Pith. sign in

Paper Citation Record · LEDGER

Quantitative spectral classification of Galactic O stars

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1805.08267.

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

pith.paper-citation-record.v1
1805.08267 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:46.065234Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T03:23:05.325995Z

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 836e1bfa-ed93-4c41-8b58-79169297109c · inbound

MUSE Imaging Spectroscopy of the Fullerene Planetary Nebula Tc 1 cites this paper.

MUSE Imaging Spectroscopy of the Fullerene Planetary Nebula Tc 1 Quantitative spectral classification of Galactic O stars

Reference 223

Resolution
verified exact
local_arxiv, observed 2026-06-26T03:18:58.003898Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a172d11b1b7571e032fa8bf64b716b5e786baf78e0a9676070705e9a77e0271a

Observation c34099b7-29fc-4f62-a752-adc034d7d07e · inbound

Southern Massive Stars at High Angular Resolution (SMaSH+): Properties of hierarchical massive triples cites this paper.

Southern Massive Stars at High Angular Resolution (SMaSH+): Properties of hierarchical massive triples Quantitative spectral classification of Galactic O stars

Reference 177

Resolution
verified exact
local_arxiv, observed 2026-06-29T03:23:05.327417Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:eb8eb9868bd4719e6c41dbd32a5cb759895f0cc8abfaa15ce0e7c86aff4644b1

Observation 0348582b-895b-43eb-b61b-a14994fb4d46 · inbound

Astro+ database. I. Description and first results cites this paper.

Astro+ database. I. Description and first results Quantitative spectral classification of Galactic O stars

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-14T04:14:15.925852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:14:15.925852Z digest=sha256:cb27e44365d9c1e41ffb519c3a23ae0ea8662873c985774e20f6880226027cba

Observation 18776ed2-fdd8-412c-bc57-394de4d9d0cd · 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 Quantitative spectral classification of Galactic O stars

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-12T12:11:54.168243Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T12:11:54.168243Z digest=sha256:12ae7c70ebf8eaab43153501ca3eb2e5fc999f9415106472a7800f7348ded908

Observation da2edfb8-bdfb-4310-adb9-10dca90afe72 · 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 Quantitative spectral classification of Galactic O stars

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:46.065234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:46.065234Z digest=sha256:38d2ed4cd7262fbd828a00a449de9f23310a3d795a83172fef9c268f573f9282