Paper Citation Record · LEDGER

The evolution of the mass-metallicity relation in IllustrisTNG

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1711.05261.

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

pith.paper-citation-record.v1
1711.05261 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 2026-08-05T06:32:48.257954+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:50:15.528621Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T15:51:01.741956Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
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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 598d369d-326b-48c1-8b54-49bbe7bae8b4 · inbound

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations cites this paper.

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations The evolution of the mass-metallicity relation in IllustrisTNG

Reference 121

Resolution: verified exact; local_arxiv, observed 2026-06-27T15:51:01.743319Z

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 fd420ee0-c877-405f-a45e-37c80ff2e98f · inbound

The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.

The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations The evolution of the mass-metallicity relation in IllustrisTNG

Reference 170

Resolution: verified exact; local_arxiv, observed 2026-06-27T04:20:32.692381Z

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 54518489-9f9d-40cd-9983-fda312c24e69 · 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 The evolution of the mass-metallicity relation in IllustrisTNG

Reference 181

Resolution: unresolved; no resolver link, observed 2026-08-02T00:50:15.528621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 11fc4b84-fff3-4a35-b62c-072fa62e615c · inbound

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The evolution of the mass-metallicity relation in IllustrisTNG

Reference 186

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.825478Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.