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Paper Citation Record · LEDGER

Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1101.3336.

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

pith.paper-citation-record.v1
1101.3336 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:20:28.210142Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T14:24:19.742423Z

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 e90d01b0-c604-4a60-84f5-fe81b506a60c · inbound

Origins of Supermassive Black Holes in Galactic Centers cites this paper.

Origins of Supermassive Black Holes in Galactic Centers Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout

Reference 11

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:24:19.843643Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:24:14.415330Z digest=sha256:8d5995ff10d653d1fa2902b5a79cce3fade60f243a47374d79440ffecfda50cc

Observation f7808864-dc22-4e47-9f80-85a3efa839e7 · inbound

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf cites this paper.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout

Reference 152

Resolution
unresolved
no resolver link, observed 2026-08-10T04:20:28.210142Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:20:28.210142Z digest=sha256:8db4cbc29da5a4be4fdad1080c1ef962c584be83285a5cb98614eab0d98c0200