{"as_of":"2026-08-19T16:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d59e2185b4a15ed1d80221958ca1fa007b0987b42a61b44dd4b62edba9804608","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":22,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":22,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":22,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":22,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T10:59:43.545887Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-02T16:07:08.605519Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-12T17:52:28.728068Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.12216","last_updated":"2025-03-13T04:28:25Z","snapshot_observed_at":"2026-08-19T02:22:40.939974Z","submitted_at":"2024-11-19T04:07:17Z","title":"Production cross sections of light and charmed mesons in $e^+e^-$ annihilation near 10.58 GeV","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T17:52:28.728068Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2411.12216"},"observation_digest":"sha256:f9f8a01a2646eb0d209096a91cdf753b0d4abe7c3ed42c72faadb7eea9a08620","observation_id":"4c78a143-0712-4681-a981-829708295997","resolution":{"observed_at":"2026-08-12T17:52:28.728068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2412.03186","last_updated":"2025-05-06T09:03:51Z","snapshot_observed_at":"2026-08-18T14:05:02.057504Z","submitted_at":"2024-12-04T10:14:24Z","title":"First Measurement of the Muon Neutrino Interaction Cross Section and Flux as a Function of Energy at the LHC with FASER","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-23T08:35:23.173867Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2412.03186"},"observation_digest":"sha256:673d7dc9cd661493b031b5c615c636663b7537ef73fd25b612bfcdcc91123868","observation_id":"d4b07920-0395-48df-bc78-1ddd8fbdfd30","resolution":{"observed_at":"2026-05-23T08:35:29.592825Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-10T22:55:38.611055Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.04714","last_updated":"2024-12-31T13:44:13Z","snapshot_observed_at":"2026-08-16T18:30:36.463634Z","submitted_at":"2024-12-31T13:44:13Z","title":"The Forward Physics Facility at the HL-LHC and its Synergies with Astroparticle Physics","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T22:55:38.611055Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2501.04714"},"observation_digest":"sha256:169228e16b89e1b7ca0339ba851672e54798df59bbca4fdccd0b8074301cde29","observation_id":"33eb3eb9-8f05-4a35-9a40-49d53d4df89f","resolution":{"observed_at":"2026-08-10T22:55:38.611055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-10T19:29:16.268010Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.10078","last_updated":"2025-01-17T09:50:13Z","snapshot_observed_at":"2026-08-17T03:58:37.758960Z","submitted_at":"2025-01-17T09:50:13Z","title":"Neutrino Experiments at the Large Hadron Collider","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T19:29:16.268010Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2501.10078"},"observation_digest":"sha256:0d2b383e7b77d6d7c1a8c2b7d7093386a3652159ead8afbdb8c7327b85179364","observation_id":"3272cae8-feee-4f02-86ee-fc769adc7089","resolution":{"observed_at":"2026-08-10T19:29:16.268010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-07T23:43:23.703068Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.08798","last_updated":"2025-05-04T12:43:14Z","snapshot_observed_at":"2026-08-15T10:51:55.061236Z","submitted_at":"2025-02-12T21:21:20Z","title":"Modified Hadronic Interactions and the future of UHECR observations","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T23:43:23.703068Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2502.08798"},"observation_digest":"sha256:482619ab258faa245e762fd9cbedd0ac96f35799ec4180035a28849de853c87a","observation_id":"2812e870-c12f-4709-bce1-657511e34d3a","resolution":{"observed_at":"2026-08-07T23:43:23.703068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-16T10:59:43.545887Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.16873","last_updated":"2025-06-22T10:58:28Z","snapshot_observed_at":"2026-08-17T09:48:54.818121Z","submitted_at":"2025-04-23T16:47:18Z","title":"A