Paper Citation Record · LEDGER

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

As of 20 August 2026, this Paper Citation Record lists 100 of 131 outbound references and 44 inbound Pith citation observations for arXiv:2412.12905.

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

pith.paper-citation-record.v1
2412.12905 v2

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measured 100 of 131 reference resolution

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measured 44 of 44 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T01:06:27.564754Z

measured 0 of 1 external citation measurements

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Source: pith, observed 2026-07-08T15:55:05.017633Z

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Outbound references

Observation 97007a7f-e3a3-4c5f-9bba-bccb9375ece3 · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.565712Z

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Observation 0a010786-948f-4086-a367-a916cb28619a · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Challenges for $\Lambda$CDM: An update

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.570089Z

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Observation bff04e44-7a25-4fb6-9020-c3e606d2daca · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.574349Z

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Observation e6f053eb-cf06-4ca7-8b4c-75864590d0d5 · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Planck 2018 results. VI. Cosmological parameters

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.578354Z

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Observation fadfeda2-d95c-4683-a955-d7a6a0ab06b7 · 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.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? 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 5

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.582812Z

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Observation 049f476a-cffa-41b0-9142-4b16ba803675 · outbound

This paper cites Measurements of the Hubble Constant: Tensions in Perspective.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Measurements of the Hubble Constant: Tensions in Perspective

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.586771Z

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Observation c02e93ac-ecf5-4c28-b726-1782ede1dfb7 · outbound

This paper cites The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.590602Z

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Observation 60e0bbd9-04f6-453e-b5f4-ace2b72820e4 · outbound

This paper cites The Hubble Constant from Infrared Surface Brightness Fluctuation Distances.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Hubble Constant from Infrared Surface Brightness Fluctuation Distances

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.594906Z

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Observation 99718dc6-d2ae-4fd9-add1-9ed0599e7585 · outbound

This paper cites Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations

Reference 9

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Observation 3269fa9f-4e40-4fa5-b2f3-ea792de19068 · outbound

This paper cites CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.602725Z

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Observation 536dc58f-bd0e-4850-b39e-8f58628aaa3a · outbound

This paper cites CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.607059Z

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Observation 7238fd11-1e43-4721-9650-61b5f556dbc7 · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.611663Z

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Observation c8916fde-5524-475f-8ae1-38234d6dc48d · outbound

This paper cites Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.615610Z

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Observation 5aa4dcd4-df7c-4bef-a338-2c2efd5c4c20 · outbound

This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.619419Z

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Observation 6602d4a5-5565-49ac-bbc4-b569de3383e2 · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.623372Z

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Observation 331e37a2-de33-4f88-8df7-c7f3e317f158 · 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.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.627487Z

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Observation d00ff5fb-1cd2-43b3-a65f-62e3a7e4040d · outbound

This paper cites TDCOSMO. I. An exploration of systematic uncertainties in the inference of $H_0$ from time-delay cosmography.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? TDCOSMO. I. An exploration of systematic uncertainties in the inference of $H_0$ from time-delay cosmography

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.631216Z

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Observation 6d91820b-5af5-499c-829d-de411f4d7c09 · outbound

This paper cites Is there an early Universe solution to Hubble tension?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Is there an early Universe solution to Hubble tension?

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.635044Z

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Observation b6b0f4ca-8e4f-40bf-9173-861069b5d539 · outbound

This paper cites Running Hubble Tension and a H0 Diagnostic.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Running Hubble Tension and a H0 Diagnostic

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.642186Z

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Observation a705abd6-a3cc-49c1-ba16-cda1fa153461 · outbound

This paper cites On the Hubble constant tension in the SNe Ia Pantheon sample.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? On the Hubble constant tension in the SNe Ia Pantheon sample

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.647752Z

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Observation d7c2db04-91b9-4368-a13c-837a563e65de · outbound

This paper cites On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.651476Z

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Observation 605b3b10-5c5d-4fb6-9874-8ff852b9034f · outbound

