Paper Citation Record · LEDGER

Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2206.03508.

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

pith.paper-citation-record.v1
2206.03508 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T06:04:38.558030Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T11:58:06.452953Z

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 90940caa-05d7-4902-bd89-854fd0bda228 · inbound

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon cites this paper.

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-05T06:04:38.558030Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 36c6faca-4524-4d21-b12b-3bc33da37c5e · inbound

X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population cites this paper.

X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

Reference 40

Resolution: metadata mismatch; arxiv_id, observed 2026-07-03T11:28:04.776967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation bf16431e-b5c2-4c4b-8682-71efc98067ce · inbound

Unification models of Active Galactic Nuclei cites this paper.

Unification models of Active Galactic Nuclei Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-07-03T11:58:06.454564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 0bc717d4-0ef6-4afb-bfe9-f9a888479ee3 · inbound

Unification models of Active Galactic Nuclei cites this paper.

Unification models of Active Galactic Nuclei Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-02T11:51:38.075544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b252f308-295f-472c-b00b-54776b6c4381 · inbound

The Lifetimes of High-redshift Quasars Suggest Magnetic Disk Support cites this paper.

The Lifetimes of High-redshift Quasars Suggest Magnetic Disk Support Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

Reference 13

Resolution: metadata mismatch; arxiv_id, observed 2026-07-01T12:35:44.161896Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 5af14067-9f34-426c-83ef-1bce856a5819 · inbound

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium

Reference 111

Resolution: unresolved; no resolver link, observed 2026-08-01T13:38:31.529260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.