Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-08T23:12:26.303970Z
Paper Citation Record · LEDGER
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
As of 10 August 2026, this Paper Citation Record lists 100 of 101 outbound references and 35 inbound Pith citation observations for arXiv:2502.04212.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T21:04:17.779578Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T05:19:36.214969Z
Reference resolution
100 of 101 outbound references displayed
- verified exact2
- verified fuzzy0
- unresolved98
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation e71ad952-d21d-470f-8233-5ff29a784a09 · outbound
This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.940113Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ae55b58-6e85-48f8-bd70-297188a132bb · outbound
This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.944703Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 285368d6-fdc8-4972-a5c9-c98e9f041340 · outbound
This paper cites A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.948642Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c91d6c7f-1141-49ab-ba76-8af55a78519f · outbound
This paper cites Planck 2018 results. VI. Cosmological parameters.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Planck 2018 results. VI. Cosmological parameters
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.952271Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5e865e6d-a5f3-4342-b844-ec5aa68515e9 · outbound
This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.956110Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6e596033-01eb-46d9-b8a1-ba52b405e2fe · outbound
This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.960154Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 30e3c253-0b78-4ece-ad26-9ac7dde6e756 · outbound
This paper cites The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.964740Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8a505817-a1a8-4343-a580-fd058d06b50c · outbound
This paper cites 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.968222Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d4c56530-e84e-4f7c-b160-a204a96d7fdb · outbound
This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.971712Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8024d9ac-a7e5-4457-b06e-9509eadb4091 · outbound
This paper cites Challenges for $\Lambda$CDM: An update.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Challenges for $\Lambda$CDM: An update
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.975312Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 030372b4-44c6-4e61-a98f-6be57eef2c67 · outbound
This paper cites The trouble with $H_0$.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The trouble with $H_0$
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.979033Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7e8e2de9-0e5f-431d-bb9d-0da9ba25293e · outbound
This paper cites Tensions between the Early and the Late Universe.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Tensions between the Early and the Late Universe
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.982550Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a42b0b2e-be4b-4af5-b3a4-8b29863614a1 · outbound
This paper cites The Hubble Hunter's Guide.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Hubble Hunter's Guide
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.986019Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ba8a8f7-db16-4d05-a5dd-ce2bee06e784 · outbound
This paper cites The Expansion of the Universe is Faster than Expected.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Expansion of the Universe is Faster than Expected
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.989700Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4bdd5133-eef2-428f-a834-b5282015d324 · outbound
This paper cites Measurements of the Hubble Constant: Tensions in Perspective.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Measurements of the Hubble Constant: Tensions in Perspective
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.993350Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2cf4fa8-1a1e-4fcb-b3ec-b228e8b88d3e · outbound
This paper cites Cosmology Intertwined III: $f \sigma_8$ and $S_8$.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Cosmology Intertwined III: $f \sigma_8$ and $S_8$
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:25.996766Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 73744bb9-bf08-4f5c-84fa-6cfb89d8054e · outbound
This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.001256Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 01d3ee5d-3dfa-4c84-933a-f62892adb5f5 · outbound
This paper cites Evidence for suppression of structure growth in the concordance cosmological model.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Evidence for suppression of structure growth in the concordance cosmological model
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.004652Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 08444cd1-6712-499b-9337-9f29f79476bb · outbound
This paper cites First detection of the Hubble variation correlation and its scale dependence.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae First detection of the Hubble variation correlation and its scale dependence
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.007985Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d6862c3b-1eb2-43aa-ba25-3f67325fa260 · outbound
This paper cites The Dark Energy Survey.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Dark Energy Survey
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.011456Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8195ff67-385e-4598-829b-c9b5c0414cfe · outbound
This paper cites Supernova Simulations and Strategies For the Dark Energy Survey.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Supernova Simulations and Strategies For the Dark Energy Survey
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.015812Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3fb30bbd-0462-42c7-95b7-327468e53869 · outbound
