Paper Citation Record · LEDGER

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior

As of 4 August 2026, this Paper Citation Record lists 68 of 68 outbound references and 5 inbound Pith citation observations for arXiv:2605.12415.

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

pith.paper-citation-record.v1
2605.12415 v1

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measured 68 of 68 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Source: pith, observed 2026-07-10T18:27:31.380180Z

Reference resolution

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External citation measurements

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Outbound references

Observation ea925b82-c42f-4f17-b7b3-43b40265ed39 · outbound

This paper cites Late-time reconstruction of non-minimally coupled gravity with a smoothness prior.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Late-time reconstruction of non-minimally coupled gravity with a smoothness prior

Reference 1

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Unresolved cited work

Reference 2

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This paper cites ShapeFit.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior ShapeFit

Reference 3

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Observation dc61be63-4695-443e-ad9e-efe562b37705 · outbound

This paper cites ShapeFit.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior ShapeFit

Reference 4

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Observation c4d36318-1adf-4f99-b715-0efd7249de47 · outbound

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

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 5

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Observation 529381e2-a58f-4769-b965-4bbadcc3c3ec · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 6

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Observation cf31405a-6b64-464d-ba9d-741b0f4ea06f · outbound

This paper cites Vikman, Phys.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Vikman, Phys

Reference 7

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Observation 69584a39-bdee-4356-b8bd-9c2ebb267c53 · outbound

This paper cites Can the dark energy equation-of-state parameter w be less than -1?.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Can the dark energy equation-of-state parameter w be less than -1?

Reference 8

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Observation e4d9c306-5113-42d8-bb0f-6e682e5d9ec5 · outbound

This paper cites Hu, Phys.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Hu, Phys

Reference 9

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Observation 3c1bfa7c-97d8-4c76-84d3-3f614b58464c · outbound

This paper cites The Effective Theory of Quintessence: the w<-1 Side Unveiled.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior The Effective Theory of Quintessence: the w<-1 Side Unveiled

Reference 10

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Observation 04c1b7e9-e91d-40f4-bd77-bb2b40de2efb · outbound

This paper cites Dark Energy Constraints from the Cosmic Age and Supernova.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark Energy Constraints from the Cosmic Age and Supernova

Reference 11

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Observation a59bbd69-4f0f-4956-acae-ca4f952b87c4 · outbound

This paper cites Hessence: A New View of Quintom Dark Energy.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Hessence: A New View of Quintom Dark Energy

Reference 12

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Observation ae6f25e9-f067-448d-84ba-f9be8d4fdf66 · outbound

This paper cites Dark-Energy Evolution Across the Cosmological-Constant Boundary.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark-Energy Evolution Across the Cosmological-Constant Boundary

Reference 13

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Observation 6406db29-8289-42a9-a0f3-d6f52278f9be · outbound

This paper cites Crossing the Phantom Divide.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Crossing the Phantom Divide

Reference 14

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Observation 7857e757-25bd-4b95-a35b-0997f9d51f4a · outbound

This paper cites On Perturbations of Quintom Bounce.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior On Perturbations of Quintom Bounce

Reference 15

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Observation a294e580-699f-4018-bfe2-fe28f1ffeae3 · outbound

This paper cites A Focused Re- view of Quintom Cosmology: From Quintom Dark Energy to Quintom Bounce.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior A Focused Re- view of Quintom Cosmology: From Quintom Dark Energy to Quintom Bounce

Reference 16

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This paper cites Modified gravity interpretation of the evolving dark energy in light of DESI data.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 17

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Observation c7160a52-c39c-4421-baa0-dc1e54cbe518 · outbound

This paper cites Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements

Reference 18

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Observation 8643e773-5e53-4356-9c50-c04e50d524a1 · outbound

This paper cites Ishak et al., (2024).

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Ishak et al., (2024)

Reference 19

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Observation 2bc2eb93-af36-4646-9031-c68ab1826957 · outbound

This paper cites Non-minimally coupled gravity constraints from DESI DR2 data.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Non-minimally coupled gravity constraints from DESI DR2 data

Reference 20

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Observation 0d259ef4-5e41-46b3-8533-085f2363cda7 · outbound

This paper cites Chudaykin, M.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Chudaykin, M

Reference 21

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Observation 065c760b-9b5f-4b6d-80f3-d0522c6e5a95 · outbound

This paper cites Matching current observational constraints with nonminimally coupled dark energy.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Matching current observational constraints with nonminimally coupled dark energy

Reference 22

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Observation 999e277f-d016-4235-bbe3-8ea7302186cf · outbound

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

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Cosmological constraints on Galileon dark energy with broken shift symmetry

Reference 23

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correction dated 2026-01-14. Source: crossref record 10.1103/bxvj-bsv1->10.1103/bxvj-bsv1:correction, observed 2026-07-11T02:56:02.203743+00:00. This notice travels one citation hop only.

