Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-09T04:10:06.881974Z
Paper Citation Record · LEDGER
As of 13 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 3 inbound Pith citation observations for arXiv:2502.03679.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-09T04:10:06.881974Z
One-hop event checks from named stored sources.
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Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T22:11:04.823185Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-17T23:30:29.450959Z
74 of 74 outbound references displayed
External citation measurements
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering V., 2016, @doi [ ] 10.3847/0004-637X/824/2/79 , http://adsabs.harvard.edu/abs/2016ApJ...824...79A 824, 79
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering Unresolved cited work
Reference 2
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering Unresolved cited work
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering S., Conroy C., Wechsler R
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering S., Wechsler R
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering S., Wechsler R
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering P., 2022, @doi [ ] 10.1093/mnras/stab3193 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.2800B 509, 2800
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering S., Ostriker J
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering E., Zennaro M., 2021, @doi [ ] 10.1093/mnras/stab1170 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.504.5205C 504, 5205
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering J., Jonsson P., Primack J
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2010.17555.x , http://adsabs.harvard.edu/abs/2011MNRAS.410.1660D 410, 1660
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering N., 2020, @doi [ ] 10.1093/mnras/staa623 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.493.5506H 493, 5506
Reference 28
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The relationship between galaxy size and halo properties: Insights from the IllustrisTNG simulations and differential clustering S., Gabrielpillai A., Bose S., Eisenstein D., Hernquist L., 2021, @doi [ ] 10.1093/mnras/stab2564 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.508..698H 508, 698
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Reference 135
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