Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-03T15:39:20.148780Z
Paper Citation Record · LEDGER
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
As of 15 August 2026, this Paper Citation Record lists 10 of 10 outbound references and 5 inbound Pith citation observations for arXiv:2512.16208.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T08:58:09.440293Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
10 of 10 outbound references displayed
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- malformed identifier5
- metadata mismatch0
External citation measurements
1
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
Observation 6cafe957-626a-4025-b1db-551fd9e56ef5 · outbound
This paper cites massive” and “quenched.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics massive” and “quenched
Reference 1
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T15:39:18.726744Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c620fd3c-a32b-47f5-8dc0-ae20caa3b4c3 · outbound
This paper cites with predictions from other galaxy formation and evolution models; here, we extend this analysis to the full redshift range2≤𝑧≤7.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics with predictions from other galaxy formation and evolution models; here, we extend this analysis to the full redshift range2≤𝑧≤7
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T15:39:18.818312Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 35d40673-bab5-47b4-9b65-226322339ac1 · outbound
This paper cites This relation becomes steeper at higher redshifts, indicating that dust is depleted after quenching, with no significant regrowth.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics This relation becomes steeper at higher redshifts, indicating that dust is depleted after quenching, with no significant regrowth
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T15:39:19.727303Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 926a2427-4e9c-4bf2-93e5-640b5a477b79 · outbound
This paper cites In the top panel, we show the galaxy size–mass relation, which extends up to𝑧=5owing to the larger volume of the L400m7 box.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics In the top panel, we show the galaxy size–mass relation, which extends up to𝑧=5owing to the larger volume of the L400m7 box
Reference 5
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T15:39:19.470934Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b963cb33-32c7-482a-8f6a-d1ab05e38d0f · outbound
This paper cites an unresolved cited work.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics Unresolved cited work
Reference 7
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T15:39:19.922942Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f706486d-0cb8-49ba-a439-f99fa0dc8fec · outbound
This paper cites This is in agreement with the observational results in (Kawinwanichakij et al.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics This is in agreement with the observational results in (Kawinwanichakij et al
Reference 8
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T15:39:19.981574Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2593240-0d0d-42ab-a90e-fecf932b2bd3 · outbound
This paper cites an unresolved cited work.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics Unresolved cited work
Reference 9
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T15:39:20.028594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7896555d-7eac-4226-8cd0-be8094263fb0 · outbound
This paper cites an unresolved cited work.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics Unresolved cited work
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T15:39:20.148780Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 88d5cb59-7f41-428e-9614-ed66b723cb23 · outbound
This paper cites (2025) versus MILES (Falcón-Barroso et al.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics (2025) versus MILES (Falcón-Barroso et al
Reference 2009
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T15:39:19.051688Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3bb64034-f1c9-4b12-b784-706d34757fdf · outbound
This paper cites (2000) dust attenuation law and uniform metallicity priors.
Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics (2000) dust attenuation law and uniform metallicity priors
Reference 2015
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T15:39:19.295265Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation ff5a734a-a805-429b-bb39-322cf001b494 · inbound
The importance of super-Eddington black hole accretion for the emergence of massive quiescent galaxies at high redshift cites this paper.
The importance of super-Eddington black hole accretion for the emergence of massive quiescent galaxies at high redshift Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T08:58:09.440293Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 83a908a6-2db0-4aae-a6b5-f1d1bd584064 · inbound
Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$ cites this paper.
Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$ Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
Reference 28
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- verified exact
- arxiv_id, observed 2026-06-01T02:02:23.299476Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation d703d2ea-b1d7-4e9a-a136-e5ca97b0f77d · inbound
Extended [CII] gas emission in and around a massive quiescent galaxy at z=7.3 cites this paper.
Extended [CII] gas emission in and around a massive quiescent galaxy at z=7.3 Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
Reference 16
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T07:09:37.500498Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation fc39b660-b4e9-455f-96dd-f710af8a4e5d · inbound
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
Reference 226
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T04:20:32.793225Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 3eb3d98f-8304-4084-b639-7b88cc07d8df · inbound
The evolution of galaxy dust scaling relations in the COLIBRE simulations cites this paper.
The evolution of galaxy dust scaling relations in the COLIBRE simulations Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:49:09.271289Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.