Pith. sign in

Paper Citation Record · LEDGER

Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0507135.

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

pith.paper-citation-record.v1
astro-ph/0507135 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 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:29:17.367914Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T12:45:44.456848Z

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 ca95c755-f00a-4db5-b476-de2e09efec33 · inbound

Electron-neutrino lepton number crossings: Variations with the supernova core physics cites this paper.

Electron-neutrino lepton number crossings: Variations with the supernova core physics Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-06T16:29:17.367914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T16:29:17.367914Z digest=sha256:6d357977b5622463483e4a878a19d37c7f4920aa51cafc9f264b7c5ebe3be84f

Observation 470de211-857a-4b20-a4a3-4df753edf9b9 · 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 Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star

Reference 37

Resolution
verified exact
local_arxiv, observed 2026-07-01T12:45:44.458251Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-07-01T01:47:53.424100Z digest=sha256:700bc509839b182d05fbef2d759a6ec5be3b2b47b0ab5e721cdcf12c5d12a54c

Observation f6735e7c-e381-485f-a7dd-284ad56fcbde · inbound

Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae cites this paper.

Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star

Reference 110

Resolution
unresolved
no resolver link, observed 2026-08-01T23:35:22.197393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T23:35:22.197393Z digest=sha256:c827eb7d9c537c244371f382ea18ee9aad86021ccbcaffa81d106a1d745892c3

Observation 4db3dfac-94eb-4a0a-8aaa-826c015120c1 · inbound

Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations cites this paper.

Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-01T04:14:01.592856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T04:14:01.592856Z digest=sha256:d9fbae0bdfdd9aad28c605d7d96a2fa3ace3d7977ae20f4f4b3427ccd4ec74c2