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Paper Citation Record · LEDGER

Neutrino-driven explosions of ultra-stripped type Ic supernovae generating binary neutron stars

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1506.08827.

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

pith.paper-citation-record.v1
1506.08827 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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T09:31:22.245618Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 3e1a76be-7a0f-4339-a28a-72d56f460189 · inbound

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions Neutrino-driven explosions of ultra-stripped type Ic supernovae generating binary neutron stars

Reference 240

Resolution
verified exact
local_arxiv, observed 2026-05-22T09:31:22.248456Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9519b7d014eff77614c7d5bc6d9f54f1f8ffb360409fed47ebc090ce18215896

Observation b240426f-af10-415e-8d4f-f84001040c7a · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins Neutrino-driven explosions of ultra-stripped type Ic supernovae generating binary neutron stars

Reference 230

Resolution
unresolved
no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:13d66589638f50baec7a29f807a0d1c970b25606d68cc7561b0420b537416c48