Observation e5ef9826-32c0-4666-80be-17edb868d390 · outbound

This paper cites Assessing cosmological evidence for non-minimal coupling.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Assessing cosmological evidence for non-minimal coupling

Reference 24

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Observation 7eaf5cef-38fe-4f9d-bdad-3ee20fffa1ff · outbound

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

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Resolving the Planck-DESI tension by nonminimally coupled quintessence

Reference 25

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Observation e7dd4043-6d2c-432c-b74a-f62bcbf6da0e · outbound

This paper cites Non-minimally coupled quintessence with sign-switching interaction.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Non-minimally coupled quintessence with sign-switching interaction

Reference 26

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Observation 0201642c-5d80-4be5-95b9-398272e91714 · outbound

This paper cites A General Model for Dark Energy Crossing the Phantom Divide.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior A General Model for Dark Energy Crossing the Phantom Divide

Reference 27

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Ye and Y

Reference 28

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This paper cites Bridge the Cosmological Tensions with Thawing Gravity.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Bridge the Cosmological Tensions with Thawing Gravity

Reference 29

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This paper cites The Effective Field Theory of Dark Energy.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior The Effective Field Theory of Dark Energy

Reference 30

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Observation 837d7dec-5e9d-4705-a8d8-6d5602891ddf · outbound

This paper cites Phenomenology of Large Scale Structure in scalar-tensor theories: joint prior covariance of $w_{\textrm{DE}}$, $\Sigma$ and $\mu$ in Horndeski.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Phenomenology of Large Scale Structure in scalar-tensor theories: joint prior covariance of $w_{\textrm{DE}}$, $\Sigma$ and $\mu$ in Horndeski

Reference 31

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This paper cites Imprints of cosmological tensions in reconstructed gravity.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Imprints of cosmological tensions in reconstructed gravity

Reference 32

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This paper cites Principal reconstructed modes of dark energy and gravity.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Principal reconstructed modes of dark energy and gravity

Reference 33

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This paper cites Fables of reconstruction: controlling bias in the dark energy equation of state.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Fables of reconstruction: controlling bias in the dark energy equation of state

Reference 34

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Observation c0b84aa1-1ac4-477a-9b02-f2d76d455af6 · outbound

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Reconstructing Gravity on Cosmological Scales

Reference 35

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Nonparametric Reconstruction of the Dark Energy Equation of State

Reference 36

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Observation 85ce4af8-51c7-4af5-8114-76ca1ad3a2d0 · outbound

This paper cites Nonparametric Dark Energy Reconstruction from Supernova Data.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Nonparametric Dark Energy Reconstruction from Supernova Data

Reference 37

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Brans and R

Reference 38

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This paper cites Models of f(R) Cosmic Acceleration that Evade Solar-System Tests.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Models of f(R) Cosmic Acceleration that Evade Solar-System Tests

Reference 39

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Chameleon Cosmology

Reference 40

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Observation c8024c94-f91d-4523-b66d-7d80910c2f75 · outbound

This paper cites Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration

Reference 41

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Observation a0f5fc97-473d-441d-8238-dab2bac9a740 · outbound

This paper cites CMB power spectra and cosmological parameters from Planck PR4 with CamSpec.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior CMB power spectra and cosmological parameters from Planck PR4 with CamSpec

Reference 42

Resolution: verified exact; arxiv_id, observed 2026-05-16T18:28:26.858538Z

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Observation c8b1ac99-475c-43da-82b4-2e5bfb935ee0 · outbound

This paper cites CMB lensing from Planck PR4 maps.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior CMB lensing from Planck PR4 maps

Reference 43

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Observation 5c726d88-6617-4632-9ab7-70d6c4595938 · outbound

This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 44

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Observation 75e6e909-bbd4-47bc-958d-e3a326b893ce · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 45

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Observation 2065ce5e-c72f-4be5-baa7-83e577e3922f · outbound

This paper cites Dark Energy or Modified Gravity? An Effective Field Theory Approach.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark Energy or Modified Gravity? An Effective Field Theory Approach

Reference 46

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.336961Z

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Observation 5a537c95-3c2d-48e4-ab61-fda1b7399c08 · outbound

This paper cites Dark Energy after GW170817 and GRB170817A.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark Energy after GW170817 and GRB170817A

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.434211Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 17008794-c701-4587-91fa-fa49b414474b · outbound

This paper cites Dark Energy after GW170817: dead ends and the road ahead.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark Energy after GW170817: dead ends and the road ahead

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.320440Z

Source-reported events for the cited work

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Observation d90982a5-6811-4528-bff8-01daacf335f6 · outbound

