Paper Citation Record · LEDGER

Model-agnostic assessment of dark energy after DESI DR1 BAO

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 28 inbound Pith citation observations for arXiv:2407.17252.

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pith.paper-citation-record.v1
2407.17252 v3

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measured 28 of 28 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 28 of 28 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:37:32.113500Z

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Source: pith, observed 2026-07-08T15:55:04.971945Z

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Pith citing papers

Observation 123d241e-31d2-483e-adbb-a5431ec2338b · inbound

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension cites this paper.

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 21

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Observation d74d6ea6-7059-4388-809c-02133954bfca · inbound

Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis cites this paper.

Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 33

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Observation e34cc018-1a63-4063-a889-a442898378d7 · inbound

A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data cites this paper.

A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 2024

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Observation 4fe0ea4c-1998-4944-9336-3b3d390ef661 · 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? Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 83

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Observation df87d6f6-954b-47e7-9484-f946e8ab8d0a · 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? Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 40

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Observation 2a93b3d6-7a99-4b0f-8bbc-40f6f65af5f7 · inbound

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

Dark energy and lensing anomaly in Planck CMB data Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 24

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Observation 0835d472-63f9-4468-bdf5-d5086caf49d9 · inbound

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

Robustness of dark energy phenomenology across different parameterizations Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 30

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Observation c73ca72f-c6c7-4d5a-9d62-e07fa67e3ddc · inbound

Extended Dark Energy analysis using DESI DR2 BAO measurements cites this paper.

Extended Dark Energy analysis using DESI DR2 BAO measurements Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 148

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Observation 1d39559b-bf7a-4733-8227-52992b0ff6aa · inbound

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background cites this paper.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 15

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Observation f90875c1-edec-434e-9ee3-c7d6c230104c · inbound

On the tension between DESI DR2 BAO and CMB cites this paper.

On the tension between DESI DR2 BAO and CMB Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 71

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Observation e69d4318-cedf-4433-8fb7-69e08f10d898 · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 30

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Observation 640a3db1-ca48-46c6-ad99-c06db919ed14 · inbound

Simple quintessence models in light of DESI-BAO observations cites this paper.

Simple quintessence models in light of DESI-BAO observations Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 48

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Observation 7c365298-abb1-4df1-89b6-e8e7865782f0 · inbound

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data cites this paper.

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 31

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Observation e8cd1c78-8a0f-4087-97f9-e413fb0ef3fc · inbound

New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 72

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Observation 501fa417-9d1b-459f-8661-316102919c97 · inbound

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 23

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Observation 8d99b621-68ec-4609-8db9-869a5421badf · inbound

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts cites this paper.

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 95

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Observation c58ceaf1-ebf5-4b83-adc7-8770ab484d45 · inbound

Cosmological constraints on Galileon dark energy with broken shift symmetry cites this paper.

Cosmological constraints on Galileon dark energy with broken shift symmetry Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 45

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Observation 645f2d0e-2f8f-48d5-9f63-0b6405ca368c · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 39

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Observation 727736ae-171a-4e94-bf21-af4918df474b · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 120

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Observation 572737d6-42f7-4d6b-93e7-3655d08a8d57 · inbound

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 93

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Observation 3e1d1281-97ee-45c7-87d0-7a9cccf83493 · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.413228Z

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Observation 1f3ff641-6803-42e7-9865-6fc229424850 · inbound

Model-independent test of the cosmic distance duality relation with recent observational data cites this paper.

Model-independent test of the cosmic distance duality relation with recent observational data Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 54

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Observation 3b65320c-3499-463f-95ed-528e39ca3d37 · inbound

Model-independent constraints on generalized FLRW consistency relations with bootstrap-based symbolic regression cites this paper.

Model-independent constraints on generalized FLRW consistency relations with bootstrap-based symbolic regression Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 28

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Observation 5e0361de-cba1-43a6-b47f-b908cd8226f0 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 78

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Observation c0129fc8-427f-499c-92e9-b546dcd15d06 · inbound

Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications cites this paper.

Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-05-11T21:26:14.100109Z

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Observation 11b9704b-47b4-48e9-ba02-2aefb25c3601 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 40

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.814557Z

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Observation 0c2b5be0-338c-45a0-800f-6051a081fdaf · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.973175Z

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Observation 9f5297cc-99b0-4b36-9888-302ea911cf03 · inbound

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction cites this paper.

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 26

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