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Paper Citation Record · LEDGER

The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2102.02135.

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

pith.paper-citation-record.v1
2102.02135 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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T10:56:50.746512Z

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

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  • verified fuzzy0
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External citation measurements

12
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation ad187e8e-8c00-4130-b7e4-d482bbd274c6 · inbound

The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy cites this paper.

The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations

Reference 113

Resolution
verified exact
local_arxiv, observed 2026-07-12T07:08:35.583498Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-12T07:07:35.219491Z digest=sha256:f47d962442caea5f63ca2ad47cc89b666073d917a85679205a0132aa6ed372ba

Observation 58651479-06d9-4d87-bcaa-df4c5d2b8d2f · 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 The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-04T10:56:50.746512Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T10:56:50.746512Z digest=sha256:49ca61167f5d195e3cc6d10415c004a5bfcfe9ad8944fc9a74e44684e821955e