{"as_of":"2026-08-23T16:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:63c9d3c62eed444d79505774a52290f80c20885785dbc7b4564e58027c3b5cf5","coverage":[{"denominator":36,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":36,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-30T19:52:33.605384Z","state":"measured"},{"denominator":36,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":36,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2605.15360/citation-record","integrity":"/paper/2605.15360/integrity","json":"/paper/2605.15360/citation-record.json","paper":"/paper/2605.15360"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.111.021103","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"G., Abbasi, R., Abdou, Y., et al","venue":"Physical Review Letters","work_id":"f8ccbe43-0dad-4745-837a-9f5ceb7c85d5","year":2013},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:e32185e2163cab1fd26250a7bd4f6314c573d632d40b984e0d3fd2f271cb42e8","observation_id":"26cfda8f-5b20-4ba4-9d5f-c5d41535b761","resolution":{"observed_at":"2026-06-30T19:55:00.447215Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:51.800218+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:51.800218+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.124.051103","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and others","venue":"Physical Review Letters","work_id":"f6d53919-f2ba-4b7a-ad79-7eae2d082d13","year":1910},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:d13a5fe0cdcafd9d1901324eaa06c7b51411655fc0a52b1c1af0369ac3a23e25","observation_id":"f8465279-fb5a-4b6b-9fdf-412231e8b899","resolution":{"observed_at":"2026-06-30T19:55:00.402691Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-20T20:52:17.184842+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-20T20:52:17.184842+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1126/science.abg3395","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Abbasi, et al., Evidence for neutrino emission from the nearby active galaxy NGC 1068, Science 378 (6619) (2022) 538–543","venue":"Science","work_id":"94196903-d815-4dfb-96f1-cca0a89279a9","year":2022},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:caf0f14928a87a688c0a08396be7a1f647245da5e6473f11078af5265f213daa","observation_id":"4252bf02-45c0-4ddf-9932-51bc7e681261","resolution":{"observed_at":"2026-06-30T19:55:00.411596Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-03T19:38:37.818235+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T19:38:37.818235+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2406.07601","doi":"10.48550/arxiv.2406.07601","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Abbasi, M","venue":null,"work_id":"1e4b39bf-fa9e-46f4-8f8f-91e763044d03","year":2024},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:725e87561a1fe4f2b07212895c491061b7ce3ea35dfa19604f588468efa613e4","observation_id":"c30e24b5-d6f2-4d26-af44-d9adcb5cae80","resolution":{"observed_at":"2026-06-30T19:55:00.372181Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:52.132349+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:52.132349+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/acbb6a","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, ApJS, 265, 31, doi: 10.3847/1538-4365/acbb6a","venue":"arXiv (Cornell University)","work_id":"57c30e5b-1191-426b-97dd-7c70adab7a7b","year":2023},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:d61e02283debac2f1640a5a104484cad5d384cbd175c276db2a83c5331f56e36","observation_id":"1de6cd48-2b18-46d1-861e-94beceec3245","resolution":{"observed_at":"2026-06-30T19:55:00.413752Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-08T03:38:02.04603+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T03:38:02.04603+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/810/1/14","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"B., et al","venue":"The Astrophysical Journal","work_id":"40365971-220b-4259-b60b-6d464fd0bbb8","year":2015},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:8b45ea05f56e839618db9ef1330825f90fb7fe535f63619ccc87652708b2c8bf","observation_id":"f2308562-e821-44b2-aaaa-66213f028396","resolution":{"observed_at":"2026-06-30T19:55:00.396942Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-22T08:24:17.523122+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-22T08:24:17.523122+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/2041-8205/815/2/l23","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"L., Ansoldi, S., Antonelli, L","venue":"The Astrophysical