Paper Citation Record · LEDGER

Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2412.05242.

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

pith.paper-citation-record.v1
2412.05242 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T14:33:59.090975Z

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

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 2026-08-07T06:34:17.273281+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 2026-08-07T06:34:17.273281+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 2026-08-07T06:34:17.273281+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.