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Paper Citation Record · LEDGER

Supernova Model Discrimination with Hyper-Kamiokande

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2101.05269.

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

pith.paper-citation-record.v1
2101.05269 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 2026-05-11T01:00:34.989861Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T04:55:56.034366Z

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 5eae8377-48dd-40f1-95a6-fe2be0a9a9f6 · inbound

Probing Cosmic-Ray-Boosted and Supernova-Sourced Sub-GeV Dark Matter with Paleo-Detectors cites this paper.

Probing Cosmic-Ray-Boosted and Supernova-Sourced Sub-GeV Dark Matter with Paleo-Detectors Supernova Model Discrimination with Hyper-Kamiokande

Reference 82

Resolution
verified exact
arxiv_id, observed 2026-05-10T11:30:19.803365Z

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=pdf_text observed=2026-05-10T04:51:01.292668Z digest=sha256:da893ade52069d19656a0c58f80004a18a7d5fea34b412fa89f0ae8f59852e36

Observation de8362c8-ae84-494e-bd93-e44327385c50 · inbound

Neutrino-Antineutrino Conversion from Ultralight Vector Dark Matter cites this paper.

Neutrino-Antineutrino Conversion from Ultralight Vector Dark Matter Supernova Model Discrimination with Hyper-Kamiokande

Reference 70

Resolution
verified exact
arxiv_id, observed 2026-05-11T04:55:56.045387Z

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=pdf_text observed=2026-05-11T01:00:34.989861Z digest=sha256:bcd33a30c1b9fbde068319886040e6e9cbc7f4a19afec04039e7ca4505f200bc