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Paper Citation Record · LEDGER

Constraints on Dark Energy Models Using Late Universe Probes

As of 16 August 2026, this Paper Citation Record lists 100 of 181 outbound references and 5 inbound Pith citation observations for arXiv:2506.12709.

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

pith.paper-citation-record.v1
2506.12709 v3

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measured 100 of 181 reference resolution

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Outbound references

Observation 63b29165-dec2-4132-aa5e-256d5a29f97e · outbound

This paper cites Including SNe Ia data, namely PantheonPlus compilation, decreases w0 to −0.827 ± 0.063 [86].

Constraints on Dark Energy Models Using Late Universe Probes Including SNe Ia data, namely PantheonPlus compilation, decreases w0 to −0.827 ± 0.063 [86]

Reference 1

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Observation 03b0e30f-216a-43a3-ad0c-d2ae56e825ea · outbound

This paper cites • Zheng et al.

Constraints on Dark Energy Models Using Late Universe Probes • Zheng et al

Reference 2

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Observation e91ba466-b859-4985-91cc-1426b686fe54 · outbound

This paper cites • Similar to BA parameterization, the central value of wa is consistent within 1 σ with out results.

Constraints on Dark Energy Models Using Late Universe Probes • Similar to BA parameterization, the central value of wa is consistent within 1 σ with out results

Reference 3

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Observation a48abb93-2fb4-4bc9-a0d1-6ffc2102db06 · outbound

This paper cites PARAM SEV A.

Constraints on Dark Energy Models Using Late Universe Probes PARAM SEV A

Reference 4

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Observation 986801ca-fe7d-4835-bb92-cde5c289e587 · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Constraints on Dark Energy Models Using Late Universe Probes Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 5

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Observation 988a4cb7-e846-4402-a661-dd9744b0350d · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

Constraints on Dark Energy Models Using Late Universe Probes Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 6

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Observation 2dc1af83-2f43-4c15-83f7-4d920e0580db · outbound

This paper cites Cosmological parameters from SDSS and WMAP.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological parameters from SDSS and WMAP

Reference 7

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Observation 4f306494-db8a-4fcc-95f3-f101f34071c8 · outbound

This paper cites Physical Evidence for Dark Energy.

Constraints on Dark Energy Models Using Late Universe Probes Physical Evidence for Dark Energy

Reference 9

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Observation cec14754-3613-45e7-be94-7e542a6fd551 · outbound

This paper cites Cosmological Results from High-z Supernovae.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological Results from High-z Supernovae

Reference 10

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Observation 457a857c-9805-41e9-b695-21889a3471e7 · outbound

This paper cites New Constraints on $\Omega_M$, $\Omega_\Lambda$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST.

Constraints on Dark Energy Models Using Late Universe Probes New Constraints on $\Omega_M$, $\Omega_\Lambda$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST

Reference 11

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Observation 81b9b966-7da6-48b7-9e0c-63f56290842e · outbound

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

Constraints on Dark Energy Models Using Late Universe Probes Dark Energy Constraints from the Cosmic Age and Supernova

Reference 12

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Observation 8e80e0d5-84d8-4a57-87eb-51223279778d · outbound

This paper cites The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set.

Constraints on Dark Energy Models Using Late Universe Probes The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set

Reference 13

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Observation 3740678c-83a3-44ee-acab-33886e88270c · outbound

This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies.

Constraints on Dark Energy Models Using Late Universe Probes Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

Reference 14

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Observation 18318eee-1931-4ba4-9eda-3027c8f55573 · outbound

This paper cites Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak.

Constraints on Dark Energy Models Using Late Universe Probes Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak

Reference 15

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Observation 4b02eabe-5068-4291-b445-296580138db1 · outbound

This paper cites Cosmological Constraints from the SDSS Luminous Red Galaxies.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological Constraints from the SDSS Luminous Red Galaxies

Reference 16

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Observation 992175c2-7cd9-4043-ba53-0bd5e4fcbf77 · outbound

This paper cites Reconstructing Dark Energy.

Constraints on Dark Energy Models Using Late Universe Probes Reconstructing Dark Energy

Reference 17

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Observation 0a65f25f-f8fa-4a12-98e1-633c078267a5 · outbound

This paper cites Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey.

