Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{*,sph}$ and $M_{BH}$-$M_{*,gal}$
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1903.04738.
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 2026-06-28T01:01:27.159453Z
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 4400747e-91a2-4e77-acc5-b7ea64860b7d · inbound
Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31 cites this paper.
Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31 Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{*,sph}$ and $M_{BH}$-$M_{*,gal}$
Reference 97
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T16:03:33.217738Z
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 22d9a414-5493-46d1-ae6a-e8c1fc13b5cc · 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 Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{*,sph}$ and $M_{BH}$-$M_{*,gal}$
Reference 23
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T01:01:27.160762Z
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 5ac1d2be-ae97-4448-8510-ac3e2fb98da5 · inbound
The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes cites this paper.
The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{*,sph}$ and $M_{BH}$-$M_{*,gal}$
Reference 148
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T15:31:00.994865Z
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.