Paper Citation Record · LEDGER

The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2502.11434.

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

pith.paper-citation-record.v1
2502.11434 v1

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measured 0 of 0 reference resolution

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measured 10 of 10 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 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T18:31:25.291585Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T14:57:04.689121Z

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Outbound references

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Pith citing papers

Observation 80cb41b0-666e-4f42-b24e-b7333625dab7 · inbound

Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data cites this paper.

Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T22:35:20.680257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ff5937d-7fdc-4d5b-8254-486ae2502f74 · inbound

`Dark' Matter Effect as a Novel Solution to the KM3-230213A Puzzle cites this paper.

`Dark' Matter Effect as a Novel Solution to the KM3-230213A Puzzle The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T13:09:35.144740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db124f82-8770-46ee-ae6b-b8e91817256d · inbound

The Highest-Energy Neutrino Event Constrains Dark Matter-Neutrino Interactions cites this paper.

The Highest-Energy Neutrino Event Constrains Dark Matter-Neutrino Interactions The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T05:04:03.320712Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 521af43c-29ca-42b4-be4e-bae2a43d6abc · inbound

Road through Dark$\nu$ess: Probing dark matter-neutrino interactions using KM3-230213A cites this paper.

Road through Dark$\nu$ess: Probing dark matter-neutrino interactions using KM3-230213A The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 111

Resolution: unresolved; no resolver link, observed 2026-08-15T18:31:25.291585Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d8e0943-001c-4d6f-b5aa-4d0e8a556a28 · inbound

Interpreting the KM3-230213A PeV Neutrino Event via Vector Dark Matter Decay and Its Multi-Messenger Signatures cites this paper.

Interpreting the KM3-230213A PeV Neutrino Event via Vector Dark Matter Decay and Its Multi-Messenger Signatures The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-06T12:57:16.442714Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c042f0e-5126-4db9-8616-239ec234aeb7 · inbound

Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A cites this paper.

Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-04T18:04:14.473611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b1c5cc7c-da4b-473e-a67f-6e86e32bed92 · inbound

Does the spectral break in the IceCube diffuse neutrino spectrum originate from AGN evolution? cites this paper.

Does the spectral break in the IceCube diffuse neutrino spectrum originate from AGN evolution? The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:46:53.749816Z

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 d7abe0d3-f469-4c5e-ac81-4eb7dc9a7c68 · inbound

Lepton interactions from GeV to EeV cites this paper.

Lepton interactions from GeV to EeV The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 228

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:57:04.690478Z

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 1a76b88b-a266-4877-8a2c-0d14b3cd63a3 · inbound

The KM3NeT 220 PeV event: a neutrino messenger from the grand unification scale? cites this paper.

The KM3NeT 220 PeV event: a neutrino messenger from the grand unification scale? The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 34

Resolution: unresolved; no resolver link, observed 2026-07-14T09:28:09.877419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e695c02-88ec-41e4-a5a4-df8cd7bd95e4 · inbound

Earth rotation turns event timing into a geometric probe of UHE neutrino origin cites this paper.

Earth rotation turns event timing into a geometric probe of UHE neutrino origin The blazar PKS 0605-085 as the origin of the KM3-230213A ultra high energy neutrino event

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-01T09:57:48.679891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.