Constraints on Dark Energy Models Using Late Universe Probes Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey

Reference 18

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Observation 67436b44-0bc5-4014-a043-cb0c53fdf69b · outbound

This paper cites Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints.

Constraints on Dark Energy Models Using Late Universe Probes Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints

Reference 19

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Observation 272410b0-3105-44e8-952e-7780ac3ab185 · outbound

This paper cites Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements.

Constraints on Dark Energy Models Using Late Universe Probes Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements

Reference 20

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Observation 8e893b48-5e92-4118-9b15-74d916d96e49 · outbound

This paper cites Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements.

Constraints on Dark Energy Models Using Late Universe Probes Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements

Reference 21

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Observation 0bc8d9ba-21ee-4ae6-92ee-79ce2248deb7 · outbound

This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results.

Constraints on Dark Energy Models Using Late Universe Probes Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results

Reference 22

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Observation aefd43d9-d107-4b06-92d8-d54ea6084165 · outbound

This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results.

Constraints on Dark Energy Models Using Late Universe Probes Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

Reference 23

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Observation abb13eb5-6ea8-438d-92c2-120bcdd32ace · outbound

This paper cites The Baryon Oscillation Spectroscopic Survey of SDSS-III.

Constraints on Dark Energy Models Using Late Universe Probes The Baryon Oscillation Spectroscopic Survey of SDSS-III

Reference 24

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Observation 633ef0c3-49f3-4aa8-a816-d03c76ca82f5 · outbound

This paper cites The Kilo-Degree Survey.

Constraints on Dark Energy Models Using Late Universe Probes The Kilo-Degree Survey

Reference 25

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Constraints on Dark Energy Models Using Late Universe Probes The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples

Reference 26

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Observation d68d8ed2-1cc8-4acc-a65e-1b3b3f7f74f6 · outbound

This paper cites Observational Probes of Cosmic Acceleration.

Constraints on Dark Energy Models Using Late Universe Probes Observational Probes of Cosmic Acceleration

Reference 27

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This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles.

Constraints on Dark Energy Models Using Late Universe Probes The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles

Reference 28

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Observation 7933e8a1-668b-4f81-9b83-f2d300ac8485 · outbound

This paper cites Baryon Acoustic Oscillations in the Ly{\alpha} forest of BOSS DR11 quasars.

Constraints on Dark Energy Models Using Late Universe Probes Baryon Acoustic Oscillations in the Ly{\alpha} forest of BOSS DR11 quasars

Reference 29

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This paper cites The Dark Energy Survey: more than dark energy - an overview.

Constraints on Dark Energy Models Using Late Universe Probes The Dark Energy Survey: more than dark energy - an overview

Reference 30

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This paper cites Strong evidence for an accelerating universe.

Constraints on Dark Energy Models Using Late Universe Probes Strong evidence for an accelerating universe

Reference 31

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This paper cites Dark energy two decades after: Observables, probes, consistency tests.

Constraints on Dark Energy Models Using Late Universe Probes Dark energy two decades after: Observables, probes, consistency tests

Reference 32

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This paper cites Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear.

Constraints on Dark Energy Models Using Late Universe Probes Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear

Reference 33

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Observation 1e50b2a8-9747-4943-b0df-bb9261a27901 · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Constraints on Dark Energy Models Using Late Universe Probes Planck 2018 results. I. Overview and the cosmological legacy of Planck

Reference 35

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

Constraints on Dark Energy Models Using Late Universe Probes Planck 2018 results. VI. Cosmological parameters

Reference 36

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This paper cites Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach.

Constraints on Dark Energy Models Using Late Universe Probes Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach

Reference 37

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This paper cites The evidence of cosmic acceleration and observational constraints.

Constraints on Dark Energy Models Using Late Universe Probes The evidence of cosmic acceleration and observational constraints

Reference 38

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

Constraints on Dark Energy Models Using Late Universe Probes The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 39

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This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Constraints on Dark Energy Models Using Late Universe Probes The Pantheon+ Analysis: Cosmological Constraints

Reference 40

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Observation e55f07c4-689e-4241-83b8-cc479bcd17df · outbound

This paper cites H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology.

