{"as_of":"2026-08-17T15:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e54d358a9c6ee15018782e5c999bfb115e7dda8a1b8c63b8bdb660526c299595","coverage":[{"denominator":55,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":55,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T17:03:19.134236Z","state":"measured"},{"denominator":59,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":59,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-30T20:23:28.071405Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"cited_work":{"arxiv_id":"2507.11993","doi":"10.48550/arxiv.2507.11993","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.11993","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv preprint arXiv:2507.11993, doi: 10.48550/arXiv.2507.11993","venue":"ArXiv.org","work_id":"463a8abc-96da-4f8e-9f60-40a50570012a","year":2025},"citing_paper":{"arxiv_id":"2509.09590","last_updated":"2026-02-20T17:10:50Z","snapshot_observed_at":"2026-08-13T05:14:15.436183Z","submitted_at":"2025-09-11T16:29:11Z","title":"Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-18T17:43:40.852227Z"},"links":{"cited_paper":"/paper/2507.11993","citing_paper":"/paper/2509.09590"},"observation_digest":"sha256:450a3c4dff15ec2768e0ebeb60fc49fe512cf8f3053e7d7d44ebd6e6b9c81ba0","observation_id":"23a8d084-8ade-4b2b-834e-1f62bf11c7d9","resolution":{"observed_at":"2026-05-18T17:46:42.277429Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"cited_work":{"arxiv_id":"2507.11993","doi":"10.48550/arxiv.2507.11993","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.11993","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv preprint arXiv:2507.11993, doi: 10.48550/arXiv.2507.11993","venue":"ArXiv.org","work_id":"463a8abc-96da-4f8e-9f60-40a50570012a","year":2025},"citing_paper":{"arxiv_id":"2603.13476","last_updated":"2026-05-22T10:49:56Z","snapshot_observed_at":"2026-08-16T20:40:43.117012Z","submitted_at":"2026-03-13T18:00:07Z","title":"Implications of a Cosmogenic Origin of KM3-230213A for Ultra-High-Energy Protons","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-25T07:24:45.543013Z"},"links":{"cited_paper":"/paper/2507.11993","citing_paper":"/paper/2603.13476"},"observation_digest":"sha256:9dd7abccc5c7f6597798a8310ca2bc3d3b28d2c608497c127d93760793c2e18b","observation_id":"ffc26bb8-56ce-4d78-83b2-1ee1006d250f","resolution":{"observed_at":"2026-05-25T07:25:27.480164Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"cited_work":{"arxiv_id":"2507.11993","doi":"10.48550/arxiv.2507.11993","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.11993","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv preprint arXiv:2507.11993, doi: 10.48550/arXiv.2507.11993","venue":"ArXiv.org","work_id":"463a8abc-96da-4f8e-9f60-40a50570012a","year":2025},"citing_paper":{"arxiv_id":"2605.07641","last_updated":"2026-05-08T12:08:42Z","snapshot_observed_at":"2026-08-13T07:52:35.212527Z","submitted_at":"2026-05-08T12:08:42Z","title":"KM3-230213A and potential astrophysical sources","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-11T01:52:37.944334Z"},"links":{"cited_paper":"/paper/2507.11993","citing_paper":"/paper/2605.07641"},"observation_digest":"sha256:dc598c62f35f5a5bb3beacce3f3395bc76d377fc743324f11d9f1870bbcac826","observation_id":"84b1f68c-8b74-4f7e-9c6b-74bd65f25fe4","resolution":{"observed_at":"2026-05-11T04:15:57.770251Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"cited_work":{"arxiv_id":"2507.11993","doi":"10.48550/arxiv.2507.11993","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.11993","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv preprint arXiv:2507.11993, doi: 10.48550/arXiv.2507.11993","venue":"ArXiv.org","work_id":"463a8abc-96da-4f8e-9f60-40a50570012a","year":2025},"citing_paper":{"arxiv_id":"2605.14869","last_updated":"2026-05-14T14:17:37Z","snapshot_observed_at":"2026-08-14T02:17:16.305663Z","submitted_at":"2026-05-14T14:17:37Z","title":"Self-confinement of ultra-high-energy nuclei in cosmic filaments: implications for the UHECR spectrum and composition","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-06-30T20:23:28.071405Z"},"links":{"cited_paper":"/paper/2507.11993","citing_paper":"/paper/2605.14869"},"observation_digest":"sha256:fc3eea84a23e995213ac0e3929d98a98994d153cbf612d7e9c83ad5d158a0499","observation_id":"4d8eb1dc-6dc3-44d4-86af-0cc0798db0dd","resolution":{"observed_at":"2026-06-30T20:25:02.423041Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.11993/citation-record","integrity":"/paper/2507.11993/integrity","json":"/paper/2507.11993/citation-record.json","paper":"/paper/2507.11993"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.973737Z","title":"Aiello et al","venue":null,"work_id":"647df29f-c379-43f8-90a8-ea78580d11bf","year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:14.968331Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:cb6fb07fb0cb2836e13e6a72f86b0234ff0b5fe93121f009c54214cef81cc389","observation_id":"197a02da-067c-446c-8ccc-e767cf597783","resolution":{"observed_at":"2026-08-06T17:03:22.064939Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.04361","last_updated":"2023-08-08T16:03:57Z","snapshot_observed_at":"2026-08-16T15:09:55.306772Z","submitted_at":"2023-08-08T16:03:57Z","title":"Cosmic