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Paper Citation Record · LEDGER

Dust in Little Red Dots

As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2407.05094.

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

pith.paper-citation-record.v1
2407.05094 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:57:55.930708Z

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

2
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 01d80f71-559a-452f-9d00-51de37aca1f3 · inbound

A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission cites this paper.

A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission Dust in Little Red Dots

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-12T00:57:55.930708Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T00:57:55.930708Z digest=sha256:ea976a5e9f3184a659283706c1cdc11276f03be7a650c678ee34e78ed02bbf66

Observation 94bd10c5-5287-453b-9b23-f6aa03206157 · inbound

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI cites this paper.

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI Dust in Little Red Dots

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-05T15:21:40.776794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T15:21:40.776794Z digest=sha256:56912d3dab2e4bb235ec57163d1d678e45f81adfd8dbdaf75785ceac3272a5f3

Observation b2729c51-1727-488d-9ce6-c64e5a509308 · 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 Dust in Little Red Dots

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-04T18:47:40.789623Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:47:40.789623Z digest=sha256:d47787f13d181bbf98f9f70149e294139bb0d2f3e2437ceb1a0b0f8ed70718cb

Observation 30f98a47-673d-41b0-a8f7-d3326b4e20de · inbound

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts cites this paper.

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts Dust in Little Red Dots

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-18T14:41:29.676413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-18T14:36:35.824494Z digest=sha256:1ec3e9cc4daa6c9c182c067139b2ccc94b6513fb3927de0051c40ab3191a6a38

Observation 1031cf61-8401-4565-995e-bc1c202cf2e2 · 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 $z < 0.35$ Dust in Little Red Dots

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-08T16:36:20.577681Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:36:20.577681Z digest=sha256:46d0f87e4b2753b84eee5610d35e00612236ec4ff70caf53cb7551e6dcc45fc1