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Source: paper_references, paper_reference_links, observed 2026-05-17T05:42:44.912403Z
Paper Citation Record · LEDGER
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements
As of 2 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 1 inbound Pith citation observation for arXiv:2511.18657.
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58 of 58 outbound references displayed
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Outbound references
Observation b1153e62-cbdc-4acc-9452-01d5ce152d79 · outbound
This paper cites The details of these datasets and their implementation in our analysis are discussed in the following subsections.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The details of these datasets and their implementation in our analysis are discussed in the following subsections
Reference 1
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Observation 643a058d-0b93-44fa-b690-11e3acdb5a13 · outbound
This paper cites As another method to overcome these limitations, we adopt the more robust and philosophically sound approach, namely the BE framework for model comparison.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements As another method to overcome these limitations, we adopt the more robust and philosophically sound approach, namely the BE framework for model comparison
Reference 2
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Observation f296b634-0d8b-429f-91a3-6fe19dc59c69 · outbound
This paper cites Our constraints are generally consistent across all DE parameterizations, indicating a robust de- termination of cosmology in the background level.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Our constraints are generally consistent across all DE parameterizations, indicating a robust de- termination of cosmology in the background level
Reference 3
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Observation fa1ee97e-040b-49ff-96e5-9cbcd88edb23 · outbound
This paper cites The results are sum- marized in Table VII.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The results are sum- marized in Table VII
Reference 4
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Observation 8c72e660-668a-4cf8-9702-526bf75a2f9c · outbound
This paper cites The strength of the BF is interpreted using Jeffreys’ scale.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The strength of the BF is interpreted using Jeffreys’ scale
Reference 5
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Observation 7b31b6f6-afc4-4f3b-8cbd-01e8550d9b96 · outbound
This paper cites The constraints on Ω m andH 0 are broadly consistent with those obtained from the Pan- theonPlus sample, indicating a stable background cos- mology across both SN Ia compilations.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The constraints on Ω m andH 0 are broadly consistent with those obtained from the Pan- theonPlus sample, indicating a stable background cos- mology across both SN Ia compilations
Reference 6
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Observation 78fdee5c-7831-4390-9614-aaa12efb52eb · outbound
This paper cites In general, our findings support a stronger preference for evolving DE, as detailed below.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements In general, our findings support a stronger preference for evolving DE, as detailed below
Reference 7
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Observation 5b1b688c-aa28-4f31-b9e6-a75cd545ae06 · outbound
This paper cites an unresolved cited work.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Unresolved cited work
Reference 8
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Observation 3cc258db-8499-498a-9a4a-7f670eff4f9b · outbound
This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Reference 9
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Observation 17f8f968-279d-42a8-9658-420f378b825e · outbound
This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Measurements of Omega and Lambda from 42 High-Redshift Supernovae
Reference 10
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Observation 437c825b-a919-4cde-8a86-1063c4815ab1 · outbound
This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Planck 2018 results. V. CMB power spectra and likelihoods
Reference 11
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Observation b1036cc4-3d79-4659-bdf5-6c5be2b151bd · outbound
This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
Reference 12
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Observation 50a8d747-1d4e-4657-9b65-6fee5864954f · outbound
This paper cites Planck 2013 results. XVI. Cosmological parameters.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Planck 2013 results. XVI. Cosmological parameters
Reference 13
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Observation 189bdc9c-ba4f-4c73-a340-9d6f68962909 · outbound
This paper cites Planck 2018 results. VI. Cosmological parameters.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Planck 2018 results. VI. Cosmological parameters
Reference 14
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Observation 8dbec489-ba9d-43cd-aa7a-f7a24f08c342 · outbound
This paper cites an unresolved cited work.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Unresolved cited work
Reference 15
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Observation be21004d-02a9-4581-9b2f-48bedf28e6d4 · outbound
This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
Reference 17
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Observation 92dee9e5-ec12-46d3-be5c-c38ffab2dcb4 · outbound
This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
Reference 18
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Observation 07147e65-dc72-4b78-94ed-02d966e89503 · outbound
This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
Reference 19
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Observation 4b07dc2d-9f8b-42aa-9721-a0b823e095bd · outbound
This paper cites Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
Reference 20
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Observation 2f27520a-5c7b-45da-b150-8d84a94e1bb7 · outbound
This paper cites Electron-phonon coupling in quasi free-standing graphene.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Electron-phonon coupling in quasi free-standing graphene
Reference 21
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Observation e73285ba-7de6-4ed6-bf30-4ad1d43dbd4c · outbound
This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
Reference 22
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Observation 70852fda-1605-4e70-8bcf-7d7b922a365d · outbound
This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
Reference 23
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Observation b049884d-ec93-4f53-b89a-3d64db8ecb6d · outbound
This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
Reference 24
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Observation f5cee150-e6b9-4e6e-bb4c-a5bc3355fb78 · outbound
This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
Reference 25
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Observation 50f110b1-a5ee-47db-8fea-14a1a164d80c · outbound
This paper cites Weinberg, Rev.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Weinberg, Rev
Reference 26
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Observation c8cd79bc-b4e6-48df-9626-4cc2fa8f064b · outbound
This paper cites Cosmological Constant - the Weight of the Vacuum.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Cosmological Constant - the Weight of the Vacuum
Reference 27
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Observation 107fa7fa-4d84-4322-9dad-0c3cb539dd1e · outbound
This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
Reference 28
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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.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements 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 29
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This paper cites Heavy-quark opportunities and challenges at FCC-ee.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Heavy-quark opportunities and challenges at FCC-ee
Reference 30
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Observation dbb38a74-35b6-49c4-bac3-eb6681d4dc47 · outbound
This paper cites On the well-posedness in Besov-Herz spaces for the inhomogeneous incompressible Euler equations.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements On the well-posedness in Besov-Herz spaces for the inhomogeneous incompressible Euler equations
Reference 31
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How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Challenges for $\Lambda$CDM: An update
Reference 32
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This paper cites Modified gravity models of dark energy.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Modified gravity models of dark energy
Reference 33
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How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Dynamics of dark energy
Reference 34
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This paper cites Cosmological Imprint of an Energy Component with General Equation of State.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Cosmological Imprint of an Energy Component with General Equation of State
Reference 35
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This paper cites Armendariz-Picon, V.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Armendariz-Picon, V
Reference 36
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How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Unresolved cited work
Reference 37
- Resolution
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No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.
