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Paper Citation Record · LEDGER

A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1801.01293.

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

pith.paper-citation-record.v1
1801.01293 v2

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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T04:54:21.953406Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T08:09:40.859383Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 4997de1b-d6c4-41d7-930d-2405055d31b2 · inbound

A grid of fast-rotating, chemically-homogeneous, supernova and/or long-GRB progenitors cites this paper.

A grid of fast-rotating, chemically-homogeneous, supernova and/or long-GRB progenitors A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole

Reference 142

Resolution
verified exact
local_arxiv, observed 2026-07-04T08:09:40.861275Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-06-26T12:13:20.611828Z digest=sha256:82b59d1fc9e682e303aea02b33b4b241637bac92f8a1368b281eee8e6d1378bb

Observation c81fcf3e-a7d5-48a1-8843-b080bb3f155f · inbound

The petit four of color-superconducting phases in proto-neutron star evolution cites this paper.

The petit four of color-superconducting phases in proto-neutron star evolution A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole

Reference 80

Resolution
unresolved
no resolver link, observed 2026-07-14T04:54:21.953406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T04:54:21.953406Z digest=sha256:00b4ccf85fa816aa6a90c5e57a4aeabf1b6e42f3ee931d3b28957c41c34db29e