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Paper Citation Record · LEDGER

Improving Predictions for Helium Emission Lines

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9810087.

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

pith.paper-citation-record.v1
astro-ph/9810087 v1

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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T15:45:57.195634Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T09:21:49.564146Z

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 f960fa0c-5be7-418b-8552-6e624b425cf0 · inbound

Fifty years of primordial helium abundances: A statistical reanalysis cites this paper.

Fifty years of primordial helium abundances: A statistical reanalysis Improving Predictions for Helium Emission Lines

Reference 10

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T09:21:49.565464Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3ced0df970edc283659dfa0b07a45aecb56310de4b2e1721c42917d09b4d4c9a

Observation e47c719b-9afd-44b2-8cb4-8151fa1e19db · inbound

A Self-Consistent 3D Hydrodynamic Model for Helium Transit Signatures in Evaporating Hot Jupiters cites this paper.

A Self-Consistent 3D Hydrodynamic Model for Helium Transit Signatures in Evaporating Hot Jupiters Improving Predictions for Helium Emission Lines

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-01T15:45:57.195634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T15:45:57.195634Z digest=sha256:67f54e6693e6fca864d065c215ae27aec707e0a25e68aba3865452fcd671fae9