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Paper Citation Record · LEDGER

The fast radio burst population evolves, consistent with the star-formation rate

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2101.07998.

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

pith.paper-citation-record.v1
2101.07998 v2

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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:25:43.223792Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 19e7d9d3-ad85-4bff-af3d-79344aa61699 · inbound

The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes cites this paper.

The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes The fast radio burst population evolves, consistent with the star-formation rate

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-03T19:05:24.169532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T19:05:24.169532Z digest=sha256:be969e5bc691f6a81f032ca68c51ecc7a6d765b49f174ec2a224e04c43810b49

Observation 89106bbc-47fc-491e-9892-fd1ec4913340 · inbound

Two new highly scattered fast radio bursts: evidence for scatter broadening by the circumsource medium cites this paper.

Two new highly scattered fast radio bursts: evidence for scatter broadening by the circumsource medium The fast radio burst population evolves, consistent with the star-formation rate

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-15T14:25:43.223792Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:25:43.223792Z digest=sha256:27c6f45da30510e35b1c5062c08b95760f80ecfa5544d862c82490274a2536b1