34bfaf58 · outbound

This paper cites C., Dame T.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation C., Dame T

Reference 14

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Observation 6e09263b-9ff1-40e9-9757-e368c8743df4 · outbound

This paper cites The Origin and Universality of the Stellar Initial Mass Function.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation The Origin and Universality of the Stellar Initial Mass Function

Reference 15

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 16

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 17

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

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This paper cites H., Schechter P., 1974, @doi [ ] 10.1086/152650 , https://ui.adsabs.harvard.edu/abs/1974ApJ...187..425P 187, 425.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation H., Schechter P., 1974, @doi [ ] 10.1086/152650 , https://ui.adsabs.harvard.edu/abs/1974ApJ...187..425P 187, 425

Reference 19

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This paper cites H., et al., 2008, @doi [ ] 10.1088/0004-6256/135/6/2245 , https://ui.adsabs.harvard.edu/abs/2008AJ....135.2245R 135, 2245.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation H., et al., 2008, @doi [ ] 10.1088/0004-6256/135/6/2245 , https://ui.adsabs.harvard.edu/abs/2008AJ....135.2245R 135, 2245

Reference 20

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Observation 60a3d82f-582a-4e71-ad61-21ee54314a09 · outbound

This paper cites E., 1955, @doi [ ] 10.1086/145971 , https://ui.adsabs.harvard.edu/abs/1955ApJ...121..161S 121, 161.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation E., 1955, @doi [ ] 10.1086/145971 , https://ui.adsabs.harvard.edu/abs/1955ApJ...121..161S 121, 161

Reference 21

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Observation 66380ae9-8328-4cc7-88b9-63ee35ebf90b · outbound

This paper cites The impact of UV variability on the abundance of bright galaxies at $z \geq 9$.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation The impact of UV variability on the abundance of bright galaxies at $z \geq 9$

Reference 22

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 23

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation S., Steinhardt C

Reference 24

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This paper cites L., Kokorev V., Rusakov V., Garcia E., Sneppen A., 2023, @doi [The Astrophysical Journal Letters] 10.3847/2041-8213/acdef6 , 951, L40.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation L., Kokorev V., Rusakov V., Garcia E., Sneppen A., 2023, @doi [The Astrophysical Journal Letters] 10.3847/2041-8213/acdef6 , 951, L40

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This paper cites Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn

Reference 26

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

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This paper cites Exploring the nature of UV-bright $z \gtrsim 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Exploring the nature of UV-bright $z \gtrsim 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?

Reference 28

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation Unresolved cited work

Reference 29

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Observation 5e866d87-fd0c-47a4-ad02-ae360ed33224 · outbound

This paper cites JADES: Using NIRCam Photometry to Investigate the Dependence of Stellar Mass Inferences on the IMF in the Early Universe.

Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation JADES: Using NIRCam Photometry to Investigate the Dependence of Stellar Mass Inferences on the IMF in the Early Universe

Reference 30

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation G., 2004, @doi [ ] 10.1086/382351 , https://ui.adsabs.harvard.edu/abs/2004ApJS..152..211Z 152, 211

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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation write newline

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Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies cites this paper.

Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation

Reference 177

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How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function cites this paper.

How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation

Reference 184

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How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function cites this paper.

Reference 151

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What becomes of JWST/NIRCam-selected high-redshift massive galaxies? cites this paper.

What becomes of JWST/NIRCam-selected high-redshift massive galaxies? Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation

Reference 132

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