Constraints on Dark Energy Models Using Late Universe Probes H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology

Reference 41

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Observation 8822c8cf-7f05-41af-ba48-5c914bdfccbe · outbound

This paper cites H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes.

Constraints on Dark Energy Models Using Late Universe Probes H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

Reference 42

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Observation 27a0d12b-033a-4d69-b7f7-8c545e51b430 · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

Constraints on Dark Energy Models Using Late Universe Probes In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 43

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Observation 196561f7-6dbb-4bc3-a8d5-bc5aedb79c54 · outbound

This paper cites Tensions between the Early and the Late Universe.

Constraints on Dark Energy Models Using Late Universe Probes Tensions between the Early and the Late Universe

Reference 44

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Observation 173a5a55-3cfe-4a8c-be4b-c28b13732b2c · outbound

This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Constraints on Dark Energy Models Using Late Universe Probes Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 45

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Observation 07a75993-5ea0-403f-8ab5-70ac41b663f8 · outbound

This paper cites Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition.

Constraints on Dark Energy Models Using Late Universe Probes Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition

Reference 46

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Observation cc85dd46-7960-42a9-a320-3206d96948e2 · outbound

This paper cites Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results.

Constraints on Dark Energy Models Using Late Universe Probes Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results

Reference 47

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source=pdf_text observed=2026-08-07T00:54:42.535710Z digest=sha256:9ec4ff46af835a9d209b8092d52b2fd2609f6aa565d1cffa578d63690e8f97f8

Observation 67f1b487-7774-4808-8423-9bc0911b3040 · outbound

This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.

Constraints on Dark Energy Models Using Late Universe Probes A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team

Reference 48

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Observation fc5b9960-c3a9-4283-8849-65b1c736600d · outbound

This paper cites The Hubble Hunter's Guide.

Constraints on Dark Energy Models Using Late Universe Probes The Hubble Hunter's Guide

Reference 49

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source=pdf_text observed=2026-08-07T00:54:42.692044Z digest=sha256:c83bfd06362806c3129b44385debef3f01645604f8f703272aa5edf0108ed0e9

Observation 9038aac6-cf86-4ba3-ba4b-80c9698b0e56 · outbound

This paper cites The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023.

Constraints on Dark Energy Models Using Late Universe Probes The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023

Reference 50

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Observation 27ab6315-3c42-4f80-8a0a-5cdc7a6dcfe5 · outbound

This paper cites Chameleon Early Dark Energy and the Hubble Tension.

Constraints on Dark Energy Models Using Late Universe Probes Chameleon Early Dark Energy and the Hubble Tension

Reference 51

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Observation 33f7f7c0-7ac2-4b2d-89b7-be5cee45a24d · outbound

This paper cites Early Dark Energy Can Resolve The Hubble Tension.

Constraints on Dark Energy Models Using Late Universe Probes Early Dark Energy Can Resolve The Hubble Tension

Reference 52

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Observation 19c7ce77-8a07-4803-85a4-8b073fa38ced · outbound

This paper cites Thermal Friction as a Solution to the Hubble Tension.

Constraints on Dark Energy Models Using Late Universe Probes Thermal Friction as a Solution to the Hubble Tension

Reference 53

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source=pdf_text observed=2026-08-07T00:54:43.036786Z digest=sha256:0c16abdc293cd9aad893f2cc364743da6a4ae1097f6fe9668138a35869608766

Observation f7b5796e-fe79-4efc-b131-7130415c1a66 · outbound

This paper cites The Hubble Tension and Early Dark Energy.

Constraints on Dark Energy Models Using Late Universe Probes The Hubble Tension and Early Dark Energy

Reference 54

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source=pdf_text observed=2026-08-07T00:54:43.113302Z digest=sha256:ff839cf374958b74fda0ebd6c5ae7432d6634de0abdfe5c42f97164cb0629400

Observation 9afe78e8-24ff-4821-95cb-7c87743b23a6 · outbound

This paper cites Rock 'n' Roll Solutions to the Hubble Tension.