This paper cites Revealing the late-time transition of $H_{0}$: relieve the Hubble crisis.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Revealing the late-time transition of $H_{0}$: relieve the Hubble crisis

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.655284Z

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Observation 48dbd911-d0a8-4b02-a77d-aed7c66ef382 · outbound

This paper cites Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.658951Z

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Observation 2d090643-657c-4933-9268-ab97db89d01c · outbound

This paper cites Putting Flat $\Lambda$CDM In The (Redshift) Bin.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Putting Flat $\Lambda$CDM In The (Redshift) Bin

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.663237Z

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Observation 497fdefc-4816-4ddd-8996-9df1f6372639 · outbound

This paper cites Evidence of a decreasing trend for the Hubble constant.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Evidence of a decreasing trend for the Hubble constant

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.667015Z

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Observation 45d8451e-cf7c-4503-be59-c841858cd103 · outbound

This paper cites Uncorrelated estimations of $H_0$ redshift evolution from DESI baryon acoustic oscillation observations.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Uncorrelated estimations of $H_0$ redshift evolution from DESI baryon acoustic oscillation observations

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.670763Z

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Observation a1737a49-b12f-41a4-9107-571a99bd3dba · outbound

This paper cites Cosmological constraints from the Hubble diagram of quasars at high redshifts.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmological constraints from the Hubble diagram of quasars at high redshifts

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.674333Z

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Observation a2e74529-f9d5-48f7-a2ae-a03a59c8a12c · outbound

This paper cites Quasars as standard candles III. Validation of a new sample for cosmological studies.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Quasars as standard candles III. Validation of a new sample for cosmological studies

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.678186Z

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Observation 47cc54ea-e78b-4f3d-b783-a532f40aa394 · outbound

This paper cites Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.681692Z

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Observation 2248d2c2-b981-4b40-9b29-5e84ef9505d8 · outbound

This paper cites Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.685615Z

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Observation 56eb58d6-4843-4588-8274-7f73b114d6f6 · outbound

This paper cites No-go guide for the Hubble tension: late-time or local-scale new physics.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? No-go guide for the Hubble tension: late-time or local-scale new physics

Reference 31

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Observation e26268e6-0616-45ec-9d1b-72757382205b · outbound

This paper cites Do high redshift QSOs and GRBs corroborate JWST?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Do high redshift QSOs and GRBs corroborate JWST?

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.693241Z

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Observation c888a2ef-dd5f-4e6d-b081-1a5d1edabb25 · outbound

This paper cites Narrowing down the Hubble tension to the first two rungs of distance ladders.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Narrowing down the Hubble tension to the first two rungs of distance ladders

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.697699Z

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Observation 3c1b6491-11f8-4884-aead-8065246d51d4 · outbound

This paper cites Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.701523Z

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Observation e263c487-26b7-4151-b9a1-8e3138c83695 · outbound

This paper cites The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data

Reference 35

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Observation e1ca4d36-e867-4e4a-95cc-b767cb4f77f8 · outbound

This paper cites Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium

Reference 36

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Observation 3dfe817d-b739-4222-a6be-e65b1522f9e2 · outbound

This paper cites More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey

Reference 37

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Observation 4cd94edd-6549-4dc0-99ad-fd7a0ff39f0a · outbound

This paper cites Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.717007Z

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Observation 591d8bb0-b357-4c77-9e6b-04224461f597 · outbound

This paper cites $S_8$ increases with effective redshift in $\Lambda$CDM cosmology.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.721183Z

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Observation 09feb980-43c0-47f0-9c7a-a4c2d93b8f15 · outbound

This paper cites Further support for $S_8$ increasing with effective redshift.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Further support for $S_8$ increasing with effective redshift

Reference 40

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Observation 71fa556b-214c-4219-9294-618140d17e9e · outbound

This paper cites The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.728656Z

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Observation 97641485-a9c0-47b1-8826-41ee81cd666f · outbound

