Pith. sign in

Paper Citation Record · LEDGER

How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements

As of 5 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 2 inbound Pith citation observations for arXiv:2511.18657.

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

pith.paper-citation-record.v1
2511.18657 v1

Coverage vector

measured 58 of 58 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-17T05:42:44.912403Z

measured 60 of 60 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T13:11:12.277830Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

58 of 58 outbound references displayed

  • verified exact31
  • verified fuzzy11
  • unresolved3
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch13

External citation measurements

No source-named external measurement is stored.

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.615894Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:4419ad0e1598273372d64b944ba0f908802fa0c35c1d59ae9d09e01232e6bf49

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.612927Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:ec209c1dca7f9c0f09d69e5a61dd488940b694c3abbf701ffc11fd05484273b1

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.626391Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:2568c9cbe1d359b05cda81e75738cacd9c67371c6f1162d276a401bdcca9ffe0

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.623966Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:1bea8f6e44a40c3f97e5cd6a44b0aa642d282f4114876ab79cf9f42fe111cb63

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.610131Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:64eba42a1dd2b673f06d861d0754652c4ca6afe4a2b4f191d79038628d1fe4c4

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.618992Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:e2f6b5c9d85e9815635a823564be4e26e86d035b3f8701d73775f144975b6f0d

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.621526Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:44e17ecf92bfb27064bfd07e2dc7f1f6468237211321dbadd4fdaf6db758b4fb

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

Resolution
unresolved
raw_fallback, observed 2026-05-17T05:44:08.599013Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:1869a7782a21ec325f7f8604f83d0f5d9257256a80f7a68324ebc7e66c9f349f

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.457605Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:f23c6357ca731cd78b19de64751951736d27231890f52adef2449b4d29002eee

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.368985Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:60ad7f0d4790855c5b82a2bf96fdc0945ad7999ca05af05658f82a465d3d82a8

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.383947Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:a1063a04ca4aa04b3051b62e6bff2b26b423db998afd13d6d31b0de899bc9840

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.355938Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:ec1e53bc6de5859776e6067310924cd321db19d1e18732110ab468a785bd7a29

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.427868Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:577f7a2e44786b36e9719d948045adf069c54c89e235141e2091f584a49a64e5

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.446077Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:6451921924c791b267fd6ea6a29e3015d7ee49a92d54c8d99cce18480ee0ccd9

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

Resolution
unresolved
raw_fallback, observed 2026-05-17T05:44:08.594268Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:45993e744432059259c63f2c4268708a116dc8e9b7bcde5c12583359f5b6dd03

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

Resolution
verified exact
arxiv_id, observed 2026-05-19T09:35:13.685919Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:015212fa5b89e0b43e2d1cd0d52435a9b3e11600350a433128f2dacc07968ceb

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.403378Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:9a0a80c967e297550670296120ae60a3f6072317c023eec8e16f407558cc5f0a

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.372787Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:5da5b5d4b57291334a98bcf65df29628dcfe11b366ba2b0a837ac6ec5fafe917

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.376738Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:c8a8a92591a6f3a6615c1f6a998d173a7d542f24a36c8d52c436def7bec33c47

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.479224Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:f084679e659b7455216da0cc8e4fcb3d16174b933c85b0263b520c5403c93180

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.521211Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:55a097a5549cfcce0dadb828f6ba57cc09b2195452c153d0976dedb604edddd0

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.488297Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:664a8085f87630a022c640eee79cd79d7e05a52c24e50be338e322d47e2e3936

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.493198Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:92edf8473eb38486f4ebe793728c15abe3e8a927d441a8a2f8544fff73df4238

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.498454Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:0acf39174bcfed00463557c568d6d96f28974415af5201fb10b40906dfb9fd3c

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.603490Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:04045683696e9026d9ef44c47efe9ce19bb0c59af5b7107f27cd0b006b68e087

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.503098Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:488810919a8c106e628869778d93b427f187fa6540e4f8bccbe59969449d2520

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.351192Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:e2a2efeb7731cdebc68c2ba29d5f85108347a40dab017f70ce693d846f77e2e0

Observation eefa9671-c882-4afa-872b-a4c858994723 · 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.

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.537020Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:302ed43b59f4070c3d107eca18ff7d9b4bd8cc602c42d5d7a7ab66751d019e13

Observation 13f45fdb-486d-4a0d-bf39-a67d3ed4bf40 · outbound

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

Resolution
verified exact
arxiv_id, observed 2026-05-17T05:44:07.396256Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:2fb0ab01ff16fe3f10da89e3c0f2765af3951eedcfe60cb7e6b8260081ec6652

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

Resolution
verified exact
arxiv_id, observed 2026-05-17T05:44:07.359629Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:3344c63d9532ed734aa6a0ec7fe833a25a8a9fd6334429c2eeafefeff81ba10c

Observation b1523b67-3e9a-4935-976a-c8f8b45abd35 · outbound

This paper cites Challenges for $\Lambda$CDM: An update.

How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Challenges for $\Lambda$CDM: An update

Reference 32

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.532923Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:95dbcbe285104aa6f9ed7e902a244290f3b8f0653a9beb05d047ca6fe878f866

Observation 44cb6b87-e823-40af-ba7b-b08712e1681b · outbound

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.517065Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:30c1ab6f6245e0b55f917467c743e795f0d42573cd204e451cb7b274f224a90a

Observation 861d0c7f-5268-4cce-927b-29c7129a4d41 · outbound

This paper cites Dynamics of dark energy.

