Paper Citation Record · LEDGER

The Host Galaxy (If Any) of the Little Red Dots

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2411.04446.

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

pith.paper-citation-record.v1
2411.04446 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T23:10:37.688452Z

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
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malformed identifier0
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External citation measurements

0
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 2a516ae0-9215-497f-a33a-e6d08159877f · inbound

Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$ cites this paper.

Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$ The Host Galaxy (If Any) of the Little Red Dots

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-11T23:10:37.688452Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5527162-fdcb-4026-a817-cd7bac7389ef · inbound

Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion cites this paper.

Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion The Host Galaxy (If Any) of the Little Red Dots

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-11T22:20:27.202561Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4bca256c-9d1f-4b7a-982b-5ee77ee06316 · inbound

An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy cites this paper.

An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy The Host Galaxy (If Any) of the Little Red Dots

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T21:29:42.458149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0619cd01-aa4c-4880-a267-b5a30ff9e046 · inbound

Discovery of Local Analogs to JWST's Little Red Dots cites this paper.

Discovery of Local Analogs to JWST's Little Red Dots The Host Galaxy (If Any) of the Little Red Dots

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-11T17:56:08.252932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3059a512-9663-48c9-b566-1b7151be5f09 · 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 The Host Galaxy (If Any) of the Little Red Dots

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-23T06:37:39.054548Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation d5bd5153-84a6-4a07-a281-9971480fe34b · inbound

Little Red reionization factories cites this paper.

Little Red reionization factories The Host Galaxy (If Any) of the Little Red Dots

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-05T19:03:20.177549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8521c4d-09b2-4775-a7e2-6f5f2283251e · inbound

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots cites this paper.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The Host Galaxy (If Any) of the Little Red Dots

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:29.882499Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2480e028-c9e7-42f7-b8d4-209a0074ad39 · inbound

Undermassive Hosts of $z = 4-6 $ AGN from JWST/NIRCam Image Decomposition with CONGRESS, FRESCO, and JADES cites this paper.

Undermassive Hosts of $z = 4-6 $ AGN from JWST/NIRCam Image Decomposition with CONGRESS, FRESCO, and JADES The Host Galaxy (If Any) of the Little Red Dots

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-03T08:47:00.546062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e20c15e-aeab-4096-b7d9-88d81d42cfac · 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 The Host Galaxy (If Any) of the Little Red Dots

Reference 206

Resolution: verified exact; arxiv_id, observed 2026-05-19T16:22:39.249387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 1716e842-dcc2-4b21-b5af-1023f907a299 · 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 The Host Galaxy (If Any) of the Little Red Dots

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.224618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 765f7191-34be-4835-b5eb-91177a56792c · 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 The Host Galaxy (If Any) of the Little Red Dots

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:37.242246Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9d67b0d-cbd9-4a4f-9a18-a01cb41a831f · 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 $z < 0.35$ The Host Galaxy (If Any) of the Little Red Dots

Reference 125

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.808998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.