Constraints on Dark Energy Models Using Late Universe Probes Rock 'n' Roll Solutions to the Hubble Tension

Reference 55

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Observation 325598b0-4506-4c5e-8cd6-16b9868c53fe · outbound

This paper cites Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension.

Constraints on Dark Energy Models Using Late Universe Probes Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 56

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source=pdf_text observed=2026-08-07T00:54:43.318362Z digest=sha256:cfdb2ae586080eeb8cf4bf6d9929c9a0c8c9c3697382969e89536588b4dafcb0

Observation 65dc56ea-f1bb-401b-a993-b7c49e474938 · outbound

This paper cites Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension.

Constraints on Dark Energy Models Using Late Universe Probes Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 57

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source=pdf_text observed=2026-08-07T00:54:43.407504Z digest=sha256:41c11271dcd6203313356488c95307c2606b2d6032813fbe81e8461224163d1c

Observation 72d0703b-f6de-49b3-a4db-e3e44316ade1 · outbound

This paper cites Reconstructing Gravity on Cosmological Scales.

Constraints on Dark Energy Models Using Late Universe Probes Reconstructing Gravity on Cosmological Scales

Reference 58

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Observation 3a61fea8-390f-40cb-a67d-fee719ac3f96 · outbound

This paper cites Implications of a transition in the dark energy equation of state for the $H_0$ and $\sigma_8$ tensions.

Constraints on Dark Energy Models Using Late Universe Probes Implications of a transition in the dark energy equation of state for the $H_0$ and $\sigma_8$ tensions

Reference 59

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Observation 701b87e3-9b64-4512-85d1-4dbee55a6951 · outbound

This paper cites 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.

Constraints on Dark Energy Models Using Late Universe Probes 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

Reference 60

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Observation d0a98ea9-18ef-4843-a077-c726d6a2f442 · outbound

This paper cites The Case for a Positive Cosmological Lambda-term.

Constraints on Dark Energy Models Using Late Universe Probes The Case for a Positive Cosmological Lambda-term

Reference 61

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Observation 6af34762-058d-40c8-aca7-315d33cb13da · outbound

This paper cites The Cosmological Constant.

Constraints on Dark Energy Models Using Late Universe Probes The Cosmological Constant

Reference 62

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source=pdf_text observed=2026-08-07T00:54:43.847923Z digest=sha256:21ec80c915ffad09df90dbc14c5a5696a60f25411a18ce574aac50dee691d0e9

Observation 3d02c9ff-cc9e-4748-acae-2bc68a974b9f · outbound

This paper cites The Cosmological Constant and Dark Energy.

Constraints on Dark Energy Models Using Late Universe Probes The Cosmological Constant and Dark Energy

Reference 63

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source=pdf_text observed=2026-08-07T00:54:43.908217Z digest=sha256:98082646296a9232579c73dfea81fab141defa9d8f1315f49cb9e5c737a5ce17

Observation 667c4545-c428-4cd1-a60e-959182a9fa29 · outbound

This paper cites Cosmological Constant - the Weight of the Vacuum.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological Constant - the Weight of the Vacuum

Reference 64

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Observation 387ba7b8-a066-4611-a716-def392e7595f · outbound

This paper cites Dynamics of dark energy.

Constraints on Dark Energy Models Using Late Universe Probes Dynamics of dark energy

Reference 65

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Observation ce7172f8-2c49-400b-89e5-327bef177704 · outbound

This paper cites The Physics of Cosmic Acceleration.

Constraints on Dark Energy Models Using Late Universe Probes The Physics of Cosmic Acceleration

Reference 66

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Observation e15ce264-9b67-40c1-a26b-52c5b77af891 · outbound

This paper cites Dark Energy.

Constraints on Dark Energy Models Using Late Universe Probes Dark Energy

Reference 67

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Observation e4217bba-9a5b-4746-b7bb-ca372dd421c5 · outbound

This paper cites Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask).

Constraints on Dark Energy Models Using Late Universe Probes Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)

Reference 68

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Observation af00b396-571f-49db-957f-f49e8425c09d · outbound

This paper cites The Cosmological Constant is Back.

Constraints on Dark Energy Models Using Late Universe Probes The Cosmological Constant is Back

Reference 69

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Observation e268c00f-640c-4782-ac57-5246d4123033 · outbound

This paper cites Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests.

