Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Cosmological structure formation in a homogeneous dark energy background
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0508156.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T14:43:16.579694Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-29T03:13:04.110227Z
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 e41bfba6-25e8-4384-8f74-4a691d2becae · inbound
Cosmo-Learn: code for learning cosmology using different methods and mock data cites this paper.
Cosmo-Learn: code for learning cosmology using different methods and mock data Cosmological structure formation in a homogeneous dark energy background
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:43:16.579694Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2d4a2bea-9e9b-4ed3-969a-b451352f653a · inbound
Large-scale structures of the Universe: physics, phenomenology, statistics cites this paper.
Large-scale structures of the Universe: physics, phenomenology, statistics Cosmological structure formation in a homogeneous dark energy background
Reference 93
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-29T03:13:04.111565Z
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 372af385-9548-4041-b69a-289bdddbe015 · inbound
Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model cites this paper.
Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model Cosmological structure formation in a homogeneous dark energy background
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:07:58.367289Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.