Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-10T17:51:45.096450Z
Paper Citation Record · LEDGER
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
As of 5 August 2026, this Paper Citation Record lists 7 of 7 outbound references and 9 inbound Pith citation observations for arXiv:2604.09177.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T13:59:31.645447Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T12:15:01.137692Z
Reference resolution
7 of 7 outbound references displayed
- verified exact0
- verified fuzzy2
- unresolved3
- parse uncertain0
- malformed identifier1
- metadata mismatch1
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 0ddb4d28-cbd3-442f-9ee9-714c1b668555 · outbound
This paper cites 2026, arXiv e-prints, arXiv:2601.22214, doi: 10.48550/arXiv.2601.22214.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ 2026, arXiv e-prints, arXiv:2601.22214, doi: 10.48550/arXiv.2601.22214
Reference 1
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T05:56:00.684699Z
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.
Observation 53b9c12d-b154-4caf-a9f5-2d1be862418d · outbound
This paper cites an unresolved cited work.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ Unresolved cited work
Reference 2
- Resolution
- unresolved
- raw_fallback, observed 2026-05-17T08:39:18.288234Z
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.
Observation 7619c719-9784-4f6e-9c87-65a3e40ab488 · outbound
This paper cites an unresolved cited work.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ Unresolved cited work
Reference 3
- Resolution
- unresolved
- raw_fallback, observed 2026-05-17T08:39:18.278110Z
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.
Observation 2be764a3-0b49-4590-8df5-0079d5a445a3 · outbound
This paper cites Model 2 favours an instrument gradient opposite to what measured inThe Cliff(panelb),implyinganevenstrongervelocitygradientthanthemeasured -15 km s−1 shown in Fig.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ Model 2 favours an instrument gradient opposite to what measured inThe Cliff(panelb),implyinganevenstrongervelocitygradientthanthemeasured -15 km s−1 shown in Fig
Reference 4
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T08:39:18.294364Z
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.
Observation a07b3a99-0c6c-4301-86f4-4e54e0f0dbaa · outbound
This paper cites an unresolved cited work.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ Unresolved cited work
Reference 5
- Resolution
- unresolved
- raw_fallback, observed 2026-05-17T08:39:18.299834Z
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.
Observation 19b7a14b-91c4-4f46-a586-61f809bc6dc3 · outbound
This paper cites The horizontal pink line indicates the upper limit on dynamical mass derived in Section 4.4.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ The horizontal pink line indicates the upper limit on dynamical mass derived in Section 4.4
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T08:39:18.283964Z
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.
Observation 4925fd4a-8b71-4c1b-b787-c59e4d3c3908 · outbound
This paper cites Aesopicaintroduces targeted updates for modelling the growth of infant SMBHs in the early Universe.
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ Aesopicaintroduces targeted updates for modelling the growth of infant SMBHs in the early Universe
Reference 7
- Resolution
- malformed identifier
- arxiv_id, observed 2026-05-11T05:56:00.674881Z
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.
Pith citing papers
Observation e8616f6f-b2df-4fa3-bb3e-6839b21594f8 · 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 The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T13:59:31.645447Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 768994ba-f5b7-490a-a45e-955bea764788 · inbound
Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots cites this paper.
Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 41
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:32:15.158479Z
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.
Observation 1fc5ee89-d6ea-40fa-9054-43838a18addd · inbound
ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement cites this paper.
ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 56
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-02T08:56:49.371946Z
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.
Observation c1a057ab-60b8-4c6e-94ff-c88fcbef7260 · 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 The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 39
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-02T14:27:04.233055Z
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.
Observation c4b2f202-b551-47ec-a9e6-908e0392cc47 · inbound
JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity cites this paper.
JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 82
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T12:20:54.778322Z
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.
Observation 2a9b9518-6664-4890-a2ff-6778fefcd88a · inbound
Little Red Dots as Supermassive Analogs of SS 433 cites this paper.
Little Red Dots as Supermassive Analogs of SS 433 The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 77
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-26T14:09:31.501960Z
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.
Observation 8840bd72-5c5e-4792-afef-bed0d92a16c4 · 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 The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 151
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-26T13:39:30.437621Z
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.
Observation 874e7f4f-4a55-4bbf-b14b-c4c0d7659c02 · 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 The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 93
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-01T12:15:43.947806Z
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.
Observation cd05b027-9050-4a10-9074-fe8c75961e13 · 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 The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
Reference 190
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:25:45.474286Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.