Paper Citation Record · LEDGER

Information criteria for astrophysical model selection

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 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 23 of 23 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T16:29:44.394566Z

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

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Pith citing papers

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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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Neutrinophilic $\mathbf{\Lambda}$CDM Extension for EMPRESS, DESI and Hubble Tension cites this paper.

Neutrinophilic $\mathbf{\Lambda}$CDM Extension for EMPRESS, DESI and Hubble Tension Information criteria for astrophysical model selection

Reference 68

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Observational implications of Wald-Gauss-Bonnet topological dark energy cites this paper.

Observational implications of Wald-Gauss-Bonnet topological dark energy Information criteria for astrophysical model selection

Reference 69

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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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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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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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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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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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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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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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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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Observation 55b30fa5-29ec-4e2d-bbab-d8d3f8905b09 · inbound

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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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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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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Observation dff2be65-7159-44f5-b294-30898a1beb84 · inbound

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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Observation e2d98bbb-cb38-40c1-bc6f-0e1bd1b6cb6d · inbound

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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Observation 57ab239b-d4e7-46b3-98ca-723e323581bd · inbound

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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