Paper Citation Record · LEDGER

Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1410.4875.

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

pith.paper-citation-record.v1
1410.4875 v3

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 2026-08-09T06:31:02.800959+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T19:17:16.716960Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T04:15:21.378859Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 116629b9-acf7-4022-9ab0-d558af4aca87 · inbound

The History of Galaxy Mergers in IllustrisTNG cites this paper.

The History of Galaxy Mergers in IllustrisTNG Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-04T19:17:16.716960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 518ddddd-4909-4f58-86ea-6803501be6dc · inbound

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

Can current models predict the local black hole merger rate? Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS

Reference 299

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.567471Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 176d57e0-ea93-4005-afbd-2815ae21f4a6 · 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? Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS

Reference 197

Resolution: verified exact; local_arxiv, observed 2026-07-01T04:15:21.380322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1a78eb08-ab27-4679-8659-8a5646dbe39d · inbound

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba cites this paper.

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS

Reference 232

Resolution: unresolved; no resolver link, observed 2026-08-01T08:26:20.521222Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.