LOFAR-style reconstruction of cosmic-ray air showers with SKA-Low","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-16T10:59:43.545887Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2504.16873"},"observation_digest":"sha256:54f9df3645252ff5f78852f7e68bcbae23ca46492d48e8a987ced0d99009a989","observation_id":"7c302fe3-db12-47b0-9b87-22a4e1b3f9c1","resolution":{"observed_at":"2026-08-16T10:59:43.545887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-15T21:45:00.673403Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.09111","last_updated":"2025-05-14T03:40:59Z","snapshot_observed_at":"2026-08-19T11:30:02.401038Z","submitted_at":"2025-05-14T03:40:59Z","title":"Measuring the Cosmic Ray Spectrum with Next Generation Neutrino Detectors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T21:45:00.673403Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2505.09111"},"observation_digest":"sha256:3a174996cee714a517dae61230c821998aa59f7292fd63acd7c27bc892e5f113","observation_id":"b869883a-bd2e-4ef6-bb59-13d5d54e393e","resolution":{"observed_at":"2026-08-15T21:45:00.673403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-06T22:46:46.235790Z","title":"Gaisser, Todor Stanev, Hadronic interaction model Sibyll 2.3d and extensive air showers, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.20855","last_updated":"2026-05-28T02:15:59Z","snapshot_observed_at":"2026-08-16T14:37:35.698857Z","submitted_at":"2025-06-25T22:00:37Z","title":"Neutrino Physics and Astrophysics at Colliders","version":2},"reference_index":126,"source":"pdf_text","source_observed_at":"2026-08-06T22:46:46.235790Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2506.20855"},"observation_digest":"sha256:a3d818d7302a9c8e0731d4cf8f2a9248efac6bea9a046295d6f3ce893f5a9ed3","observation_id":"3ba83b46-a694-40f6-ad67-a8afc2ffdd4a","resolution":{"observed_at":"2026-08-06T22:46:46.235790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-06T18:15:11.123844Z","title":"Riehn et al.,Hadronic interaction model Sibyll 2.3d and extensive air showers,Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.08997","last_updated":"2025-07-11T19:57:57Z","snapshot_observed_at":"2026-08-18T19:20:31.474631Z","submitted_at":"2025-07-11T19:57:57Z","title":"Constraints on the spread of nuclear masses in ultra-high-energy cosmic rays based on the Phase I hybrid data from the Pierre Auger Observatory","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T18:15:11.123844Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2507.08997"},"observation_digest":"sha256:60e562c447afecc96ca4fab0fa33f8368e4e9398e8142862e481c2e3897dd461","observation_id":"4b0fde6d-219f-4ce0-b342-111611c9a4f3","resolution":{"observed_at":"2026-08-06T18:15:11.123844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-06T12:21:43.180595Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.21856","last_updated":"2025-07-29T14:29:11Z","snapshot_observed_at":"2026-08-16T06:05:11.521955Z","submitted_at":"2025-07-29T14:29:11Z","title":"Chromo: A High-Performance Python Interface to Hadronic Event Generators for Collider and Cosmic-Ray Simulations","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T12:21:43.180595Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2507.21856"},"observation_digest":"sha256:1b39ca45b69adf2adf44f4a5dd60f54d538656fca16b61171520ea1f517ad88e","observation_id":"87bac284-1252-48dd-b096-d58b1cd9684f","resolution":{"observed_at":"2026-08-06T12:21:43.180595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-06T11:45:35.534547Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.22463","last_updated":"2025-09-05T09:29:13Z","snapshot_observed_at":"2026-08-16T22:24:13.590158Z","submitted_at":"2025-07-30T08:10:02Z","title":"A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors","version":3},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-06T11:45:35.534547Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2507.22463"},"observation_digest":"sha256:1ad6889b0baf454103ea364b8e4c5960c3493460f1365f1a46d6b4f9ad14071f","observation_id":"b94aa1fa-991e-4722-b170-1855e594525b","resolution":{"observed_at":"2026-08-06T11:45:35.534547Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-06T10:48:04.438838Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.23552","last_updated":"2025-07-31T13:41:26Z","snapshot_observed_at":"2026-08-16T06:05:15.196087Z","submitted_at":"2025-07-31T13:41:26Z","title":"Latest