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Paper Citation Record · LEDGER

Lyman Continuum leakage from massive leaky starbursts: A different class of emitters?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2410.13254.

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

pith.paper-citation-record.v1
2410.13254 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:19:12.306603Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7f387335-8d4e-4b7c-849f-fe56fa90939d · inbound

Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic $\beta_{UV}$ slope at z=8.5 cites this paper.

Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic $\beta_{UV}$ slope at z=8.5 Lyman Continuum leakage from massive leaky starbursts: A different class of emitters?

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-10T20:19:12.306603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T20:19:12.306603Z digest=sha256:afd36c191190486cedd120a30289f6b5a389cc89feb47a0ed3161d6f1bca72f0

Observation b32f0341-e47a-4bd7-b9ca-db17f07ef0ee · inbound

pySTARBURST99: The Next Generation of STARBURST99 cites this paper.

pySTARBURST99: The Next Generation of STARBURST99 Lyman Continuum leakage from massive leaky starbursts: A different class of emitters?

Reference 109

Resolution
unresolved
no resolver link, observed 2026-08-07T12:35:51.120034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T12:35:51.120034Z digest=sha256:8507ef383a24069b37e0f4f3a55cc359007ce4cb53157f970be29385fe95c1a4

Observation 1161f8e7-ce37-42d4-828d-c32e28ff651a · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Lyman Continuum leakage from massive leaky starbursts: A different class of emitters?

Reference 61

Resolution
verified exact
arxiv_id, observed 2026-06-26T18:09:41.586281Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-06-26T07:09:31.413097Z digest=sha256:ee4db023875995789a5c9765d7ac73dabebc4d789adaf152f595284d784a5535