Paper Citation Record · LEDGER

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample

As of 17 August 2026, this Paper Citation Record lists 85 of 85 outbound references and 2 inbound Pith citation observations for arXiv:2501.19117.

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

pith.paper-citation-record.v1
2501.19117 v1

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measured 85 of 85 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Reference resolution

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Outbound references

Observation 9e22f755-2a2a-42a5-8fa2-b345ccd7ae10 · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample write newline

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

Reference 2

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This paper cites E., Contreras S., Ondaro-Mallea L., Pellejero-Iba \ n ez M., Zennaro M., 2021, @doi [ ] 10.1093/mnras/stab1911 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.4070A 506, 4070.

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample E., Contreras S., Ondaro-Mallea L., Pellejero-Iba \ n ez M., Zennaro M., 2021, @doi [ ] 10.1093/mnras/stab1911 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.4070A 506, 4070

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample M., Corasaniti P

Reference 12

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

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Reference 17

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample R., Hearin A

Reference 19

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample arXiv:2406.18274

Reference 20

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Weak Lensing and the Measurement of q0 from Type Ia Supernovae

Reference 22

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample E., 2024, @doi [ ] 10.1088/1475-7516/2024/08/024 , https://ui.adsabs.harvard.edu/abs/2024JCAP...08..024G 2024, 024

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample J., Hobson M

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample R., et al., 2020, @doi [Nature] 10.1038/s41586-020-2649-2 , 585, 357

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample D., 2007, @doi [Computing in Science & Engineering] 10.1109/MCSE.2007.55 , 9, 90

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample C., Pewsey A., 2009, @doi [Biometrika] 10.1093/biomet/asp053 , 96, 761

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample J., Tr \"o ster T., Heymans C., Van Waerbeke L., McCarthy I

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Resolution: unresolved; no resolver link, observed 2026-08-09T21:24:36.692772Z

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Observation 17d3a86e-92d0-4134-9be3-53a7da09b935 · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample J., Brieden S., Tr \"o ster T., Heymans C., 2021, @doi [ ] 10.1093/mnras/stab082 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.1401M 502, 1401

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Observation 99ad8d35-a64a-493d-aee0-a66a1578ea42 · outbound

This paper cites Y., 2018, @doi [ ] 10.3847/1538-4357/aad3b1 , https://ui.adsabs.harvard.edu/abs/2018ApJ...863..173M 863, 173.

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Y., 2018, @doi [ ] 10.3847/1538-4357/aad3b1 , https://ui.adsabs.harvard.edu/abs/2018ApJ...863..173M 863, 173

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This paper cites an unresolved cited work.

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

Reference 55

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

Reference 56

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

Reference 57

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Observation 3e4ecd5e-6799-4f24-a080-e7072d6436a8 · outbound

This paper cites F., Frenk C.

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample F., Frenk C

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

Reference 59

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Observation 9d5edf9f-d8de-4a7b-8621-da2733a16a78 · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample D., 2024, @doi [The Open Journal of Astrophysics] 10.33232/001c.117419 , https://ui.adsabs.harvard.edu/abs/2024OJAp....7E..34P 7, 34

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample O., et al., 2024, @doi [ ] 10.3847/1538-4357/ad739a , https://ui.adsabs.harvard.edu/abs/2024ApJ...975....5S 975, 5

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample E., Le Brun A

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Observation 779659aa-e903-44d1-a657-a6cc1efba4fa · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Constraints on compact objects from the Dark Energy Survey five-year supernova sample

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Observation 1608e68f-d81e-4ade-ad3e-d5d62332929b · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample K., Mo H

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Resolution: verified exact; arxiv_id_nonexistent, observed 2026-08-09T21:24:37.598669Z

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Observation 08a8e287-a4d4-4588-b79a-85687a14855d · outbound

This paper cites E., et al., 2003, @doi [ ] 10.1046/j.1365-8711.2003.06503.x , https://ui.adsabs.harvard.edu/abs/2003MNRAS.341.1311S 341, 1311.

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Observation 0bd8c6a0-da1c-45ed-9cc7-f017e8ed6f9a · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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Observation 3ac23f2a-e136-43a8-91ab-a41a5b5498d0 · outbound

This paper cites Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present.

It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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Observation 844b7945-48d4-4e26-b6a9-1c1ded157d7a · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample S., Gao L., Jenkins A., Springel V., White S

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Resolution: unresolved; no resolver link, observed 2026-08-09T21:24:36.772902Z

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Observation 960f4f04-f610-4bce-a6bc-fe2a521778a2 · outbound

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample H., Jing Y

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample Unresolved cited work

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Unavailable: canonical work link unavailable.

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It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample P., McCarthy I

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Pith citing papers

Observation 88bfbe3b-fc4f-44ff-ad28-626a19e68746 · inbound

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Positive neutrino masses with DESI DR2 via matter conversion to dark energy It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample

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Observation d8736040-59e1-4451-8b4f-15f56393379d · inbound

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Gravitational particle production, the cosmological tensions and fast radio bursts It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample

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Resolution: verified exact; arxiv_id, observed 2026-05-18T20:51:50.398846Z

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