This paper cites The Dark Energy Survey: more than dark energy - an overview.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Dark Energy Survey: more than dark energy - an overview
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.019208Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 432ffecb-396e-418f-848d-0a1ce1f76e11 · outbound
This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.023011Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a9664840-026c-4f1d-86c3-aad15ea44cb8 · outbound
This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.026689Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3e6c1f2e-e373-4589-936a-8367f6416889 · outbound
This paper cites DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.030728Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2f5dfdc-f60b-401f-ab6b-fb6ae7fe1aef · outbound
This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.034033Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b7f687b2-dbc2-4ef7-9dac-94eeb9dce537 · outbound
This paper cites The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.037594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8e4a4771-4237-4c66-98ca-c06fd3a0d96e · outbound
This paper cites DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.040912Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2011c885-27a4-4422-899f-a41ac0dd650f · outbound
This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.044202Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 926e3e81-b428-4e2b-8be3-cd8f0302bad9 · outbound
This paper cites Quintessential interpretation of the evolving dark energy in light of DESI.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Quintessential interpretation of the evolving dark energy in light of DESI
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.048335Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 154d47eb-d211-419e-b5e4-a81d0e957335 · outbound
This paper cites Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.053046Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 223d4a1c-6055-4ddb-8392-ae6837160e07 · outbound
This paper cites Assessing observational constraints on dark energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Assessing observational constraints on dark energy
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.057673Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3c03681f-77fd-445a-a8bb-66d55ec86559 · outbound
This paper cites DESI Constraints on Exponential Quintessence.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI Constraints on Exponential Quintessence
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.061628Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 592a8230-53c5-4c74-b0f0-682665c79f0d · outbound
This paper cites Cosmological constraints on curved quintessence.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Cosmological constraints on curved quintessence
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.065180Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8ac42b03-5561-4f83-b4b5-17e07998f0f0 · outbound
This paper cites Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.069386Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0e7f1f29-85bd-4587-86c4-e33d659ecf8b · outbound
This paper cites Reduced Hubble Tension in Dark Radiation Models after DESI 2024.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Reduced Hubble Tension in Dark Radiation Models after DESI 2024
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.072994Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc0f30f1-7025-4d9c-9331-c972960e7de6 · outbound
This paper cites DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.076923Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 55590b40-163a-467a-b458-f530dd270243 · outbound
This paper cites Quintom cosmology and modified gravity after DESI 2024.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Quintom cosmology and modified gravity after DESI 2024
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.080815Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0eab95e8-1900-4606-87eb-8dcf9e4aef75 · outbound
This paper cites $f(T)$ gravity after DESI Baryon Acoustic Oscillation and DES Supernovae 2024 data.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae $f(T)$ gravity after DESI Baryon Acoustic Oscillation and DES Supernovae 2024 data
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.084527Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 055c1961-4b7e-4b56-9f3b-57f2c3d1bf86 · outbound
This paper cites Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.087965Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b437240b-3a69-4717-8d34-7b8784841649 · outbound
This paper cites Dynamical dark energy in light of cosmic distance measurements I: a demonstration using simulated datasets.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Dynamical dark energy in light of cosmic distance measurements I: a demonstration using simulated datasets
Reference 41
- Resolution
- verified exact
- local_arxiv, observed 2026-08-08T23:12:27.363153Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 5ce85100-35ac-45a5-8a37-4d0dc385282b · outbound
This paper cites Dynamical dark energy in light of cosmic distance measurements II: a study using current observations.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-08-08T23:12:27.348889Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation a80af285-7250-4bf0-b6db-fa113cf80bac · outbound
This paper cites Interpreting DESI's evidence for evolving dark energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Interpreting DESI's evidence for evolving dark energy
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.098176Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fdf1ab36-a759-4897-80f7-9c8bd1c166ef · outbound
This paper cites Does DESI 2024 Confirm $\Lambda$CDM?.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Does DESI 2024 Confirm $\Lambda$CDM?
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.102448Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3b144e72-d954-43bd-b94b-2772bfaf0a9b · outbound
This paper cites Does dark energy really revive using DESI 2024 data?.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Does dark energy really revive using DESI 2024 data?
