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Paper Citation Record · LEDGER

A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

As of 15 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1208.6512.

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

pith.paper-citation-record.v1
1208.6512 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 2026-07-15T06:30:58.975436+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T04:05:20.592279Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 927f7dec-307a-4262-99c4-179491608c7a · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

Reference 297

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.877508Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-15T06:30:58.975436+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:553d01c7773541800070621bf8c83bffcddcd61bb694f51088da9ece193d952f

Observation 16594e3a-5f32-4f65-8033-1c27e9d95047 · inbound

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? cites this paper.

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

Reference 224

Resolution
verified exact
local_arxiv, observed 2026-07-01T04:05:20.593645Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-15T06:30:58.975436+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:face2d2a67376da0aeab863f9826a0a335b945f66121bd0c721f74c62ba02d49