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Paper Citation Record · LEDGER

Gas-phase metallicity gradients in galaxies at $z \sim 6-8$

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2403.03977.

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

pith.paper-citation-record.v1
2403.03977 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-05-18T08:40:11.481931Z

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

4
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 63b82698-ed25-4e91-9f5f-4e25a19e5be5 · inbound

Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations cites this paper.

Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations Gas-phase metallicity gradients in galaxies at $z \sim 6-8$

Reference 95

Resolution
verified exact
arxiv_id, observed 2026-05-18T08:41:07.598193Z

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.

source=pdf_text observed=2026-05-18T08:40:11.481931Z digest=sha256:c9869e8ae672d07c2206979ae42fdc81f110fc269e73a8bc231dc76cf029e907

Observation 1d903912-0ad3-45b2-af35-628afc4bd590 · inbound

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift cites this paper.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Gas-phase metallicity gradients in galaxies at $z \sim 6-8$

Reference 152

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.645666Z

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.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:379b3af99f5b0f29a6cd04773fdc5acd49fc91da72113babce1a023f62050130