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.106013Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 98213401-6107-4104-9bf1-d317f7a4ff5b · outbound
This paper cites DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.109599Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 26f4dc72-df1f-4efa-856a-6128cd4d7a27 · outbound
This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.114074Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f39f5104-71c9-4f80-992e-ff2181df8ddd · outbound
This paper cites Model independent cosmographic constraints from DESI 2024.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Model independent cosmographic constraints from DESI 2024
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.117649Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6d18bf14-3da8-4ffe-9fbc-ddcd5ec0521d · outbound
This paper cites Model- independent cosmological inference post DESI DR1 BAO measurements,.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Model- independent cosmological inference post DESI DR1 BAO measurements,
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.121553Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e2061418-17e9-4473-833a-0bbadc40a159 · outbound
This paper cites A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.124757Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5bf2625e-8ca3-4401-8635-7f1e58243be7 · outbound
This paper cites The Dark Energy Survey Supernova Program: Investigating Beyond-$\Lambda$CDM.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Dark Energy Survey Supernova Program: Investigating Beyond-$\Lambda$CDM
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.128273Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b7fa834-9f64-4c0e-b2ab-aac483e2d638 · outbound
This paper cites Revisiting holographic dark energy after DESI 2024.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Revisiting holographic dark energy after DESI 2024
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.131843Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c960f933-572b-427e-bd98-0adb62a9e29f · outbound
This paper cites On the evidence of dynamical dark energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae On the evidence of dynamical dark energy
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.135286Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c324ca3c-4d0a-4e69-bee9-6d053801514c · outbound
This paper cites A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.138825Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 045d8f2a-1d28-4512-b686-f4ea3be5b3b4 · outbound
This paper cites Prob- ing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data,.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Prob- ing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data,
Reference 55
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.143211Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 69a12525-686c-4e59-9537-0b4318265e3b · outbound
This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.146533Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 33ca6360-e4c4-4211-9344-41152a6cce72 · 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.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae 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 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.149898Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e1a31702-4702-4524-b52d-873b6e61b826 · outbound
This paper cites The Pantheon+ Analysis: Cosmological Constraints.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Pantheon+ Analysis: Cosmological Constraints
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.153714Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bef6d92d-7ee7-4665-bfcc-8bf29d9272e2 · outbound
This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.157389Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7495864c-6667-4f78-8e66-8d1702f6d3da · outbound
This paper cites The Pantheon+ Analysis: SuperCal-Fragilistic Cross Calibration, Retrained SALT2 Light Curve Model, and Calibration Systematic Uncertainty.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Pantheon+ Analysis: SuperCal-Fragilistic Cross Calibration, Retrained SALT2 Light Curve Model, and Calibration Systematic Uncertainty
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.160864Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c2db4c9-acf8-4a68-860c-77383b2e57fd · outbound
This paper cites The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.164118Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df43478c-0739-4490-af3e-9a7059b90903 · outbound
This paper cites The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.167642Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 54b4c831-fd23-4bd6-ab30-1202d3e8878f · outbound
This paper cites The Pantheon+ Analysis: Forward-Modeling the Dust and Intrinsic Colour Distributions of Type Ia Supernovae, and Quantifying their Impact on Cosmological Inferences.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Pantheon+ Analysis: Forward-Modeling the Dust and Intrinsic Colour Distributions of Type Ia Supernovae, and Quantifying their Impact on Cosmological Inferences
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.171295Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fb5de902-a962-48a7-9d73-a899d93b99df · outbound
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?.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.174471Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fcf69485-f640-48c0-af2f-dad6b6c81b9b · outbound
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?.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.177828Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5c072c8-009a-45d1-b7a4-3a21122f67f7 · outbound
This paper cites Impact of LRG1 and LRG2 in DESI 2024 BAO data on dark energy evolution.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Impact of LRG1 and LRG2 in DESI 2024 BAO data on dark energy evolution
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.182115Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d744406d-ae2a-4104-a175-b643d8834c27 · outbound
This paper cites Implications of DES 5YR SNe Dataset for $\Lambda$CDM.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Implications of DES 5YR SNe Dataset for $\Lambda$CDM
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.185625Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47743180-6287-4f9f-a974-c6603a39bb86 · outbound
This paper cites DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?.
