Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-06-28T04:24:31.631297Z
Paper Citation Record · LEDGER
On the potential for inhomogeneities to mimic an evolving dark energy
As of 22 August 2026, this Paper Citation Record lists 68 of 68 outbound references and 1 inbound Pith citation observation for arXiv:2606.05479.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T09:39:53.309158Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
68 of 68 outbound references displayed
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- unresolved7
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 4b51876d-b169-467c-982e-6b35a66bd31c · outbound
This paper cites 5 We use a continuous fluid approximation for dark matter and thus only sample scales above bound objects; see e.g.
On the potential for inhomogeneities to mimic an evolving dark energy 5 We use a continuous fluid approximation for dark matter and thus only sample scales above bound objects; see e.g
Reference 1
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Observation 60805d3b-ec4f-4131-99f2-389be9f8db77 · outbound
This paper cites an unresolved cited work.
On the potential for inhomogeneities to mimic an evolving dark energy Unresolved cited work
Reference 2
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Observation a11ff784-ecbe-4364-80b1-87a42615100f · outbound
This paper cites Is the Observable Universe Consistent with the Cosmological Principle?.
On the potential for inhomogeneities to mimic an evolving dark energy Is the Observable Universe Consistent with the Cosmological Principle?
Reference 3
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Observation 4f5f7e41-2dec-4dd4-b85c-e9aa8a5d8be9 · outbound
This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.
On the potential for inhomogeneities to mimic an evolving dark energy Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
Reference 4
- Resolution
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Source-reported events for the cited work
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Observation 7b214435-82e2-4e00-9a6a-03f97685a49e · outbound
This paper cites Challenges for $\Lambda$CDM: An update.
On the potential for inhomogeneities to mimic an evolving dark energy Challenges for $\Lambda$CDM: An update
Reference 5
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Observation 92a1a798-d9d9-4024-bfe8-1a7d46965e85 · outbound
This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.
On the potential for inhomogeneities to mimic an evolving dark energy DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
Reference 6
- Resolution
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Observation 5b00b152-a364-4015-8bd7-6ccf4ab46eda · outbound
This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.
On the potential for inhomogeneities to mimic an evolving dark energy Extended Dark Energy analysis using DESI DR2 BAO measurements
Reference 7
- Resolution
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Source-reported events for the cited work
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Observation a3cc7898-5135-42e9-9ec8-2c2288f0fe62 · outbound
This paper cites Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data.
On the potential for inhomogeneities to mimic an evolving dark energy Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data
Reference 8
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation 12af7e0f-7928-4f85-8820-45b08786fdc6 · outbound
This paper cites The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters.
On the potential for inhomogeneities to mimic an evolving dark energy The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
Reference 10
- Resolution
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Source-reported events for the cited work
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Observation 5e1b35f8-96fe-43f3-9b0a-2d3f1361df5a · outbound
This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.
On the potential for inhomogeneities to mimic an evolving dark energy The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
Reference 11
- Resolution
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Source-reported events for the cited work
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Observation 11da6f81-255f-40dc-af4c-cfed90a66f1a · outbound
This paper cites The Pantheon+ Analysis: Cosmological Constraints.
On the potential for inhomogeneities to mimic an evolving dark energy The Pantheon+ Analysis: Cosmological Constraints
Reference 12
- Resolution
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Source-reported events for the cited work
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Observation 009a66f7-142f-433c-81b2-fc93197ced6b · outbound
This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.
On the potential for inhomogeneities to mimic an evolving dark energy Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
Reference 13
- Resolution
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Source-reported events for the cited work
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Observation 53882fa9-74ad-4c4c-93ec-8b481515deca · outbound
This paper cites Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey.
On the potential for inhomogeneities to mimic an evolving dark energy Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey
Reference 15
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation d49dec03-0a21-471a-b59e-9cdd9b79f78b · outbound
This paper cites A Reassessment of the Pantheon+ and DES 5YR Calibration Uncertainties: Dovekie.
