Pith. sign in

Paper Citation Record · LEDGER

The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing at the origin of chemical abundance variations

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2007.09153.

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

pith.paper-citation-record.v1
2007.09153 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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:57:04.977844Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T10:57:05.727053Z

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 a15d6f1c-3a82-4052-b3d1-6e4f21593260 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing at the origin of chemical abundance variations

Reference 152

Resolution
verified exact
local_arxiv, observed 2026-08-05T10:57:05.730900Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-05T10:57:04.977844Z digest=sha256:b15a2f6bb042072fa262d768a9ae18429c4caca8f73b4d3ced70e77220aea8cd

Observation ddabf093-df41-4795-9b99-2f33ff6bda3f · inbound

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis cites this paper.

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing at the origin of chemical abundance variations

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-01T16:32:14.646822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T16:32:14.646822Z digest=sha256:b8dd7525ff618721d20ba51dfb42369895b1659a9f4fb671abb87ccd17f73cd5