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Paper Citation Record · LEDGER

Using $^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2210.10804.

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

pith.paper-citation-record.v1
2210.10804 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:56.240936Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T20:25:20.894011Z

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 d05d7983-a1cb-46b3-b26b-ea045565cf36 · inbound

Type Ia supernovae cites this paper.

Type Ia supernovae Using $^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors

Reference 58

Resolution
verified exact
local_arxiv, observed 2026-08-12T20:25:20.898288Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-12T20:25:19.802304Z digest=sha256:ceacb598627032f0b705cb58bb591a395d3b31f7cb16fc938b02f8ee432357de

Observation c697d5d6-114b-4962-a3dd-d2ccdb0c9834 · inbound

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves cites this paper.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Using $^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors

Reference 111

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.240936Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.240936Z digest=sha256:e840a53c1a5758c9c5c8bfb5e627ca1cc52e31a6f1d3d2ec9f4ab666a72f4a2a