Constraints on Dark Energy Models Using Late Universe Probes Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests

Reference 70

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Observation 052957ce-e6c1-4d42-b0fd-011fe9294f54 · outbound

This paper cites Observational constraints on dynamical dark energy with pivoting redshift.

Constraints on Dark Energy Models Using Late Universe Probes Observational constraints on dynamical dark energy with pivoting redshift

Reference 71

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Observation c5229a7e-9cd7-44de-8e75-0fcdc4f9435e · outbound

This paper cites Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension.

Constraints on Dark Energy Models Using Late Universe Probes Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension

Reference 72

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Observation 342b55c8-8b22-4aad-b35b-880ad115a703 · outbound

This paper cites Dynamical dark energy after Planck CMB final release and $H_0$ tension.

Constraints on Dark Energy Models Using Late Universe Probes Dynamical dark energy after Planck CMB final release and $H_0$ tension

Reference 73

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Observation d4d6a876-a697-4847-85f7-08af8166852f · outbound

This paper cites Can dark energy be dynamical?.

Constraints on Dark Energy Models Using Late Universe Probes Can dark energy be dynamical?

Reference 74

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Observation 6ab77519-ff87-4bcd-af68-4a539c69f16e · outbound

This paper cites Modeling Dynamical Dark Energy.

Constraints on Dark Energy Models Using Late Universe Probes Modeling Dynamical Dark Energy

Reference 75

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Observation a0a92e12-789d-4324-99e1-ffaef7ae5261 · outbound

This paper cites The case for dynamical dark energy revisited.

Constraints on Dark Energy Models Using Late Universe Probes The case for dynamical dark energy revisited

Reference 76

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Observation 674f1b54-5744-409b-9621-d6d74bfac437 · outbound

This paper cites Dynamical dark energy or variable cosmological parameters?.

Constraints on Dark Energy Models Using Late Universe Probes Dynamical dark energy or variable cosmological parameters?

Reference 77

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Observation 932da266-6fbd-476e-81c3-b68e53a19ac9 · outbound

This paper cites Dynamical dark energy versus $\Lambda=$const. in light of observations.

Constraints on Dark Energy Models Using Late Universe Probes Dynamical dark energy versus $\Lambda=$const. in light of observations

Reference 78

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Observation e2c449f0-e4a0-47bf-90be-bcb2580d85d6 · outbound

This paper cites Cosmological Dark Energy: Prospects for a Dynamical Theory.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological Dark Energy: Prospects for a Dynamical Theory

Reference 79

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Observation 303d9656-a2bc-4089-8123-78f9bac03d26 · outbound

This paper cites Examining the evidence for dynamical dark energy.

Constraints on Dark Energy Models Using Late Universe Probes Examining the evidence for dynamical dark energy

Reference 80

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Observation a56bbe3c-294b-4eb2-8b2e-c703113c9b61 · outbound

This paper cites Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations

Reference 81

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Observation e792dd13-fcf5-4f91-8caa-df9d2ef5d8de · outbound

This paper cites Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension.

Constraints on Dark Energy Models Using Late Universe Probes Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension

Reference 82

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Observation b479d7c1-859c-4b81-8d56-def631d5f0ed · outbound

This paper cites Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues.

Constraints on Dark Energy Models Using Late Universe Probes Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues

Reference 83

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Observation f4b6acd2-c115-4955-a362-b1c30a1f7999 · outbound

This paper cites Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data.

Constraints on Dark Energy Models Using Late Universe Probes Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

Reference 84

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Observation a26551e4-ea06-4724-a46e-b954bb954318 · outbound

This paper cites an unresolved cited work.

Constraints on Dark Energy Models Using Late Universe Probes Unresolved cited work

Reference 85

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Observation 81302c1f-03d6-4a00-a3d3-37a0d707dec9 · outbound

This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result.

Constraints on Dark Energy Models Using Late Universe Probes Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result

Reference 86

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Observation bf04adcc-abb9-45d5-9ffd-daa661f1a51b · outbound

This paper cites Constraining Dark Energy Dynamics in Extended Parameter Space.

