{"as_of":"2026-08-10T08:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4a3260f31f231d7e31a0f8463a12612fc4da982ecebcf29643b26033298464b4","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":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T15:18:08.334267Z","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":"2026-07-01T20:36:11.136541Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2506.04212","last_updated":"2026-05-06T18:45:15Z","snapshot_observed_at":"2026-08-03T05:26:45.391048Z","submitted_at":"2025-06-04T17:56:48Z","title":"Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-19T10:45:37.848326Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2506.04212"},"observation_digest":"sha256:f6b3ff2ed9c04533fc15aad8580bda78ccfb56d1da04a66452aa781ceb281f04","observation_id":"45a65eac-134f-4f42-b9b5-a780b6fd4824","resolution":{"observed_at":"2026-05-09T02:33:42.760028Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2506.21403","last_updated":"2026-04-29T21:40:00Z","snapshot_observed_at":"2026-08-03T21:55:51.647032Z","submitted_at":"2025-06-26T15:50:46Z","title":"3C403: a candidate neutrino-emitting radio galaxy","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-19T07:49:42.780148Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2506.21403"},"observation_digest":"sha256:51fddd44eb82d70a68b6cf2d0d71bac12242f8063ace5f0cd1142c3d0d86bc29","observation_id":"a74cad94-3438-4eab-bb1e-3d06c32fc510","resolution":{"observed_at":"2026-05-19T07:52:09.440709Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-08-06T15:18:08.334267Z","title":"Inoue, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.16551","last_updated":"2025-07-22T13:03:49Z","snapshot_observed_at":"2026-08-08T20:02:28.196749Z","submitted_at":"2025-07-22T13:03:49Z","title":"Exploring the properties of newborn pulsars with high-energy neutrinos","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T15:18:08.334267Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2507.16551"},"observation_digest":"sha256:d2f318ccc81808083c5322041b0091f575a0733fb4e9f810a5d863f22aa77fcd","observation_id":"59297f10-2be6-4502-8dc7-ee1a70353f9c","resolution":{"observed_at":"2026-08-06T15:18:08.334267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2603.15754","last_updated":"2026-05-21T09:00:01Z","snapshot_observed_at":"2026-08-04T09:43:05.150527Z","submitted_at":"2026-03-16T18:00:10Z","title":"Single-source-class interpretation of the diffuse astrophysical neutrino flux","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-22T10:15:07.047534Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2603.15754"},"observation_digest":"sha256:3bc091eb4f5cf07213528de7464f0834eac367dd9cd6355d65c5c86576677098","observation_id":"976c2d02-f8ad-4ae6-96c2-4ab6075112cc","resolution":{"observed_at":"2026-05-22T10:16:22.713668Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2604.23726","last_updated":"2026-05-11T18:24:39Z","snapshot_observed_at":"2026-08-04T05:00:36.335256Z","submitted_at":"2026-04-26T14:13:19Z","title":"A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-08T05:35:10.178971Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2604.23726"},"observation_digest":"sha256:8d4a142582dcb795b95af9746e216686d4efae48d9b8379e9eb11af1f43d9715","observation_id":"06572a49-d5bf-418f-bcf3-4d20d1a0d6c6","resolution":{"observed_at":"2026-05-11T21:26:16.899138Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2604.23726","last_updated":"2026-05-11T18:24:39Z","snapshot_observed_at":"2026-08-04T05:00:36.335256Z","submitted_at":"2026-04-26T14:13:19Z","title":"A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-13T07:37:10.999134Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2604.23726"},"observation_digest":"sha256:2765bfca75c1b4d6d902eb4d13cf9ee5f2e4d7d7ced4272cd82a7fe3364bd70a","observation_id":"46c8d450-479f-4000-b112-490ec6a6a843","resolution":{"observed_at":"2026-05-13T07:37:29.022248Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2605.13588","last_updated":"2026-05-13T14:23:24Z","snapshot_observed_at":"2026-08-02T09:18:43.216302Z","submitted_at":"2026-05-13T14:23:24Z","title":"On the Apparent Correlation between X-ray and Neutrino Luminosities of Active Galactic Nuclei","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-14T18:03:05.359872Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2605.13588"},"observation_digest":"sha256:503def6e74e90378aa6f4d87a935d499e1870732b9a6f97bb4918956e558230f","observation_id":"a6a4deb6-cb2e-4556-9226-d3820f006e07","resolution":{"observed_at":"2026-05-14T18:07:33.956038Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2605.13968","last_updated":"2026-05-13T18:00:05Z","snapshot_observed_at":"2026-07-06T23:25:25.361350Z","submitted_at":"2026-05-13T18:00:05Z","title":"Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-15T05:21:13.326499Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2605.13968"},"observation_digest":"sha256:c149fba18bf2977ff65fd55760a732502442e8994947397e5f3bc5ea9c3855fb","observation_id":"eb9e73d2-7032-467d-9a43-7a95ef73fac4","resolution":{"observed_at":"2026-05-15T05:25:04.204978Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":"1909.02239","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-01T20:36:11.136541Z","title":"Inoue, D","venue":null,"work_id":"1a01d3c2-a1bd-4e5c-9724-ab015febcc10","year":2020},"citing_paper":{"arxiv_id":"2606.00249","last_updated":"2026-05-29T18:29:27Z","snapshot_observed_at":"2026-08-09T15:51:19.990885Z","submitted_at":"2026-05-29T18:29:27Z","title":"The