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Paper Citation Record · LEDGER

The connection between galaxy structure and quenching efficiency

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1402.3394.

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

pith.paper-citation-record.v1
1402.3394 v3

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

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T02:35:16.882588Z

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 9349a49b-069c-4aa4-8789-859c9f236c44 · inbound

Empirical estimates of how massive galaxies can be in {\Lambda}CDM cites this paper.

Empirical estimates of how massive galaxies can be in {\Lambda}CDM The connection between galaxy structure and quenching efficiency

Reference 219

Resolution
verified exact
local_arxiv, observed 2026-05-14T21:09:27.389414Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:923858f3c20a8c0039f35dc5d02c8158aa53b55084176db2d31cd8e5e8b95a83

Observation 6b50ad43-d98a-463f-93c3-d34428398da7 · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The connection between galaxy structure and quenching efficiency

Reference 210

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:59:08.762136Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7de9d89657fcd819d4dad9cc69b0892f592056342ac17df61bbbadc7b37a1bc8

Observation 4ad9fbff-5561-41fa-89ed-07cf110d48b7 · inbound

A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon cites this paper.

A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon The connection between galaxy structure and quenching efficiency

Reference 12

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T02:35:16.884656Z

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.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:d3c8d83d2301ef741fdddbbb8e4a18a1b506fc9f1630f8c3261a26f3fa8b2f49