Paper Citation Record · LEDGER

Simulating the dust content of galaxies: successes and failures

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1606.02714.

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

pith.paper-citation-record.v1
1606.02714 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:50:14.890197Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T18:07:15.568388Z

Reference resolution

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External citation measurements

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Outbound references

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Pith citing papers

Observation 83fc01d5-a2c6-46df-aebe-c49f7768860e · inbound

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization Simulating the dust content of galaxies: successes and failures

Reference 154

Resolution: verified exact; local_arxiv, observed 2026-05-19T16:17:39.038496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 91e86716-b659-4bb8-a350-ee86d48c3ba4 · inbound

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 cites this paper.

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 Simulating the dust content of galaxies: successes and failures

Reference 111

Resolution: verified exact; local_arxiv, observed 2026-05-20T03:58:02.295263Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6e98f88d-c650-422b-9796-7a54ed8a38a1 · inbound

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 cites this paper.

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 Simulating the dust content of galaxies: successes and failures

Reference 111

Resolution: verified exact; local_arxiv, observed 2026-05-21T07:49:49.312094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ce46e307-425c-481f-a627-dec43aa1cb26 · inbound

Grain-size evolution and rapid dust growth in high-redshift galaxies cites this paper.

Grain-size evolution and rapid dust growth in high-redshift galaxies Simulating the dust content of galaxies: successes and failures

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-06-28T00:51:27.413586Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 50916350-b69b-45df-8fa3-ab76f46057fd · inbound

Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6 cites this paper.

Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6 Simulating the dust content of galaxies: successes and failures

Reference 171

Resolution: verified exact; local_arxiv, observed 2026-07-02T18:07:15.569651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 9195f06a-a367-48a6-81dc-4abb31a37c60 · inbound

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster cites this paper.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Simulating the dust content of galaxies: successes and failures

Reference 112

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f6f4679-29d6-4051-a2b1-4779ed0ab395 · inbound

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations Simulating the dust content of galaxies: successes and failures

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-02T00:50:14.890197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.