Paper Citation Record · LEDGER

X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2404.19010.

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

pith.paper-citation-record.v1
2404.19010 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 19 of 19 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 19 of 19 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T20:15:57.141612Z

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

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 9e40e29e-7ba9-4558-89d6-327264b1c6a4 · 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" X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-11T20:15:57.141612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9312e65-b0ce-4ae8-8827-fe78e26091ad · 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 X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 3

Resolution: verified exact; arxiv_id, observed 2026-05-23T06:37:39.021396Z

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 4e6e1061-8145-4d37-93b5-acc332c40e94 · inbound

Little Red Dots from Small-Scale Primordial Black Hole Clustering cites this paper.

Little Red Dots from Small-Scale Primordial Black Hole Clustering X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-06T19:01:56.143832Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82d56938-dc03-4394-bc46-67f0e761d6d2 · inbound

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot cites this paper.

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-04T18:47:40.761168Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a05ce21f-af26-4aff-b502-36ebc8a63814 · inbound

Little Red Dots as Hidden Neutrino Sources cites this paper.

Little Red Dots as Hidden Neutrino Sources X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-16T13:42:56.280856Z

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 9be8926e-84d2-4bc0-ad9e-6da6afbd6b2b · inbound

Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters cites this paper.

Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 132

Resolution: verified exact; arxiv_id, observed 2026-05-13T21:23:17.569133Z

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 f1e7db64-6f6c-46fd-aae6-f78102661d5b · inbound

The Two Orbital, Interacting Hatano-Nelson Model cites this paper.

The Two Orbital, Interacting Hatano-Nelson Model X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 27

Resolution: unresolved; no resolver link, observed 2026-07-12T20:13:28.839499Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9040f4c-6c8e-4b54-adda-c90f18ce17d8 · inbound

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe cites this paper.

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-10T11:10:09.313572Z

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 2cfb9b8a-ef9f-45bd-b9f8-94fe09a46986 · inbound

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe cites this paper.

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T16:17:40.355954Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5cc6556a-4d64-4323-80fc-cdae9d523eda · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 11

Resolution: malformed identifier; arxiv_id, observed 2026-07-02T00:36:24.462013Z

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 807f55fe-f77e-455e-9dfa-115f18783c34 · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 11

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:26.057994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 824a26fb-fda9-4899-952b-64385c530ec1 · 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 X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:06:51.602708Z

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 03f472f0-176c-4722-a6d8-7257719c0971 · inbound

SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds cites this paper.

SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 2

Resolution: verified exact; arxiv_id, observed 2026-06-29T05:13:07.366542Z

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 7431a519-a5d9-4d96-9e9b-3af27e07e5be · inbound

AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN cites this paper.

AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 114

Resolution: unresolved; no resolver link, observed 2026-07-12T09:44:28.146054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ec02d52-74aa-4b6d-a3f1-17b9e6ce66ad · inbound

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 268

Resolution: unresolved; no resolver link, observed 2026-07-11T06:23:06.110361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 659fa78d-973e-48ef-8f2a-1a2d6cfc57b8 · 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 X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 226

Resolution: unresolved; no resolver link, observed 2026-08-01T13:38:42.006733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d03cde38-bf07-42de-8ef5-9675c31afd15 · 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 X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 121

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:39.147268Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 243bab8e-5e0f-4c88-8d96-eb4e98b6f17c · inbound

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry cites this paper.

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-03T00:41:19.198069Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e051070-3043-4a5b-bb05-9644ff20435e · 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 $z < 0.35$ X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.565941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.