Paper Citation Record · LEDGER

Modeling the Evolution from Massive Stars to Supernovae and Supernova Remnants

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2311.05612.

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

pith.paper-citation-record.v1
2311.05612 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T20:33:14.791007Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

3
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b922dea6-b083-45fb-8407-b2198afa6454 · inbound

Lecture Notes: WISPs in gamma-ray astrophysics cites this paper.

Lecture Notes: WISPs in gamma-ray astrophysics Modeling the Evolution from Massive Stars to Supernovae and Supernova Remnants

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-15T20:33:14.791007Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c7c33b6-4044-4e0f-8c53-8ff15609119a · inbound

Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets cites this paper.

Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets Modeling the Evolution from Massive Stars to Supernovae and Supernova Remnants

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-13T03:32:11.218578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation b1e664e9-a637-47cc-8a0a-e326637b12f8 · inbound

Building three-dimensional giant stellar models for common envelope simulations cites this paper.

Building three-dimensional giant stellar models for common envelope simulations Modeling the Evolution from Massive Stars to Supernovae and Supernova Remnants

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-06-27T08:30:45.580157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 623bdfa1-75f7-4b83-9412-ae908de99739 · inbound

Stellar black hole binaries from two common envelope evolution phases in triple stellar systems cites this paper.

Stellar black hole binaries from two common envelope evolution phases in triple stellar systems Modeling the Evolution from Massive Stars to Supernovae and Supernova Remnants

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-06-26T03:38:58.902507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.