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Paper Citation Record · LEDGER

Information criteria for astrophysical model selection

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:astro-ph/0701113.

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pith.paper-citation-record.v1
astro-ph/0701113 v2

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measured 21 of 21 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 21 of 21 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:42:47.258578Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T18:27:31.717200Z

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Pith citing papers

Observation ec64f6e6-bf0e-41cb-9b5e-8f8bc3186995 · inbound

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

DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations Information criteria for astrophysical model selection

Reference 220

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arxiv_id, observed 2026-05-12T02:13:10.947866Z

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Observation ebfbf22f-9c7c-4754-be9a-4e1d49e66ac8 · inbound

Teleparallel dark energy in a nonflat universe cites this paper.

Teleparallel dark energy in a nonflat universe Information criteria for astrophysical model selection

Reference 94

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A novel test of gravity: Does spacetime geometry track matter density? cites this paper.

A novel test of gravity: Does spacetime geometry track matter density? Information criteria for astrophysical model selection

Reference 60

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Revisiting $\Lambda$CDM extensions in light of re-analyzed CMB data cites this paper.

Revisiting $\Lambda$CDM extensions in light of re-analyzed CMB data Information criteria for astrophysical model selection

Reference 73

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local_arxiv, observed 2026-05-19T09:27:15.125175Z

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Observation 8f035433-b19f-47e8-82f0-2305d703b826 · inbound

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach cites this paper.

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach Information criteria for astrophysical model selection

Reference 92

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Observation e6d6b2d8-9598-4cca-87a9-f0649dfccb5e · inbound

Exponential $f(R)$ cosmology with massive neutrinos as a dynamical dark energy framework cites this paper.

Exponential $f(R)$ cosmology with massive neutrinos as a dynamical dark energy framework Information criteria for astrophysical model selection

Reference 77

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Observation 4f061fe4-647f-485d-acfe-5cd0d2510576 · inbound

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations cites this paper.

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations Information criteria for astrophysical model selection

Reference 120

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local_arxiv, observed 2026-05-16T05:20:39.698557Z

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Observation e0a6e7c2-32df-4f9f-ad1b-be758a8414bf · inbound

Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History cites this paper.

Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History Information criteria for astrophysical model selection

Reference 62

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arxiv_id, observed 2026-05-10T11:10:09.569270Z

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Observation 4b32246d-0f09-47c6-b8b4-5960848844dd · inbound

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension cites this paper.

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension Information criteria for astrophysical model selection

Reference 71

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arxiv_id, observed 2026-05-11T12:11:05.210311Z

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Observation fefec6fb-782a-4efb-9b94-cd12b3cdb190 · inbound

Generalizing the CPL Parametrization through Dark Sector Interaction cites this paper.

Generalizing the CPL Parametrization through Dark Sector Interaction Information criteria for astrophysical model selection

Reference 83

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arxiv_id, observed 2026-05-12T00:31:17.070367Z

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Observation 2d15096d-a3c3-4495-9e77-535a118f5e07 · inbound

Generalizing the CPL Parametrization through Dark Sector Interaction cites this paper.

Generalizing the CPL Parametrization through Dark Sector Interaction Information criteria for astrophysical model selection

Reference 83

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Observation 46aec25f-284b-446b-bc48-29f246d213da · inbound

Single field matter bounce with dark energy era: comparison with CMB Planck 2018 data and best fit parameters cites this paper.

Single field matter bounce with dark energy era: comparison with CMB Planck 2018 data and best fit parameters Information criteria for astrophysical model selection

Reference 31

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local_arxiv, observed 2026-05-15T02:08:29.706327Z

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Observation 5f8e0c05-2e76-4983-b41e-a46b96afd7fb · inbound

Dark Energy in Ghost-free non-local Gravity cites this paper.

Dark Energy in Ghost-free non-local Gravity Information criteria for astrophysical model selection

Reference 79

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local_arxiv, observed 2026-05-22T05:24:38.077556Z

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Late-time Quantum Vacuum Decay and its Cosmological Implications cites this paper.

Late-time Quantum Vacuum Decay and its Cosmological Implications Information criteria for astrophysical model selection

Reference 86

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local_arxiv, observed 2026-06-29T05:43:08.226416Z

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Observation 64803d0c-dbb2-42b7-9765-5d3e512fabfe · inbound

The Coherence Principle: A Falsifiable Prior for Model Selection from the Grammar of Theories cites this paper.

The Coherence Principle: A Falsifiable Prior for Model Selection from the Grammar of Theories Information criteria for astrophysical model selection

Reference 4

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local_arxiv, observed 2026-07-03T23:09:01.688179Z

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Observation d7766939-3575-4b1d-9711-5fd96ef7a6f3 · inbound

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

The Status of Single Scalar Field Dark Energy Information criteria for astrophysical model selection

Reference 133

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Phenomenology of EDE-photon coupling I: constant photon-sector deviation cites this paper.

Phenomenology of EDE-photon coupling I: constant photon-sector deviation Information criteria for astrophysical model selection

Reference 37

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Constraints on unimodular diffusion models with latest observables cites this paper.

Constraints on unimodular diffusion models with latest observables Information criteria for astrophysical model selection

Reference 36

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Observation 4bf3ca1d-3562-4872-b234-ab38ce6fd074 · inbound

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Information criteria for astrophysical model selection

Reference 107

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A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background cites this paper.

A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background Information criteria for astrophysical model selection

Reference 97

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Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements cites this paper.

Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements Information criteria for astrophysical model selection

Reference 67

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