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Paper Citation Record · LEDGER

3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2002.07457.

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

pith.paper-citation-record.v1
2002.07457 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T10:56:50.632563Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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Pith citing papers

Observation 647f61c2-b3d1-4b55-a149-a034fa183445 · inbound

Origin of the Long-Period Radial Velocity Variation in the Red Supergiant HD 216946 (V424 Lac) cites this paper.

Origin of the Long-Period Radial Velocity Variation in the Red Supergiant HD 216946 (V424 Lac) 3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations

Reference 207

Resolution
unresolved
no resolver link, observed 2026-08-01T11:43:05.630004Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T11:43:05.630004Z digest=sha256:f4d80fa0d672c764556816b8608272d0015fc242d22e4935b54b2f60cd96d3b9

Observation 77af7588-aec2-4a6e-aea8-566fd5d5c65c · inbound

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum cites this paper.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum 3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-04T10:56:50.632563Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T10:56:50.632563Z digest=sha256:715fd788bc24d1b4c591a0ac1c4064f9454211834dea889c06e0137addef0015