Pith. sign in

Paper Citation Record · LEDGER

Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2012.08568.

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

pith.paper-citation-record.v1
2012.08568 v3

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 2026-08-18T06:34:40.430872+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:38:39.812211Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T03:14:31.333466Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 c9953a66-76ec-4cdf-adf3-1f71123c3dc3 · inbound

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

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 131

Resolution
verified exact
arxiv_id, observed 2026-05-19T09:35:12.667882Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-19T09:35:12.156800Z digest=sha256:59ea03154dca398948ae5339827a8a4c7f6e6e4a8abef565f1287e0309a8e20c

Observation aba8f523-78f7-4bc2-833c-eed125d5df0b · inbound

Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing cites this paper.

Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-11T18:38:39.812211Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T18:38:39.812211Z digest=sha256:ab2abc23916bfde7870ab1828a8746cbd8675e7a7a301331a465a580c54dad91

Observation 9efe453c-defc-46f2-8eed-49aadf30686c · inbound

Pixelization effects in cosmic shear angular power spectra cites this paper.

Pixelization effects in cosmic shear angular power spectra Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T20:26:55.014631Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T20:26:55.014631Z digest=sha256:8ebbcdf22e1af3667e1e9456accd6504d002b8144e4495e83e24875413d9ff56

Observation 701a7823-aa76-45cf-b747-584b8cb24d81 · 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: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-18T06:15:58.407493Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-18T06:13:13.345307Z digest=sha256:605c50e5b11bb2dfa02b74d2d3c7c20852c4e6eb06f47f9d5a817f80e4692a75

Observation 7153bfc7-c45f-4129-9e0d-139627051ac4 · 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: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 54

Resolution
metadata mismatch
arxiv_id, observed 2026-05-13T01:52:05.955449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-13T01:10:38.364185Z digest=sha256:44c40804e5f100094603d243070584d66936b6cde4e0dd57eaf8d2283ae4dad7

Observation 51b49a2d-d231-42ca-a6bc-d3203bc185c7 · 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: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 54

Resolution
metadata mismatch
arxiv_id, observed 2026-07-04T01:39:23.718834Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-07-04T01:35:31.698704Z digest=sha256:5a150f9a734e150857e30b69c8bb065ef663ded640f8cc77b26290149bd21367

Observation efc0f764-49c1-4990-8c7c-5b49a9c9cefb · inbound

Analytical method for computing the covariance matrix of cosmic shear two-point correlation function cites this paper.

Analytical method for computing the covariance matrix of cosmic shear two-point correlation function Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 14

Resolution
verified exact
arxiv_id, observed 2026-05-20T16:13:34.463911Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-20T16:10:04.825506Z digest=sha256:a1c010a79d60bd4e490c4b42196d4bd81cd868388f7f4866c7f08e9129781b40

Observation 82e02014-cbd8-47b3-b994-51278a9e41a5 · inbound

Complex yet Hermitian: Gaussian covariance of cross-correlation and multi-tracer power spectra cites this paper.

Complex yet Hermitian: Gaussian covariance of cross-correlation and multi-tracer power spectra Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-07-03T13:08:08.997726Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-27T08:24:36.251007Z digest=sha256:7510140744f8151d22879472592df66ce7a43eec8574004ae5cc3a65b3662e8f

Observation 37857d07-1160-455c-915a-36b650fdaab5 · inbound

One with HI: Modelling HI Intensity Mapping one-point statistics including systematics cites this paper.

One with HI: Modelling HI Intensity Mapping one-point statistics including systematics Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-07-08T03:14:31.334809Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:36ed1effe7d7e48f5d648f4daa65130da435fe2e6a4fcf1c524f18b166bcdc34

Observation e56d8fb3-ae21-4575-a73d-a0740b1e8433 · inbound

Analytical covariances for catalogue-based pseudo-$C_\ell$s cites this paper.

Analytical covariances for catalogue-based pseudo-$C_\ell$s Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-02T00:58:36.386469Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T00:58:36.386469Z digest=sha256:0bb56b33fecb5b79156af92cbc709fce2f893fd66ba28c129571aed8a25de276

Observation 0a14239b-169e-4e0f-86ca-9e5b7cb9b6c9 · inbound

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

Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit

Reference 9

Resolution
unresolved
no resolver link, observed 2026-07-31T11:14:46.751838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T11:14:46.751838Z digest=sha256:ec3b5e30ad6073f731eb0123621e7b6d683eb2e3ea307bab49c091bec477d85b