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Paper Citation Record · LEDGER

The impact of intrinsic magnetic field on the absorption signatures of elements probing the upper atmosphere of HD209458b

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2112.01128.

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

pith.paper-citation-record.v1
2112.01128 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T15:45:57.345431Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-13T07:19:26.935851Z

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 c8c9aa9e-4929-4304-bd9b-0559075a9efc · inbound

Magnetic activity in cool stars: manifestations and relevance to exoplanets cites this paper.

Magnetic activity in cool stars: manifestations and relevance to exoplanets The impact of intrinsic magnetic field on the absorption signatures of elements probing the upper atmosphere of HD209458b

Reference 8

Resolution
verified exact
local_arxiv, observed 2026-07-13T07:19:26.937783Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-07-13T07:12:16.870340Z digest=sha256:30acb122904eec4d5aa94ba9e6c6a9c28252efbc057a74b11bdd189d41a03d1c

Observation 949ee720-25c8-4737-8562-dc9b3f9d3031 · 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 The impact of intrinsic magnetic field on the absorption signatures of elements probing the upper atmosphere of HD209458b

Reference 133

Resolution
unresolved
no resolver link, observed 2026-08-01T15:45:57.345431Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T15:45:57.345431Z digest=sha256:ed7e191d18fd46d4752125ea8147cd6bf40fdcdf1dd71774d58c1663246d05d9