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Paper Citation Record · LEDGER

The evolution of surface magnetic fields in young solar-type stars I: the first 250 Myr

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1601.00684.

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

pith.paper-citation-record.v1
1601.00684 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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T03:58:35.317650Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

188
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 59007a8d-f909-4af4-8998-f170df0c12fd · inbound

Exploring Activity Across the Stellar Main Sequence with the Sun as a Benchmark cites this paper.

Exploring Activity Across the Stellar Main Sequence with the Sun as a Benchmark The evolution of surface magnetic fields in young solar-type stars I: the first 250 Myr

Reference 63

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:18:24.838397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d865f4d69842e4ecdc052b828015640f5aba3033b2796a8a7f5b8c3f7b84066e

Observation bf2d2083-d224-4698-8248-93d61db7551e · inbound

Unstable magnetospheric accretion on the T Tauri star TW Hya cites this paper.

Unstable magnetospheric accretion on the T Tauri star TW Hya The evolution of surface magnetic fields in young solar-type stars I: the first 250 Myr

Reference 279

Resolution
unresolved
no resolver link, observed 2026-07-14T03:58:35.317650Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T03:58:35.317650Z digest=sha256:e3089b22616b85fad8dd2857f1a57a87b8645ac35f48182f656647bc9d77f2f0