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Paper Citation Record · LEDGER

Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2405.20989.

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

pith.paper-citation-record.v1
2405.20989 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:47:24.310105Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1f79a432-3e91-4e1e-9072-c69ed96a3afa · inbound

SN 2023ixf: The Closest Supernova of the Decade cites this paper.

SN 2023ixf: The Closest Supernova of the Decade Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-06T18:34:12.164693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:34:12.164693Z digest=sha256:bdace62ee9fc875542ed58dfcf2c4ab6cd70ccd374fb52c5750f281e68d31ae0

Observation 097ed114-2ddd-46cd-9d0f-ee7724661a6f · inbound

SN 2023ixf in M101: physical parameters from bolometric light curve modeling cites this paper.

SN 2023ixf in M101: physical parameters from bolometric light curve modeling Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-05T22:43:50.991505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T22:43:50.991505Z digest=sha256:84a2157c152c58c726e3fae65bf917bba4c596bbe0793d3ee90708eb07df7800

Observation 5e7641c4-4c22-4c06-bc2e-96ae0fca2816 · inbound

Evidence for Asymmetric Ejecta and Circumstellar Material in SN 2023ixf Inferred from Extensive Nebular-phase Observations cites this paper.

Evidence for Asymmetric Ejecta and Circumstellar Material in SN 2023ixf Inferred from Extensive Nebular-phase Observations Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf

Reference 194

Resolution
verified exact
local_arxiv, observed 2026-07-12T06:38:33.525866Z

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=pdf_text observed=2026-07-12T06:33:42.823481Z digest=sha256:54af4c45cacc352068db66b8b0ebd9a91263603cdf3c9b87e9f894187a0f3db6

Observation 360043f3-99b8-4ed0-8e97-4563abd20932 · inbound

SN 2022xus: bridging the gap between Type IIP and IIL supernovae cites this paper.

SN 2022xus: bridging the gap between Type IIP and IIL supernovae Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf

Reference 126

Resolution
unresolved
no resolver link, observed 2026-08-01T02:50:51.305385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:50:51.305385Z digest=sha256:475ea576f94bc2c0155e9b39fd9af0c29637f30c12b1d15bdda24c20cab51e9c

Observation 5b70e62a-ede4-4a3e-9440-a110dc49b9c1 · inbound

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf cites this paper.

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf

Reference 119

Resolution
unresolved
no resolver link, observed 2026-08-14T13:47:24.310105Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:47:24.310105Z digest=sha256:172344350b476d56e3dfbf2988248eadad911ee88b20a58e8885442ee4546e39