On the potential for inhomogeneities to mimic an evolving dark energy A Reassessment of the Pantheon+ and DES 5YR Calibration Uncertainties: Dovekie
Reference 16
- Resolution
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Source-reported events for the cited work
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Observation 22d25bc0-3214-4c00-a565-ea5a10bf95fb · outbound
This paper cites An overview of what current data can (and cannot yet) say about evolving dark energy.
On the potential for inhomogeneities to mimic an evolving dark energy An overview of what current data can (and cannot yet) say about evolving dark energy
Reference 17
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation fa1ed6b4-3596-4118-9b17-e6bbebeeb5c4 · outbound
This paper cites Capozziello, H.
On the potential for inhomogeneities to mimic an evolving dark energy Capozziello, H
Reference 18
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation 427d9cc8-b195-4cc0-b5a1-f9d7f14c9499 · outbound
This paper cites Khoury, M.-X.
On the potential for inhomogeneities to mimic an evolving dark energy Khoury, M.-X
Reference 19
- Resolution
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Source-reported events for the cited work
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Observation e508c977-23f7-4324-ac8e-782f096f8e16 · outbound
This paper cites Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO.
On the potential for inhomogeneities to mimic an evolving dark energy Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO
Reference 20
- Resolution
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Source-reported events for the cited work
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Observation 3cfdfd84-f35d-426e-8cc6-99728c14e0e6 · outbound
This paper cites Non-minimally coupled gravity constraints from DESI DR2 data.
On the potential for inhomogeneities to mimic an evolving dark energy Non-minimally coupled gravity constraints from DESI DR2 data
Reference 21
- Resolution
- verified exact
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Observation f4f80639-0145-4d86-be43-261046b28367 · outbound
This paper cites Scalar field dark energy models: Current and forecast constraints.
On the potential for inhomogeneities to mimic an evolving dark energy Scalar field dark energy models: Current and forecast constraints
Reference 22
- Resolution
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Observation 7beec8c9-5fef-4891-a611-c8184b9472a7 · outbound
This paper cites Ishak et al., (2024).
On the potential for inhomogeneities to mimic an evolving dark energy Ishak et al., (2024)
Reference 23
- Resolution
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Source-reported events for the cited work
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Observation 8d6082ce-5dd8-4d4f-87be-a4f0a5327633 · outbound
This paper cites Evolving Dark Sector and the Dark Dimension Scenario.
On the potential for inhomogeneities to mimic an evolving dark energy Evolving Dark Sector and the Dark Dimension Scenario
Reference 24
- Resolution
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Source-reported events for the cited work
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Observation 81e149bf-2482-4ee4-afa3-868bbcadfa3c · outbound
This paper cites It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2.
On the potential for inhomogeneities to mimic an evolving dark energy It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2
Reference 25
- Resolution
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Source-reported events for the cited work
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Observation a998691e-a2e1-4013-80cd-a29033de3961 · outbound
This paper cites Fern´ andez-Garc´ ıa, R.
On the potential for inhomogeneities to mimic an evolving dark energy Fern´ andez-Garc´ ıa, R
Reference 26
- Resolution
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Source-reported events for the cited work
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Observation cee2f3fc-38fa-4bdb-b9d7-5d382f475bb6 · outbound
This paper cites Sailer, G.
On the potential for inhomogeneities to mimic an evolving dark energy Sailer, G
Reference 27
- Resolution
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Source-reported events for the cited work
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Observation 10fd65b0-ea5a-405a-bca1-58539553fe82 · outbound
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On the potential for inhomogeneities to mimic an evolving dark energy Unresolved cited work
Reference 28
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Observation 5883033c-851e-49a4-bee3-cb1425b2ae16 · outbound
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On the potential for inhomogeneities to mimic an evolving dark energy Unresolved cited work
Reference 29
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Observation fd0cf6d5-ca80-4ab9-8d09-cfcb6f1947d0 · outbound
This paper cites Futamase, Approximation scheme for constructing a clumpy universe in general relativity, Phys.
