Paper Citation Record · LEDGER

Cosmological parameter inference with Bayesian statistics

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1903.11127.

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

pith.paper-citation-record.v1
1903.11127 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T12:01:08.840716Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T14:27:03.406182Z

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 04104296-a65e-464f-8131-141ef742044c · inbound

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach cites this paper.

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach Cosmological parameter inference with Bayesian statistics

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-06T12:01:08.840716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6813a7d6-2072-43c1-825f-3c0d9c2cdafc · 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 Cosmological parameter inference with Bayesian statistics

Reference 249

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 725559dc-6bcc-4a35-b3e0-9b12ec41a1ef · inbound

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations cites this paper.

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations Cosmological parameter inference with Bayesian statistics

Reference 159

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:27:03.407651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7e8438e2-b0dc-4012-a325-0ab06f463a2e · inbound

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime cites this paper.

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime Cosmological parameter inference with Bayesian statistics

Reference 144

Resolution: unresolved; no resolver link, observed 2026-08-04T12:59:05.787293Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.