Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2412.05242.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.885294Z
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
1
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 a2df814e-4bea-4168-bbec-d3a83b002c9c · inbound
Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales cites this paper.
Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 37
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T06:37:39.046341Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation b022f16d-5da0-4292-a73e-1d45c03ac6cd · inbound
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ cites this paper.
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 156
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:33:59.090975Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 01ee6c22-7b73-4d33-8133-01b31e0930bf · inbound
Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? cites this paper.
Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:09:00.465727Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1d2d5760-c348-461b-8abd-739385a44e6b · inbound
Do Little Red Dots Vary? cites this paper.
Do Little Red Dots Vary? Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T10:54:53.333856Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4b11cec3-6de6-4c3a-b311-4e49f93ba18b · inbound
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 185
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-19T16:17:39.883845Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 72e7bfb8-0e61-4e51-aece-7fa205b07687 · inbound
Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations cites this paper.
Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 19
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T10:06:51.623784Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 912649a8-60ba-44bb-9118-870df3944fb0 · inbound
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:25:32.135109Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a8d26450-bd3a-456a-8350-2876d3cc6daa · inbound
Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ cites this paper.
Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations
Reference 138
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T16:36:20.885294Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.