ray interactions with matter and radiation","version":1},"cited_work":{"arxiv_id":"2308.04361","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.04361","snapshot_observed_at":"2026-08-06T17:03:20.433149Z","title":"Cosmic ray interactions with matter and radiation","venue":"astro-ph.HE","work_id":"eb1bc1cc-735f-4c79-8d9e-d3b476e3713d","year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.076333Z"},"links":{"cited_paper":"/paper/2308.04361","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:e6e94474b5748d3459c03196ee70400c1c012d903c94f7d7cd9be93d4bd68f45","observation_id":"272ee444-8ccd-4a28-a5a3-d731e4c6bd32","resolution":{"observed_at":"2026-08-06T17:03:20.513925Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.12743","last_updated":"2023-09-22T09:44:55Z","snapshot_observed_at":"2026-08-16T14:58:29.917925Z","submitted_at":"2023-09-22T09:44:55Z","title":"Cosmic-ray propagation in extragalactic space and secondary messengers","version":1},"cited_work":{"arxiv_id":"2309.12743","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.12743","snapshot_observed_at":"2026-08-06T17:03:20.267734Z","title":"Cosmic-ray propagation in extragalactic space and secondary messengers","venue":"astro-ph.HE","work_id":"60d45d2e-36d7-4056-8e5c-695b2628f5fb","year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.131064Z"},"links":{"cited_paper":"/paper/2309.12743","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:eb54aa4d7a418bf3aa86cf1e9fc49ba8b68407adb9fe355efb2aa17c6d6d7195","observation_id":"8b442598-ef33-43f4-9079-cad499587e54","resolution":{"observed_at":"2026-08-06T17:03:20.364967Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.03989","last_updated":"2016-03-13T03:53:34Z","snapshot_observed_at":"2026-08-14T22:06:18.852058Z","submitted_at":"2016-03-13T03:53:34Z","title":"High energy electromagnetic cascades in extragalactic space: physics and features","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.03989","snapshot_observed_at":"2026-08-06T17:03:15.203124Z","title":"Berezinsky and O","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.203124Z"},"links":{"cited_paper":"/paper/1603.03989","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:761be8488427275fff7ef3a8a3b308b96ee3803b71c071b10a24dcfb09a4ae82","observation_id":"4fbc7048-aaf2-4710-82ce-1820aa33fe7c","resolution":{"observed_at":"2026-08-06T17:03:15.203124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.06486","last_updated":"2020-10-06T12:41:09Z","snapshot_observed_at":"2026-08-16T04:52:53.829514Z","submitted_at":"2020-08-14T17:43:36Z","title":"Measurement of the cosmic-ray energy spectrum above $2.5{\\times} 10^{18}$ eV using the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.06486","snapshot_observed_at":"2026-08-06T17:03:15.307165Z","title":"Aab et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.307165Z"},"links":{"cited_paper":"/paper/2008.06486","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:96d7c506fb97c4be34d0fb3e488957da687a79a403e7fda1b167cddba593c70f","observation_id":"71b9bcbe-4c04-4df6-aa90-20df2020a831","resolution":{"observed_at":"2026-08-06T17:03:15.307165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.843485Z","title":"Abreu et al","venue":null,"work_id":"d18bbc63-5970-42ff-b646-405a3154ca6d","year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.374120Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:3a3fb9f8e662f4a16a4f55bd0838138ebd4dac34b0b369dd7e47db9ef4de8c00","observation_id":"f9a834fe-c2c4-4781-9159-ef57ad4b3e37","resolution":{"observed_at":"2026-08-06T17:03:21.910950Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.684366Z","title":"Abdul Halim et al","venue":null,"work_id":"7d2412d4-25bb-4983-9f4e-d41ca9e8aa1e","year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.462578Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:a6e7e677eeb79ba3cf2b4f9dfb6aef629ed287a9127ba3c96d650733ffa73bdb","observation_id":"45607313-6636-4338-b5c0-14fe2a81d624","resolution":{"observed_at":"2026-08-06T17:03:21.763119Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.04020","last_updated":"2015-10-06T15:40:54Z","snapshot_observed_at":"2026-08-14T22:48:26.695967Z","submitted_at":"2015-05-15T10:54:17Z","title":"Cosmogenic neutrinos and ultra-high energy cosmic ray models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.04020","snapshot_observed_at":"2026-08-06T17:03:15.525291Z","title":"Aloisio, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.525291Z"},"links":{"cited_paper":"/paper/1505.04020","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:6d8c36de4182243fbb8c2b4684c3d9da200b6a548d9fcb66e83ab668cae6ff54","observation_id":"951d2184-b3f3-4b6d-a609-c11b2f74beb0","resolution":{"observed_at":"2026-08-06T17:03:15.525291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.05988","last_updated":"2016-07-15T14:23:56Z","snapshot_observed_at":"2026-08-14T22:17:54.173377Z","submitted_at":"2015-12-18T15:22:03Z","title":"Cosmogenic Neutrinos Challenge the