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Paper Citation Record · LEDGER

A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2603.28335.

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

pith.paper-citation-record.v1
2603.28335 v3

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 2026-08-12T06:34:41.77262+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:21.034849Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 839c8105-dd70-4103-b1d3-1b2a2ff0a5f5 · inbound

A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability cites this paper.

A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 86

Resolution
verified exact
arxiv_id, observed 2026-06-19T17:09:53.567007Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-15T02:46:55.074673Z digest=sha256:0bf4c4cda65423a4a129e8999a0429fa5b1547390f289a34ee0633b1a8957f1b

Observation e1d02b35-208c-4b71-9664-4f1f0ece5752 · inbound

The quasi-star model for Little Red Dots: potential and challenges cites this paper.

The quasi-star model for Little Red Dots: potential and challenges A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 76

Resolution
verified exact
local_arxiv, observed 2026-07-02T14:27:04.209005Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-28T00:26:52.824241Z digest=sha256:67aff54afd027bf4cf3a03587242510aec758c30b0d056cf2456220cb1043433

Observation a3a72433-5cfd-4039-8957-0499e554f876 · inbound

TBD LBD: The nature of `little blue dots' cites this paper.

TBD LBD: The nature of `little blue dots' A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 33

Resolution
verified exact
local_arxiv, observed 2026-07-03T11:58:05.846276Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-27T09:18:14.075506Z digest=sha256:d353de93b5afab7af5e46b5d16a80c667ce81116cbaf07ec149ff22247e0038c

Observation 86ceaf91-fcf1-47d0-bb01-88afcdac8936 · inbound

Little Red Dots as Supermassive Analogs of SS 433 cites this paper.

Little Red Dots as Supermassive Analogs of SS 433 A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-06-26T14:09:31.534850Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-06-26T14:02:19.397772Z digest=sha256:4eba8e1a3c887a83bab83ef9cf3d1a2070ba95dace56631ec29c1053ebab463e

Observation f7e5a0ae-eadf-48a2-913a-8bea06b27842 · inbound

Little Red and Blue Dots: AGN-excited narrow lines, Lyman-$\alpha$ emission, and resemblance to standard quasars cites this paper.

Little Red and Blue Dots: AGN-excited narrow lines, Lyman-$\alpha$ emission, and resemblance to standard quasars A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 143

Resolution
verified exact
local_arxiv, observed 2026-06-26T13:39:30.274257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-06-26T13:36:30.180504Z digest=sha256:f89232d6bfd5087a2774c3d2a97e3946f99add33a57370b01393c9dece130c4d

Observation ffbcd04a-8db0-423e-a00b-39528c32f0d6 · inbound

Constraints on the Gas Geometry Surrounding Little Red Dots through Narrow-Line Diagnostics cites this paper.

Constraints on the Gas Geometry Surrounding Little Red Dots through Narrow-Line Diagnostics A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-06-26T08:09:10.012375Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-26T08:07:54.650186Z digest=sha256:9a8269b6649fc0cb351171bbf17aeb588556e09733684b7a2cd6f7bfdeedde1d

Observation 6a656e0c-53fc-43ed-aa9d-91bbfae320a7 · inbound

Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $\eta$ Carinae cites this paper.

Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $\eta$ Carinae A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 211

Resolution
verified exact
local_arxiv, observed 2026-07-01T12:15:43.784803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-01T02:15:32.123527Z digest=sha256:c471042bb04c0b58e614253fd4988503448bd385ecb4bca1bb087345e6533f38

Observation 919ac773-d538-4b8e-902c-86e17ebfcd5b · inbound

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys cites this paper.

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 17

Resolution
verified exact
local_arxiv, observed 2026-07-01T06:25:28.512331Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-01T01:25:40.167166Z digest=sha256:fdbba6caba6bc2d35b0b392e189a01198ac79248af3a40e9af2f34ba537e0f4b

Observation 9c8a90db-b27d-4f01-b1ce-b4679a645158 · 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 A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 185

Resolution
unresolved
no resolver link, observed 2026-08-01T00:25:45.106859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:25:45.106859Z digest=sha256:03f205943607b2ed0230683c11ba2bc9dff9f8c01c9e94ba58c67642f6f1bad6

Observation 35a91a16-e1d9-40e8-a6b5-880665f0e025 · 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 $z < 0.35$ A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7

Reference 168

Resolution
unresolved
no resolver link, observed 2026-08-08T16:36:21.034849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:36:21.034849Z digest=sha256:f66cfae674c84bb7e1516ce896a773d1beb6955f9a3e27730062b4b09dec5277