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Paper Citation Record · LEDGER

Little Red Dots as Direct-collapse Black Hole Nurseries

As of 15 August 2026, this Paper Citation Record lists 3 of 3 outbound references and 3 inbound Pith citation observations for arXiv:2508.14897.

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

pith.paper-citation-record.v1
2508.14897 v1

Coverage vector

measured 3 of 3 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T18:19:59.331754Z

measured 6 of 6 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T00:30:25.492661Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-11T06:27:50.535212Z

Reference resolution

3 of 3 outbound references displayed

  • verified exact0
  • verified fuzzy2
  • unresolved1
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation efd4e0b6-17ac-480e-8e9d-1698dc179942 · outbound

This paper cites COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly.

Little Red Dots as Direct-collapse Black Hole Nurseries COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-05T18:19:59.146373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T18:19:59.146373Z digest=sha256:a0a36301dd534141383bd6b5c0a8bb82f1332626345c54606d977d67e0b7e1e6

Observation 7133efe9-42a7-42ec-87e2-5cf3b09759ff · outbound

This paper cites On average, low-redshift haloes have both lower central gas densities and higher metal- licities.

Little Red Dots as Direct-collapse Black Hole Nurseries On average, low-redshift haloes have both lower central gas densities and higher metal- licities

Reference 3

Resolution
verified fuzzy
raw_fallback, observed 2026-08-05T18:19:59.735138Z

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.

source=pdf_text observed=2026-08-05T18:19:59.220212Z digest=sha256:25eeecfebfb174ce75e46fbf4e420559682b5b8d3506272e1a8c031613637628

Observation f6691914-73b8-45ce-abf4-4db8aab110cc · outbound

This paper cites Gas-phase metallicity (Z) in all haloes in our simulations, as a function of redshift, in different simulations, in three different halo mass bins.

Little Red Dots as Direct-collapse Black Hole Nurseries Gas-phase metallicity (Z) in all haloes in our simulations, as a function of redshift, in different simulations, in three different halo mass bins

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-08-05T18:19:59.566632Z

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.

source=pdf_text observed=2026-08-05T18:19:59.331754Z digest=sha256:265edcbb31c44c2ff71947575bc3adeb8311feebb7b1034d4ec36d715f6204a0

Pith citing papers

Observation bcf23899-1457-4942-a52b-fb9138c7c2fb · 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 $z\simeq5.23$ Little Red Dots as Direct-collapse Black Hole Nurseries

Reference 20

Resolution
verified exact
local_arxiv, observed 2026-07-11T06:27:50.537694Z

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.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:e352436c4f1f667bed32153ab1901546566ba2e1d1da78d3dead5a87f45c3206

Observation aa6b4805-f806-4534-baed-c2fa5b07ac97 · 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 $z < 0.35$ Little Red Dots as Direct-collapse Black Hole Nurseries

Reference 204

Resolution
unresolved
no resolver link, observed 2026-08-08T16:36:21.215339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:36:21.215339Z digest=sha256:6a7dae38f6170a025b55ea9bbceb976c7fb220543da7195dc56bba51abcd7834

Observation 194e646e-7d55-4f68-9c18-ea731712b992 · inbound

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models cites this paper.

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models Little Red Dots as Direct-collapse Black Hole Nurseries

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-11T00:30:25.492661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T00:30:25.492661Z digest=sha256:61d9205292906cfd1243ff31a160fd6e51b3a2a2b61b4253810618960eb7b924