Paper Citation Record · LEDGER

Evolution of dark energy reconstructed from the latest observations

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:1807.03772.

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

pith.paper-citation-record.v1
1807.03772 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T02:14:28.102833Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

125
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 29833fc2-bd30-445f-a6ff-8e2bef5182d6 · 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 Evolution of dark energy reconstructed from the latest observations

Reference 137

Resolution: verified exact; local_arxiv, observed 2026-05-15T11:50:21.257589Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation d84376ad-d54f-4859-ab50-6d40b4488b10 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Evolution of dark energy reconstructed from the latest observations

Reference 97

Resolution: verified exact; local_arxiv, observed 2026-05-24T03:53:54.833355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation c9acba76-a1f8-43a3-a56f-f1081dbab4b7 · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 Evolution of dark energy reconstructed from the latest observations

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-05-19T13:12:18.826615Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7835ce99-5074-4adf-8ebb-177c34f4e593 · inbound

Evidence for evolving dark energy from DESI DR2 BAO and Pantheon$^+$, DES-Dovekie, and Union3 cites this paper.

Evidence for evolving dark energy from DESI DR2 BAO and Pantheon$^+$, DES-Dovekie, and Union3 Evolution of dark energy reconstructed from the latest observations

Reference 97

Resolution: verified exact; local_arxiv, observed 2026-05-25T07:50:28.668733Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation f82253a3-d16c-4c79-b9da-09213792fabb · 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 Evolution of dark energy reconstructed from the latest observations

Reference 149

Resolution: verified exact; local_arxiv, observed 2026-05-18T04:50:55.103994Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 815c8c18-c4d0-456f-a13c-b8f1e54b7fcc · 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 Evolution of dark energy reconstructed from the latest observations

Reference 104

Resolution: verified exact; local_arxiv, observed 2026-05-21T13:30:12.244936Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation ae71541b-90dd-45b2-978e-b1149f063d2b · 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 Evolution of dark energy reconstructed from the latest observations

Reference 114

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 01b05168-dd17-4455-8e8d-1fd138ca15d4 · 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? Evolution of dark energy reconstructed from the latest observations

Reference 90

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:20:31.070106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 642ab887-a304-411a-b5e0-6a2a1d64a437 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Evolution of dark energy reconstructed from the latest observations

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:03:55.475043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation aa52e48b-4405-494b-8461-13b16a57a81a · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Evolution of dark energy reconstructed from the latest observations

Reference 92

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1851dadd-d694-49e6-a973-5540e49df5d5 · inbound

Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey cites this paper.

Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey Evolution of dark energy reconstructed from the latest observations

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-07-09T13:46:17.337342Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 78527f92-05a3-4625-8543-1d1bf5a1e1ef · inbound

No preference for generalized emergent dark energy from current cosmological data cites this paper.

No preference for generalized emergent dark energy from current cosmological data Evolution of dark energy reconstructed from the latest observations

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T02:14:28.102833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.