Cosmic Ray Proton Dip Model","version":4},"cited_work":{"arxiv_id":"1512.05988","doi":null,"metadata_source":"pith","pith_arxiv_id":"1512.05988","snapshot_observed_at":"2026-08-06T17:03:20.076355Z","title":"Cosmogenic Neutrinos Challenge the Cosmic Ray Proton Dip Model","venue":"astro-ph.HE","work_id":"427d655b-4fb3-477e-932d-d71ae745571a","year":2015},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.594081Z"},"links":{"cited_paper":"/paper/1512.05988","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:95de7c1e0f9744f6b124b2ada499e41de19be067cfdbc37545d8126dcd95151d","observation_id":"3e2b4cf4-1b76-4834-ab1c-0c2172ecbf0c","resolution":{"observed_at":"2026-08-06T17:03:20.190331Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.10879","last_updated":"2019-01-03T19:02:21Z","snapshot_observed_at":"2026-08-14T18:58:07.025130Z","submitted_at":"2018-06-28T11:10:30Z","title":"Cosmogenic photon and neutrino fluxes in the Auger era","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.10879","snapshot_observed_at":"2026-08-06T17:03:15.685998Z","title":"Alves Batista, R","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.685998Z"},"links":{"cited_paper":"/paper/1806.10879","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:f10d8dc5c04fdac8a19ddf0f7237e9f3c0ecba35329a3657a28e935106d961eb","observation_id":"147c4251-2229-48de-928b-08fed1b26fa5","resolution":{"observed_at":"2026-08-06T17:03:15.685998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03338","last_updated":"2019-02-11T16:36:01Z","snapshot_observed_at":"2026-08-17T03:55:12.375034Z","submitted_at":"2019-01-10T19:00:02Z","title":"A new view on Auger data and cosmogenic neutrinos in light of different nuclear disintegration and air-shower models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03338","snapshot_observed_at":"2026-08-06T17:03:15.760735Z","title":"Heinze, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.760735Z"},"links":{"cited_paper":"/paper/1901.03338","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:a417fe00355781732343a9ec15685a8141b34b2ad9ed415564e7fbf25ff7d14d","observation_id":"139649ad-6a7e-4d84-a60d-b30dd6b188ed","resolution":{"observed_at":"2026-08-06T17:03:15.760735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.07321","last_updated":"2024-03-06T15:37:22Z","snapshot_observed_at":"2026-08-16T15:40:20.936089Z","submitted_at":"2023-04-14T18:00:08Z","title":"Constraints on the proton fraction of cosmic rays at the highest energies and the consequences for cosmogenic neutrinos and photons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.07321","snapshot_observed_at":"2026-08-06T17:03:15.836690Z","title":"Ehlert, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.836690Z"},"links":{"cited_paper":"/paper/2304.07321","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:d9cc895d835600c3982692b700ac6b14064378f1e8a527a941f6dc989fd70641","observation_id":"2d09021b-cca6-4027-a55e-555b4753bef2","resolution":{"observed_at":"2026-08-06T17:03:15.836690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.01899","last_updated":"2019-09-03T12:25:30Z","snapshot_observed_at":"2026-08-15T11:41:33.986472Z","submitted_at":"2019-01-07T16:19:09Z","title":"Determining the fraction of cosmic-ray protons at ultra-high energies with cosmogenic neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.01899","snapshot_observed_at":"2026-08-06T17:03:15.895512Z","title":"van Vliet, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.895512Z"},"links":{"cited_paper":"/paper/1901.01899","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:f779368608eb1f691294e5f3aaba4b1d4998fdd413433dbdaedf02737725fb16","observation_id":"cd00a73c-0fe6-4205-8aeb-39282169762d","resolution":{"observed_at":"2026-08-06T17:03:15.895512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07422","last_updated":"2019-10-16T17:51:24Z","snapshot_observed_at":"2026-08-16T04:52:50.660939Z","submitted_at":"2019-06-18T07:45:55Z","title":"Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07422","snapshot_observed_at":"2026-08-06T17:03:15.977436Z","title":"Aab et al","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:15.977436Z"},"links":{"cited_paper":"/paper/1906.07422","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:bc8e968c3a03239ad3395730b6b0df1f1fe792f04eefe5f4eb450218ea1a50cd","observation_id":"325e1618-24a3-4df7-bcd7-cd2cdc259894","resolution":{"observed_at":"2026-08-06T17:03:15.977436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.521990Z","title":"Abdul Halim et al","venue":null,"work_id":"9d394171-b4d1-4db0-b6dd-fbf3005a8497","year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.023858Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:6edaabc8572fa0415fe5805951ed019bbbbfdc79fd8de7607d463c6bbcada532","observation_id":"20d27da6-109b-4b03-9f92-db3c90f9ad9f","resolution":{"observed_at":"2026-08-06T17:03:21.592479Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.04170","last_updated":"2023-05-14T18:09:22Z","snapshot_observed_at":"2026-08-16T15:50:01.846404Z","submitted_at":"2023-03-07T19:00:03Z","title":"Prospects for joint cosmic ray and