Paper Citation Record · LEDGER

The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:1906.02747.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1906.02747 v1

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measured 16 of 16 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:47:46.824763Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-10T18:07:31.395912Z

Reference resolution

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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 2e90a550-a70f-4099-8e48-df0176c5bc6d · inbound

The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship cites this paper.

The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG

Reference 65

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Observation 855b70cb-59e9-4d01-bc4d-d29bd2e697fd · inbound

The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas cites this paper.

The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG

Reference 127

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Source-reported events for the cited work

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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.

Reference 141

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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

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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

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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

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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

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