Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0307202.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T00:16:22.974745Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-21T07:49:49.185480Z
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 7717af0e-7c35-4129-85dc-073394b17ee4 · inbound
COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 cites this paper.
COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
Reference 132
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T03:58:01.957590Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 04154a8e-893f-44d1-8876-2773426e65d1 · inbound
COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 cites this paper.
COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
Reference 132
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T07:49:49.187519Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 63cde8ea-6615-49a0-8993-2e97ab6988be · inbound
The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data cites this paper.
The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T00:16:22.974745Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.