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Paper Citation Record · LEDGER

Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2105.13544.

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

pith.paper-citation-record.v1
2105.13544 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-07-22T06:31:00.163083+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-15T12:01:04.317365Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T01:39:23.542205Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8b167016-8808-4c03-ae7e-09ed378ca242 · inbound

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA cites this paper.

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 11

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verified exact
arxiv_id, observed 2026-05-18T06:15:58.350070Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

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Observation 408c3046-ae3b-440a-a550-efd536ac84b0 · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 53

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verified exact
arxiv_id, observed 2026-05-18T04:50:54.698025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

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Observation 6ef5d234-86c5-454b-a922-ee8e20e5d59e · inbound

Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI cites this paper.

Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 11

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verified exact
arxiv_id, observed 2026-05-17T06:29:10.042282Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

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Observation 06080f03-4eed-44dc-ab87-b7820d819de8 · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 37

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unresolved
no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:71e8958a2b85e5fe91cd438956e0e8836beba21e9a49e06ec8d6538d428850b3

Observation 8a2b3573-4030-4720-970a-bf7efcc1edd6 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 18

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verified exact
arxiv_id, observed 2026-05-11T11:36:01.921667Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

source=pdf_text observed=2026-05-10T14:10:57.749079Z digest=sha256:a8def7530ad01bd821c3d221241e5dafaa3e6d9d1393926111b6c2169f61f6dd

Observation f1421021-2449-4fb0-a003-3c1174a5d433 · inbound

Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts cites this paper.

Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 57

Resolution
malformed identifier
arxiv_id, observed 2026-05-10T05:46:09.960740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

source=pdf_text observed=2026-05-10T05:45:46.799115Z digest=sha256:f833b089a4e0373933e82856573d7e0447835401ba0b5058e5a6e4b42ded3c7d

Observation e7349b10-29cd-4eeb-b267-1b1455495aba · inbound

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback cites this paper.

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 4

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verified exact
arxiv_id, observed 2026-05-11T16:11:07.693768Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

source=pdf_text observed=2026-05-09T18:38:12.253954Z digest=sha256:9561ca27fb9d1f87df2585c26ad347b9d01a6cd0ad17fb44f2e952edc73ab6c8

Observation 16bbdbb0-593a-48ab-830e-22f921dbca9e · inbound

Density-Shear Baryon Acoustic Oscillation as a Cosmological Consistency Check cites this paper.

Density-Shear Baryon Acoustic Oscillation as a Cosmological Consistency Check Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 36

Resolution
verified exact
arxiv_id, observed 2026-05-13T01:52:05.908833Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

source=pdf_text observed=2026-05-13T01:10:38.364185Z digest=sha256:9e01a50b43b1c21317a3efab0275cfe7263aafacbd318b37bd30154424451d1b

Observation 4f941325-407d-4514-8d32-cf9fca144331 · inbound

Density-Shear Baryon Acoustic Oscillation as a Cosmological Consistency Check cites this paper.

Density-Shear Baryon Acoustic Oscillation as a Cosmological Consistency Check Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 36

Resolution
verified exact
arxiv_id, observed 2026-07-04T01:39:23.544980Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

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Observation 282bf514-48ec-4afe-8981-99918bbab744 · inbound

The sound of dynamical dark energy and modified gravity cites this paper.

The sound of dynamical dark energy and modified gravity Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 93

Resolution
verified exact
arxiv_id, observed 2026-06-28T20:52:37.736376Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

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Observation ff3789b2-9472-4721-a442-9bc243eda797 · inbound

AKRA 3.0: A matrix-free Inversion Framework for Weak Lensing Mass Mapping and Its Application to DES Y3 Data cites this paper.

AKRA 3.0: A matrix-free Inversion Framework for Weak Lensing Mass Mapping and Its Application to DES Y3 Data Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 17

Resolution
verified exact
arxiv_id, observed 2026-07-02T15:17:08.446373Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

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