Pith. sign in

Paper Citation Record · LEDGER

Using the helium triplet as a tracer of the physics of giant planet outflows

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2412.05258.

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

pith.paper-citation-record.v1
2412.05258 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:24:38.442994Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation c81897e2-41dc-4331-acf1-c22607d1320c · 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 Using the helium triplet as a tracer of the physics of giant planet outflows

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-07T05:24:38.442994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:24:38.442994Z digest=sha256:0f14c79364d9be7905c6320a48d07599755ce27d634b749c3b79774713146727

Observation 7d2a869e-d109-463b-bcef-5e6c7b2ce218 · 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 the helium triplet as a tracer of the physics of giant planet outflows

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-05T14:38:51.564214Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:38:51.564214Z digest=sha256:252c26e411b61d7f6347c4112e618cb7899a655c0439078ab3065090e8586b8a

Observation 934e42a9-fc47-4088-bfea-ae36e1263567 · inbound

Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b cites this paper.

Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b Using the helium triplet as a tracer of the physics of giant planet outflows

Reference 51

Resolution
verified exact
arxiv_id, observed 2026-05-10T21:25:53.538324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-10T16:35:51.172834Z digest=sha256:69ab601cc96d305808b2d9dcc5c7c8c6f515ddda7b95cc5885f2cb3ebfe6f27e

Observation 2af3e9fa-a18d-4ff3-912b-aa991727cd85 · inbound

Magnetic field strengths of hot giant exoplanets consistent with Solar System values cites this paper.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Using the helium triplet as a tracer of the physics of giant planet outflows

Reference 274

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.394841Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:2adc6f726b0ca202b71d789537a1ddf439968d6ff4ac6915eeb4e2d54c7b7fc4

Observation 50da267d-cc72-4767-b974-37feb8bfc500 · 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 the helium triplet as a tracer of the physics of giant planet outflows

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-01T15:45:57.165080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T15:45:57.165080Z digest=sha256:fed370640ce163eb1bef9634481488b383582ae76a7eeb21193b65acb4cc296f