Delta Resonance in the Neutrino Sky","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-06-28T21:02:18.735963Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2606.00249"},"observation_digest":"sha256:87f67990e6146ede69edf22323b6376822314d2e47cd5878b85e7f1c05d510d5","observation_id":"c35aa54c-dbf2-4ace-b435-9bce902c6773","resolution":{"observed_at":"2026-07-01T20:36:11.138345Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-14T16:57:50.370612Z","title":"891(2):L33","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2606.30764","last_updated":"2026-07-12T21:55:27Z","snapshot_observed_at":"2026-08-02T08:18:53.119406Z","submitted_at":"2026-06-29T18:01:35Z","title":"Active Galactic Nuclei as high-energy neutrino sources","version":2},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-07-14T16:57:50.370612Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2606.30764"},"observation_digest":"sha256:6fea6480130237c1a1847c3ad7b4493abe943ea51578920122114f51e8217945","observation_id":"bcea2011-7044-4277-8593-4ecc0ab246af","resolution":{"observed_at":"2026-07-14T16:57:50.370612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-13T06:23:15.280807Z","title":"Inoue, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.08833","last_updated":"2026-07-09T18:00:10Z","snapshot_observed_at":"2026-08-03T18:31:01.553379Z","submitted_at":"2026-07-09T18:00:10Z","title":"Flavorful Interactions of AGN Neutrinos with Dark Matter Spike","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-13T06:23:15.280807Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2607.08833"},"observation_digest":"sha256:b1b52b43a0f56834d0eb56b2d5d2646282835575dffa0fa682ce56b7a3915d92","observation_id":"73031b31-2cd9-4282-8e4c-44cbcce50c60","resolution":{"observed_at":"2026-07-13T06:23:15.280807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-07-13T05:54:31.458711Z","title":"On the Origin of High-energy Neutrinos from NGC 1068: The Role of Nonthermal Coronal Activity,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.08904","last_updated":"2026-07-09T19:58:36Z","snapshot_observed_at":"2026-08-05T22:56:59.843293Z","submitted_at":"2026-07-09T19:58:36Z","title":"Revisiting bounds on neutrino dark matter interaction at spikes","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-13T05:54:31.458711Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2607.08904"},"observation_digest":"sha256:893a602a70c67895df0c9da5d5107bfa4051a6cfa30a57bf47769a2d22eb5b05","observation_id":"cf8cad35-ac25-4fee-a59d-d06cf6cfa2f6","resolution":{"observed_at":"2026-07-13T05:54:31.458711Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-08-01T13:06:18.243759Z","title":"Inoue, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19254","last_updated":"2026-07-21T16:24:37Z","snapshot_observed_at":"2026-08-05T16:12:05.848042Z","submitted_at":"2026-07-21T16:24:37Z","title":"Astrophysical Neutrino Sources as Colliders","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T13:06:18.243759Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2607.19254"},"observation_digest":"sha256:e664482f6e3c2f2160378a87d1dd118ba95e7fe675c02a448ea5c8ec3b4539eb","observation_id":"f93e4df5-6ca0-4b4f-84ce-ade3c7d80cea","resolution":{"observed_at":"2026-08-01T13:06:18.243759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.02239","snapshot_observed_at":"2026-08-01T03:56:35.607216Z","title":"On the Origin of High-energy Neutrinos from NGC 1068: The Role of Nonthermal Coronal Activity","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.27658","last_updated":"2026-07-30T04:16:19Z","snapshot_observed_at":"2026-08-08T03:51:14.711967Z","submitted_at":"2026-07-30T04:16:19Z","title":"On the Blueprint of Active Galaxies Producing Neutrinos","version":1},"reference_index":148,"source":"arxiv_source","source_observed_at":"2026-08-01T03:56:35.607216Z"},"links":{"cited_paper":"/paper/1909.02239","citing_paper":"/paper/2607.27658"},"observation_digest":"sha256:12f6dbfcd91b8c4dffb2aa64bbcc4b78ba652d1219b13ee193369d5acf31b5ff","observation_id":"8015f1dd-8400-48e0-9abe-10dab03769a1","resolution":{"observed_at":"2026-08-01T03:56:35.607216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1909.02239/citation-record","integrity":"/paper/1909.02239/integrity","json":"/paper/1909.02239/citation-record.json","paper":"/paper/1909.02239"},"outbound":[],"paper":{"arxiv_id":"1909.02239","last_updated":"2020-02-19T02:58:09Z","latest_version":4,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T08:19:18.253814Z","submitted_at":"2019-09-05T07:15:41Z","title":"On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1909.02239."}