Paper Citation Record · LEDGER

New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1610.06939.

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pith.paper-citation-record.v1
1610.06939 v1

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measured 0 of 0 reference resolution

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measured 4 of 4 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.729985Z

measured 0 of 1 external citation measurements

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Source: pith, observed 2026-07-02T07:36:44.340153Z

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Pith citing papers

Observation 191c5e16-b7b9-454a-8fb0-90e5a9f64f20 · inbound

Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope cites this paper.

Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies

Reference 111

Resolution: verified exact; local_arxiv, observed 2026-05-25T03:55:19.195083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 46d6ad13-0329-4f84-9d01-c3601a2468ce · inbound

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies

Reference 106

Resolution: verified exact; local_arxiv, observed 2026-06-27T18:01:07.815606Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation ddaa0b24-22a2-4365-96d2-f31109a1f613 · inbound

Bridging the gap between SLSNe and SE-SNe. Multi-wavelength analysis of the SLSN-Ib SN 2024jlc cites this paper.

Bridging the gap between SLSNe and SE-SNe. Multi-wavelength analysis of the SLSN-Ib SN 2024jlc New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-07-02T07:36:44.341749Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 4be10376-94e4-4202-9711-2e9edf20e69b · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies

Reference 252

Resolution: unresolved; no resolver link, observed 2026-08-16T00:12:18.729985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.