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Paper Citation Record · LEDGER

Galaxy populations in protoclusters at cosmic noon

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2410.08412.

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

pith.paper-citation-record.v1
2410.08412 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 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T22:15:06.987670Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4e0806cb-0fd8-454b-b98c-c5b4a5fef869 · inbound

Evidence for environmental effects in the $z\,{=}\,4.3$ protocluster core SPT2349$-$56 cites this paper.

Evidence for environmental effects in the $z\,{=}\,4.3$ protocluster core SPT2349$-$56 Galaxy populations in protoclusters at cosmic noon

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-11T22:15:06.987670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T22:15:06.987670Z digest=sha256:b48653d29046be12a48f6a385ef4401bcc4bcc16cdf84bf825049e130ca16779

Observation 67831124-5483-4d1c-b961-e8ed879defd9 · inbound

Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys cites this paper.

Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys Galaxy populations in protoclusters at cosmic noon

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-09T20:39:54.871895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-09T20:39:54.871895Z digest=sha256:252a4d4b4395b770b6dacd8a9652f30b42d05d0ddcab3f64f34e36b1a3a5b73c

Observation 101bfcc5-fe94-4456-8679-af8ed31d1b7b · inbound

Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging cites this paper.

Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging Galaxy populations in protoclusters at cosmic noon

Reference 151

Resolution
verified exact
arxiv_id, observed 2026-05-21T04:43:58.303766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-05-21T04:39:53.459827Z digest=sha256:66c7e8119311fce17f6dd0f31878eed13a391444c3c6b571f10ebc65aa13a96d