Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Helium escape signatures are generally strongest during younger ages but this age dependence is lost in the diversity of observed exoplanets
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2504.02578.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T05:24:38.202219Z
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 f3c36b86-eff3-4ba0-9a1a-d86684780041 · inbound
A Multi-Species Atmospheric Escape Model with Excited Hydrogen and Helium: Application to HD209458b cites this paper.
A Multi-Species Atmospheric Escape Model with Excited Hydrogen and Helium: Application to HD209458b Helium escape signatures are generally strongest during younger ages but this age dependence is lost in the diversity of observed exoplanets
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:24:38.202219Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1f424032-d186-424a-9083-e7e25c0d259b · 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 Helium escape signatures are generally strongest during younger ages but this age dependence is lost in the diversity of observed exoplanets
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T15:45:57.068835Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.