On the potential for inhomogeneities to mimic an evolving dark energy Futamase, Approximation scheme for constructing a clumpy universe in general relativity, Phys
Reference 30
- Resolution
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Source-reported events for the cited work
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Observation be2c9e43-a981-40df-a0f1-0e5fb209ac53 · outbound
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On the potential for inhomogeneities to mimic an evolving dark energy Unresolved cited work
Reference 31
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Observation 2ea04773-01ef-4a73-a24a-c0fac3cd41f1 · outbound
This paper cites Dark Energy from structure: a status report.
On the potential for inhomogeneities to mimic an evolving dark energy Dark Energy from structure: a status report
Reference 32
- Resolution
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Observation acbd01b8-0d15-4be1-804b-082aeddc3961 · outbound
This paper cites Backreaction in late-time cosmology.
On the potential for inhomogeneities to mimic an evolving dark energy Backreaction in late-time cosmology
Reference 33
- Resolution
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Source-reported events for the cited work
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Observation 96968fea-fc2b-4a3f-a832-aabb5b0186b8 · outbound
This paper cites A Complete Treatment of CMB Anisotropies in a FRW Universe.
On the potential for inhomogeneities to mimic an evolving dark energy A Complete Treatment of CMB Anisotropies in a FRW Universe
Reference 34
- Resolution
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Source-reported events for the cited work
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Observation 20020dcc-cab6-4081-8c28-d2c87b39450c · outbound
This paper cites Fluctuations of the luminosity distance.
On the potential for inhomogeneities to mimic an evolving dark energy Fluctuations of the luminosity distance
Reference 35
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation 8676d666-98c1-4bb4-b5bd-5e5d6ff548ec · outbound
This paper cites Correlated Fluctuations in Luminosity Distance and the (Surprising) Importance of Peculiar Motion in Supernova Surveys.
On the potential for inhomogeneities to mimic an evolving dark energy Correlated Fluctuations in Luminosity Distance and the (Surprising) Importance of Peculiar Motion in Supernova Surveys
Reference 36
- Resolution
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Observation 54830033-7167-417e-b94e-b10c71d99c17 · outbound
This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.
On the potential for inhomogeneities to mimic an evolving dark energy Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
Reference 37
- Resolution
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Source-reported events for the cited work
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Observation 1db5da74-fc8b-4daa-ba69-e8367d21b8fa · outbound
This paper cites KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey.
On the potential for inhomogeneities to mimic an evolving dark energy KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey
Reference 38
- Resolution
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Observation 1944f5e7-fa44-45eb-8aa6-ee5abfa6150b · outbound
This paper cites Joint analysis of 6dFGS and SDSS peculiar velocities for the growth rate of cosmic structure and tests of gravity.
On the potential for inhomogeneities to mimic an evolving dark energy Joint analysis of 6dFGS and SDSS peculiar velocities for the growth rate of cosmic structure and tests of gravity
Reference 39
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 5261a9ad-e020-4d8a-be08-5a6779880add · outbound
This paper cites Cosmological Parameters from the Comparison of the 2MASS Gravity Field with Peculiar Velocity Surveys.
On the potential for inhomogeneities to mimic an evolving dark energy Cosmological Parameters from the Comparison of the 2MASS Gravity Field with Peculiar Velocity Surveys
Reference 40
- Resolution
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Source-reported events for the cited work
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Observation 3f6dc7e6-8855-40e0-9eb7-317db211aca1 · outbound
This paper cites an unresolved cited work.
On the potential for inhomogeneities to mimic an evolving dark energy Unresolved cited work
Reference 41
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation b92548a4-0705-4674-b67d-1474bbcfd3d6 · outbound
This paper cites On the Bias of the Distance-Redshift Relation from Gravitational Lensing.
On the potential for inhomogeneities to mimic an evolving dark energy On the Bias of the Distance-Redshift Relation from Gravitational Lensing
Reference 42
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation b74ae956-6e64-4ba0-9d87-5a1344653733 · outbound
This paper cites Hubble Diagram Dispersion From Large-Scale Structure.
