Paper Citation Record · LEDGER

The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:astro-ph/9605073.

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

pith.paper-citation-record.v1
astro-ph/9605073 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:39:44.659478Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T17:02:23.862298Z

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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 2c629c10-e689-43bc-b600-592153604707 · inbound

Supermassive black holes and their surroundings: MeV signatures cites this paper.

Supermassive black holes and their surroundings: MeV signatures The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T21:05:50.929899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 284ed7e5-e2ac-4b7b-b86b-75f40115cc73 · inbound

Astrophysical X-Ray Polarization cites this paper.

Astrophysical X-Ray Polarization The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 11

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:31:13.194803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation ac486e35-d062-468c-a979-63e2ee168ad0 · inbound

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 cites this paper.

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.213188Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 4e11c801-3745-4dad-815b-b6b165099102 · inbound

The first IXPE view of the eclipsing ADC source 4U 1822-37 cites this paper.

The first IXPE view of the eclipsing ADC source 4U 1822-37 The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-05-20T04:18:02.632876Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 9f45d2ae-082e-4be6-97a1-3a3400cba3ee · inbound

Photon Escape from Slab Thomson Media: A Scattering-order-resolved Recursive Formalism for Comptonization Applications cites this paper.

Photon Escape from Slab Thomson Media: A Scattering-order-resolved Recursive Formalism for Comptonization Applications The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-06-28T17:02:23.863632Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 586e1d98-51d1-471a-876c-6bdd89d1cb6f · inbound

Unchanged X-Ray Polarization During Accretion Dips in the Low Hard State of Cygnus X-1 cites this paper.

Unchanged X-Ray Polarization During Accretion Dips in the Low Hard State of Cygnus X-1 The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T00:44:27.728152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a95a31e7-a7de-4b15-8d1b-0e56bded7948 · inbound

AT2021yky: A Fast-Rising Optical Transient with Evolving Broad Hydrogen Emission Consistent with an Ambiguous Nuclear Transient cites this paper.

AT2021yky: A Fast-Rising Optical Transient with Evolving Broad Hydrogen Emission Consistent with an Ambiguous Nuclear Transient The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-15T14:39:44.659478Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8163348-1492-451b-8da6-e5d483c40100 · inbound

ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo cites this paper.

ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo The Two-Phase Pair Corona Model for Active Galactic Nuclei and X-ray Binaries: How to Obtain Exact Solutions

Reference 115

Resolution: unresolved; no resolver link, observed 2026-08-15T14:20:14.118297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.