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Paper Citation Record · LEDGER

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$

As of 10 August 2026, this Paper Citation Record lists 5 of 5 outbound references and 3 inbound Pith citation observations for arXiv:2511.05647.

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

pith.paper-citation-record.v1
2511.05647 v2

Coverage vector

measured 5 of 5 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-03T23:34:08.613409Z

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T03:09:03.916396Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T00:16:24.755483Z

Reference resolution

5 of 5 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved3
  • parse uncertain0
  • malformed identifier2
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation f923065e-d134-4ee4-99df-77fdad5271d4 · outbound

This paper cites EPOCHS III: Unbiased UV continuum slopes at 6.5<z<13 from combined PEARLS GTO and public JWST NIRCam imaging.

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$ EPOCHS III: Unbiased UV continuum slopes at 6.5<z<13 from combined PEARLS GTO and public JWST NIRCam imaging

Reference 1

Resolution
malformed identifier
no resolver link, observed 2026-08-03T23:34:08.217286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:34:08.217286Z digest=sha256:40cb020fa958eb380b3b3d361fc7de67ceee75275154e03e89417ab24ca7b726

Observation 61f4c945-ad56-4312-84f5-c4f2465c5b08 · outbound

This paper cites The best-fit stellar mass is log10(M⋆[M⊙])=10±0.1, with a V-band dust attenuation of AV =2.0 +0.4 −0.2.

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$ The best-fit stellar mass is log10(M⋆[M⊙])=10±0.1, with a V-band dust attenuation of AV =2.0 +0.4 −0.2

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-03T23:34:08.302489Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:34:08.302489Z digest=sha256:9b4a7a904e1607ea53d89f14b2968fb16d73cdad24634443a2ddb7178ae2170f

Observation a6f38f74-d5b7-4cc7-8e98-1bf13cf261a2 · outbound

This paper cites It is clear that when modelled with purely stellar populations, the LRDs (red data points) have significantly higher stellar mass surface densities than the sample ofz>5 galaxies.

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$ It is clear that when modelled with purely stellar populations, the LRDs (red data points) have significantly higher stellar mass surface densities than the sample ofz>5 galaxies

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-03T23:34:08.613409Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:34:08.613409Z digest=sha256:41cc3ded55740a80da50943d2ecd9500b78f4e7b0bad06a9323dea05310a4280

Observation 18af9d7e-752c-4e8a-b4b5-7ba07b95a2fd · outbound

This paper cites an unresolved cited work.

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$ Unresolved cited work

Reference 2024

Resolution
unresolved
no resolver link, observed 2026-08-03T23:34:08.476773Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:34:08.476773Z digest=sha256:a49ad0b0c4f4530faa2bac468fc99a159630a0c4843de5e7544ba2536135118b

Observation 34026e06-ebf5-40d0-ad69-98e92f01b7b0 · outbound

This paper cites an unresolved cited work.

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$ Unresolved cited work

Reference 2025

Resolution
malformed identifier
no resolver link, observed 2026-08-03T23:34:08.397390Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:34:08.397390Z digest=sha256:28509e8ec39a1bc75bb634f75db5baade220804bcb6a22c16e67d7596b451a28

Pith citing papers

Observation ae5fa9b1-3805-490d-a596-a559c8f143a9 · inbound

All the Massive Galaxy Overdensities during Reionization: JWST Rest-Frame Optical Selection Reveals Young, Chemically Evolved Galaxies Embedded in Dense, Neutral Gas at z > 5 cites this paper.

All the Massive Galaxy Overdensities during Reionization: JWST Rest-Frame Optical Selection Reveals Young, Chemically Evolved Galaxies Embedded in Dense, Neutral Gas at z > 5 Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-03T03:09:03.916396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T03:09:03.916396Z digest=sha256:736e66ea8c33264aa634618352bad4c84a44d50441dbf81e2aa57dd3ee0b4da0

Observation 1feef50b-fc12-4e00-813c-f1bcb870cd85 · inbound

The birth of the intracluster medium: the evolution of multiphase gas and Lyman-$\alpha$ haloes in a simulated $z\sim3$ protocluster cites this paper.

The birth of the intracluster medium: the evolution of multiphase gas and Lyman-$\alpha$ haloes in a simulated $z\sim3$ protocluster Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$

Reference 108

Resolution
unresolved
no resolver link, observed 2026-08-02T18:00:53.534336Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T18:00:53.534336Z digest=sha256:dc7bc4c6d139782c6c4afb769f53cfb20105161cfaf2316bccf8cf6613e5705b

Observation 576ad5b6-a5b5-4fa1-a240-492ab773334d · inbound

A Cosmic Archipelago of lensed metal-poor galaxies at $z\sim6$ cites this paper.

A Cosmic Archipelago of lensed metal-poor galaxies at $z\sim6$ Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$

Reference 195

Resolution
verified exact
local_arxiv, observed 2026-07-02T00:16:24.757578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-28T13:28:57.785289Z digest=sha256:f1bda0c4b11cc133d5b8e66f5e5474070b92c951a945dc68e7c088a93aa5b0e5