Paper Citation Record · LEDGER

Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2412.03653.

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

pith.paper-citation-record.v1
2412.03653 v2

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measured 9 of 9 standing notices

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

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:03:27.076648Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T06:37:39.090379Z

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Outbound references

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Pith citing papers

Observation 9574047e-b98b-45e1-9a01-cdbf65183618 · 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 Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-05-23T06:37:39.092642Z

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 b875a7f9-1e30-43da-95d9-bb2cbb4b4a6b · inbound

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$ cites this paper.

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$ Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T14:03:27.076648Z

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Unavailable: canonical work link unavailable.

Observation 6a8cbba7-1689-4e10-920c-df92615624d1 · inbound

Measurements of the z=4-10 X-ray Luminosity Function: the high space density of moderate-luminosity, obscured AGN cites this paper.

Measurements of the z=4-10 X-ray Luminosity Function: the high space density of moderate-luminosity, obscured AGN Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T23:53:18.397509Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fe726c8-86b0-488f-946d-9830fbbdc346 · inbound

The $z=7.08$ quasar ULAS J1120+0641 May Never Reach a "Normal" Black Hole to Stellar Mass Ratio cites this paper.

The $z=7.08$ quasar ULAS J1120+0641 May Never Reach a "Normal" Black Hole to Stellar Mass Ratio Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-06T16:30:44.347249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db0b7ac0-3773-4f43-928c-7e1ec319b907 · 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 $5.71 \le z \le 7.02$ Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-05T14:33:54.802841Z

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Unavailable: canonical work link unavailable.

Observation 5809cb45-e64d-4ac4-ad1b-24ed4197c2a9 · inbound

Do Little Red Dots Vary? cites this paper.

Do Little Red Dots Vary? Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-05T10:54:53.075291Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0dd19fb3-0159-4cee-b7a5-73487096a8cb · inbound

The WISSH quasar project. XII. X-ray view of the most luminous quasi-stellar objects at Cosmic Noon cites this paper.

The WISSH quasar project. XII. X-ray view of the most luminous quasi-stellar objects at Cosmic Noon Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-04T21:28:19.179809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42afe6b7-0d52-43c1-8c88-6511742f685f · inbound

The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics cites this paper.

The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-04T15:38:07.867651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b71e7b0-0bed-42b9-aded-2bce0f9bb848 · 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 Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion

Reference 269

Resolution: unresolved; no resolver link, observed 2026-08-01T13:38:46.955530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.