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Paper Citation Record · LEDGER

How does radiative feedback from a UV background impact reionization?

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1301.6781.

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

pith.paper-citation-record.v1
1301.6781 v1

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 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T16:14:56.784192Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T16:14:57.258132Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 e38054ad-b3f3-4a2b-8da3-06d475dc5740 · inbound

Simulation-based inference on warm dark matter from HERA forecasts cites this paper.

Simulation-based inference on warm dark matter from HERA forecasts How does radiative feedback from a UV background impact reionization?

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-08-11T16:14:57.262672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-11T16:14:56.784192Z digest=sha256:b87cbd18d17d99689718413b79866ef143e09457a5bb0a7c0a6785f371101879

Observation 8961fb33-bb0a-4eb3-9d4c-a0a4badfba2f · inbound

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter cites this paper.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter How does radiative feedback from a UV background impact reionization?

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-03T21:29:40.373116Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T21:29:40.373116Z digest=sha256:0d02ac67047a963f74bf4ab1a9cf054a3b2c9111008ea9bac8b057974290375a

Observation b112416e-191f-44e2-9faa-96f6ebf9488f · inbound

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity How does radiative feedback from a UV background impact reionization?

Reference 180

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:56.798123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:10:56.798123Z digest=sha256:9fbead5383bdbd2fbd2891667b95818c554be9057a10fefaacf6226ae0bdc054