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Paper Citation Record · LEDGER

On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2102.05670.

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

pith.paper-citation-record.v1
2102.05670 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:46.919595Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T12:11:56.432083Z

Reference resolution

0 of 0 outbound references displayed

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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 3fa42d10-f4b4-41b5-8946-ed757419029a · inbound

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-05T20:04:22.175532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 232412f1-7601-48f7-8008-7ba932cdb345 · inbound

Characterization of the variability of the blue supergiant HD 14134 cites this paper.

Characterization of the variability of the blue supergiant HD 14134 On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-06T18:25:19.528486Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:25:19.528486Z digest=sha256:1a727ebe93f7dd72ec1a1f13050f2ee94de14f56e9739a1758217f1996bea606

Observation c41dc39f-bcfd-4593-a766-9f302e3c9853 · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

Reference 75

Resolution
verified exact
local_arxiv, observed 2026-08-12T12:11:56.451238Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-08-12T12:11:54.344314Z digest=sha256:55b7a1aa027acaead74f93ea82670df6370002e521e2c130d55eb7857248cb34

Observation 49656e73-65ca-456c-8369-d25059d5b7a8 · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:46.919595Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:46.919595Z digest=sha256:fa6e699721c6d3412f14ecc7c51e7a233af8c283492a764b0eac016eb626b15f