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Paper Citation Record · LEDGER

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

As of 23 August 2026, this Paper Citation Record lists 39 of 39 outbound references and 18 inbound Pith citation observations for arXiv:2412.04430.

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

pith.paper-citation-record.v1
2412.04430 v2

Coverage vector

measured 39 of 39 reference resolution

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:00:38.007117Z

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Source: arxiv_reference, observed 2026-07-04T02:19:23.500241Z

Reference resolution

39 of 39 outbound references displayed

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Outbound references

Observation f4dbb811-ce83-4643-b676-dc60af1ea99a · outbound

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes , " * write output.state after.block = add.period write newline

Reference 1

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes write newline

Reference 2

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes C լY痩: 606**ʦ8##G@ɓG -ҠA2]' Zxw 5h 7nh v`xҥk kVfMoOϹs4 x=S*X*T= j̘1ڲem6 qqqU ,ɛ7>3øYfjѢEY_s͖ UV- * 6<\|Y -]T 52n 믿dɒV L׈Ըq >c#u e˖ez paʔ)ngȑ1 ʕ+UX,kР̙c8T /

Reference 3

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This paper cites 2023, Publications of the Astronomical Society of Australia, 40, 10.1017/pasa.2023.40.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2023, Publications of the Astronomical Society of Australia, 40, 10.1017/pasa.2023.40

Reference 4

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Observation 6b3b26ed-01f5-4b0b-9695-3c353c058aba · outbound

This paper cites V., Kable, J.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes V., Kable, J

Reference 5

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Observation 47e4d7ce-2b9b-4a24-b803-b3a3bce217e8 · outbound

This paper cites 2021, The Astrophysical Journal, 909, 26, 10.3847/1538-4357/abd69b.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2021, The Astrophysical Journal, 909, 26, 10.3847/1538-4357/abd69b

Reference 6

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This paper cites 2022, The Astrophysical Journal, 938, 110.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2022, The Astrophysical Journal, 938, 110

Reference 7

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2022, , 938, 111, 10.3847/1538-4357/ac8bcc

Reference 8

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Observation bf3e1db6-35cb-4d1f-85ad-10549cfe3ef8 · outbound

This paper cites R., Stubbs, C.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes R., Stubbs, C

Reference 9

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This paper cites The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder

Reference 10

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This paper cites A., Clayton , G.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes A., Clayton , G

Reference 11

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This paper cites 2019, Journal of Cosmology and Astroparticle Physics, 2019, 028.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2019, Journal of Cosmology and Astroparticle Physics, 2019, 028

Reference 12

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2024, , 973, L14, 10.3847/2041-8213/ad6f9f

Reference 13

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This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 15

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This paper cites 2020, The Astrophysical Journal, 894, 54, 10.3847/1538-4357/ab7fb0.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2020, The Astrophysical Journal, 894, 54, 10.3847/1538-4357/ab7fb0

Reference 16

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Unresolved cited work

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes W., Lang, D., & Goodman, J

Reference 18

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Unresolved cited work

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes R., Millman, K

Reference 20

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This paper cites Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Unresolved cited work

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Procoli: Profiles of cosmological likelihoods

Reference 23

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes D., Jones , D

Reference 24

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2009, The Astrophysical Journal Supplement Series, 180, 330

Reference 25

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2020, Nature, 587, 210

Reference 26

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This paper cites 2020, Astronomy & Astrophysics, 641, A6.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2020, Astronomy & Astrophysics, 641, A6

Reference 27

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Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2023, Astrophys

Reference 28

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This paper cites Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO

Reference 29

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This paper cites G., Yuan, W., Macri, L.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes G., Yuan, W., Macri, L

Reference 30

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Observation 69fddc99-9466-4a4e-b391-49761b167c5d · outbound

This paper cites P., Tollerud, E.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes P., Tollerud, E

Reference 31

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This paper cites 2015, The Astrophysical Journal, 813, 137, 10.1088/0004-637x/813/2/137.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2015, The Astrophysical Journal, 813, 137, 10.1088/0004-637x/813/2/137

Reference 32

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

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 33

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Observation 30481f73-e3b5-446c-b5ab-86a907d1b99e · outbound

This paper cites The Dark Energy Survey Six-Year Calibration Star Catalog.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes The Dark Energy Survey Six-Year Calibration Star Catalog

Reference 34

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Observation 5b9e9e7d-86f6-4e5a-8ad3-5d1c65f288a0 · outbound

This paper cites 2022, The Astrophysical Journal, 938, 113, 10.3847/1538-4357/ac8b7a.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2022, The Astrophysical Journal, 938, 113, 10.3847/1538-4357/ac8b7a

Reference 35

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Observation 2f518018-2fb2-42c3-ac09-17224a618058 · outbound

This paper cites The Dark Energy Survey Supernova Program: Light curves and 5-Year data release.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes The Dark Energy Survey Supernova Program: Light curves and 5-Year data release

Reference 36

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Observation 6838515c-60b5-41f3-823e-fa42db5a3ed7 · outbound

This paper cites 2024, Physical Review D, 109, L121305.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2024, Physical Review D, 109, L121305

