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Paper Citation Record · LEDGER

The Rate of Supernovae. II. the Selection Effects and the Frequencies Per Unit Blue Luminosity

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9302017.

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

pith.paper-citation-record.v1
astro-ph/9302017 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:15:31.865714Z

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

  • verified exact0
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External citation measurements

6
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 875e8e92-c11c-40ec-8a11-3f5614bc7919 · inbound

An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo cites this paper.

An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo The Rate of Supernovae. II. the Selection Effects and the Frequencies Per Unit Blue Luminosity

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-14T14:15:31.865714Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:15:31.865714Z digest=sha256:06533cd6c31cba45b513698bcdf33e9739f448ebb4dee19bf4a76c9ead0106e5

Observation 1b7e98dc-86c7-488b-8803-65c2dc9b46c0 · inbound

What shall we learn from a future supernova? cites this paper.

What shall we learn from a future supernova? The Rate of Supernovae. II. the Selection Effects and the Frequencies Per Unit Blue Luminosity

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-11T10:58:39.557410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T10:58:39.557410Z digest=sha256:feb9a8a12a2af8078d96a72a951040dfcf60c201d0bcd9b09319088193d38fd4

Observation 4ac9d8b1-47b2-4855-8d3a-d0210b7411ab · inbound

Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors cites this paper.

Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors The Rate of Supernovae. II. the Selection Effects and the Frequencies Per Unit Blue Luminosity

Reference 174

Resolution
verified exact
local_arxiv, observed 2026-07-09T20:56:34.269388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-09T20:48:05.724078Z digest=sha256:5e31f6f056e30fe5ea16eddc63dabf4c9fb3411865ad13e5b7868b8fbbc2cb17