neutrino constraints on the evolution of trans-GZK proton sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.04170","snapshot_observed_at":"2026-08-06T17:03:16.085704Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.085704Z"},"links":{"cited_paper":"/paper/2303.04170","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:4e8ccfbdc949d89bec48abdf208bb35e3c8c1bee915a7214fad67a113d157c73","observation_id":"8def2f13-664a-4a10-b944-09ef2cc9e727","resolution":{"observed_at":"2026-08-06T17:03:16.085704Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:16.167383Z","title":"Abbasi et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.167383Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:9110790d6d442154f945358c0b95bd9f61d7eedb120aadf6cffd1753f4aa317f","observation_id":"94938849-103f-4e5c-993f-e108b2ad6b9e","resolution":{"observed_at":"2026-08-06T17:03:16.167383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.08508","last_updated":"2025-02-12T15:43:30Z","snapshot_observed_at":"2026-08-17T08:53:58.301263Z","submitted_at":"2025-02-12T15:43:30Z","title":"On the potential cosmogenic origin of the ultra-high-energy event KM3-230213A","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.08508","snapshot_observed_at":"2026-08-06T17:03:16.224553Z","title":"Adriani et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.224553Z"},"links":{"cited_paper":"/paper/2502.08508","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:050640e470f05c67bcea862d2e4ce04eeadbfbb47ac24e08e89a89b1949436fb","observation_id":"17bba9aa-23f2-4559-a295-7ad23e45c8ee","resolution":{"observed_at":"2026-08-06T17:03:16.224553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04508","last_updated":"2025-02-26T23:41:29Z","snapshot_observed_at":"2026-08-16T16:13:33.281785Z","submitted_at":"2025-02-06T21:17:34Z","title":"Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04508","snapshot_observed_at":"2026-08-06T17:03:16.289495Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.289495Z"},"links":{"cited_paper":"/paper/2502.04508","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:37b9f6fa31abb45d807df027fadd16adacd04e1014e1744356569367737586cc","observation_id":"caf0eb37-509d-4d52-bbac-2eb6058bba7c","resolution":{"observed_at":"2026-08-06T17:03:16.289495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.10378","last_updated":"2025-07-18T04:01:20Z","snapshot_observed_at":"2026-08-16T12:41:16.171929Z","submitted_at":"2025-04-14T16:24:52Z","title":"Cosmogenic Neutrino Point Source and KM3-230213A","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.10378","snapshot_observed_at":"2026-08-06T17:03:16.363568Z","title":"Zhang, T.-Q","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.363568Z"},"links":{"cited_paper":"/paper/2504.10378","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:614ab16108c2dde9057bd61d1f95317aae997da8152f9139429693360d85acbd","observation_id":"3e356d75-621f-4e16-99fe-9f0f58ad77eb","resolution":{"observed_at":"2026-08-06T17:03:16.363568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.06944","last_updated":"2025-02-12T19:16:57Z","snapshot_observed_at":"2026-08-17T14:07:46.444044Z","submitted_at":"2025-02-10T19:00:01Z","title":"Emergence of a neutrino flux above 5 PeV and implications for ultrahigh energy cosmic rays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.06944","snapshot_observed_at":"2026-08-06T17:03:16.445504Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.445504Z"},"links":{"cited_paper":"/paper/2502.06944","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:e205a9f8a011175a1c10e89a630e6482192982fa293c8ecc903a7f47fc508bf8","observation_id":"e6dbf3de-fa84-447f-8bb0-339f98e191c0","resolution":{"observed_at":"2026-08-06T17:03:16.445504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:16.510908Z","title":"Abdul Halim et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.510908Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:23574a99fc47f02aa2f6d5681511c3759a8976ab7edb2827143c82b252d1bc97","observation_id":"2ea10d24-2ee6-48f9-9750-ee92e3a34ba9","resolution":{"observed_at":"2026-08-06T17:03:16.510908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.08173","last_updated":"2025-02-12T07:27:40Z","snapshot_observed_at":"2026-08-16T06:37:13.172397Z","submitted_at":"2025-02-12T07:27:40Z","title":"The ultra-high-energy event KM3-230213A within the global neutrino landscape","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.08173","snapshot_observed_at":"2026-08-06T17:03:16.598859Z","title":"Adriani et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.598859Z"},"links":{"cited_paper":"/paper/2502.08173","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:1d35e6108083ffee34fa220aaaa894e92b594c037105036d6480b1a71f838d2d","observation_id":"7981c390-1a55-47bf-b1a7-5c92c25369cc","resolution":{"observed_at":"2026-08-06T17:03:16.598859Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.3696","last_updated":"2014-10-14T14:05:04Z","snapshot_observed_at":"2026-08-14T23:15:48.113740Z","submitted_at":"2014-10-14T14:05:04Z","title":"The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.3696","snapshot_observed_at":"2026-08-06T17:03:16.682427Z","title":"Ackermann