Pith. sign in

Paper Citation Record · LEDGER

Modelling the He I triplet absorption at 10830 Angstroms in the atmosphere of HD 209458 b

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2003.04872.

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

pith.paper-citation-record.v1
2003.04872 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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T23:49:15.933933Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 5eb79f0c-3f11-4f1d-aa46-70cdac53eee8 · inbound

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae cites this paper.

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae Modelling the He I triplet absorption at 10830 Angstroms in the atmosphere of HD 209458 b

Reference 294

Resolution
unresolved
no resolver link, observed 2026-08-03T23:49:15.933933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:49:15.933933Z digest=sha256:8aa644ad14b7ffb52b0d8f25b2840a071a4e5b75c10347a3b563d2711fab03d1

Observation 7dc3cd89-fabf-4c6f-91aa-df7de9826e97 · 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 Modelling the He I triplet absorption at 10830 Angstroms in the atmosphere of HD 209458 b

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-01T15:45:57.205304Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T15:45:57.205304Z digest=sha256:704a78c247d6b77dcd2f93846f19919ffbee4a6ba58a41d1f8dd191cbb2d49d5