On the potential for inhomogeneities to mimic an evolving dark energy Hubble Diagram Dispersion From Large-Scale Structure
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.226459Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 54784e97-1cd5-4e78-935f-ff36c70aa449 · outbound
This paper cites Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe.
On the potential for inhomogeneities to mimic an evolving dark energy Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
Reference 44
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.249473Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 2670dad7-6d38-4d08-8c0c-66b448cf9a91 · outbound
This paper cites Interpretation of the Hubble diagram in a nonhomogeneous universe.
On the potential for inhomogeneities to mimic an evolving dark energy Interpretation of the Hubble diagram in a nonhomogeneous universe
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.246477Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation d1e12258-063e-4037-bfed-9d6a8288c387 · outbound
This paper cites Ginat and P.G.
On the potential for inhomogeneities to mimic an evolving dark energy Ginat and P.G
Reference 46
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 8f75316b-9cf0-4261-9feb-296aa7303932 · outbound
This paper cites Camarena, K.
On the potential for inhomogeneities to mimic an evolving dark energy Camarena, K
Reference 47
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 0e81cb9a-4fca-4b1a-bb43-9677c91424b6 · outbound
This paper cites Efficient Computation of CMB anisotropies in closed FRW models.
On the potential for inhomogeneities to mimic an evolving dark energy Efficient Computation of CMB anisotropies in closed FRW models
Reference 48
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.292437Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 1d7ca7f8-727b-411a-beb7-bac7852e8cfb · outbound
This paper cites General Relativistic Corrections to the Weak Lensing Convergence Power Spectrum.
On the potential for inhomogeneities to mimic an evolving dark energy General Relativistic Corrections to the Weak Lensing Convergence Power Spectrum
Reference 49
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.237754Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 0a6fe957-c95f-47ca-bcce-6234db9a5c73 · outbound
This paper cites Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions.
On the potential for inhomogeneities to mimic an evolving dark energy Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions
Reference 50
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.262176Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation d8f4a904-941d-4637-84d0-d8ec1bd7b6c6 · outbound
This paper cites arXiv e-prints , keywords =.
On the potential for inhomogeneities to mimic an evolving dark energy arXiv e-prints , keywords =
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.229808Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation ad098cec-1fd2-4973-a310-1754b1fb234f · outbound
This paper cites HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere.
On the potential for inhomogeneities to mimic an evolving dark energy HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.143407Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 1604e91a-40a8-4fc1-a141-3ee0d413438b · outbound
This paper cites Einstein's Universe: Cosmological structure formation in numerical relativity.
On the potential for inhomogeneities to mimic an evolving dark energy Einstein's Universe: Cosmological structure formation in numerical relativity
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.308991Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation fadc6504-f49d-4802-8116-e3ac8d7410f4 · outbound
This paper cites The trouble with Hubble: Local versus global expansion rates in inhomogeneous cosmological simulations with numerical relativity.
On the potential for inhomogeneities to mimic an evolving dark energy The trouble with Hubble: Local versus global expansion rates in inhomogeneous cosmological simulations with numerical relativity
Reference 54
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.269184Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation b3060ee6-e023-46f3-8466-6cc79aa95011 · outbound
This paper cites Theoretical and numerical perspectives on cosmic distance averages.
On the potential for inhomogeneities to mimic an evolving dark energy Theoretical and numerical perspectives on cosmic distance averages
Reference 55
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.283100Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation a3179dfe-4b5e-4b7c-808b-1cafe326d620 · outbound
This paper cites an unresolved cited work.
On the potential for inhomogeneities to mimic an evolving dark energy Unresolved cited work
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-06-28T04:24:31.631297Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2ee1a5bf-ff44-47a2-9b70-27e7cd83b9a4 · outbound
This paper cites Data Release 1 of the Dark Energy Spectroscopic Instrument.
