Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5<z<2.5
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1607.03107.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-01T05:45:26.354128Z
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 da40741b-04a9-499d-8d49-609e24f31a2b · inbound
Empirical estimates of how massive galaxies can be in {\Lambda}CDM cites this paper.
Empirical estimates of how massive galaxies can be in {\Lambda}CDM Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5<z<2.5
Reference 210
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T21:09:27.743482Z
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 94b886fe-9973-4d73-9ec4-7551bc9238b9 · inbound
A big step forward with SHARP: spatially resolved stellar population properties in passive galaxies at z > 1.5 cites this paper.
A big step forward with SHARP: spatially resolved stellar population properties in passive galaxies at z > 1.5 Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5<z<2.5
Reference 39
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T05:45:26.357916Z
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.