Journal Letters","work_id":"9117c867-3bca-4a49-8627-b8120d9ca585","year":2015},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:1d02ad6582e11d08b1d84a11290c9f7a1c07a52c200c355509f2db7d48e0786d","observation_id":"e8b4db52-50f3-452d-bd7d-56186096b613","resolution":{"observed_at":"2026-06-30T19:55:00.423016Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:38.075683+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:38.075683+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2024.102976","doi":"10.1016/j.astropartphys.2024.102976","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"L., Biermann, P","venue":"Astroparticle Physics","work_id":"23aff4e4-5351-44b8-a29d-3a593f482d3b","year":2024},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:4227881e9cfa9025c4e30cb7499b57ee7dd10240b427a4f366fe4abb19e1eb06","observation_id":"2cde249c-dffd-49dc-a59e-e1878223a197","resolution":{"observed_at":"2026-06-30T19:55:00.389729Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:53.653227+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:53.653227+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201322068","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T02:17:44.936438Z","title":"P., Tollerud, E","venue":"Astronomy &amp; Astrophysics","work_id":"aeafa8f2-1c15-4f27-9682-a76b6bf42e2b","year":2013},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:9cc567d7d1f2d13f8ee054b2e2a451ef9361b8e875be91a3d6174c4b59c35854","observation_id":"c8ccdbaf-133a-46e9-9e9f-871b34b3e5de","resolution":{"observed_at":"2026-06-30T19:55:00.392560Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-10T15:38:31.005157+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-10T15:38:31.005157+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/318742","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., Cowie, L","venue":"The Astronomical Journal","work_id":"d5f7bcdd-70e1-4b95-ae67-d319d8ca88f1","year":2001},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:92a0687e7b9497b178fe19fa0289f988a9a3ffc8f326392e41afe607308fb2b5","observation_id":"0cf66872-45e4-49d7-8cb3-310e6fe30bdb","resolution":{"observed_at":"2026-06-30T19:55:00.439403Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:54.090047+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:54.090047+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/revmodphys.56.255","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Reviews of Modern Physics , year = 1984, month = apr, volume =","venue":"Reviews of Modern Physics","work_id":"c6cfc67f-2f6e-440c-91df-d0c449d52c67","year":1984},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:15d7e22712fd1dc326ec78a8d22fa4acfbe76c3177f40caa35eedbc6a6ebf7b7","observation_id":"fe0d2fc8-8da6-43ee-a81f-1cbe16407772","resolution":{"observed_at":"2026-06-30T19:55:00.380496Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-20T12:55:56.745981+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-20T12:55:56.745981+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac9588","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2022, ApJ, 939, 43, doi: 10.3847/1538-4357/ac9588","venue":"The Astrophysical Journal","work_id":"adb906d3-ec61-4dd4-b4a6-95cebe9cd356","year":2022},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:bca3f2a15e304c955808a31e694609b9762a0a29ab8abba1fac9f623e2b6c2bb","observation_id":"d8455149-7eee-4dc3-85c7-82c97e9cc228","resolution":{"observed_at":"2026-06-30T19:55:00.415779Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-03T19:38:53.53025+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T19:38:53.53025+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/186171","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Maraschi, L","venue":"The Astrophysical Journal","work_id":"25fd2448-aaa5-48ef-8b43-68cb8493bd2b","year":1991},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:3b481a0eafcbd4a5ed7f240fb793e45ec651a75c3aa48589d67831704c68e22c","observation_id":"ca090852-84f0-42ec-971c-d962dd219a7f","resolution":{"observed_at":"2026-06-30T19:55:00.417706Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-22T06:23:32.323446+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-22T06:23:32.323446+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1142/s0218271822300038","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2022, International Journal of Modern Physics D, 31, 2230003, doi: 10.1142/S0218271822300038","venue":"International Journal of Modern Physics