Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
Paper Citation Record · LEDGER
A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling
As of 7 August 2026, this Paper Citation Record lists 3 of 3 outbound references and 3 inbound Pith citation observations for arXiv:2605.30414.
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 2026-08-01T00:39:49.419962Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
3 of 3 outbound references displayed
- verified exact2
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch1
External citation measurements
0
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
Observation 624fca09-8728-498f-a8b5-fc00376d9c77 · outbound
This paper cites A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy.
A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy
Reference 1
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-29T06:33:11.304555Z
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 f5ab6b86-2f27-4b98-af0d-698391896813 · outbound
This paper cites E., Sanders, R.
A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling E., Sanders, R
Reference 2
- Resolution
- verified exact
- doi, observed 2026-06-29T06:33:11.306608Z
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 b2254ad0-80a6-4f15-9925-561efa42be8d · outbound
This paper cites Source ID R.A.
A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling Source ID R.A
Reference 4
- Resolution
- verified exact
- arxiv_id, observed 2026-06-29T06:33:11.905671Z
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.
Pith citing papers
Observation b1984acc-6770-4d7c-9652-bbcfda39d04c · inbound
General Relativistic Shock Wave Solutions with Black Hole Formation: The Singular Isothermal Sphere Case cites this paper.
General Relativistic Shock Wave Solutions with Black Hole Formation: The Singular Isothermal Sphere Case A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling
Reference 12
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-30T01:54:11.620848Z
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 9f0976df-5636-4c92-a8da-673a3b126b43 · inbound
Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $\eta$ Carinae cites this paper.
Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $\eta$ Carinae A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling
Reference 69
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-01T12:15:43.976136Z
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 d8e62cbb-268f-42ae-87ff-cd0ca9c99137 · inbound
How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations cites this paper.
How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling
Reference 225
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:39:49.419962Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.