neutrino results from the FASER experiment and their implications for forward hadron production","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T10:48:04.438838Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2507.23552"},"observation_digest":"sha256:4a74e73be15c729bd0a8a8e79d43101c211305c1b0d401cc248f8f3838a25db3","observation_id":"38507696-432f-45ba-afe8-05b661d13065","resolution":{"observed_at":"2026-08-06T10:48:04.438838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2510.26260","last_updated":"2025-10-30T08:40:59Z","snapshot_observed_at":"2026-08-13T00:00:24.186606Z","submitted_at":"2025-10-30T08:40:59Z","title":"Letter of Intent: The Forward Physics Facility","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-21T20:59:22.363015Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2510.26260"},"observation_digest":"sha256:90569a5c29988081f9b0bd0ff4a794ad057fd562d9738d52b068a37e591e73a2","observation_id":"de8584f0-0c83-4f63-820d-348e96d0cda5","resolution":{"observed_at":"2026-05-21T21:00:38.994556Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-03T09:52:24.082593Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2601.12422","last_updated":"2026-07-20T09:25:26Z","snapshot_observed_at":"2026-08-13T18:12:12.829829Z","submitted_at":"2026-01-18T14:09:19Z","title":"Modified hadronic interactions in 3-dimensional simulations","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T09:52:24.082593Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2601.12422"},"observation_digest":"sha256:773f102297b83857a7a6d3b5b9fa63e92de26800df3d3bb56389330f65ce599f","observation_id":"5abbbb4d-9fbb-4e25-a603-072482969264","resolution":{"observed_at":"2026-08-03T09:52:24.082593Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-02T19:36:47.164363Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.01744","last_updated":"2026-06-09T13:24:04Z","snapshot_observed_at":"2026-08-16T22:44:56.708461Z","submitted_at":"2026-03-02T11:15:26Z","title":"The PYTHIA Facility","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-02T19:36:47.164363Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2603.01744"},"observation_digest":"sha256:b072cc74d7dcf55e6c66a9202ca981403b631f24fedbf6c66f8687637bc27939","observation_id":"c808b0b8-c6e4-442e-a400-8982180c09ee","resolution":{"observed_at":"2026-08-02T19:36:47.164363Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2604.05512","last_updated":"2026-04-07T07:06:50Z","snapshot_observed_at":"2026-08-13T20:22:08.442299Z","submitted_at":"2026-04-07T07:06:50Z","title":"Measurement of charged-particle production in $\\sqrt{s_\\text{NN}}=9.62$ TeV proton-oxygen collisions as a probe of cosmic-ray air showers with the ATLAS detector","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-10T19:20:21.397820Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2604.05512"},"observation_digest":"sha256:f0041fa02f102fa8d961740d59c3a0da7dcc8f1b87f62e1fef04fc360b6e651a","observation_id":"3425e9ce-3582-4868-9ada-51ddf2c36ca8","resolution":{"observed_at":"2026-05-10T23:05:50.130547Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2604.22083","last_updated":"2026-04-23T21:29:02Z","snapshot_observed_at":"2026-08-15T05:00:33.086859Z","submitted_at":"2026-04-23T21:29:02Z","title":"Downward ultra-high-energy neutrino detection in the air with radio antennas at ground-based observatories","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-09T20:12:01.985148Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2604.22083"},"observation_digest":"sha256:a5e813b19f8ae79a45934c2ad8c3c0e7b909913ee4979bb320892fe28f88c88f","observation_id":"769f30bd-1bb1-4edb-a2f4-40ce278162ce","resolution":{"observed_at":"2026-05-11T15:21:08.328785Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2604.22462","last_updated":"2026-04-24T11:29:09Z","snapshot_observed_at":"2026-08-10T21:23:44.507379Z","submitted_at":"2026-04-24T11:29:09Z","title":"Machine