This paper cites an unresolved cited work.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Unresolved cited work

Reference 42

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Observation 6ab71e68-a859-48a4-a1dd-8692a72384ff · outbound

This paper cites DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.735625Z

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Observation 60cfa6d7-2e23-42e7-8c25-d42b490607b9 · outbound

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.739073Z

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Observation bf996a66-ab16-4308-ac02-c4ca98d6b156 · outbound

This paper cites Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.743415Z

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Observation 0c6d107a-371a-439f-827e-3e48b3b920ba · outbound

This paper cites The Atacama Cosmology Telescope DR6 and DESI: Structure growth measurements from the cross-correlation of DESI Legacy Imaging galaxies and CMB lensing from ACT DR6 and Planck PR4.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Atacama Cosmology Telescope DR6 and DESI: Structure growth measurements from the cross-correlation of DESI Legacy Imaging galaxies and CMB lensing from ACT DR6 and Planck PR4

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.732161Z

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Observation 3d02fdc0-2fbc-4b0b-b29c-6738c098858e · outbound

This paper cites Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.751096Z

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Observation 85e8ed6a-5443-46c7-98f8-bf2e96e55bc6 · outbound

This paper cites Mukherjee and A.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Mukherjee and A

Reference 48

Resolution: verified exact; raw_fallback, observed 2026-08-11T13:41:25.269135Z

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Observation 2016212f-7095-4aaa-9256-63a7a4cb76fd · outbound

This paper cites $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.758572Z

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Observation 577586c7-ace0-4fea-8b5d-c45cd0612e81 · outbound

This paper cites A test for the redshift dependence of $\sigma_8$ using $f\sigma_8$ measurements.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? A test for the redshift dependence of $\sigma_8$ using $f\sigma_8$ measurements

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.747394Z

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Observation 117a56f7-c4cb-49e4-bc6a-5c9336b1bb72 · outbound

This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

Reference 51

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Pantheon+ Analysis: Cosmological Constraints

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

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This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

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This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Dark Energy Survey Supernova Program: Light curves and 5-Year data release

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This paper cites Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?

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This paper cites Dark energy in light of recent DESI BAO and Hubble tension.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Dark energy in light of recent DESI BAO and Hubble tension

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result

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This paper cites Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?

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This paper cites Cosmological constraints on curved quintessence.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmological constraints on curved quintessence

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This paper cites On the evidence of dynamical dark energy.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? On the evidence of dynamical dark energy

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Quintessential interpretation of the evolving dark energy in light of DESI

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This paper cites Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements

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This paper cites First Constraints on a Pixelated Universe in Light of DESI.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? First Constraints on a Pixelated Universe in Light of DESI

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This paper cites DESI Constraints on Exponential Quintessence.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI Constraints on Exponential Quintessence

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This paper cites Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model

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This paper cites Solar chameleons: Novel channels.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Solar chameleons: Novel channels

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This paper cites Bhattacharya, G.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Bhattacharya, G

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements

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

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Matching current observational constraints with nonminimally coupled dark energy

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This paper cites Consistency tests between SDSS and DESI BAO measurements.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Consistency tests between SDSS and DESI BAO measurements

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This paper cites Bridge the Cosmological Tensions with Thawing Gravity.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Bridge the Cosmological Tensions with Thawing Gravity

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This paper cites Revisiting holographic dark energy after DESI 2024.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Revisiting holographic dark energy after DESI 2024

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This paper cites Model independent cosmographic constraints from DESI 2024.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Model independent cosmographic constraints from DESI 2024

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This paper cites Model-agnostic assessment of dark energy after DESI DR1 BAO.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Model-agnostic assessment of dark energy after DESI DR1 BAO

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This paper cites $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

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This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data

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This paper cites Mukherjee and A.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Mukherjee and A

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This paper cites DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes

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This paper cites Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

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This paper cites Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs

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This paper cites What if string theory has a de Sitter excited state?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? What if string theory has a de Sitter excited state?