et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.682427Z"},"links":{"cited_paper":"/paper/1410.3696","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:07aebe616c2bd9ed3bfcd56002246b9d6ca1a7a0d31ecc1e9fe2877159dd5125","observation_id":"08416719-0462-4b0c-a9c4-734484cc8609","resolution":{"observed_at":"2026-08-06T17:03:16.682427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.13400","last_updated":"2022-04-20T13:22:22Z","snapshot_observed_at":"2026-08-16T17:53:37.251654Z","submitted_at":"2021-09-27T23:54:49Z","title":"The energy spectrum of cosmic rays beyond the turn-down around $10^{17}$ eV as measured with the surface detector of the Pierre Auger Observatory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.13400","snapshot_observed_at":"2026-08-06T17:03:16.746100Z","title":"Abreu et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.746100Z"},"links":{"cited_paper":"/paper/2109.13400","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:d8b153376f917e3c85d6c1aa60d46443bbd85a02c92bffa95fce5260e4338da5","observation_id":"08e9ebdf-d249-44d7-944c-f8ebf36335bb","resolution":{"observed_at":"2026-08-06T17:03:16.746100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.379395Z","title":null,"venue":null,"work_id":"ff069c28-aa3d-4a73-ab23-6fd81077b294","year":2018},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.822689Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:186e8ccffa289e9b1f997d850a5705455cfcb85b144a22be8ef84d016ff7753f","observation_id":"28be9b36-0f7b-436a-ba43-c9bc7f790f30","resolution":{"observed_at":"2026-08-06T17:03:21.444459Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.04317","last_updated":"2019-11-12T19:06:25Z","snapshot_observed_at":"2026-08-14T16:17:47.114771Z","submitted_at":"2019-06-10T23:13:25Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV Using 3 Years of Data From IceTop and IceCube","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.04317","snapshot_observed_at":"2026-08-06T17:03:16.888320Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.888320Z"},"links":{"cited_paper":"/paper/1906.04317","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:2d9b4186ceaacfdf97fe2779f9cfc17f0d9acc3bdb994b1015215d4e95452f53","observation_id":"1e985c20-6168-459b-9976-40f4b72968ba","resolution":{"observed_at":"2026-08-06T17:03:16.888320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:16.937276Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:16.937276Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:5ea1fcae02f00480d39d319c9dec61e9f3705e3991d8a6c04664900664927e4f","observation_id":"36dee60c-e6c2-4f92-b67e-5c0e1ffb44d5","resolution":{"observed_at":"2026-08-06T17:03:16.937276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:17.015922Z","title":"Abbasi et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.015922Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:8aff7b3cf099c65e6662657ea60bd77f729aad51d9b5c31f63f2bb8d8b082b28","observation_id":"eba758f1-a6b8-4b5b-be83-73e11d38405c","resolution":{"observed_at":"2026-08-06T17:03:17.015922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:17.110410Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.110410Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:3385ecb3523746a4e7894f0a49631b0c03a56ed8329b9da8a17ea31af5274fcd","observation_id":"5127de43-7af9-4846-81a5-d38553bc92ff","resolution":{"observed_at":"2026-08-06T17:03:17.110410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00328","last_updated":"2024-08-27T06:45:08Z","snapshot_observed_at":"2026-08-17T04:20:56.816458Z","submitted_at":"2024-06-29T06:06:00Z","title":"Constraints on the energy spectrum of the diffuse cosmic neutrino flux from the ANTARES neutrino telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00328","snapshot_observed_at":"2026-08-06T17:03:17.196335Z","title":"Albert et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.196335Z"},"links":{"cited_paper":"/paper/2407.00328","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:86f47429aae55a2ccc2a5eb389531f7f28835c315e631ffa15776f4ccb27ea4a","observation_id":"d07a99e2-f687-4208-bb72-a4e79e391404","resolution":{"observed_at":"2026-08-06T17:03:17.196335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.06315","last_updated":"2025-02-06T14:49:48Z","snapshot_observed_at":"2026-08-16T13:44:32.472249Z","submitted_at":"2024-06-10T14:32:10Z","title":"Inference of the Mass Composition of Cosmic Rays with energies from $\\mathbf{10^{18.5}}$ to $\\mathbf{10^{20}}$ eV using the Pierre Auger Observatory and Deep Learning","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.06315","snapshot_observed_at":"2026-08-06T17:03:17.282146Z","title":"Abdul Halim et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.282146Z"},"links":{"cited_paper":"/paper/2406.06315","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:7f04b266c40ae2cee2ed1db73888cfe62304c6113d3c18f3fb4719f5990adcd9","observation_id":"7316a29d-5908-43d8-94ca-12c3bef41f9a","resolution":{"observed_at":"2026-08-06T17:03:17.282146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.02483","last_updated":"2021-03-31T13:18:26Z","snapshot_observed_at":"2026-08-17T12:41:08.167872Z","submitted_at":"2020-11-04T19:00:00Z","title":"Starburst