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 6afef57e-f725-46d9-8c40-24de84292f62 · outbound
This paper cites The role of LRG1 and LRG2's monopole in inferring the DESI 2024 BAO cosmology.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The role of LRG1 and LRG2's monopole in inferring the DESI 2024 BAO cosmology
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.192436Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d019e1fb-6651-4ded-9756-9f46efe8e655 · outbound
This paper cites Key drivers of the preference for dynamic dark energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Key drivers of the preference for dynamic dark energy
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.195708Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eda1940b-0d86-456e-b419-ad192dec3127 · outbound
This paper cites The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.200474Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7cb046ed-2b47-4f7d-a314-91ef0bb69f03 · outbound
This paper cites Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.204461Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d2963e63-707e-4452-b46a-aaac97e8f49c · outbound
This paper cites Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.207929Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e67c6e41-4f42-4546-9619-66c363dfec58 · outbound
This paper cites Evolving Dark Energy or Supernovae Systematics?.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Evolving Dark Energy or Supernovae Systematics?
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.211635Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6d53f37c-1098-438b-8a61-babcd83cfe17 · outbound
This paper cites BAO vs. SN evidence for evolving dark energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae BAO vs. SN evidence for evolving dark energy
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.215685Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a9ab532e-1f08-4006-a218-2d96d653e0bc · outbound
This paper cites Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.219182Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4e88a307-f0c8-4936-9937-e79ba91e3aaf · outbound
This paper cites Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on "Evolving Dark Energy or Supernovae systematics?".
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on "Evolving Dark Energy or Supernovae systematics?"
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.222665Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b49a0f5d-a5e1-4263-80da-a173413c127d · outbound
This paper cites The Carnegie Supernova Project I: Third Photometry Data Release of Low-Redshift Type Ia Supernovae and Other White Dwarf Explosions.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Carnegie Supernova Project I: Third Photometry Data Release of Low-Redshift Type Ia Supernovae and Other White Dwarf Explosions
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.225928Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 73fefc38-bdf8-4b0d-b72e-4756c85e1637 · outbound
This paper cites CfA3: 185 Type Ia Supernova Light Curves from the CfA.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae CfA3: 185 Type Ia Supernova Light Curves from the CfA
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.229494Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 545b53dc-0050-4ae1-adf4-8d3ac09bea1a · outbound
This paper cites CfA4: Light Curves for 94 Type Ia Supernovae.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae CfA4: Light Curves for 94 Type Ia Supernovae
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.232789Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e8aa698e-0e32-4089-bd06-c73d4b57f56e · outbound
This paper cites The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.236682Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e0bdb775-b6cb-41a0-b924-daa4e06470aa · outbound
This paper cites No-go guide for the Hubble tension: late-time or local-scale new physics.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae No-go guide for the Hubble tension: late-time or local-scale new physics
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.240232Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bf7686a6-d104-4552-a73f-d7c9ccc2ac32 · outbound
This paper cites Narrowing down the Hubble tension to the first two rungs of distance ladders.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Narrowing down the Hubble tension to the first two rungs of distance ladders
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.243555Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 25bff443-1d8d-47f6-8fc9-916924cd8a7b · outbound
This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.246879Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e7dcd73a-bd09-4aca-945d-54279a20e346 · outbound
This paper cites Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.250134Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6da8b4f1-cbe6-465c-8119-bb2d359e5c6f · outbound
This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.253494Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 00d72346-84d7-41ba-8fb7-7855918a25a0 · outbound
This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.257397Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e06a7b74-b793-48fa-80b0-e7f586f48065 · outbound
This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Extended Dark Energy analysis using DESI DR2 BAO measurements
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.260771Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 31658183-1333-40c8-bd69-c0f4f65175fb · outbound
This paper cites Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.264044Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 778d34a8-fdef-4bb7-acf0-05b57afd88bd · outbound
This paper cites Cosmological Evolution of a Quintom Model of Dark Energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Cosmological Evolution of a Quintom Model of Dark Energy
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.267568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 922ca0ce-dd5a-476e-a51a-05ffdd623536 · outbound
This paper cites Dark energy constraints from the cosmic age and super- nova,.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Dark energy constraints from the cosmic age and super- nova,