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This paper cites Model-Independent Test of Prerecombination New Physics: Measuring the Sound Horizon with Gravitational Wave Standard Sirens and the Baryon Acoustic Oscillation Angular Scale.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Model-Independent Test of Prerecombination New Physics: Measuring the Sound Horizon with Gravitational Wave Standard Sirens and the Baryon Acoustic Oscillation Angular Scale

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This paper cites Quantification of 2D vs 3D BAO tension using SNIa as a redshift interpolator and test of the Etherington relation.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Quantification of 2D vs 3D BAO tension using SNIa as a redshift interpolator and test of the Etherington relation

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This paper cites Can recent DESI BAO measurements accommodate a negative cosmological constant?.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Can recent DESI BAO measurements accommodate a negative cosmological constant?

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This paper cites The Cosmological Preference for Negative Neutrino Mass.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? The Cosmological Preference for Negative Neutrino Mass

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This paper cites an unresolved cited work.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Unresolved cited work

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This paper cites Impact of evolving dark energy on the search for primordial gravitational waves.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Impact of evolving dark energy on the search for primordial gravitational waves

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Cosmological constraints from calibrated $E_p-E_{iso}$ gamma-ray burst correlation by using DESI 2024 data release

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This paper cites Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis

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Observation 4c7a8531-d031-435a-852c-1ac6864686c6 · outbound

This paper cites Arjona and S.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Arjona and S

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50bd8e14-3d94-4b74-91d0-574444d146e8 · inbound

Tuning the cosmic instrument: robust cosmology through combined probes cites this paper.

Tuning the cosmic instrument: robust cosmology through combined probes DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-09T14:46:06.550296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 47743180-6287-4f9f-a974-c6603a39bb86 · inbound

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-08T23:12:26.188946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28ad7101-f891-4310-b8e8-ffb65d5c015b · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-08T22:04:59.451872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83665ba1-751d-4e0b-8f14-57482ab2743b · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.705968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3bd8737-908e-4ffc-84ed-b91778b78e6e · inbound

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions cites this paper.

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-08T17:56:51.936732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0036e1ca-c4d1-40e4-93f3-37bf1663fdf7 · inbound

On the tension between DESI DR2 BAO and CMB cites this paper.

On the tension between DESI DR2 BAO and CMB DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-16T01:06:27.564754Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 72b703df-f824-4778-b910-8960bb73a018 · inbound

The matter with(in) CPL cites this paper.

The matter with(in) CPL DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-15T22:00:18.119696Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f3af7a7-aa82-4dc6-868e-ea1495d64f8e · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 111

Resolution: verified exact; arxiv_id, observed 2026-05-19T13:12:18.750206Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 6440c24a-ece6-4113-8c50-99950e84c2d9 · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.353704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dcf8f4d6-d429-4d38-ba43-1ca11b478f93 · inbound

Uncalibrated Cosmic Standards as a Robust Test on Late-Time Cosmological Models cites this paper.

Uncalibrated Cosmic Standards as a Robust Test on Late-Time Cosmological Models DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T10:50:52.110174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 199f838b-4681-4a66-ad47-d892e4787fd3 · inbound

Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data cites this paper.

Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-06T21:34:26.662248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 122e1715-1dab-46bd-8458-9bf4c58d908c · inbound

New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:22:06.259094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 9a320c14-c6bc-4cc0-a34d-90bf61eb52d9 · inbound

Revisiting cosmic acceleration with DESI BAO cites this paper.

Revisiting cosmic acceleration with DESI BAO DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T11:39:53.234165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd5d076d-1a8e-41e9-afa5-535a68345bca · inbound

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

Resolving the Planck-DESI tension by nonminimally coupled quintessence DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-19T01:36:57.984521Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 1d46001f-521b-4551-9832-7efba630134c · inbound

Constraints on transition redshift utilizing the latest H(z) measurements and comments on the Hubble tension cites this paper.

