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Paper Citation Record · LEDGER

Star formation quenching in massive galaxies

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1809.00722.

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

pith.paper-citation-record.v1
1809.00722 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T13:38:42.394522Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T06:25:28.138415Z

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 e29dabac-cfe0-42f9-964a-cc1ac47ed532 · inbound

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon cites this paper.

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon Star formation quenching in massive galaxies

Reference 236

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T03:30:27.394016Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:82c63c0b6138d51eba6baba9def826d52e495cef2f4eef992805f29bbf67aef2

Observation 368d4b39-3469-4d62-bdcd-0e3b720dd8e0 · 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 Star formation quenching in massive galaxies

Reference 171

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T07:59:08.483465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3661c11dd25c206d0d02f03da096029fb1e80a48986f1bbbf46a93b38cc8cd93

Observation fdbafaac-6ce8-459c-9728-75ccbbb80475 · inbound

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys cites this paper.

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys Star formation quenching in massive galaxies

Reference 192

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T06:25:28.139976Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d644052954cd608d47809afd3a551356996dc852476fd4be9be33c68fd96c508

Observation e17c26cb-922d-4733-a900-d4c1a20fa6ee · inbound

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N cites this paper.

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N Star formation quenching in massive galaxies

Reference 35

Resolution
unresolved
no resolver link, observed 2026-07-12T05:06:34.225475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:06:34.225475Z digest=sha256:cfd50d085d986df57f8d5f92b046aa2f6c87ca9d7b4db288dfe282a0f4a19ca4

Observation 313ca7c0-3f36-4bdf-a86a-6e5efc64192b · inbound

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster cites this paper.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Star formation quenching in massive galaxies

Reference 46

Resolution
unresolved
no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T05:32:07.775931Z digest=sha256:3bd5122c4834fe532abeb76dbe01e4e999e523a491203d6daf008d821a99c22e

Observation 5139608b-84fb-4303-be0e-eef420b6fd2d · inbound

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars Star formation quenching in massive galaxies

Reference 231

Resolution
unresolved
no resolver link, observed 2026-08-01T13:38:42.394522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:38:42.394522Z digest=sha256:c03e73bae200964af366939f6f3e70ad74ff4c9907ef035db6e2f7a0f6379eb4

Observation d6c81fc3-07a6-4234-b37e-603fac760287 · inbound

Outflows in the Early Universe: Neutral gas Absorption in Galaxies at z > 3 from low-resolution JWST Spectroscopy cites this paper.

Outflows in the Early Universe: Neutral gas Absorption in Galaxies at z > 3 from low-resolution JWST Spectroscopy Star formation quenching in massive galaxies

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-01T09:56:46.511586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T09:56:46.511586Z digest=sha256:50adc9db5d26e119580fe966ac842967df7cdfaced683f35b409d0b4ec512081