Learning for Multi-messenger Probes of New Physics and Cosmology: A Review and Perspective","version":1},"reference_index":232,"source":"pdf_text","source_observed_at":"2026-05-08T11:02:17.987425Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2604.22462"},"observation_digest":"sha256:d38472d27ba74608dbad251e301e784cd324f39cb0541c17e470fd1690638038","observation_id":"fbcc9f4e-903e-4108-b578-a6515b6b251a","resolution":{"observed_at":"2026-05-11T19:46:14.786039Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2606.06029","last_updated":"2026-06-04T11:22:14Z","snapshot_observed_at":"2026-08-14T10:06:57.141920Z","submitted_at":"2026-06-04T11:22:14Z","title":"Mountain Muography for China Jinping Underground Laboratory","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-27T23:03:40.799637Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2606.06029"},"observation_digest":"sha256:ef7fa03926145c9f4c7c109b57ab3161eadcc6a40aa8f162feef2df009429e12","observation_id":"735ed3c0-f848-487f-9d0b-3f9cbca9f8d4","resolution":{"observed_at":"2026-07-02T16:07:08.607620Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":"1912.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-02T16:07:08.605519Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","venue":null,"work_id":"5eedcbee-8f8d-44fe-a921-a20f7b8a6812","year":2020},"citing_paper":{"arxiv_id":"2606.13062","last_updated":"2026-06-11T08:48:21Z","snapshot_observed_at":"2026-08-07T03:19:00.001462Z","submitted_at":"2026-06-11T08:48:21Z","title":"Optimization of muon suppression using sweeper magnets for the Forward Physics Facility at the HL-LHC","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-27T05:24:37.445155Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2606.13062"},"observation_digest":"sha256:d27370bef170f479430e50c90208a2bf545766f630e9357fa58732a21ae64616","observation_id":"3ad0ee96-8964-4e93-ae01-a98b559eb7e9","resolution":{"observed_at":"2026-06-27T05:30:35.970952Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-07-12T08:01:48.933771Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.02644","last_updated":"2026-07-07T18:37:06Z","snapshot_observed_at":"2026-08-17T13:59:32.576571Z","submitted_at":"2026-07-02T17:52:41Z","title":"High-Energy Neutrino Tomography of the Earth's Interior with IceCube","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-12T08:01:48.933771Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2607.02644"},"observation_digest":"sha256:0226b4b4ed9a78b95dcab0a7749f5818a3975e4c743ee1a07915f811ec0799ca","observation_id":"af17432f-8a06-4384-badf-d528a42cd88f","resolution":{"observed_at":"2026-07-12T08:01:48.933771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03300","snapshot_observed_at":"2026-08-16T00:28:47.964264Z","title":"Riehn, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.11862","last_updated":"2026-08-12T09:48:58Z","snapshot_observed_at":"2026-08-18T20:07:52.867634Z","submitted_at":"2026-08-12T09:48:58Z","title":"SPORE: An Event-Level Sampling Pipeline for Multi-Telescope Neutrino Astronomy","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T00:28:47.964264Z"},"links":{"cited_paper":"/paper/1912.03300","citing_paper":"/paper/2608.11862"},"observation_digest":"sha256:5b28a3fe77aef724775671641c6525a38e07d96331767411cb919ccc55de60c0","observation_id":"9790148e-827c-4958-a0f5-61f3daebbfe7","resolution":{"observed_at":"2026-08-16T00:28:47.964264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1912.03300/citation-record","integrity":"/paper/1912.03300/integrity","json":"/paper/1912.03300/citation-record.json","paper":"/paper/1912.03300"},"outbound":[],"paper":{"arxiv_id":"1912.03300","last_updated":"2020-09-04T18:00:17Z","latest_version":3,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-18T00:28:04.147508Z","submitted_at":"2019-12-06T18:59:56Z","title":"Hadronic interaction model Sibyll 2.3d and extensive air showers"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:1912.03300."}