Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2405.02242.
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 2026-08-14T04:17:46.966533Z
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
6
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 1d1d4241-e887-4916-a569-f5f8b7ef9bbf · inbound
Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "Little Red Dots" cites this paper.
Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "Little Red Dots" The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T20:15:56.493120Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5746b549-8eb1-4554-8d7e-7f8c84e6bc11 · inbound
Cosmic quenching cites this paper.
Cosmic quenching The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T14:45:24.422607Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b3db56d2-9ecb-44a9-9ab0-1b9d113d9357 · inbound
Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$ cites this paper.
Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$ The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 5
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T23:42:16.285791Z
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 9e2dc0db-3b9a-467d-8b9d-6a4be16ccc77 · inbound
A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots cites this paper.
A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 32
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T08:53:14.739514Z
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 f6926b01-3570-45b5-b471-2cc42b6b5066 · inbound
DeepDive: A deep dive into the physics of the first massive quiescent galaxies in the Universe cites this paper.
DeepDive: A deep dive into the physics of the first massive quiescent galaxies in the Universe The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:10:20.073639Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2b1b153-2d28-4be7-94d9-08120db9fe28 · inbound
Are Nucleosynthetic Yields Universal? Interpreting the Multi-Elemental Abundances of Quiescent Galaxies over Cosmic Time Using Milky Way Stars cites this paper.
Are Nucleosynthetic Yields Universal? Interpreting the Multi-Elemental Abundances of Quiescent Galaxies over Cosmic Time Using Milky Way Stars The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 85
- Resolution
- verified exact
- arxiv_id, observed 2026-05-08T18:08:54.164588Z
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 d543f497-c29d-48c4-80d8-e78e9b2ca04f · 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 The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 238
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:38:43.120172Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28687ad0-82f2-41a7-99e7-6ac1d8ea532c · inbound
Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy cites this paper.
Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T04:17:46.966533Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.