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Paper Citation Record · LEDGER

The Most Luminous Supernovae

As of 18 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1812.01428.

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

pith.paper-citation-record.v1
1812.01428 v1

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 2026-07-18T06:30:57.431901+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T04:51:42.156415Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T07:32:00.422476Z

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 68a3ed1b-eea0-4309-9e52-2d3aba719a25 · inbound

On the Gamma-ray Efficiency of Superluminous Supernovae: Potential Detections and Population-Level Constraints cites this paper.

On the Gamma-ray Efficiency of Superluminous Supernovae: Potential Detections and Population-Level Constraints The Most Luminous Supernovae

Reference 3

Resolution
verified exact
arxiv_id, observed 2026-05-10T07:32:00.423881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-18T06:30:57.431901+00:00.

source=pdf_text observed=2026-05-10T07:28:20.494507Z digest=sha256:318f858e9b259b0633771b8a270a3184caae8a559e1c16a6385bb737082a60e7

Observation 0ca4e140-7f16-438b-a8f6-b87f93a0d585 · inbound

AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission cites this paper.

AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission The Most Luminous Supernovae

Reference 64

Resolution
unresolved
no resolver link, observed 2026-07-14T04:51:42.156415Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T04:51:42.156415Z digest=sha256:549523a0a7720a0ee11ff063797e294c1dd67c2f744ec88843c5c7eb308cfca4