galaxies strike back: a multi-messenger analysis with Fermi-LAT and IceCube data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.02483","snapshot_observed_at":"2026-08-06T17:03:17.335001Z","title":"Ambrosone, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.335001Z"},"links":{"cited_paper":"/paper/2011.02483","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:c397cd9e42a73b8e8847a9189a5c273e1985f9fac35e0acce87ff28987e0180a","observation_id":"b6487383-a373-4b71-9c1b-8e3f45249ef3","resolution":{"observed_at":"2026-08-06T17:03:17.335001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.05301","last_updated":"2015-01-21T21:00:05Z","snapshot_observed_at":"2026-08-16T15:10:37.719215Z","submitted_at":"2015-01-21T21:00:05Z","title":"The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.05301","snapshot_observed_at":"2026-08-06T17:03:17.432985Z","title":"Ajello et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.432985Z"},"links":{"cited_paper":"/paper/1501.05301","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:ad1d907d77fdec5507825e4e382742ca9c27ef912a7217cfc8234ee657b7ddf2","observation_id":"e1f0f90d-9662-48e9-b31d-fa3a9c54b502","resolution":{"observed_at":"2026-08-06T17:03:17.432985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.04101","last_updated":"2017-01-11T15:47:15Z","snapshot_observed_at":"2026-08-14T21:52:57.473709Z","submitted_at":"2016-06-13T20:00:00Z","title":"Deciphering Contributions to the Extragalactic Gamma-Ray Background from 2 GeV to 2 TeV","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.04101","snapshot_observed_at":"2026-08-06T17:03:17.521546Z","title":"Lisanti, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.521546Z"},"links":{"cited_paper":"/paper/1606.04101","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:7ca5494dc667e3ac575d7848bd30195eeb88b5b32bdb3684c96454c1148b708d","observation_id":"f9bc737e-4455-447b-8857-f92af281416a","resolution":{"observed_at":"2026-08-06T17:03:17.521546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.00693","last_updated":"2015-11-02T21:00:04Z","snapshot_observed_at":"2026-08-14T22:25:10.083270Z","submitted_at":"2015-11-02T21:00:04Z","title":"Resolving the Extragalactic $\\gamma$-ray Background above 50 GeV with Fermi-LAT","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.00693","snapshot_observed_at":"2026-08-06T17:03:17.590467Z","title":"Ackermann et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.590467Z"},"links":{"cited_paper":"/paper/1511.00693","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:7ed97cb121056983cbca376389567d710152685cbed154dcbce80f4f08825f24","observation_id":"e49685a4-0329-4e38-a279-c44579772894","resolution":{"observed_at":"2026-08-06T17:03:17.590467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.236639Z","title":"Cermenati et al., 2025, in preparation","venue":null,"work_id":"b44495cb-6da5-47a3-bf8c-ad1e7daa5770","year":2025},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.660066Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:db58abd3fb16de7dfe6853abed7516d2ac0a530482463f622997eef35b562cbc","observation_id":"d58d2c0b-15ad-41c8-8e2d-9a4cbebc0c43","resolution":{"observed_at":"2026-08-06T17:03:21.312134Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.02857","last_updated":"2023-04-17T10:11:13Z","snapshot_observed_at":"2026-08-16T16:18:25.226837Z","submitted_at":"2022-11-05T09:11:37Z","title":"Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.02857","snapshot_observed_at":"2026-08-06T17:03:17.750867Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.750867Z"},"links":{"cited_paper":"/paper/2211.02857","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:bef009dec98f277428cda0a929a7504d74249ca9cd8ad64d7887b58050217a47","observation_id":"b1407230-631a-4043-9e6a-1be8b2b6db69","resolution":{"observed_at":"2026-08-06T17:03:17.750867Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.04472","last_updated":"2019-05-11T07:45:24Z","snapshot_observed_at":"2026-08-16T12:07:59.182405Z","submitted_at":"2019-05-11T07:45:24Z","title":"AugerPrime: the Pierre Auger Observatory Upgrade","version":1},"cited_work":{"arxiv_id":"1905.04472","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.04472","snapshot_observed_at":"2026-08-06T17:03:19.561423Z","title":"AugerPrime: the Pierre Auger Observatory Upgrade","venue":"astro-ph.HE","work_id":"fe6bfff6-b03e-4e6d-8dca-6afcb58bf829","year":2019},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.822302Z"},"links":{"cited_paper":"/paper/1905.04472","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:b1f325adda3950ca53a72f73d7476b2b3891ef1e5b44ee475dec7c5aab4b72d5","observation_id":"14d9fe7c-bf08-4af5-b986-5ec4c449f53a","resolution":{"observed_at":"2026-08-06T17:03:19.650505Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12922","last_updated":"2025-02-11T20:58:36Z","snapshot_observed_at":"2026-08-15T15:05:14.111060Z","submitted_at":"2024-11-19T23:20:12Z","title":"Instrument