Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The gas fractions of dark matter haloes hosting simulated $\sim L^\star$ galaxies are governed by the feedback history of their black holes
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1810.07696.
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 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-27T01:00:20.832125Z
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 bd2eb397-9524-473f-85c6-c805240930b2 · 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 The gas fractions of dark matter haloes hosting simulated $\sim L^\star$ galaxies are governed by the feedback history of their black holes
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T16:03:33.363370Z
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 7440a42d-54f9-4756-acd4-b4776263d8fb · inbound
On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ cites this paper.
On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ The gas fractions of dark matter haloes hosting simulated $\sim L^\star$ galaxies are governed by the feedback history of their black holes
Reference 251
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T20:09:57.529989Z
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 58dee072-894d-4c2e-a0d4-b47cebf5cd84 · inbound
Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array cites this paper.
Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array The gas fractions of dark matter haloes hosting simulated $\sim L^\star$ galaxies are governed by the feedback history of their black holes
Reference 161
- Resolution
- verified exact
- local_arxiv, observed 2026-06-25T21:38:29.189484Z
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 5b86b14b-cb31-4a91-8072-eaa732f8e376 · inbound
Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium cites this paper.
Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium The gas fractions of dark matter haloes hosting simulated $\sim L^\star$ galaxies are governed by the feedback history of their black holes
Reference 174
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T01:00:20.833816Z
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.