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Paper Citation Record · LEDGER

Cosmology with SKA Radio Continuum Surveys

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1501.03825.

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

pith.paper-citation-record.v1
1501.03825 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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-25T23:05:16.735340Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T18:00:01.538805Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 d121c84c-27a9-4646-8a05-da553a5ac8dd · inbound

How to augment cosmic shear measurements with radio polarimetry of galaxies? cites this paper.

How to augment cosmic shear measurements with radio polarimetry of galaxies? Cosmology with SKA Radio Continuum Surveys

Reference 6

Resolution
verified exact
arxiv_id, observed 2026-05-12T08:31:26.283984Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-12T00:59:48.132631Z digest=sha256:5dedf57510aab41e4b4ce4f2083d95bc6e97678a5d806e5c65973f9adeb1a1e2

Observation ee544f04-9fda-4655-af3d-fd71729a037c · inbound

Using SKAO to Understand the Clustering of Gravitational Wave Sources cites this paper.

Using SKAO to Understand the Clustering of Gravitational Wave Sources Cosmology with SKA Radio Continuum Surveys

Reference 27

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T18:00:01.540473Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-06-25T23:05:16.735340Z digest=sha256:2c70effe5dbcdd15b5f263bce7e0f6e2d69ba530b8fc2eaa56a5c663ce1d9cd9