Constraints on Dark Energy Models Using Late Universe Probes Constraining Dark Energy Dynamics in Extended Parameter Space

Reference 87

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Observation f9875cf7-62fd-47d5-a76c-994106f01acf · outbound

This paper cites Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments.

Constraints on Dark Energy Models Using Late Universe Probes Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments

Reference 88

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Observation 419a33ca-9c3f-4e21-8eaf-b3b22f8c0582 · outbound

This paper cites Cosmological constraints in extended parameter space from the Planck 2018 Legacy release.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological constraints in extended parameter space from the Planck 2018 Legacy release

Reference 89

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Observation a88e510b-fd60-491c-9590-a2176d81ebc0 · outbound

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

Constraints on Dark Energy Models Using Late Universe Probes DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 90

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Observation 10ffb329-708c-4d45-ba82-dba683bc5036 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Constraints on Dark Energy Models Using Late Universe Probes Accelerating Universes with Scaling Dark Matter

Reference 91

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Observation e81800ff-4f78-4f4d-9b40-adba4658c112 · outbound

This paper cites Exploring the Expansion History of the Universe.

Constraints on Dark Energy Models Using Late Universe Probes Exploring the Expansion History of the Universe

Reference 92

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Observation f37097d0-7fa4-4541-9556-af52e646416d · outbound

This paper cites A parametric model for dark energy.

Constraints on Dark Energy Models Using Late Universe Probes A parametric model for dark energy

Reference 93

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Observation ee1e1dc6-fdfd-4a33-8668-71bc61149e71 · outbound

This paper cites Observational constraints on low redshift evolution of dark energy: How consistent are different observations?.

Constraints on Dark Energy Models Using Late Universe Probes Observational constraints on low redshift evolution of dark energy: How consistent are different observations?

Reference 94

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Observation 58d1740a-5735-4344-81b8-d39e50134015 · outbound

This paper cites Dynamical dark energy confronted with multiple CMB missions.

Constraints on Dark Energy Models Using Late Universe Probes Dynamical dark energy confronted with multiple CMB missions

Reference 95

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Observation 839ecb9a-79f2-4b7f-bf1f-250ecbd74f23 · outbound

This paper cites Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters.

Constraints on Dark Energy Models Using Late Universe Probes Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters

Reference 96

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Observation 3bfb4bdf-0eab-48ea-9d9c-ba57eefb56aa · outbound

This paper cites Addressing the Hubble tension with cosmic chronometers.

Constraints on Dark Energy Models Using Late Universe Probes Addressing the Hubble tension with cosmic chronometers

Reference 97

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Observation 5c66b37b-4db0-41d2-9e8d-e0c5b441550e · outbound

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Constraints on Dark Energy Models Using Late Universe Probes The Megamaser Cosmology Project. XI. A geometric distance to CGCG 074-064

Reference 98

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Observation 8c0744e2-33ca-443d-904e-b0473458f65e · outbound

This paper cites Cosmological constraints on dark energy models using DESI BAO 2024.

Constraints on Dark Energy Models Using Late Universe Probes Cosmological constraints on dark energy models using DESI BAO 2024

Reference 99

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Observation a6fe9f65-3225-4a26-92f9-973498ff587b · outbound

This paper cites Comparison of dark energy models using late-universe observations.

Constraints on Dark Energy Models Using Late Universe Probes Comparison of dark energy models using late-universe observations

Reference 100

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Observation 31805a0c-6dc9-4ae2-a9d6-beae1d9d6f19 · outbound

This paper cites an unresolved cited work.

Constraints on Dark Energy Models Using Late Universe Probes Unresolved cited work

Reference 101

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Observation 5eaeb395-3155-4aaf-a1d2-027f3d78644f · outbound

This paper cites Underdetermination of dark energy.

Constraints on Dark Energy Models Using Late Universe Probes Underdetermination of dark energy

Reference 102

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Pith citing papers

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Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Constraints on Dark Energy Models Using Late Universe Probes

Reference 29

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Observation fc98218f-7973-4980-b09b-d6682d8c864e · inbound

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Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Constraints on Dark Energy Models Using Late Universe Probes

Reference 49

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Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Constraints on Dark Energy Models Using Late Universe Probes

Reference 126

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Reference 46

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Reference 54

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