Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for S\'ersic and Core-S\'ersic Galaxies
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1303.5490.
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 2026-08-13T06:32:02.005865+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 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
143
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 4da86088-bd8f-411c-9db1-a7186645bb12 · inbound
Mapping the nuclear environments of extreme coronal line emitting galaxies cites this paper.
Mapping the nuclear environments of extreme coronal line emitting galaxies The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for S\'ersic and Core-S\'ersic Galaxies
Reference 105
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T09:11:49.509678Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 855cd564-bf49-4d06-8f8f-b72acdce8d54 · inbound
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations cites this paper.
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for S\'ersic and Core-S\'ersic Galaxies
Reference 66
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T01:01:26.864119Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.