Constraints on transition redshift utilizing the latest H(z) measurements and comments on the Hubble tension DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-05T23:25:36.592233Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ffa7031c-815d-482f-8412-e9e6d5f9e703 · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:46:16.666674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 410db800-809c-4c19-ab80-350d64582361 · inbound

Crosschecking Cosmic Distances from DESI BAO and DES SNe cites this paper.

Crosschecking Cosmic Distances from DESI BAO and DES SNe DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:32:33.857388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 4fc247fa-9fdf-4fa9-845b-01bd6507f3a4 · inbound

Crosschecking Cosmic Distances from DESI BAO and DES SNe cites this paper.

Crosschecking Cosmic Distances from DESI BAO and DES SNe DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-04T11:34:09.414604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d7d9152-e2ee-4b50-bbed-5cf4908110fb · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 112

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:21.190629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 960b6dd7-e0ce-4210-a6a7-2d4bb0514029 · inbound

DESI constraints on two-field quintessence with exponential potentials cites this paper.

DESI constraints on two-field quintessence with exponential potentials DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-04T08:18:50.581465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f7274ea-cdd9-47ee-ace7-de4d3b057dfb · inbound

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM cites this paper.

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-03T18:51:46.262584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80dbbca6-24a9-41ec-a019-6ec4cc6bf6da · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.433543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b51538f-5cdf-440f-9e35-039b5547cdd7 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 150

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.995267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b7928cb-d6c1-4d12-9b1d-667b96bccc1c · inbound

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-16T02:27:10.063580Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 0f0f6064-6fc8-4b5d-8189-e6d0d3f27f3f · inbound

Mapping the redshift drift at various redshifts through cosmography cites this paper.

Mapping the redshift drift at various redshifts through cosmography DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-13T18:38:07.456074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation ed036ebe-61b0-451a-a137-ab1ce39e26ca · inbound

Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.

Breaking Free from the Swampland of Impossible Universes through the DESI Portal DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-02T14:29:23.253844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad9e7e72-a52b-4509-adce-fce27fa8e5f9 · inbound

A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-07-01T21:46:15.850126Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 1f509e89-c6a5-447e-9448-22c1330908e7 · inbound

A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T12:40:02.711551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b97afb1-7395-4693-be8c-e4ed53511c94 · inbound

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements cites this paper.

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-07-03T15:38:34.040238Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation ca645464-17f8-43d8-8fbc-1346abd31363 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 133

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:19:23.617817Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 68042e03-fbd0-43b4-81de-d51a0cc6a7f6 · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 268

Resolution: verified exact; arxiv_id, observed 2026-07-02T06:16:43.190898Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation a3b60f7a-85b8-4118-b307-3374bbf79db4 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:05.018866Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 948cf7cd-c83e-4538-abe4-fc8448d4ca92 · inbound

Evaporating cosmologically coupled black holes cites this paper.

Evaporating cosmologically coupled black holes DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 257

Resolution: unresolved; no resolver link, observed 2026-08-02T03:36:03.719306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cde0bcd-25e4-4488-9227-69babe230479 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 297

Resolution: unresolved; no resolver link, observed 2026-08-01T08:09:03.729947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd3ea272-4f26-44cf-ab7a-e6ae3a55f1b9 · inbound

Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ cites this paper.

Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 49

Resolution: unresolved; no resolver link, observed 2026-07-31T11:14:46.860699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea65fd28-5167-4c6c-94e1-e0a177ddb26c · inbound

A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal cites this paper.

A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-03T17:20:49.356567Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d92f815b-229a-48f9-a494-01171dbc2c9f · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.190153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9947ecac-7951-4d33-ad32-8fe6bffd5686 · inbound

Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB cites this paper.

Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-08T19:17:22.472790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d19cd7a2-5172-4b5e-b04f-dc77ebf8c355 · inbound

Evolution of matter perturbations in the context of cosmic slowing down cites this paper.

Evolution of matter perturbations in the context of cosmic slowing down DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-15T14:42:16.880292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.