Pith. sign in

Paper Citation Record · LEDGER

The Spiral Modes of the Standing Accretion Shock Instability

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1003.1730.

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

pith.paper-citation-record.v1
1003.1730 v2

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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:14.242738Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T12:45:44.504675Z

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 de4c3684-4173-42f6-957a-bbccd9c818d9 · inbound

Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass cites this paper.

Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass The Spiral Modes of the Standing Accretion Shock Instability

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-05-20T08:13:08.611709Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-20T08:10:13.936279Z digest=sha256:942b133a659bd7ca12ca4bff4f83ba20bf54f2c0dbceee7b1563e5580fea8233

Observation 2604a7d5-d3d6-4bd2-a44d-093740664cf9 · inbound

Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube cites this paper.

Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube The Spiral Modes of the Standing Accretion Shock Instability

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-07-01T12:45:44.506550Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-07-01T01:47:53.424100Z digest=sha256:6b02cce216d1445f92f95aa14564310caffca80c74bb530096736bd24c303a6c

Observation 9861a829-310d-4abd-be7f-8bb5e27ca0e2 · inbound

A "Neutrino Fog" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory cites this paper.

A "Neutrino Fog" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory The Spiral Modes of the Standing Accretion Shock Instability

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:14.242738Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:15:14.242738Z digest=sha256:5451f829c5226d85d3b0b12e86198e91a98293764acec70916abd5086affdc3f