Paper Citation Record · LEDGER

The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2408.07745.

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

pith.paper-citation-record.v1
2408.07745 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 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 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:31:00.577535Z

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

2
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 10e61887-191e-4898-be22-6bb229a042da · inbound

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots cites this paper.

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:53:14.778564Z

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 bfb687d4-7410-4711-b2de-a8b83beac04e · inbound

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots cites this paper.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.577535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b6890cd-71fc-44a0-949d-3e8faa6eee1f · inbound

Little Red reionization factories cites this paper.

Little Red reionization factories The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T19:03:20.011104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8e1f1a0-3e91-41d0-bff9-18d65f492156 · inbound

The BlueDOG at Cosmic Noon: A Possible Analog to Little Red Dots? cites this paper.

The BlueDOG at Cosmic Noon: A Possible Analog to Little Red Dots? The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-05T15:44:27.233207Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 10526df7-2ec7-47bc-8cc5-f691c753de0d · inbound

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI cites this paper.

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-05T15:21:40.734540Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbc22dab-7c41-4866-8dcb-021bcda7ac9e · inbound

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon cites this paper.

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-05T06:04:32.704748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 57377696-d7e9-4afa-9934-e23e4b2623b5 · 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 Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:29.843284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 548d7180-b38a-4596-aa5c-66d7712af362 · 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 The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-04T18:47:40.806654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ff52c974-1523-4525-9cb9-58520cff54b1 · 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 The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 4

Resolution: verified exact; arxiv_id, observed 2026-06-29T05:13:07.382103Z

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 abfb6a2f-eb7c-4640-96d8-b2fbac2c6e98 · 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 The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-03T00:41:20.753667Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.