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Paper Citation Record · LEDGER

The vela supernova remnant: The unique morphological features of jittering jets

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2409.02626.

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

pith.paper-citation-record.v1
2409.02626 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T21:35:45.719699Z

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

1
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 84a5d06b-3e38-4334-931c-7b9a16740a94 · inbound

The two alternative explosion mechanisms of core-collapse supernovae: 2024 status report cites this paper.

The two alternative explosion mechanisms of core-collapse supernovae: 2024 status report The vela supernova remnant: The unique morphological features of jittering jets

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-12T21:35:45.719699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T21:35:45.719699Z digest=sha256:0f556bf1362e4a98a35846e527433d9291d5941ea99df7dc20051332ed2db503

Observation 754edc7a-9a9c-48e2-bc58-3db63b058cc1 · inbound

The main jet axis of the W49B supernova remnant cites this paper.

The main jet axis of the W49B supernova remnant The vela supernova remnant: The unique morphological features of jittering jets

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-07T21:09:31.070157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T21:09:31.070157Z digest=sha256:f104a3db0e0fa994a4dea73d78868f67a7045d34eff3564435211b9a594914ea

Observation 23550a2d-3543-4743-b202-20797b074144 · inbound

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

Building three-dimensional giant stellar models for common envelope simulations The vela supernova remnant: The unique morphological features of jittering jets

Reference 101

Resolution
verified exact
arxiv_id, observed 2026-06-27T08:30:45.300283Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-06-27T08:27:59.759564Z digest=sha256:81706ea4b102b30fecc27739e894d1cf4cfce0523db1b9ddbf2aefd24d96febd