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Paper Citation Record · LEDGER

An Effective Model for the Cosmic-Dawn 21-cm Signal

As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2302.08506.

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

pith.paper-citation-record.v1
2302.08506 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:34:41.215931Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T02:29:23.458407Z

Reference resolution

0 of 0 outbound references displayed

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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 25f669fc-ab19-478b-9b48-562473343958 · inbound

Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method cites this paper.

Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-12T12:42:57.116802Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 457cfd7f-ee08-47f8-ad97-379ad419b433 · inbound

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos cites this paper.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 123

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unresolved
no resolver link, observed 2026-08-16T11:34:41.215931Z

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Unavailable: canonical work link unavailable.

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Observation 2722bdc8-1e1d-4a19-95f8-edb1469a6a58 · inbound

Tracing the Neutrino-Induced Phase Shift in the 21-cm Spectrum cites this paper.

Tracing the Neutrino-Induced Phase Shift in the 21-cm Spectrum An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 39

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unresolved
no resolver link, observed 2026-08-05T10:55:46.204580Z

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Unavailable: canonical work link unavailable.

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Observation 2d5edb7a-f59b-463f-bebb-ec84ae4c22fb · inbound

A New Boundary Condition on Reionization cites this paper.

A New Boundary Condition on Reionization An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-04T20:07:41.042802Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 6db6f3f9-bbb4-4ae3-b0eb-0cf120783af4 · inbound

Primordial Magnetic Fields at Cosmic Dawn: 21-cm Forecasts with HERA and SKA cites this paper.

Primordial Magnetic Fields at Cosmic Dawn: 21-cm Forecasts with HERA and SKA An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 48

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verified exact
arxiv_id, observed 2026-05-11T18:16:12.505771Z

Source-reported events for the cited work

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Observation bc89dd03-3173-4e66-93ea-c6fd1af69121 · inbound

A self-consistent analytical model for both the photoionization rate and reionization history cites this paper.

A self-consistent analytical model for both the photoionization rate and reionization history An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 61

Resolution
verified exact
arxiv_id, observed 2026-07-04T02:29:23.460006Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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Observation 4613facf-56f9-46cd-9df0-1298b45a9cd2 · inbound

The Rise and Fall of Acoustic Oscillations at Cosmic Dawn cites this paper.

The Rise and Fall of Acoustic Oscillations at Cosmic Dawn An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 80

Resolution
unresolved
no resolver link, observed 2026-07-14T15:06:13.177523Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 38e8bc90-5691-40ba-bcdb-8c40b25e7408 · inbound

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal cites this paper.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-01T09:49:23.783028Z

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Unavailable: canonical work link unavailable.

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Observation 1421878a-d6b4-43f3-a49c-080d3f876659 · inbound

Searching for Population III stars with line intensity mapping cross-correlations cites this paper.

Searching for Population III stars with line intensity mapping cross-correlations An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-03T00:21:45.491266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 729d4ac7-14c0-4b2d-8bd1-7c321a5a3bda · inbound

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations cites this paper.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-15T14:54:41.740447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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