Reference 37

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No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-08-11T21:30:33.406080Z digest=sha256:3fd2706b861603257f04de443477a0685a70cc0cf9557b8ad3fd994f8b9468d8

Observation 4800fd76-6fed-4a73-b56e-c82242cb0ad6 · outbound

This paper cites E., et al.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes E., et al

Reference 38

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no resolver link, observed 2026-08-11T21:30:33.410412Z

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source=arxiv_source observed=2026-08-11T21:30:33.410412Z digest=sha256:24dd6a78fb55917fe06a672e2ba1e05ac3b177379382d8943ce0b910df6904d1

Observation b69cf316-721f-4cbb-877b-3470db6c6d7a · outbound

This paper cites 2024, Astrophys.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes 2024, Astrophys

Reference 39

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no resolver link, observed 2026-08-11T21:30:33.414792Z

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source=arxiv_source observed=2026-08-11T21:30:33.414792Z digest=sha256:4beaa9f22a57f5182b02c92a3ed01767cf36a3ad8c692826bf39df9fa77070b2

Observation b6caa44b-8523-49fe-9497-b25e12deb20c · outbound

This paper cites E., et al.

Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes E., et al

Reference 40

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no resolver link, observed 2026-08-11T21:30:33.419266Z

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source=arxiv_source observed=2026-08-11T21:30:33.419266Z digest=sha256:d32c11c312a10d2d9e229f7ce73fe6b0420bbaa6018542bc1bb2ad9b2f4b530c

Pith citing papers

Observation 7e472628-9d95-40d7-bf4c-af41cd99d722 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 103

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Observation f94c84fc-b400-4afc-b6b8-4ee51c1c1fdf · inbound

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 56

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unresolved
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source=pdf_text observed=2026-08-10T22:00:59.894159Z digest=sha256:dc90698e940c82a80257e5b2d51c9d7948a05279cc931f61d47db03278f47706

Observation 0fd8f325-51b7-4755-b4d3-71349a49aae6 · inbound

The case for a low dark matter density in dynamical dark energy model from local probes cites this paper.

The case for a low dark matter density in dynamical dark energy model from local probes Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 4

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unresolved
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Observation 2da92e3f-7be8-4c41-9c45-ae4d75d2ca76 · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 83

Resolution
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no resolver link, observed 2026-08-08T22:04:59.648655Z

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source=pdf_text observed=2026-08-08T22:04:59.648655Z digest=sha256:c5c0d6ad5f716402d59c09de50e12be53fe69dcbfb90dee1a03dae5713835fde

Observation 402f4963-af62-45aa-9ac3-162a1c1e0c12 · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 59

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Observation 9993121d-9b7f-4333-957b-0b7d2b150524 · inbound

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Reference 132

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:56:03.389538Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 4223870c-fcd3-4353-b672-110070e4ebd3 · inbound

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Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 183

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verified exact
arxiv_id, observed 2026-05-16T17:46:23.344612Z

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No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation a8098b7f-609b-4643-80c2-de67a673962c · inbound

Turning a negative neutrino mass into a positive optical depth cites this paper.

Turning a negative neutrino mass into a positive optical depth Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 14

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Observation 13059100-e16b-48fc-a39f-2de1bb180680 · inbound

Dynamical dark energy and gravitational coupling from moving geometries cites this paper.

Dynamical dark energy and gravitational coupling from moving geometries Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 10

Resolution
unresolved
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Observation 5230eb0f-5cc7-40e6-abad-5d494e46608b · inbound

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension cites this paper.

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 81

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unresolved
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Observation d972b54b-ec94-4d29-aa5b-3f7563d30c8d · inbound

Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.

Bayesian and frequentist perspectives agree on dynamical dark energy Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 13

Resolution
unresolved
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Observation 95f5c847-7450-46a4-bf3c-b222113d08fd · inbound

Type II Seesaw Leptogenesis in a Majoron background cites this paper.

Type II Seesaw Leptogenesis in a Majoron background Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 104

Resolution
verified exact
arxiv_id, observed 2026-05-19T07:52:10.077139Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation dceb52c2-cde5-4240-afc1-e657ca23729c · inbound

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 89

Resolution
unresolved
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Unavailable: canonical work link unavailable.

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Observation 2d9419cd-0934-4a96-8f49-f247a0805eab · inbound

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Reference 92

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unresolved
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Observation d54483b9-4972-48cf-8324-1d7d29194ec8 · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 81

Resolution
verified exact
arxiv_id, observed 2026-07-02T14:57:04.202699Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 15dd65d8-2966-4e59-b25c-72e77564f7b6 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 134

Resolution
verified exact
arxiv_id, observed 2026-07-04T02:19:23.501584Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 300bd0d5-b445-44ec-b1cf-39072b9d7e22 · inbound

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 9

Resolution
unresolved
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Unavailable: canonical work link unavailable.

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Observation 4fed44a3-6c62-4e3e-9406-45a3d145bb04 · inbound

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 9

Resolution
unresolved
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Unavailable: canonical work link unavailable.

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