Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Using helium 10830 {\AA} transits to constrain planetary magnetic fields
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2302.10947.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T20:55:36.041485Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
2
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation cb2babbd-1d30-4f54-94c7-ea4c423437f5 · inbound
Using the helium triplet as a tracer of the physics of giant planet outflows cites this paper.
Using the helium triplet as a tracer of the physics of giant planet outflows Using helium 10830 {\AA} transits to constrain planetary magnetic fields
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T20:55:36.041485Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0218dc6d-b68c-4b22-8bcb-2e0858613e4b · inbound
Stringent Upper Bounds on Atmospheric Mass Loss from Three Neptune-Sized Planets in the TOI-4010 System cites this paper.
Stringent Upper Bounds on Atmospheric Mass Loss from Three Neptune-Sized Planets in the TOI-4010 System Using helium 10830 {\AA} transits to constrain planetary magnetic fields
Reference 63
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T14:38:55.020029Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation df2ceb9c-2d78-4ad2-8fde-37a32518edcc · 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 Using helium 10830 {\AA} transits to constrain planetary magnetic fields
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T15:45:57.044740Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.