D","work_id":"da2e342c-eeeb-448b-ae17-e75050c8199e","year":2022},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:c86dc8e62f36ad5ac1eea52abf497f88e5392a3f1fba556feb246f8bc228cd69","observation_id":"7aa5fc5b-eaf9-4a76-8a95-d93cb69a820c","resolution":{"observed_at":"2026-06-30T19:55:00.428683Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:55.056175+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:55.056175+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2010","doi":"10.1111/j.1365-2966.2010","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"J., Reeves J","venue":null,"work_id":"b11220ca-ed53-44f4-8db3-b381c41c3d0a","year":2010},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:253bf02673b458d281fb31fb94d895b20cb7f4f1c9cf9c97a08ebed9862bfbfb","observation_id":"d8349366-3fcd-4498-b901-625c59cc0b45","resolution":{"observed_at":"2026-06-30T19:55:00.437157Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-12T18:20:04.642004+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T18:20:04.642004+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1008.4686","last_updated":"2010-08-27T10:29:25Z","snapshot_observed_at":"2026-08-19T18:02:33.920831Z","submitted_at":"2010-08-27T10:29:25Z","title":"Data analysis recipes: Fitting a model to data","version":1},"cited_work":{"arxiv_id":"1008.4686","doi":"10.48550/arxiv.1008.4686","metadata_source":"pith","pith_arxiv_id":"1008.4686","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Data analysis recipes: Fitting a model to data","venue":"astro-ph.IM","work_id":"53ca9ded-71c2-4f36-9fdf-d6879552d19c","year":2010},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"cited_paper":"/paper/1008.4686","citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:7a9dd3b07f9692c1c8f90d7eceff52ae01e9c1287c5913d8b347745f74303e95","observation_id":"b249fccc-c5c2-4d87-950a-83b4458d45c0","resolution":{"observed_at":"2026-06-30T19:55:00.386401Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:49:49.578506+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:49:49.578506+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ab7661","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2020, ApJL, 891, L33, doi: 10.3847/2041-8213/ab7661","venue":"The Astrophysical Journal Letters","work_id":"2f32d993-9cf0-4fd0-a737-03f078fb721e","year":2041},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:668ab169ccff9a4c63c64dd189a591848df1df5b095ee84b5954f38590e0a945","observation_id":"efc208bc-8106-4e63-84e9-0223cbd855bf","resolution":{"observed_at":"2026-06-30T19:55:00.409002Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-03T19:39:11.865518+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T19:39:11.865518+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac8794","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2022, ApJ, 938, 87, doi: 10.3847/1538-4357/ac8794","venue":"The Astrophysical Journal","work_id":"c9136a19-56d4-4c63-9614-140cf3454c6b","year":2022},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:b887e031b706bb4dfe5d63debdda19b5251f6bd3414305b3d5af9a9f035b6c5f","observation_id":"112eff41-fcf4-4f98-88c3-1a9c05a6918b","resolution":{"observed_at":"2026-06-30T19:55:00.394747Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-11T18:20:06.919023+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T18:20:06.919023+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s10509-007-9622-5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"I., Kovalev, Y","venue":"Astrophysics and Space Science","work_id":"e6e52788-74ac-4805-8371-dc6c2df07253","year":2007},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:18dc2ba0e1f6a77563c53fb7d2ac5b148e063c3d408030dff168ec7910cbc0ca","observation_id":"202f48d2-4a39-40c7-afb1-0fbb0d043071","resolution":{"observed_at":"2026-06-30T19:55:00.378086Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:56.505725+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:56.505725+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/519947","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"C., 2007, @doi [ ] 10.1086/519947 , https://ui.adsabs.harvard.edu/abs/2007ApJ...665.1489K 665","venue":"The Astrophysical Journal","work_id":"246adb7a-b1a3-4fd9-827b-672237516a29","year":2007},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:a5ca197309e82b03781696faac79f1dfbfe467ba3814444278d9600de9b428de","observation_id":"7c1d490f-e9bb-4fee-8a07-8ca3db77594d","resolution":{"observed_at":"2026-06-30T19:55:00.443363Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-10T21:38:25.765851+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-10T21:38:25.765851+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/ac6c05","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., Ricci, C., Trakhtenbrot, B., et