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Paper Citation Record · LEDGER

Can we believe the strong-line abundances in giant HII regions and emission-line galaxies?

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1906.04520.

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

pith.paper-citation-record.v1
1906.04520 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T05:28:10.199252Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T21:17:48.773000Z

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 44508bcc-5a40-4298-8dc7-a70bb574cc90 · inbound

Gas accretion as fuel for residual star formation in Galaxy Zoo elliptical galaxies cites this paper.

Gas accretion as fuel for residual star formation in Galaxy Zoo elliptical galaxies Can we believe the strong-line abundances in giant HII regions and emission-line galaxies?

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-14T05:28:10.199252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T05:28:10.199252Z digest=sha256:1aa64f3198b87c097a76b71e2084d22071dc7db37efa56d74e14e216dea2eec9

Observation 4065eba8-a70e-4afd-aa92-0579f48636a3 · inbound

Nebular emission from composite star-forming galaxies -- I. A novel modelling approach cites this paper.

Nebular emission from composite star-forming galaxies -- I. A novel modelling approach Can we believe the strong-line abundances in giant HII regions and emission-line galaxies?

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-08-10T21:17:48.779437Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-10T21:17:48.393928Z digest=sha256:b907021ba6c995a75f715bc13a35af2859778ced1121ea222734989b6a707519