This paper cites Investigating dark energy experiments with principal components.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Investigating dark energy experiments with principal components

Reference 49

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.375490Z

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Observation 3b54edd1-6b79-4d5b-8679-ce5e989b6a0e · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Planck 2018 results. VI. Cosmological parameters

Reference 50

Resolution: metadata mismatch; local_arxiv, observed 2026-05-13T04:07:13.365928Z

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Observation 42f4068d-cc73-4acc-a18a-eddd342a6c46 · outbound

This paper cites Phenomenology of Horndeski Gravity under Positivity Bounds.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Phenomenology of Horndeski Gravity under Positivity Bounds

Reference 51

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.278209Z

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Observation a4a11c0f-e14a-4c31-92fe-c906aaa540b1 · outbound

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

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 52

Resolution: metadata mismatch; arxiv_id, observed 2026-05-14T21:04:04.151127Z

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Observation 28654528-03e3-4534-9324-8fdcaced49d3 · outbound

This paper cites Reconstructing the dark energy density in light of DESI BAO observations.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Reconstructing the dark energy density in light of DESI BAO observations

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.311697Z

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Observation d91a21be-83ee-475b-b5d1-dcaf1593f506 · outbound

This paper cites Effective Field Theory of Cosmic Acceleration: an implementation in CAMB.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Effective Field Theory of Cosmic Acceleration: an implementation in CAMB

Reference 54

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.397272Z

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Observation eb439bcd-6877-4e5b-90b1-9ab1242101c6 · outbound

This paper cites Effective Field Theory of Cosmic Acceleration: constraining dark energy with CMB data.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Effective Field Theory of Cosmic Acceleration: constraining dark energy with CMB data

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.300880Z

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Observation 99d3fb73-c978-4597-bf50-551fedbcd03b · outbound

This paper cites an unresolved cited work.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Unresolved cited work

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.369198Z

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Observation 01a4719e-0f21-4009-86b2-985a75d8dd41 · outbound

This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Efficient Computation of CMB anisotropies in closed FRW models

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.449624Z

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Observation 3e294616-4cb2-4473-b4a4-73c16bc2b6cb · outbound

This paper cites Cobaya: Code for Bayesian Analysis of hierarchical physical models.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-05-14T21:57:22.456194Z

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Observation 9dd4ccee-1ac2-42bd-a76a-7e66f6a4e728 · outbound

This paper cites Cobaya: Bayesian analysis in cosmology.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Cobaya: Bayesian analysis in cosmology

Reference 59

Resolution: verified fuzzy; raw_fallback, observed 2026-05-13T12:07:44.914721Z

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Observation de29bfaa-9932-4627-85cf-f6c087a63ec8 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Planck 2018 results. V. CMB power spectra and likelihoods

Reference 60

Resolution: metadata mismatch; arxiv_id, observed 2026-05-15T21:56:29.613337Z

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Observation 08099823-017f-4ebf-93eb-089167d535ce · outbound

This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 61

Resolution: metadata mismatch; arxiv_id, observed 2026-05-16T08:30:11.136343Z

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Observation 118ad13b-026e-467f-bcc4-f35633186edf · outbound

This paper cites CosmoSIS: modular cosmological parameter estimation.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior CosmoSIS: modular cosmological parameter estimation

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.296920Z

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Observation d9922b67-2e7b-4821-9df7-2fd45b124a1e · outbound

This paper cites Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.266583Z

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Observation 1fd204a9-8d68-45ab-b98b-3d052fd21298 · outbound

This paper cites Effective Theory of Dark Energy at Redshift Survey Scales.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Effective Theory of Dark Energy at Redshift Survey Scales

Reference 64

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.390978Z

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Observation 93e5c80f-2eb9-467d-9c5a-5894648519de · outbound

This paper cites What can Cosmology tell us about Gravity? Constraining Horndeski with Sigma and Mu.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior What can Cosmology tell us about Gravity? Constraining Horndeski with Sigma and Mu

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.393925Z

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Observation 95d2d405-1e62-447b-b03e-fcef258df8f9 · outbound

This paper cites DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

Reference 66

Resolution: verified exact; arxiv_id, observed 2026-05-17T06:00:50.118019Z

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Observation ccaf1f50-4342-4804-8df0-302978460e8b · outbound

This paper cites ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD

Reference 67

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.446396Z

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Observation f135e353-d74f-458e-8c44-5bc3467d1573 · outbound

This paper cites Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck III: Combined cosmological constraints.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck III: Combined cosmological constraints

Reference 68

Resolution: verified exact; arxiv_id, observed 2026-05-13T04:07:13.443196Z

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Pith citing papers

Observation ea925b82-c42f-4f17-b7b3-43b40265ed39 · inbound