Paper Citation Record · LEDGER

Constraining Early Dark Energy with Large-Scale Structure

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 24 inbound Pith citation observations for arXiv:2006.11235.

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

pith.paper-citation-record.v1
2006.11235 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 24 of 24 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 24 of 24 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T11:45:58.370689Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T05:19:36.123766Z

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 d3716251-7eca-4108-ba61-3ae9644409bc · inbound

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

In the Realm of the Hubble tension $-$ a Review of Solutions Constraining Early Dark Energy with Large-Scale Structure

Reference 102

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:50:21.111610Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e60db5e3-6068-476c-90ba-893b2cadbff4 · inbound

The Hubble Tension and Early Dark Energy cites this paper.

The Hubble Tension and Early Dark Energy Constraining Early Dark Energy with Large-Scale Structure

Reference 141

Resolution: verified exact; arxiv_id, observed 2026-05-17T23:41:11.260551Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 038defcc-686c-40d0-9155-342ea964014d · inbound

Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure cites this paper.

Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure Constraining Early Dark Energy with Large-Scale Structure

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-09T11:45:58.370689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75da2591-3238-4c94-b136-26f2868de7ef · inbound

$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum cites this paper.

$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum Constraining Early Dark Energy with Large-Scale Structure

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T20:33:58.122303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ab3735e-fd72-4d3e-9630-5d5b09789a40 · inbound

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

Can the universe experience an AdS landscape since matter-radiation equality? Constraining Early Dark Energy with Large-Scale Structure

Reference 128

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.707890Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ee0b670-4b72-4528-9c04-e3036eef26df · inbound

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Early Dark Energy with Large-Scale Structure

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T21:30:54.963624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95d2311c-c72c-482b-b9f4-e456ceda2a75 · inbound

The BAO-CMB Tension and Implications for Inflation cites this paper.

The BAO-CMB Tension and Implications for Inflation Constraining Early Dark Energy with Large-Scale Structure

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-06T16:53:14.203967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc175f8d-8bbb-491a-ad57-5b30b53babc0 · 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 Constraining Early Dark Energy with Large-Scale Structure

Reference 74

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.583503Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 0123b5dd-2418-413b-a9e8-0a0e10d05c5e · inbound

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Constraining Early Dark Energy with Large-Scale Structure

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-03T08:41:57.962163Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa4217f4-934d-4bc5-b7b8-405ec25a36de · inbound

Hubble Tension as an Effect of Horizon Entanglement Nonequilibrium cites this paper.

Hubble Tension as an Effect of Horizon Entanglement Nonequilibrium Constraining Early Dark Energy with Large-Scale Structure

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-03T08:14:18.396253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 038d6ee0-d386-44af-bdde-12679a848f22 · inbound

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework cites this paper.

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework Constraining Early Dark Energy with Large-Scale Structure

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.610920Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b0dc7c98-05da-4ed7-8596-94ed5b720c70 · inbound

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors cites this paper.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Constraining Early Dark Energy with Large-Scale Structure

Reference 116

Resolution: unresolved; no resolver link, observed 2026-08-02T22:01:26.452054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9c8d1b41-811d-4c2e-913e-8ff6dfaadfb4 · 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 Constraining Early Dark Energy with Large-Scale Structure

Reference 50

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e105be8c-1e08-4866-bb1a-2511547335ba · inbound

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension cites this paper.

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension Constraining Early Dark Energy with Large-Scale Structure

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-11T12:11:05.488542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f16380f3-1150-416e-9907-729669057d2c · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Constraining Early Dark Energy with Large-Scale Structure

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:21:26.619693Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 03f8560c-46ba-4919-b593-039cb82d4ac6 · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Constraining Early Dark Energy with Large-Scale Structure

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-11T22:01:13.954593Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation ba77c804-f97b-4c57-a917-0f361d138a5c · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Constraining Early Dark Energy with Large-Scale Structure

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.348186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 8cb56323-6d04-4729-b1eb-fa2871737fd6 · inbound

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

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Constraining Early Dark Energy with Large-Scale Structure

Reference 66

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:19:23.582622Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 2521b701-dd63-46a6-b6e3-2569cb79fff9 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Constraining Early Dark Energy with Large-Scale Structure

Reference 290

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:19:36.125498Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation d7ea2c1d-9a0e-482a-a0c4-039874d13885 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Constraining Early Dark Energy with Large-Scale Structure

Reference 290

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 b42c5f15-9657-4880-8cd5-a2dac290e5c0 · inbound

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics cites this paper.

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics Constraining Early Dark Energy with Large-Scale Structure

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-07-01T12:25:44.432527Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1dbc8600-a4bd-429e-9e4c-dd72fc19fef0 · inbound

The $H_0$ World Cup. I. Summary of the baseline group stage results cites this paper.

The $H_0$ World Cup. I. Summary of the baseline group stage results Constraining Early Dark Energy with Large-Scale Structure

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-02T05:41:37.309148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb5fa631-6705-4a31-a49a-49262406c40a · inbound

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions Constraining Early Dark Energy with Large-Scale Structure

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:10.972335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 425cc9bb-eb3d-4d37-b6ac-4e4791bd7e0e · inbound

Hubble tension: a short review of theoretical explanations cites this paper.

Hubble tension: a short review of theoretical explanations Constraining Early Dark Energy with Large-Scale Structure

Reference 161

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:07.996057Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.