Paper Citation Record · LEDGER

Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2410.07340.

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

pith.paper-citation-record.v1
2410.07340 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T22:03:27.890848Z

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

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External citation measurements

1
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 334630e3-72d8-4cfb-90de-7c1cdee616f2 · inbound

Little Red Dots are Tidal Disruption Events in Runaway-Collapsing Clusters cites this paper.

Little Red Dots are Tidal Disruption Events in Runaway-Collapsing Clusters Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T22:03:27.890848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f05bfca-04a4-4545-a548-64b9d30bd2f7 · 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 Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:53:14.733300Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 397a0505-5ce7-47a1-ac4e-93780bee2f55 · inbound

Measurements of the z=4-10 X-ray Luminosity Function: the high space density of moderate-luminosity, obscured AGN cites this paper.

Measurements of the z=4-10 X-ray Luminosity Function: the high space density of moderate-luminosity, obscured AGN Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-06T23:53:18.240525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24649e2d-f56a-4f37-9aa3-30fafd703cf5 · 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 Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 207

Resolution: verified exact; arxiv_id, observed 2026-05-19T16:22:39.172089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 764f3bfc-2f8e-4a02-bc1e-37185b204e25 · 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 Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 178

Resolution: verified exact; arxiv_id, observed 2026-07-02T18:27:16.477496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 28b960e9-801f-4a86-bebc-0915b19c527b · inbound

Two Peas in a Pod: The First Confirmed Dual Active Galactic Nucleus within a Green Pea Galaxy System cites this paper.

Two Peas in a Pod: The First Confirmed Dual Active Galactic Nucleus within a Green Pea Galaxy System Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-01T17:12:35.328305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 012d5e19-49f5-4f13-b305-e6fd5da9c641 · 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 Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 197

Resolution: unresolved; no resolver link, observed 2026-08-01T13:38:39.301252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1d2772c-245a-4712-a9ac-b85f89bcd397 · inbound

NEXUS: Spectral Variability of Little Red Dots and Blue Active Galactic Nuclei at $2 \lesssim z \lesssim 6$ cites this paper.

NEXUS: Spectral Variability of Little Red Dots and Blue Active Galactic Nuclei at $2 \lesssim z \lesssim 6$ Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-04T23:44:40.143450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.