How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Dynamics of dark energy

Reference 34

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.436068Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:ec2802479bca864ebfb70f363a8c5396a58b95f8150caca4b29c8728bc5dc735

Observation 9d29bb3f-0979-49b2-b18d-8691cb6017da · outbound

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.363575Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:d0ff0d1ab9bfb8d066da73901a15c8ec6acf9f317719cbfc664e530bf16a3c26

Observation 4b5406da-14a3-4cc5-be3b-3d85da98bf11 · outbound

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

Resolution
verified exact
arxiv_id, observed 2026-05-17T05:44:07.422610Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:61d16e4fdce0fb630d23c14eda1e6bd34b273cbb52428ff60b1ef44d122f1ae3

Observation 77438699-53de-4b83-b081-69e031c98ae8 · 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 37

Resolution
verified exact
arxiv_id, observed 2026-05-17T05:44:07.507610Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:aa63de68e75b4cde4576f734722dcddea7123c9307ba99b6977697a802c41f20

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.418903Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:c3c9882dd8f9fdbb7fabcbc9b610c314d2439415efc0f5ab40f0695ef65ada64

Observation 6c34030c-e380-47f9-a0d4-4e76006874a9 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements Accelerating Universes with Scaling Dark Matter

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.399847Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:220c91f49f496c405832fb915fbe2bfac921715631e4f1795d2c8b947704aa19

Observation 154529ad-a748-40c4-b922-f200531a525b · outbound

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.483755Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:8a66ccdf5b527e215d21a20883ead98581faaa5e765ab3699bdcbc33377f8627

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
verified exact
arxiv_id, observed 2026-05-17T05:44:07.346184Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:37cbef630d76153054f2d34b33ac538ead3875f3782799c4d1b372412483c321

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.547983Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:0d5f9dd0de0631a6f6d9c8428f8098e3b891fd55f997328dc2e0a9ece5460c28

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.525603Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:695dd8e073becb6dac18ba966103f43ef0c9d4b22950b7bc9d6c5d0a7a4020f7

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

Resolution
verified exact
arxiv_id, observed 2026-05-17T05:44:07.380021Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:f636590f19b5bc4ce4e7d115400b67032ff9a9f4bb001998b5a822c061b99e3f

Observation 1c7cce95-385e-4d6f-9acd-a890b5d5c8bd · outbound

This paper cites Constraints to dark energy using PADE parameterisations.

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.511392Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:833cd9813ef49548e074f572ed1f58d7c3e312cc41dbd6885375384e327374ca

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.529349Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:7e31dfb13791c14dbf76fade0de79b8bfcb854d23c17d162fe893008b1c885b3

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

Reference 47

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.440859Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:a19bccc45ccdedc53773602ec6597868e69e2de2c977a958bdeac19ee4603cc5

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

Resolution
verified exact
arxiv_id, observed 2026-06-09T02:06:02.692145Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:581ed2663facbef1c4eb15f21f5eb8cf36b5d33ba2d9835817e44f0cbdc1167f

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

Resolution
verified exact
arxiv_id, observed 2026-05-17T06:34:55.175109Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:81c3f182484c67867b75f86330314fac3e666441b07b270f7f5a73c2ca30b8cf

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

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

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:bc353262fefcebeb98a2db9dadbcaf899701166ce555c737c43082a9e6599075

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.450749Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:50833ea6d3357f1a842eb37ffd04ee799944a38854e5ba335a127d1c10961b5d

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

Resolution
unresolved
raw_fallback, observed 2026-05-17T05:44:08.608043Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:bfb3fc4d501de6a3d919b594e5a8a424604ec46f1978a793340575f301347d32

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.472752Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:cdf960c6ad410acb216952b37fa972a4385301b9e84d89e57594123a4931f0f9

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

Resolution
verified exact
local_arxiv, observed 2026-05-17T05:44:07.542365Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:ab360503ff04ad3c435d860adc65c33dc2764c5abcd68a6e879720672a136c44

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.410421Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:9113d40ea51995af899bd1f3b92bf4a67e0b64f39e7baae8cf9ea112b74d2d5f

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.601044Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:d65ff0dde04db2bfcf222c51c52f846c2deab77d8f57dcec7d1cae7b85707d91

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

Resolution
metadata mismatch
local_arxiv, observed 2026-05-17T05:44:07.406889Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:ae125e75550c0e8966b6589cb7961fbb907c686128214f0de87235bdbbbfecb2

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.605811Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:997077adc4481d422863cabec4782ce1ac9bdacfa76bfda52be8eed05a330582

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

Resolution
verified fuzzy
raw_fallback, observed 2026-05-17T05:44:08.596722Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-05-17T05:42:44.912403Z digest=sha256:b5c5a4781250417aaebf16e49da1d714883e6541126bc6d3cd2ff1144d76f4d5

Pith citing papers

Observation 6db5ea7e-8bbe-4919-b194-3607123b0e45 · inbound

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks cites this paper.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-03T13:11:12.277830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T13:11:12.277830Z digest=sha256:0d11a64a6e2a55e814e7d7f579c399c9d2bb68a7db6390366257ce7ddf95b121

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

Resolution
unresolved
no resolver link, observed 2026-08-01T02:14:30.422251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T02:14:30.422251Z digest=sha256:2fd8376ff93a075cf60c5a82c7b96d40b63a9017b9a7530b6e7bee2b9f57e695