Paper Citation Record · LEDGER

Interacting supernovae

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2405.04259.

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

pith.paper-citation-record.v1
2405.04259 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 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 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T23:47:06.178234Z

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

2
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 d88cd368-dbca-4a6b-8c5d-f7cf90e8847a · inbound

A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow cites this paper.

A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow Interacting supernovae

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T20:28:08.768652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3742fc10-37eb-48f0-bd87-2d54e735d9ee · inbound

Signatures of the Shock Interaction as an Additional Power Source in the Nebular Spectra of SN 2023ixf cites this paper.

Signatures of the Shock Interaction as an Additional Power Source in the Nebular Spectra of SN 2023ixf Interacting supernovae

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T22:24:45.238049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 93f65c82-5da3-4655-aa7d-b5fc6402faa9 · inbound

Spectropolarimetric Evolution of SN 2023ixf: an Asymmetric Explosion in a Confined Aspherical Circumstellar Medium cites this paper.

Spectropolarimetric Evolution of SN 2023ixf: an Asymmetric Explosion in a Confined Aspherical Circumstellar Medium Interacting supernovae

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-15T23:47:06.178234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 26757444-cfcf-4849-a057-0d546d9c20f7 · inbound

Explosion sites of SN 1994W-like transients cites this paper.

Explosion sites of SN 1994W-like transients Interacting supernovae

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T14:49:32.010113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e57c3b65-99f1-4160-ba97-2d9885dad08e · inbound

Giant outbursts of clumpy material preceding Type II supernova 2024qiw cites this paper.

Giant outbursts of clumpy material preceding Type II supernova 2024qiw Interacting supernovae

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-17T00:01:22.860020Z

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.

Observation 558fb560-4ac3-4877-8e0c-b6f612479492 · inbound

Evolved massive stars and their impact on their environment cites this paper.

Evolved massive stars and their impact on their environment Interacting supernovae

Reference 23

Resolution: malformed identifier; arxiv_id, observed 2026-07-04T20:50:12.666681Z

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.

Observation fd78cb96-b11c-4ca7-913a-cd1e4f7cb335 · inbound

Evolved massive stars and their impact on their environment cites this paper.

Evolved massive stars and their impact on their environment Interacting supernovae

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-06-25T19:28:17.120657Z

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.

Observation 0193f13f-096b-4213-bcb2-ef9c1a98cdd0 · inbound

Two years of shock interaction tracing three phases of evolution: the explosion of a Type IIn supernova, SN 2019vxm cites this paper.

Two years of shock interaction tracing three phases of evolution: the explosion of a Type IIn supernova, SN 2019vxm Interacting supernovae

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-06-25T19:18:16.436550Z

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.

Observation de534c0e-69af-4449-a5d6-a18461628e38 · inbound

SN 2019vxm: A luminous and long-lived Type IIn supernova with early flash-ionisation features cites this paper.

SN 2019vxm: A luminous and long-lived Type IIn supernova with early flash-ionisation features Interacting supernovae

Reference 141

Resolution: verified exact; arxiv_id, observed 2026-06-30T04:14:19.040269Z

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.

Observation bb39ab47-2831-45c9-9e01-723d7af7ba65 · inbound

Same explosion, many faces: numerical modeling reveals viewing angle as a driver of diversity for core-collapse SNe in binary systems cites this paper.

Same explosion, many faces: numerical modeling reveals viewing angle as a driver of diversity for core-collapse SNe in binary systems Interacting supernovae

Reference 27

Resolution: unresolved; no resolver link, observed 2026-07-31T04:49:53.699569Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8906bfc2-eb04-44fa-b31b-d659b437be67 · inbound

Same explosion, many faces: numerical modeling reveals viewing angle as a driver of diversity for core-collapse SNe in binary systems cites this paper.

Same explosion, many faces: numerical modeling reveals viewing angle as a driver of diversity for core-collapse SNe in binary systems Interacting supernovae

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-05T04:27:08.624623Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.