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.271072Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cd5353a6-bed2-4220-8c3d-64ae928fc6f1 · outbound
This paper cites Oscillating quintom and the recurrent uni- verse,.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Oscillating quintom and the recurrent uni- verse,
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.274678Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb48835a-c879-4d61-a2de-d01e1d1a6b95 · outbound
This paper cites Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.277928Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 360298b9-928e-41d9-af38-ccf82f38805c · outbound
This paper cites Non-minimally coupled gravity constraints from DESI DR2 data.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Non-minimally coupled gravity constraints from DESI DR2 data
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.281783Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3c0eaaab-8e70-4812-8a02-983902c76949 · outbound
This paper cites Assessing cosmological evidence for non-minimal coupling.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Assessing cosmological evidence for non-minimal coupling
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.285596Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8ba8679d-92ba-47af-b59b-172a76ac0572 · outbound
This paper cites Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.289395Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 163373ea-d6a7-457d-9970-037b778e4857 · outbound
This paper cites Matching current observational constraints with nonminimally coupled dark energy.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Matching current observational constraints with nonminimally coupled dark energy
Reference 97
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.293360Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0c036bd8-6b5d-4000-b8e8-d00cc123f2b7 · outbound
This paper cites Scant evidence for thawing quintessence.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Scant evidence for thawing quintessence
Reference 98
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.296866Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f97ff44d-177c-4d74-82db-9faa7da4d4a2 · outbound
This paper cites Chameleon dark energy can resolve the Hubble tension.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Chameleon dark energy can resolve the Hubble tension
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.300453Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ef86fef6-7cec-454b-ba27-47257d199c9c · outbound
This paper cites DESI results: Hint towards coupled dark matter and dark energy,.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae DESI results: Hint towards coupled dark matter and dark energy,
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.303970Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation 445a4a87-624c-46ce-9d68-77ce54cf518b · inbound
Robustness of dark energy phenomenology across different parameterizations cites this paper.
Robustness of dark energy phenomenology across different parameterizations The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T21:04:17.779578Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f8852ea6-447a-411d-b9d5-3091da5e01d8 · inbound
An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.
An overview of what current data can (and cannot yet) say about evolving dark energy The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 268
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T18:51:44.283531Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d8202962-1d19-413f-b05a-100d7248950f · inbound
The Quintom theory of dark energy after DESI DR2 cites this paper.
The Quintom theory of dark energy after DESI DR2 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 29
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T13:12:19.267389Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 2e0fb7c9-5a6f-4d64-9be1-ad9a7b613bd2 · inbound
Topological defects as effective dynamical dark energy cites this paper.
Topological defects as effective dynamical dark energy The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T04:41:33.543751Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c0f2a26b-8d2f-4cdb-b18a-51856afce11f · inbound
Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data cites this paper.
Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:36:59.471286Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9237c92e-8240-4eee-b615-256af3013964 · 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 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 36
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T05:22:06.323883Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 2ecadffc-23f3-46db-9b93-7bff9b840ab6 · inbound
Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.
Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:12:33.689414Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 57744f48-8d3c-447b-9136-4ae245300e17 · inbound
Revisiting cosmic acceleration with DESI BAO cites this paper.
Revisiting cosmic acceleration with DESI BAO The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T11:39:53.276298Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2fd1c9f4-b2be-4eec-956c-f1f2641b148f · inbound
Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints cites this paper.
Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 40
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T18:16:43.651730Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 44e4e4e1-c973-4dae-8fa7-91ad1f8ce86c · inbound
Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.
Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:43:12.226732Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 70c35886-05bb-46c5-8639-dec1c1d7f3bb · inbound
Crosschecking Cosmic Distances from DESI BAO and DES SNe cites this paper.
Crosschecking Cosmic Distances from DESI BAO and DES SNe The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 55
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T10:32:33.733026Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 0c231518-0685-4b6a-9ad7-231e805d03eb · inbound
Crosschecking Cosmic Distances from DESI BAO and DES SNe cites this paper.
