Paper Citation Record · LEDGER

Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 37 inbound Pith citation observations for arXiv:2406.07533.

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

pith.paper-citation-record.v1
2406.07533 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 37 of 37 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 37 of 37 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T22:00:59.804949Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-10T18:27:31.671144Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0516237b-1764-4070-ac2e-cb2ace0690cd · 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 Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 29

Resolution: metadata mismatch; arxiv_id, observed 2026-05-18T16:14:18.529100Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation c03a6b80-593a-4b24-8e37-ac18062093b9 · 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? Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T22:00:59.804949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3786f311-7abb-44aa-b666-64178f7990de · inbound

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 160

Resolution: unresolved; no resolver link, observed 2026-08-10T18:12:34.423208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 631567a3-4b2d-4e1d-bb45-777803ba765b · inbound

Scalar-Tensor Gravity and DESI 2024 BAO data cites this paper.

Scalar-Tensor Gravity and DESI 2024 BAO data Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T14:29:27.497923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea3e8753-fb68-44af-9d27-3ab84654ddf8 · inbound

Tuning the cosmic instrument: robust cosmology through combined probes cites this paper.

Tuning the cosmic instrument: robust cosmology through combined probes Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-09T14:46:06.558732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d2963e63-707e-4452-b46a-aaac97e8f49c · inbound

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-08T23:12:26.207929Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5da24b45-808b-4605-adb3-6c05e435df72 · inbound

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

Dark energy and lensing anomaly in Planck CMB data Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-08T22:04:59.370685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c80de3f7-11c3-4bfd-93f0-9bd3da33ef2d · inbound

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

Robustness of dark energy phenomenology across different parameterizations Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.615333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7edd82d0-a9cf-45c1-9e22-78508ba701c6 · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 206

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:44.040160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 38c5c595-8b08-4da8-9625-9ecc1c7e4753 · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-05-19T13:12:19.172692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 018b568f-38e0-4140-8868-944b9be0b1fb · inbound

About electroweak domain walls in Majoron models cites this paper.

About electroweak domain walls in Majoron models Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 166

Resolution: unresolved; no resolver link, observed 2026-08-07T11:21:39.210233Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ed999a0-bd83-429b-8d74-f5c581db2da6 · 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? Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.225414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 184266ef-ec32-4383-aa0d-512dd72f7c0d · inbound

Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity cites this paper.

Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:57:09.076602Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 38f943fb-0269-46c5-bbcf-ee4a98f5ac4a · 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 Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 42

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:22:06.242157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 853729c2-9527-4af2-9484-a388675e7c8b · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 9

Resolution: metadata mismatch; arxiv_id, observed 2026-05-19T01:36:57.948735Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 5ad5a39a-25b5-4174-83fd-2c44a50d8f98 · 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 Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:46:16.520227Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 8c15c53e-7d61-4b0c-a6a8-b8b4bb90d765 · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 105

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.590326Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 036c3977-9830-4a8c-818d-42b789dcfc0f · inbound

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM cites this paper.

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-03T18:51:43.791992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 238d8d88-0a8d-4a28-a176-9c9aecf5a292 · 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 Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.377002Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53664f9d-0097-4710-9b95-07d86e261326 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.657493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2095bd9b-d8cf-4843-8309-4533017b0b10 · inbound

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework cites this paper.

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 172

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.200779Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 69480a9b-e933-4d7f-9147-2b19cb97035b · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 59

Resolution: unresolved; no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d79808d-1998-4917-bfaf-3a93b59e8ebe · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 198

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2adda3a-91ec-48ce-a6bb-a52b6e09cd75 · inbound

Testing the consistency of cosmological models with multimessenger astronomy cites this paper.

Testing the consistency of cosmological models with multimessenger astronomy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 3

Resolution: verified exact; arxiv_id, observed 2026-05-12T03:01:18.056337Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 00594c18-9c02-4e79-bdad-8897e7f3424e · inbound

Testing the consistency of cosmological models with multimessenger astronomy cites this paper.

Testing the consistency of cosmological models with multimessenger astronomy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 4

Resolution: verified exact; arxiv_id, observed 2026-05-20T22:29:09.644688Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2db34c0e-3942-4d4b-803c-492d58327e92 · inbound

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

Negative neutrino mass or negative dark energy? Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 126

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.622435Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2535988a-6db2-4cf4-8bc7-42a57595cd44 · inbound

A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-07-01T21:46:16.106296Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 80c47346-5943-48da-8f7e-f418bcde57f6 · inbound

A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T12:40:01.009278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c08c9fe6-0bad-451d-9370-19ab13aaa25c · inbound

Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:56:52.499967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 18a87b7e-b316-43f3-8803-546d05848c13 · inbound

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations cites this paper.

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 77

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:27:03.558788Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 047c8898-63c4-443c-a7f5-43f7dc4c0c00 · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:57:04.294450Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation e1d87951-1f4b-4e87-8159-8b4fdf9b8959 · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 73

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.467972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a18c72dd-ead5-4423-90b4-1e82c2e4a86e · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 121

Resolution: verified exact; arxiv_id, observed 2026-07-02T06:16:43.256251Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2b84d7c4-91f1-4fc5-b8b5-30268bc4a5a0 · inbound

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

Imprint of swampland-inspired coupled early dark energy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.985009Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation b78dae36-075c-4073-a384-76c399b56406 · inbound

The Status of Single Scalar Field Dark Energy cites this paper.

The Status of Single Scalar Field Dark Energy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 126

Resolution: verified exact; local_arxiv, observed 2026-07-10T18:27:31.672460Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6314e4e1-12c3-4de9-967a-8e93fb56c915 · inbound

General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints cites this paper.

General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-01T01:25:44.084185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b41e3923-47d6-477a-a52f-44e125d99da9 · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:08.032306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.