Pith. sign in

Paper Citation Record · LEDGER

Is the bowshock of the runaway massive star HD 195592 a Fermi source?

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1212.1549.

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

pith.paper-citation-record.v1
1212.1549 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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:46.572227Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T12:11:56.729628Z

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 9bfa7071-d19f-49b1-a1d7-4b190c619efc · 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 Is the bowshock of the runaway massive star HD 195592 a Fermi source?

Reference 69

Resolution
verified exact
local_arxiv, observed 2026-08-12T12:11:56.747580Z

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=2026-08-12T12:11:54.286374Z digest=sha256:adc3646e82b7909f2386680789ca50079ec80a1a368060781c50d8b044fb7d68

Observation aafead1b-59e6-44c4-97f6-ee77fa856166 · 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 Is the bowshock of the runaway massive star HD 195592 a Fermi source?

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:46.572227Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:46.572227Z digest=sha256:f77a5740020a113820dcf646290b99078312e97d6209828530bcb43fbeecb86e