Pith. sign in

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 9 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 2026-08-09T06:31:02.800959+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 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-16T08:53:14.586891Z digest=sha256:b8a20025775db89291106842385b90a20bbc6dbedfda8684606a84713ae7e6d5

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.

source=pdf_text observed=2026-08-07T14:31:00.577535Z digest=sha256:c14c8176d9d354953562fc1fd7287d37b485eae792187dddd0e6cd9b0cbffc55

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.

source=arxiv_source observed=2026-08-05T19:03:20.011104Z digest=sha256:be4c7a988f36582e3d2c9226d4499360a63c10b3cf222987ebcade843deabfd9

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.

source=pdf_text observed=2026-08-05T15:44:27.233207Z digest=sha256:3245014f58e0a573226abe8483266d3c7a301838310a3d3ed1fb7781f2c836f2

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.

source=arxiv_source observed=2026-08-05T15:21:40.734540Z digest=sha256:3f68c8320de07e1a94819b003f70a9dcb46e01fbae2328b2eb869d9810dd9b5e

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.

source=arxiv_source observed=2026-08-05T06:04:32.704748Z digest=sha256:ed13fa9e03282b997366150d7d76a4f67fc7c41567082e58da4efde4ac6e6040

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.

source=pdf_text observed=2026-08-05T05:29:29.843284Z digest=sha256:0ca54056316c498ca633ed7cffa1df7e104fdd770d10e68744d17d465d48c253

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.

source=pdf_text observed=2026-08-04T18:47:40.806654Z digest=sha256:f01e1b83ac3156799718fa441cae3deb7007c5585b31f2bd4255b297f51cf826

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 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-29T02:06:03.427307Z digest=sha256:4593b41d8aecfe6b45e96db84eb42ed3082f7ffb3d051cf9f52cc54aeef827a3

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.

source=arxiv_source observed=2026-08-03T00:41:20.753667Z digest=sha256:063cb8d04a98f1e53ff7de7ec1ad15e585f8e2d23d2b3931e8c987cd9b588ce9