design and performance of the first seven stations of RNO-G","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12922","snapshot_observed_at":"2026-08-06T17:03:17.916625Z","title":"Agarwal, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.916625Z"},"links":{"cited_paper":"/paper/2411.12922","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:df674b81dae92cba98b4f71b4d206a1f47fd65a40a67cabcd7b57126837e2bec","observation_id":"83143d94-4fea-4a9b-a45a-229c4180e389","resolution":{"observed_at":"2026-08-06T17:03:17.916625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.09994","last_updated":"2019-07-18T13:41:23Z","snapshot_observed_at":"2026-08-14T18:10:26.118640Z","submitted_at":"2018-10-23T17:56:18Z","title":"The Giant Radio Array for Neutrino Detection (GRAND): Science and Design","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.09994","snapshot_observed_at":"2026-08-06T17:03:17.982370Z","title":"´Alvarez-Mu˜ nizet al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:17.982370Z"},"links":{"cited_paper":"/paper/1810.09994","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:8e53ae9d30dc94c27755830823d8b21051ad486f02f08108af0a27e8924f4d61","observation_id":"4fee516b-9feb-41f4-ab09-b5f2f359f391","resolution":{"observed_at":"2026-08-06T17:03:17.982370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:18.033489Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.033489Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:9d372e3fe2ba8ff8413f6b6b66d68e35500a0e10655989368891e22939389c58","observation_id":"3fb77f58-5a4a-4279-9664-123f73cba4c9","resolution":{"observed_at":"2026-08-06T17:03:18.033489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00032","last_updated":"2021-07-30T18:15:01Z","snapshot_observed_at":"2026-08-16T18:06:15.167728Z","submitted_at":"2021-07-30T18:15:01Z","title":"The Giant Radio Array for Neutrino Detection (GRAND) Project","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.00032","snapshot_observed_at":"2026-08-06T17:03:18.149838Z","title":"Kotera (GRAND), PoS ICRC2021, 1181 (2021), arXiv:2108.00032 [astro-ph.HE]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.149838Z"},"links":{"cited_paper":"/paper/2108.00032","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:44799b9fdf07343f98a1a4d81104929c6b6abc6d469cba728023f0fc95a701da","observation_id":"bba5b3c9-2b44-4654-86df-e2e06f950c40","resolution":{"observed_at":"2026-08-06T17:03:18.149838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.07945","last_updated":"2021-05-24T18:42:28Z","snapshot_observed_at":"2026-08-16T18:58:33.995093Z","submitted_at":"2020-12-14T21:20:46Z","title":"The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.07945","snapshot_observed_at":"2026-08-06T17:03:18.196495Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.196495Z"},"links":{"cited_paper":"/paper/2012.07945","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:9244d15d5bd9a77e4e2f42fce82cb1104c81c883a59f04ab5087e3b45dfa22f5","observation_id":"a5487a8f-52db-44db-b51a-4964fd337f62","resolution":{"observed_at":"2026-08-06T17:03:18.196495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0204357","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:19.298998Z","title":"Berezinsky, A","venue":null,"work_id":"1ae78c37-a15f-42ab-ac77-e24ace29acb3","year":2006},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.268476Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:465833276ed5d9b22b4d309bb028c6a14bb50eb3661b57c2bb46711311135152","observation_id":"e97cc44e-131f-43e4-b22f-36860ab11362","resolution":{"observed_at":"2026-08-06T17:03:19.359134Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:21.066885Z","title":null,"venue":null,"work_id":"33b218c4-795b-4143-bb8e-4fe5efa34e1f","year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.333797Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:36ccec5d408716fb95fe6b336f1bb707c4b5c0f71ca440d8f6e30ce891dedf78","observation_id":"bfe61923-5d25-4f7d-9cc4-0ffd38095f11","resolution":{"observed_at":"2026-08-06T17:03:21.159704Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13336","last_updated":"2024-06-19T08:36:48Z","snapshot_observed_at":"2026-08-16T13:41:32.930113Z","submitted_at":"2024-06-19T08:36:48Z","title":"Berezinsky Hidden Sources: An Emergent Tension in the High-Energy Neutrino Sky?