Paper Citation Record · LEDGER

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

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 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 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:57:34.102772Z

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

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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 b7d39f92-4e44-45c7-a36a-23ef911b9642 · inbound

Bias to CMB lensing from lensed foregrounds cites this paper.

Bias to CMB lensing from lensed foregrounds A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-14T11:57:34.102772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

Observation e2c0d650-2627-4014-9daa-47443d7486a1 · inbound

Non-Primordial Contribution to the Cosmic Microwave Background cites this paper.

Non-Primordial Contribution to the Cosmic Microwave Background A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:19.121094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.