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Paper Citation Record · LEDGER

BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2503.11752.

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

pith.paper-citation-record.v1
2503.11752 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 17 of 17 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T18:47:40.859864Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T12:15:01.137692Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 42e7a2cb-047b-4eea-851f-df721ff58383 · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-05-16T08:53:14.658027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-16T08:53:14.586891Z digest=sha256:6ce3b5c48db244a63e935cf62892bc7f6d07dda89d5a2c93ab217a843a900858

Observation 0bf4b922-5472-47b5-846c-14fdde49eb01 · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-04T18:47:40.859864Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:47:40.859864Z digest=sha256:4d42d4ca240cb8a5945b436ed3bbdd37855f60426ac6beebafcf01439c877022

Observation 9ca793c3-2ee6-4d98-8404-0f93d62fbc87 · inbound

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon cites this paper.

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 50

Resolution
metadata mismatch
local_arxiv, observed 2026-05-11T01:10:52.507418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-11T01:07:57.029580Z digest=sha256:f8cc7df518255aac62a5380545a392b63cbced11da82f25f1be93afa5cf8ac74

Observation dcfb4b4d-a5c6-433c-988d-99e72715451f · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 77

Resolution
metadata mismatch
local_arxiv, observed 2026-05-19T16:17:39.470583Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-05-19T16:15:05.216074Z digest=sha256:8afaa180ada02ab626e339b85282b4863f0e58b0c2ecded459d693ad3363d012

Observation 7ec6c9b9-ceca-442d-8deb-13cf10ef4475 · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:22:14.980868Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-06-28T13:19:50.167400Z digest=sha256:0286129c5bc6f891bb08effc71bb824a87aebdebb4bf4af132c35fa0376302fd

Observation 0c689920-09a2-473c-9120-c335d188953a · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-02T12:34:25.997241Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T12:34:25.997241Z digest=sha256:3f58f74a0697a48f87f52c0baecdb80c50c52a88f4f2b7d74797fb75b5048df9

Observation dbebe6c0-3cb8-4eac-84e7-46d50f905c44 · inbound

The Extreme Rarity and Physical Properties of Low-redshift AGNs with Balmer Absorption cites this paper.

The Extreme Rarity and Physical Properties of Low-redshift AGNs with Balmer Absorption BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 11

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T09:06:49.321530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-06-28T05:38:53.500014Z digest=sha256:4042f273a37af638834de5860869cbc41c1e7fefd081a439f804bd6c6494a338

Observation 687ab7a4-beba-4866-bf56-9800d252a0e3 · inbound

The X-ray-to-UV relation does not evolve in homogeneous quasar samples cites this paper.

The X-ray-to-UV relation does not evolve in homogeneous quasar samples BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 23

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T21:01:15.432569Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-06-27T20:56:09.146467Z digest=sha256:8a08c0cc9849c823c5bd4a14c6da1b3adc6e4d1f78d1caa488ae775ed741fe64

Observation 07204055-ef16-4961-8abe-21e101bb47ea · inbound

Between Degeneracy and Evolution: UV-to-optical Insights into the BH$^*$ Model in Little Red Dots cites this paper.

Between Degeneracy and Evolution: UV-to-optical Insights into the BH$^*$ Model in Little Red Dots BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 120

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T10:00:49.854023Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-06-27T09:21:06.539829Z digest=sha256:01e0f450f8e450276dd5c49817a2440730deb9271b6b55098d759707fb7493af

Observation 7264b075-bc2b-4699-b328-4837d5bcd6be · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 144

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T13:39:30.332151Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-06-26T13:36:30.180504Z digest=sha256:6340de518b6e3b9d3c55f99fd7d5a540e984fe31aefcaf8f3f58df04f05166f5

Observation 44387d9a-eaa2-42bf-8aa4-a02db7ce82ca · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 47

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T06:25:28.418798Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-01T01:25:40.167166Z digest=sha256:05d410b05d950b4693baa1d5ec5a85709a1d7b6a1c32c21141dc66f8e664dfff

Observation fbd0a15f-4842-4cf2-9dba-c15eec0365e1 · inbound

The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine cites this paper.

The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 213

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T05:05:23.760568Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-01T04:59:22.269454Z digest=sha256:d0f22806cd5f77eaa9ed6c5c7eade667dd96ea7b8e59321acdcd0ff7e8266806

Observation 3be48c37-75ca-47e1-96c0-abaa74ad554c · inbound

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 cites this paper.

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 186

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T18:27:16.423418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-02T18:25:22.489682Z digest=sha256:b4c12ec600151699cb65cb9f654a8975124a065e46aae30afc150ddc88e1d6d4

Observation d7354d8e-8355-42f8-ad63-739c80bb302c · 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 $z\simeq5.23$ BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 272

Resolution
unresolved
no resolver link, observed 2026-07-11T06:23:06.110361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:3b7493b2695e874deca8eb637ee583d1b34f81bbd187478702f67c32b79eee8b

Observation 1ec462c2-39cb-4037-8eb6-bbf2aca6f8e6 · 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 $z\simeq5.23$ BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 273

Resolution
unresolved
no resolver link, observed 2026-07-11T06:23:06.110361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:e73b1080b99d6d60c4ac2fcf99508142fe366f267f2d8c5fc2d682363ee2c09f

Observation 82f3f943-fb05-4e06-97b5-9c650a7fe814 · inbound

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 252

Resolution
unresolved
no resolver link, observed 2026-08-01T13:38:44.829118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:38:44.829118Z digest=sha256:b13f75d53501f5f8c20f8d56ee7ce2bc6666ec16317846e870332b0e395d622f

Observation f8ea8db8-6384-4a38-ab7d-8901c4ed79b1 · 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 BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 184

Resolution
unresolved
no resolver link, observed 2026-08-01T00:25:45.013635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:25:45.013635Z digest=sha256:0b8285e18fd2c7910f87ace9433c79d4ba623f177a2c3bb0b0ec6042bff55688