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Paper Citation Record · LEDGER

Power-law distributions in binned empirical data

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1208.3524.

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

pith.paper-citation-record.v1
1208.3524 v2

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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:13:22.209394Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T15:56:32.853634Z

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 123980d0-20d2-4884-aeb1-c7ce20af278b · inbound

On the extraction of power-law parts of the probability density functions in star-forming clouds cites this paper.

On the extraction of power-law parts of the probability density functions in star-forming clouds Power-law distributions in binned empirical data

Reference 72

Resolution
verified exact
local_arxiv, observed 2026-08-14T15:56:32.860663Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T15:56:32.797554Z digest=sha256:b65339b9c2a430461f9970ac3d864eb8090889f5608ad25fefa0e07726ab58f8

Observation 0bc0ebdd-04dc-4e5b-8c4e-e7e04e0b71db · inbound

Why is the Star Formation Rate Proportional to Dense Gas Mass? cites this paper.

Why is the Star Formation Rate Proportional to Dense Gas Mass? Power-law distributions in binned empirical data

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-15T22:15:53.812969Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T22:15:53.812969Z digest=sha256:d94e41ece02a5a0a62612b5d9430a0b6ca7f104117caf72363b97e25cd7d2e3e

Observation 29308ded-d3f0-4de8-ad0b-3bef2c3051d5 · inbound

Trace the Self-Gravitating Gas Using CO Isotopologues cites this paper.

Trace the Self-Gravitating Gas Using CO Isotopologues Power-law distributions in binned empirical data

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-16T00:13:22.209394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T00:13:22.209394Z digest=sha256:7eacefd639d113cc343f077eb96b54392d84567eb03ccdf6809a44a928c15ee5