Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A semi-cosmographic approach to study cosmological evolution in phase space
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2503.03288.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T22:23:09.642138Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T14:19:54.195564Z
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 554c7038-4224-4c46-9346-fb7371dc03a8 · inbound
Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys cites this paper.
Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys A semi-cosmographic approach to study cosmological evolution in phase space
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:23:09.642138Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 57ac68d6-1be3-4ab7-ae23-ed069c81009a · inbound
Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy cites this paper.
Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy A semi-cosmographic approach to study cosmological evolution in phase space
Reference 34
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T14:19:54.197126Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.