Crosschecking Cosmic Distances from DESI BAO and DES SNe The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 55
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:34:12.869859Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b0265588-bbdf-4def-baaf-96333d6a9fa1 · 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 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 125
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T09:59:22.769194Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 856f41ef-ed6c-488d-b64d-6ab76b783046 · inbound
Modeling nonlinear scales for dynamical dark energy cosmologies with COLA cites this paper.
Modeling nonlinear scales for dynamical dark energy cosmologies with COLA The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T06:15:58.557461Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 0967bca4-967c-4872-b138-ffefed32722f · inbound
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T07:19:40.270534Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07740211-d852-464b-b784-4b1159124992 · inbound
Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.
Revisiting the Hubble tension problem in the framework of holographic dark energy The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 54
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T22:20:23.798078Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation d960720e-ca59-49b6-b511-2e203f5a6581 · inbound
Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.
Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 27
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T04:19:00.920329Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation b8466c79-980e-434b-abf6-38ca6c56517c · inbound
Cosmological tensions in Proca-Nuevo theory cites this paper.
Cosmological tensions in Proca-Nuevo theory The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T20:12:23.338390Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1c1afff0-988e-44c2-85a1-9196a484301e · 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 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 85
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T18:51:46.766290Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c9605df0-0871-4f7e-8ebc-2e8f7f1e764c · inbound
Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing cites this paper.
Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T08:17:35.788628Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation cca71284-e26b-46a6-ac69-2809d4fdbadf · inbound
Cosmic voids evolution in modified gravity via hydrodynamics cites this paper.
Cosmic voids evolution in modified gravity via hydrodynamics The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T22:16:52.733530Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1f838d2f-4f71-4bf2-aa64-6fd87870a24e · inbound
Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.
Measuring neutrino mass in light of ACT DR6 and DESI DR2 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 41
- Resolution
- verified exact
- arxiv_id, observed 2026-05-15T13:15:50.405465Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation b9d9cb6c-f512-48c7-8389-9759e346b147 · inbound
Non-minimally coupled quintessence with sign-switching interaction cites this paper.
Non-minimally coupled quintessence with sign-switching interaction The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 27
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-13T20:48:15.306591Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 46102c81-fa72-42dc-a04a-bf238462f462 · inbound
Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy cites this paper.
Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 40
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T09:11:06.200278Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 82a26c30-b283-4057-a80e-49647563d71a · inbound
Cosmological intercept tension cites this paper.
Cosmological intercept tension The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T10:26:30.655901Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 1171d055-7083-4366-a3ae-4790764b665a · inbound
A short review on Quintom dark energy theory cites this paper.
A short review on Quintom dark energy theory The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T21:46:16.136804Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 0638205c-2a92-4b46-8bd0-101d90042369 · inbound
A short review on Quintom dark energy theory cites this paper.
A short review on Quintom dark energy theory The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:40:03.192153Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ea20f16a-b098-4b00-8fc9-6af32b8d99c3 · inbound
Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.
Neutrino mass constraints in interacting dark energy models after DESI DR2 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T10:56:52.301532Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 4bfbb58f-64d4-48d7-838d-8e4ca29eea10 · 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 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 55
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T15:38:33.955667Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 3fad8716-c098-4783-a93e-c337925a4a8b · inbound
The Hubble tension: A decade review cites this paper.
The Hubble tension: A decade review The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 116
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T05:19:36.216372Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 6cb54a05-9714-42fa-8d31-f688a3a4ade2 · inbound
The Hubble tension: A decade review cites this paper.
The Hubble tension: A decade review The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 116
- Resolution
- unresolved
- no resolver link, observed 2026-07-15T10:41:50.733215Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 110b0434-add3-43d6-b9d7-98f73fea4e13 · 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 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 202
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T06:16:43.426365Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation f1f262c4-2a5a-4680-9795-3234fcf92244 · inbound
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 105
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T04:18:55.037825Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63e8dbb4-99bc-409b-88e4-1884362ef377 · inbound
Hubble tension: a short review of theoretical explanations cites this paper.
Hubble tension: a short review of theoretical explanations The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:20:07.676060Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 22d4d46d-e0b8-40a1-b223-7ff67a005150 · 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 The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T19:17:22.415775Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.