Observation eedc2150-0597-4c71-a248-4f0704371211 · outbound
This paper cites Accelerated expansion of the universe driven by tachyonic matter.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Accelerated expansion of the universe driven by tachyonic matter
Reference 38
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How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Accelerating Universes with Scaling Dark Matter
Reference 39
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This paper cites Exploring the Expansion History of the Universe.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Exploring the Expansion History of the Universe
Reference 40
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Observation 83dc895a-d397-4a74-9e75-97c404d2c8d7 · outbound
This paper cites an unresolved cited work.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Unresolved cited work
Reference 41
- Resolution
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- arxiv_id, observed 2026-05-17T05:44:07.346184Z
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No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.
Observation 661e61f4-8fd5-46e7-82e4-56347f56f398 · outbound
This paper cites A generalized equation of state for dark energy.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements A generalized equation of state for dark energy
Reference 42
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Observation 95b452b1-3da2-47bc-bbc8-459138c0463b · outbound
This paper cites Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies
Reference 43
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No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.
Observation 2978ff0d-645c-4b4b-953d-876c09808835 · outbound
This paper cites Wetterich, Phys.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Wetterich, Phys
Reference 44
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- arxiv_id, observed 2026-05-17T05:44:07.380021Z
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No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.
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How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Constraints to dark energy using PADE parameterisations
Reference 45
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Observation d757fc95-c00f-431d-a869-8615fb003a6b · outbound
This paper cites How many dark energy parameters?.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements How many dark energy parameters?
Reference 46
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Observation 781ce78c-ca0c-410f-a938-8b0588c759f7 · outbound
This paper cites Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
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Observation 1adb5683-3aa5-45ce-92b2-e4d58f81e2ae · outbound
This paper cites To CPL, or not to CPL? What we have not learned about the dark energy equation of state.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements To CPL, or not to CPL? What we have not learned about the dark energy equation of state
Reference 48
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Observation 5e6d8442-8631-4b45-a875-ed21b3076fba · outbound
This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
Reference 49
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Observation de117bc6-5804-46cf-87f6-37af0ceb9750 · outbound
This paper cites DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 50
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Observation cdbec958-bc40-43ba-ac14-f23ae925450d · outbound
This paper cites A Bayesian Perspective on Evidence for Evolving Dark Energy.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements A Bayesian Perspective on Evidence for Evolving Dark Energy
Reference 51
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Observation 15a9b7ca-efdc-4924-984a-66612ff70858 · outbound
This paper cites an unresolved cited work.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Unresolved cited work
Reference 52
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Observation 0265be49-101a-4ed0-8ab8-254d7839b4aa · outbound
This paper cites Robust and model-independent cosmological constraints from distance measurements.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Robust and model-independent cosmological constraints from distance measurements
Reference 53
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Observation a8f9fc16-3e85-4dcd-8c3d-d694d432a718 · outbound
This paper cites Observational Constraints on Dark Energy and Cosmic Curvature.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Observational Constraints on Dark Energy and Cosmic Curvature
Reference 54
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Observation 7e51e2ea-8ef5-415e-82c2-735e619666dd · outbound
This paper cites The Pantheon+ Analysis: Cosmological Constraints.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements The Pantheon+ Analysis: Cosmological Constraints
Reference 55
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Observation 09f5d57e-6fde-424e-ab3d-17e6fc0a6360 · outbound
This paper cites Foreman-Mackey, D.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Foreman-Mackey, D
Reference 56
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Observation 6fdf8fa8-4a3d-409e-8ce8-f000591d0029 · outbound
This paper cites GetDist: a Python package for analysing Monte Carlo samples.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements GetDist: a Python package for analysing Monte Carlo samples
Reference 57
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Observation 5b5355d8-05a0-45be-bbeb-c8a739ad3d41 · outbound
This paper cites Akaike, IEEE Transactions on Automatic Control19, 716 (1974).
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Akaike, IEEE Transactions on Automatic Control19, 716 (1974)
Reference 58
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Observation 4821a407-cd24-4e49-81e5-0c71e5672c27 · outbound
This paper cites Jeffreys,The Theory of Probability, Oxford Classic Texts in the Physical Sciences (1939).
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Jeffreys,The Theory of Probability, Oxford Classic Texts in the Physical Sciences (1939)
Reference 59
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Pith citing papers
Observation 5afac2eb-7067-430a-bbf8-bbb581ac3b75 · inbound
No preference for generalized emergent dark energy from current cosmological data cites this paper.
No preference for generalized emergent dark energy from current cosmological data How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements
Reference 33
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