Paper Citation Record · LEDGER

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

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 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 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T16:48:44.774725Z

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

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 3f49b367-d26e-41d4-b437-d5404b875e66 · inbound

The Composite Spectral Energy Distribution of Quasars is Surprisingly Universal Since Cosmic Noon cites this paper.

The Composite Spectral Energy Distribution of Quasars is Surprisingly Universal Since Cosmic Noon Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-12T16:48:44.774725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29874ef1-1143-4edc-8079-f0656a10a2e6 · inbound

The ionizing photon production efficiency of star-forming galaxies at $z\sim 4-10$ cites this paper.

The ionizing photon production efficiency of star-forming galaxies at $z\sim 4-10$ Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-12T04:37:05.679218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 20375a65-39ba-4e57-a537-f0edc0147bd2 · inbound

Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$ cites this paper.

Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$ Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T23:10:37.664555Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-14T06:32:32.682623+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 2026-08-14T06:32:32.682623+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 2026-08-14T06:32:32.682623+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.