Paper Citation Record · LEDGER

Heavy element abundances in blue compact galaxies

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/9811387.

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

pith.paper-citation-record.v1
astro-ph/9811387 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.540143Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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External citation measurements

504
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 572c04bc-d61f-41ea-8e26-8bcde0e281ed · inbound

Theoretical ISM pressure and electron density diagnostics for local and high-redshift galaxies cites this paper.

Theoretical ISM pressure and electron density diagnostics for local and high-redshift galaxies Heavy element abundances in blue compact galaxies

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-14T13:20:20.438842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69bf7052-ab64-43ed-828d-11cb3951c6d0 · 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 Heavy element abundances in blue compact galaxies

Reference 262

Resolution: verified exact; local_arxiv, observed 2026-05-25T03:55:19.758775Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b4586350-d641-4b94-9345-3687a5373a68 · 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 Heavy element abundances in blue compact galaxies

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-06-27T18:01:08.003184Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 0e647374-8773-4982-814f-e42ddd4d788d · inbound

Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies cites this paper.

Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies Heavy element abundances in blue compact galaxies

Reference 146

Resolution: verified exact; local_arxiv, observed 2026-06-27T00:00:16.103053Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 4cf88b4e-d6ca-43bc-bc3f-d1d63fedeb4d · inbound

Structural and dynamical properties of Tidal dwarf galaxies in the tails and bridge of the Guitar galaxy Arp 105 cites this paper.

Structural and dynamical properties of Tidal dwarf galaxies in the tails and bridge of the Guitar galaxy Arp 105 Heavy element abundances in blue compact galaxies

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T17:08:01.132618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ffc118ef-8019-4e12-a307-0f207544640b · 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 Heavy element abundances in blue compact galaxies

Reference 213

Resolution: unresolved; no resolver link, observed 2026-08-16T00:12:18.540143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.