Paper Citation Record · LEDGER

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2502.00574.

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

pith.paper-citation-record.v1
2502.00574 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T23:21:42.547743Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T12:11:22.576878Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 d6f9e175-0266-484d-a1da-bdf27a03b4e4 · inbound

Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars cites this paper.

Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-06T23:21:42.547743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eac45310-605e-4b18-8434-86bd4d628e67 · inbound

The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results cites this paper.

The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:08.410822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a466134d-6958-4a32-9766-874ba4169a8f · inbound

The Emergence and Ionizing Feedback of Pop III.1 Stars as Progenitors for Supermassive Black Holes cites this paper.

The Emergence and Ionizing Feedback of Pop III.1 Stars as Progenitors for Supermassive Black Holes Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T11:17:50.397541Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c3919f7-520d-413d-94ad-f5b01d94bdd1 · inbound

Direct Collapse Black Hole Candidates from Decaying Dark Matter cites this paper.

Direct Collapse Black Hole Candidates from Decaying Dark Matter Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-18T12:11:22.579715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.