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Paper Citation Record · LEDGER

Blue Monsters at $z>10$. Where has all their dust gone?

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2410.19042.

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

pith.paper-citation-record.v1
2410.19042 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:58:21.933430Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-09T20:23:52.711623Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 418afea9-463b-4d0b-88e4-c5027839ead7 · inbound

No evidence (yet) for increased star-formation efficiency at early times cites this paper.

No evidence (yet) for increased star-formation efficiency at early times Blue Monsters at $z>10$. Where has all their dust gone?

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T21:58:21.933430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T21:58:21.933430Z digest=sha256:cb46e137e76eaabbaae63b6bfb645a6cc95ede7578c59fceaf14d4d48229309f

Observation 6fcd7a5b-c194-44f0-9d27-d9559c1c6f1a · inbound

Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic $\beta_{UV}$ slope at z=8.5 cites this paper.

Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic $\beta_{UV}$ slope at z=8.5 Blue Monsters at $z>10$. Where has all their dust gone?

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-10T20:19:12.181723Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T20:19:12.181723Z digest=sha256:5998c918ec393bd28d52b9ad7664a8afe429fcdd57f79ead520449b1df46c5e6

Observation eab72a88-76e1-45ca-a516-3e736a55ab22 · inbound

Low dust mass and high star-formation efficiency at $z>12$ from deep ALMA observations cites this paper.

Low dust mass and high star-formation efficiency at $z>12$ from deep ALMA observations Blue Monsters at $z>10$. Where has all their dust gone?

Reference 35

Resolution
metadata mismatch
local_arxiv, observed 2026-08-09T20:23:52.719289Z

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.

source=pdf_text observed=2026-08-09T20:23:52.207966Z digest=sha256:7127626064378395537c46a7e059c2dce56b51449d8dce80cbaa732a52928cb6

Observation b2695a97-7415-4d3e-8be2-ed6b94fda2cf · inbound

Effects of temperature-dependent optical properties on the determination of interstellar dust masses cites this paper.

Effects of temperature-dependent optical properties on the determination of interstellar dust masses Blue Monsters at $z>10$. Where has all their dust gone?

Reference 30

Resolution
unresolved
no resolver link, observed 2026-07-31T19:44:47.511306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T19:44:47.511306Z digest=sha256:3105a2dedb09dae63284320498de293673a9bb267caa5aac663adf0004a3a540