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Paper Citation Record · LEDGER

Convection and the Core $g$-mode in Proto-Compact Stars -- A detailed analysis

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2405.01449.

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

pith.paper-citation-record.v1
2405.01449 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:16:46.693084Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T04:16:48.746269Z

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 8eccb092-46fa-4ee7-9bc2-aeda8a6bf7ef · inbound

The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations cites this paper.

The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations Convection and the Core $g$-mode in Proto-Compact Stars -- A detailed analysis

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-04T05:44:58.879700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T05:44:58.879700Z digest=sha256:ff7eb7f663b451d11dd2e693cd5ce0a11871be30ffba909b9114dcb7db8f8fd5

Observation b79aec4d-2b67-4151-96b3-db0ab66c765b · inbound

On the nature of oscillating modes of proto-neutron stars cites this paper.

On the nature of oscillating modes of proto-neutron stars Convection and the Core $g$-mode in Proto-Compact Stars -- A detailed analysis

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:16:48.759532Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:16:46.693084Z digest=sha256:632df812fa8e3d82a3d69b1a25d3b132b231deb488b89d2832bc3479977b22b0