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Paper Citation Record · LEDGER

Large scale simulations of H and He reionization and heating driven by stars and more energetic sources

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2009.06631.

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

pith.paper-citation-record.v1
2009.06631 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:24:47.897838Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T04:24:08.106193Z

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 9761f74b-4203-4b0f-9b20-15194b3068bb · inbound

Patchy Helium and Hydrogen Reionization from the Kinetic Sunyaev-Zel'dovich Effect and Galaxies cites this paper.

Patchy Helium and Hydrogen Reionization from the Kinetic Sunyaev-Zel'dovich Effect and Galaxies Large scale simulations of H and He reionization and heating driven by stars and more energetic sources

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-08-07T04:24:08.109579Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-07T04:24:07.508758Z digest=sha256:beba470d54a25087fe6fe799f09f2da6fd5d5a4c554511f81f10a0f906c1aa35

Observation 867518d8-f656-4a4f-a117-894b4fc1f404 · inbound

On the Origin of the Ly$\alpha$ Damping Wing in Galaxies at $8\le z \le 10$: Explorations using the NINJA Simulations cites this paper.

On the Origin of the Ly$\alpha$ Damping Wing in Galaxies at $8\le z \le 10$: Explorations using the NINJA Simulations Large scale simulations of H and He reionization and heating driven by stars and more energetic sources

Reference 144

Resolution
unresolved
no resolver link, observed 2026-08-08T16:24:47.897838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:24:47.897838Z digest=sha256:7c5cd7e83c104d84a3caa5ddb15c41f0da03825a80807750d6da774bea071069