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13336","snapshot_observed_at":"2026-08-06T17:03:18.400455Z","title":"Ambrosone, JCAP 09, 075, arXiv:2406.13336 [astro-ph.HE]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.400455Z"},"links":{"cited_paper":"/paper/2406.13336","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:4dda82f7ebbfb96d40034ce4bab6facb42d06f42978f3e7e6705c00b6d937195","observation_id":"6c7c91be-0b4f-49e3-80a2-3beee0f58872","resolution":{"observed_at":"2026-08-06T17:03:18.400455Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-06T17:03:18.486163Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.486163Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:31d1427d2ede71052fc7e4103590c38c951bef2758b4a167f7f65f1cdf4975eb","observation_id":"3ff1642b-c711-47f1-bb85-e74d2aae86b9","resolution":{"observed_at":"2026-08-06T17:03:18.486163Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0688","last_updated":"2009-01-16T15:04:30Z","snapshot_observed_at":"2026-08-15T10:20:09.311868Z","submitted_at":"2008-03-05T15:55:57Z","title":"Energy spectra of gamma-rays, electrons and neutrinos produced at interactions of relativistic protons with low energy radiation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0688","snapshot_observed_at":"2026-08-06T17:03:18.578155Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.578155Z"},"links":{"cited_paper":"/paper/0803.0688","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:8234f0e7d2f3fe1036a04651099f88584934a0540be46fb82fa0855c95bd7d77","observation_id":"96031a60-c4c6-42a4-9873-0d7f3cef02d5","resolution":{"observed_at":"2026-08-06T17:03:18.578155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9903478","last_updated":"1999-03-31T13:36:46Z","snapshot_observed_at":"2026-07-07T01:25:23.293384Z","submitted_at":"1999-03-31T13:36:46Z","title":"Monte-Carlo simulations of photohadronic processes in astrophysics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9903478","snapshot_observed_at":"2026-08-06T17:03:18.668165Z","title":"Mucke, R","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.668165Z"},"links":{"cited_paper":"/paper/astro-ph/9903478","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:b8a1575bb986d66e3c12097449b24faa9d916bdc7f116c459fec1262297638f8","observation_id":"1489c187-f443-406f-bded-1640c4de79c3","resolution":{"observed_at":"2026-08-06T17:03:18.668165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.03035","last_updated":"2021-09-28T12:25:07Z","snapshot_observed_at":"2026-08-17T00:43:08.406391Z","submitted_at":"2020-12-05T14:10:41Z","title":"An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.03035","snapshot_observed_at":"2026-08-06T17:03:18.765598Z","title":"Saldana-Lopez, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.765598Z"},"links":{"cited_paper":"/paper/2012.03035","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:1ca009338abb05a08e4d4a911b0559fcfc617ba672fa6229494fabacbc8afbce","observation_id":"a4891926-48b2-4c3b-bc07-e5327b84ce93","resolution":{"observed_at":"2026-08-06T17:03:18.765598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:20.931484Z","title":"and Zdziarski, Andrzej A","venue":null,"work_id":"b14ab630-31c3-48d2-96fb-1fec8d1d0fcc","year":1992},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.854054Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:52a5c0bccbcbb8899179f3b0cce3c2bd2a306aef1420291fafaac26c72ba0cbc","observation_id":"6fc1415b-7bb7-4944-bfef-8354fb9cedcb","resolution":{"observed_at":"2026-08-06T17:03:21.010707Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.08901","last_updated":"2023-10-15T14:04:45Z","snapshot_observed_at":"2026-08-16T15:23:46.757483Z","submitted_at":"2023-06-15T07:09:23Z","title":"A cosmic-ray database update: CRDB v4.1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.08901","snapshot_observed_at":"2026-08-06T17:03:18.921487Z","title":"Maurin, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:18.921487Z"},"links":{"cited_paper":"/paper/2306.08901","citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:badc46be6466b0431fab675c488298e1dffe222642b6084b417a741e5612135c","observation_id":"ec604947-f71e-4688-8855-c426a6fdff75","resolution":{"observed_at":"2026-08-06T17:03:18.921487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:20.758802Z","title":null,"venue":null,"work_id":"d4f4a4d0-0acc-494d-ad3d-723d218025c2","year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:19.007229Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:89488e9f102f371344c4c8e76b6f35849b4deceac694927fc483037d03cf7ab3","observation_id":"ef291edf-9a3e-49e0-8b45-15720eb249dc","resolution":{"observed_at":"2026-08-06T17:03:20.837435Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:03:20.604104Z","title":"NUSES - A pathfinder for studying astrophysi- cal neutrinos and electromagnetic signals of seismic origin from space","venue":null,"work_id":"6287fd47-8704-45ef-ae0e-f6cce7204030","year":null},"citing_paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T17:03:19.134236Z"},"links":{"citing_paper":"/paper/2507.11993"},"observation_digest":"sha256:1561a07fd0407c57ee5283ed2af299c2ef424d261c1dc8be086d9f1f69c2f8dc","observation_id":"1a9457c3-cb56-4e70-ac98-4fd47c43619f","resolution":{"observed_at":"2026-08-06T17:03:20.698457Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.11993","last_updated":"2025-07-16T07:46:20Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T04:25:34.497470Z","submitted_at":"2025-07-16T07:46:20Z","title":"Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective"},"reference_resolution":{"displayed":55,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":43,"verified_exact":5,"verified_fuzzy":7},"total_outbound_references":55},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 55 of 55 outbound references and 4 inbound Pith citation observations for arXiv:2507.11993."}