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Paper Citation Record · LEDGER

Bulge mass is king: The dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1403.5269.

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

pith.paper-citation-record.v1
1403.5269 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 2026-08-22T06:32:14.747728+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:38:19.059445Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T13:00:56.835378Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
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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 35920418-fe82-4d89-b2dc-843a7a1ff53f · inbound

Dark Matter-Independent Orbital Decay Bounds on Ultralight Bosons from OJ287 cites this paper.

Dark Matter-Independent Orbital Decay Bounds on Ultralight Bosons from OJ287 Bulge mass is king: The dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-15T21:38:19.059445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T21:38:19.059445Z digest=sha256:6b5b2af86e37229e2fc9755b322982577bbd287bf91409926bb46fbbbb2b83c4

Observation d71765e5-ce15-4953-ad20-b888667d2500 · 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 Bulge mass is king: The dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey

Reference 206

Resolution
verified exact
local_arxiv, observed 2026-05-14T21:09:27.902817Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c9bf0b84ef04c9fa6830ad5b939fda8bf1ac802f3e4a21cd09bdc5784c3f8196

Observation 6d30d55f-db69-4110-bd59-b5ba6d05ac2b · inbound

Multiphase images of a powerful supernova-driven wind in the early Universe cites this paper.

Multiphase images of a powerful supernova-driven wind in the early Universe Bulge mass is king: The dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey

Reference 138

Resolution
verified exact
local_arxiv, observed 2026-06-27T13:00:56.836818Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6c74fc28da0a91b87a00b15b5e5e2bae3fd6a1473c85a698e7c48ac0fc475676