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Paper Citation Record · LEDGER

Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event

As of 4 August 2026, this Paper Citation Record lists 4 of 4 outbound references and 5 inbound Pith citation observations for arXiv:2512.10564.

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

pith.paper-citation-record.v1
2512.10564 v2

Coverage vector

measured 4 of 4 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-03T17:10:39.962905Z

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T01:19:32.449413Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-10T12:15:01.137692Z

Reference resolution

4 of 4 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation fec580b2-33a8-4cdf-814b-657cff764457 · outbound

This paper cites arXiv:2509.23894 Alexander K.

Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event arXiv:2509.23894 Alexander K

Reference 1

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unresolved
no resolver link, observed 2026-08-03T17:10:39.556677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:10:39.556677Z digest=sha256:1e4dbb651de3b1055304d83a10944aac57fd73dfa6bb80117d1d520f2dd66ac2

Observation fb0c3a49-2771-4718-9c92-4f9f3769ae99 · outbound

This paper cites Colours follow the scheme of Fig.8.

Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event Colours follow the scheme of Fig.8

Reference 4

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no resolver link, observed 2026-08-03T17:10:39.828179Z

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source=pdf_text observed=2026-08-03T17:10:39.828179Z digest=sha256:f32aa07e3921809715013c8c44d76ca35055e1cff0b5676c62bbac39a8838405

Observation ef070ea9-a1f4-4ad8-81a5-f6167deb02be · outbound

This paper cites (ii) Compton scattering is used as a lower limit at low densities (𝜌<10 −10g/cm3) or at high temperatures (𝑇 >6·107K).

Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event (ii) Compton scattering is used as a lower limit at low densities (𝜌<10 −10g/cm3) or at high temperatures (𝑇 >6·107K)

Reference 22

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no resolver link, observed 2026-08-03T17:10:39.962905Z

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source=pdf_text observed=2026-08-03T17:10:39.962905Z digest=sha256:dbe3fecaddfd84fe7a1d7be248d46211a0b5ef479685e14b4d06fbb1d2d4385a

Observation 4f7c74f5-6207-4c3e-b7e0-57073b085e9c · outbound

This paper cites There- fore, the rate of change of the dissipation energy is ¤𝐸irr = ¤𝐸tot− ¤𝐸rev=− ∑︁ interfaces 𝐴(𝑃∗𝒗∗−𝑃 𝑐𝒗∗−𝒗 𝑐𝑃∗)·𝒏 A,(A7) as given in Eq.(7).

Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event There- fore, the rate of change of the dissipation energy is ¤𝐸irr = ¤𝐸tot− ¤𝐸rev=− ∑︁ interfaces 𝐴(𝑃∗𝒗∗−𝑃 𝑐𝒗∗−𝒗 𝑐𝑃∗)·𝒏 A,(A7) as given in Eq.(7)

Reference 2009

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unresolved
no resolver link, observed 2026-08-03T17:10:39.657319Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:10:39.657319Z digest=sha256:f594c836b0943d14a96850ee717996bb252b8886f0959860dd49b2869ff01996

Pith citing papers

Observation dc040181-b0e3-4171-b679-9a3b95de0f79 · inbound

TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy cites this paper.

TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event

Reference 73

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unresolved
no resolver link, observed 2026-08-03T01:19:32.449413Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T01:19:32.449413Z digest=sha256:f38e9adc76030bc464706a59832d352e1b1daf76b237932f923d0a0a7e406331

Observation 7ba9470d-451e-45ab-b5ad-fb70fc864ec5 · inbound

On the origin of anomalous dissipation in simulations of tidal disruption events cites this paper.

On the origin of anomalous dissipation in simulations of tidal disruption events Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event

Reference 42

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verified exact
arxiv_id, observed 2026-06-19T17:10:18.822470Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-21T01:20:29.533556Z digest=sha256:7369600329d5fb43a13e00547178ee8089b2754a7b57a9d370bd9494c1469e94

Observation be6e97de-423b-4a03-98e6-6ff4dc2c36e5 · inbound

Low-hard to high-soft spectral state transitions in the faintest early-X-ray-detected optical tidal disruption event TDE 2025aarm cites this paper.

Low-hard to high-soft spectral state transitions in the faintest early-X-ray-detected optical tidal disruption event TDE 2025aarm Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event

Reference 176

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no resolver link, observed 2026-07-14T15:04:53.805474Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:04:53.805474Z digest=sha256:114c9a80a26d215952f683e27bab886813afcb69ae65435bc2e9c446f47c5890

Observation b341d226-1e02-4a46-8332-24f13e80ef61 · inbound

A spectacular multi-wavelength transient associated with an off-axis relativistic jet cites this paper.

A spectacular multi-wavelength transient associated with an off-axis relativistic jet Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event

Reference 136

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unresolved
no resolver link, observed 2026-07-14T00:47:36.004275Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T00:47:36.004275Z digest=sha256:6ea68affdc1b562d04425763ecc90aabcc03f0889def668b6f9029b366ec3d05

Observation 1c84eb24-4064-422b-9c61-a1acd58924a0 · inbound

Implications of the UV/optical Plateau of AT2018cow cites this paper.

Implications of the UV/optical Plateau of AT2018cow Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-01T23:24:43.339425Z

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Unavailable: canonical work link unavailable.

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