On the potential for inhomogeneities to mimic an evolving dark energy Data Release 1 of the Dark Energy Spectroscopic Instrument
Reference 57
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.275256Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation cc38689b-7f33-42ea-97bc-a1e99a71af07 · 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.
On the potential for inhomogeneities to mimic an evolving dark energy 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 58
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.287137Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 375341c4-dc29-4513-9611-31afd73da149 · outbound
This paper cites Accelerating Universes with Scaling Dark Matter.
On the potential for inhomogeneities to mimic an evolving dark energy Accelerating Universes with Scaling Dark Matter
Reference 59
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.200617Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 8314eeed-e6a6-4bae-a29f-c6badfb6b7d8 · outbound
This paper cites Exploring the Expansion History of the Universe.
On the potential for inhomogeneities to mimic an evolving dark energy Exploring the Expansion History of the Universe
Reference 60
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.163446Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 7aeb6805-bd4b-490c-a365-158f981b8d2a · outbound
This paper cites Planck 2018 results. VI. Cosmological parameters.
On the potential for inhomogeneities to mimic an evolving dark energy Planck 2018 results. VI. Cosmological parameters
Reference 61
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.150998Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 955cc846-ee0a-4aeb-b59a-48f5897067d0 · outbound
This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.
On the potential for inhomogeneities to mimic an evolving dark energy The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.241373Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 74502af4-db1a-43ee-82a2-89c0fe50a4a2 · outbound
This paper cites The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae.
On the potential for inhomogeneities to mimic an evolving dark energy The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
Reference 63
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.228522Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation f0861c0f-833a-4215-9f14-2078bc8ffa02 · outbound
This paper cites The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses.
On the potential for inhomogeneities to mimic an evolving dark energy The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses
Reference 64
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.288434Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 7bff1b56-9d86-4c2f-9a0d-dc6363594f00 · outbound
This paper cites The effect of peculiar velocities on supernova cosmology.
On the potential for inhomogeneities to mimic an evolving dark energy The effect of peculiar velocities on supernova cosmology
Reference 65
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.156615Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 0a7681b6-1dfd-4111-834b-35924dbc31b2 · outbound
This paper cites The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology.
On the potential for inhomogeneities to mimic an evolving dark energy The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology
Reference 66
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.305212Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 6f35e3e5-9c22-41e5-86ed-586a434f2fbb · outbound
This paper cites Bulk flows in the local Universe and the importance of relativistic effects.
On the potential for inhomogeneities to mimic an evolving dark energy Bulk flows in the local Universe and the importance of relativistic effects
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.262830Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation a245b5ad-d3f2-4422-b1a2-b6f53e3c1901 · outbound
This paper cites Multipole decomposition of the general luminosity distance 'Hubble law' -- a new framework for observational cosmology.
On the potential for inhomogeneities to mimic an evolving dark energy Multipole decomposition of the general luminosity distance 'Hubble law' -- a new framework for observational cosmology
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.283863Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation d6ef8f48-7b38-4465-b21a-5e2eedfc6174 · outbound
This paper cites How does the cosmic large-scale structure bias the Hubble diagram?.
On the potential for inhomogeneities to mimic an evolving dark energy How does the cosmic large-scale structure bias the Hubble diagram?
Reference 69
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T11:16:53.149145Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 091884a5-b83a-4a2a-a357-1f3546da951f · outbound
This paper cites Inhomogeneous Cosmology using General Relativistic Smoothed Particle Hydrodynamics coupled to Numerical Relativity.
On the potential for inhomogeneities to mimic an evolving dark energy Inhomogeneous Cosmology using General Relativistic Smoothed Particle Hydrodynamics coupled to Numerical Relativity
Reference 70
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T11:16:53.279279Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Pith citing papers
Observation 9aab456f-c8e3-493f-8ee6-78a690f5bd08 · inbound
Evolving Dark Energy from the Back-Reaction of Cosmological Perturbations cites this paper.
Evolving Dark Energy from the Back-Reaction of Cosmological Perturbations On the potential for inhomogeneities to mimic an evolving dark energy
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:39:53.309158Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.