Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1906.02747.
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 2026-08-12T06:34:41.77262+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 2026-07-10T18:07:31.395912Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- malformed identifier0
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External citation measurements
195
pith, observed 2026-07-10T18:07:31.395912Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 6cc814df-2e48-4e81-95c4-9d2a3a1e8e9e · inbound
Galaxy discs regulate the growth of supermassive black holes cites this paper.
Galaxy discs regulate the growth of supermassive black holes The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 82
- Resolution
- metadata mismatch
- doi, observed 2026-05-10T18:20:42.082862Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 01339a88-4bd2-4db5-ac4e-e6269ab697ca · inbound
DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Proto-clusters cites this paper.
DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Proto-clusters The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 117
- Resolution
- verified exact
- doi, observed 2026-05-09T23:09:26.096562Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation f9a2f1f6-0da4-49aa-860a-126cc79c8d98 · inbound
The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model cites this paper.
The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 88
- Resolution
- verified exact
- doi, observed 2026-05-09T00:49:28.493439Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation cec4b015-c5ae-49ed-97ea-ee16cef015f8 · inbound
Constraining the nature of active galactic nuclei through circumgalactic Lya emission at z=2-3 cites this paper.
Constraining the nature of active galactic nuclei through circumgalactic Lya emission at z=2-3 The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 78
- Resolution
- verified exact
- doi, observed 2026-05-09T01:59:36.743831Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 598226a2-e964-42aa-8c84-d331666ec6ab · inbound
Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations cites this paper.
Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 59
- Resolution
- verified exact
- doi, observed 2026-05-08T17:58:52.821854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 439f22b2-506f-4af1-950c-b53e476ddecb · inbound
ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations cites this paper.
ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 214
- Resolution
- verified exact
- doi, observed 2026-05-08T20:04:08.327581Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 009fdba7-a3f5-4a11-bd1b-c1c4a6015edc · 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 relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 114
- Resolution
- verified exact
- doi, observed 2026-05-20T16:03:33.283689Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 814d1a06-eb04-44be-822c-d076fb765a01 · 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 relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 143
- Resolution
- verified exact
- doi, observed 2026-06-28T01:01:26.932587Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ac0c7156-89ca-45d9-8242-32cf964afa55 · inbound
Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as revealed by their stellar populations cites this paper.
Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as revealed by their stellar populations The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 141
- Resolution
- metadata mismatch
- doi, observed 2026-06-27T16:51:06.511355Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 9dee3483-9b17-42d4-af0e-631f77ef00a3 · inbound
Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as revealed by their stellar populations cites this paper.
Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as revealed by their stellar populations The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 141
- Resolution
- metadata mismatch
- doi, observed 2026-06-29T02:33:05.608689Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ce80fe4b-2ae2-44f1-8943-e052c95b9400 · inbound
TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation cites this paper.
TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 35
- Resolution
- verified exact
- doi, observed 2026-06-27T00:30:17.117840Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e4fd67ae-83b0-4868-abd7-5302b1498837 · 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 relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 133
- Resolution
- verified exact
- doi, observed 2026-06-26T20:09:57.198482Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 7146d8ab-573d-4287-ab9d-50d66c0d77ab · inbound
RAD@home discovery of a bow-and-arrow radio galaxy tracing a ~560 kpc bow-shock structure in a multi-halo environment cites this paper.
RAD@home discovery of a bow-and-arrow radio galaxy tracing a ~560 kpc bow-shock structure in a multi-halo environment The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 298
- Resolution
- verified exact
- doi, observed 2026-06-26T08:29:13.121383Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8e692c03-071b-4a1d-9be7-57c172326d95 · inbound
Tracing black hole and galaxy growth across environments since cosmic noon cites this paper.
Tracing black hole and galaxy growth across environments since cosmic noon The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
Reference 61
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T18:07:31.397645Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.