al","venue":"The Astrophysical Journal Supplement Series","work_id":"0b81aaa9-fc27-4012-8af1-77334ca18b45","year":2022},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:6e9b6998bd052e15b925decc77700559da2c1ada5b45c3cb927f0e4e7c825451","observation_id":"b970003a-b2d0-41f3-b038-479f25503391","resolution":{"observed_at":"2026-06-30T19:55:00.405140Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-12T23:38:09.859666+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-12T23:38:09.859666+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202555400","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Y., Pushkarev, A","venue":"Astronomy and Astrophysics","work_id":"6812721d-057f-4b66-8633-f6b0900e0613","year":2025},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:7dfb5d95b3bf45748ed8f60ce0cb79331b35eccf9cfc74cfe24060e8f088b306","observation_id":"23a439b7-c65b-4c05-aacd-f208d3886511","resolution":{"observed_at":"2026-06-30T19:55:00.434432Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:58.003011+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:58.003011+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202346710","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, A&A, 679, A46, doi: 10.1051/0004-6361/202346710","venue":"Astronomy and Astrophysics","work_id":"2d58c01b-cb13-4324-96e6-543d7155f288","year":2023},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:3b7d5e14dfdccc43172acc59ee62fd8b01b967854070d1f3f3a1692bf9e3bdeb","observation_id":"fc6ce704-975c-4a8f-8f79-64f6f2188420","resolution":{"observed_at":"2026-06-30T19:55:00.421452Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:58.512011+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:58.512011+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/abf1ec","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"B., et al","venue":"The Astrophysical Journal Letters","work_id":"70a1cf3c-3b21-461f-beff-b6f451005cf7","year":2041},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:a4c513c92b44c7076fcf8d37656b9aaf6aecefa962ada316e86d9c967b9fe12a","observation_id":"646dd252-5fc3-4c81-b7a5-eb9bee45f521","resolution":{"observed_at":"2026-06-30T19:55:00.398891Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:58.991361+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:58.991361+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.110.123014","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"B., et al","venue":"Physical review. D/Physical review. D.","work_id":"e9d68de5-e01f-4779-83fd-ccb69894b324","year":2024},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:0ab9ddb77658ac25792774749ff60e32b031b0cf85fda125dbd61a6603bad62b","observation_id":"1729717d-6485-4340-b8c2-759ee15b3e15","resolution":{"observed_at":"2026-06-30T19:55:00.432530Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:59.416132+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:59.416132+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2605.13588","last_updated":"2026-05-13T14:23:24Z","snapshot_observed_at":"2026-08-12T14:17:42.053457Z","submitted_at":"2026-05-13T14:23:24Z","title":"On the Apparent Correlation between X-ray and Neutrino Luminosities of Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":"2605.13588","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.13588","snapshot_observed_at":"2026-06-30T19:55:01.361140Z","title":"On the Apparent Correlation between X-ray and Neutrino Luminosities of Active Galactic Nuclei","venue":"astro-ph.HE","work_id":"4e097296-fa0a-4ba8-8b3d-7de2df25f001","year":2026},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"cited_paper":"/paper/2605.13588","citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:36340a2d70e6912e38578e2160cee9390c1ddfa19be0d948d7815d0940b73341","observation_id":"e24dfb20-025b-43e1-ab28-8601b30cebf3","resolution":{"observed_at":"2026-06-30T19:55:01.362731Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-07T22:34:12.954550Z","title":"S., French, H","venue":null,"work_id":"fa0ed543-c3c9-479c-9b1a-6d28b949b1ec","year":1978},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:ebe5dd7594bea098104991b1668705107691468444fed0b923509345b23e3402","observation_id":"8b46d5d0-d77b-4947-9c36-2060e2532a8d","resolution":{"observed_at":"2026-07-07T22:34:12.956343Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.125.011101","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"S., & M´ esz´ aros, P","venue":"Physical Review Letters","work_id":"1d85d61b-f16b-4fb2-9133-1819c2472a6a","year":2020},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:b7112b8463d089f908b2c79b10dc5e5f4641d28ac960fd6161f5a2f573b9d2d9","observation_id":"1d8c24ac-c125-4d5c-a194-88d8c5b020ba","resolution":{"observed_at":"2026-06-30T19:55:00.374603Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:25:59.887394+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:25:59.887394+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.132.101002","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Physical Review Letters","work_id":"5b05e45b-b6e8-4180-a9bc-f1e99c80a273","year":2024},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:91d78a8afa3a796482c5cb34c316feced6406da7b849c64aac5d7bb3841d4c7c","observation_id":"5894ef0d-d93d-48a5-b7fc-28a7c36c891f","resolution":{"observed_at":"2026-06-30T19:55:00.424830Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:26:00.317157+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:26:00.317157+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01882","last_updated":"2018-01-05T19:00:01Z","snapshot_observed_at":"2026-08-14T19:57:37.448460Z","submitted_at":"2018-01-05T19:00:01Z","title":"The 105 month Swift-BAT all-sky hard X-ray survey","version":1},"cited_work":{"arxiv_id":"1801.01882","doi":"10.3847/1538-4365/aaa7fd","metadata_source":"pith","pith_arxiv_id":"1801.01882","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"B., et al","venue":"astro-ph.HE","work_id":"31dae4d3-1ada-4dd0-9198-b829d960eabe","year":2018},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"cited_paper":"/paper/1801.01882","citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:742b715a122b6c4bf924d46832bb354ad17f6198bbaff546471e99811e8bc43c","observation_id":"d8509b15-f072-412d-9fe5-e5421dae2c1e","resolution":{"observed_at":"2026-06-30T19:55:00.426924Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-22T05:38:30.411456+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-22T05:38:30.411456+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s00159-017-0102-9","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"M., Assef, R","venue":"The Astronomy and Astrophysics Review","work_id":"d06b83b2-dc20-4293-822b-12c7dc6f4aaf","year":2017},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:a0c4804b061bc78c1b8330281ec4dfd814ae357dec3c5a82fc640eee843b89bf","observation_id":"8aa6d098-d846-4ec1-b21c-f1a2ac21ff32","resolution":{"observed_at":"2026-06-30T19:55:00.441436Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-13T22:20:55.830681+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T22:20:55.830681+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stw472","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2016, MNRAS, 458, 2836, doi: 10.1093/mnras/stw472","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"da0b4717-3d1b-421a-a200-dfbb9747bd7a","year":2016},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:c4764803c59f288ebfb8c8febf690e52c6d34cf8f04e76706e97e3eb91f6c503","observation_id":"740b35ae-f6cd-4a67-85a0-2c2835cf3fed","resolution":{"observed_at":"2026-06-30T19:55:00.445273Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:26:00.749653+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:26:00.749653+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2024/05/133","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"V., Burenin, R","venue":"Journal of Cosmology and Astroparticle Physics","work_id":"ca2a5722-438b-4d7d-8361-23941d10f2a3","year":2024},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:f42f73fd4de3784bc1d6c2b8b6e9317f1965baf660015c89924a8687a6984a81","observation_id":"5a89bc7e-7e03-4f34-8d5e-5da1bc7aac90","resolution":{"observed_at":"2026-06-30T19:55:00.419658Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T13:26:01.24547+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T13:26:01.24547+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/acda27","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, ApJL, 952, L28, doi: 10.3847/2041-8213/acda27","venue":"The Astrophysical Journal Letters","work_id":"536fed35-2547-42d5-9baf-77ddbbd97ea2","year":2041},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:b0a2e17d26ac6ff12ab519ef525706f368100283734808ad7c8e854c278507bc","observation_id":"269e6206-fab2-4425-ae51-da63cb1ba369","resolution":{"observed_at":"2026-06-30T19:55:00.407174Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-12T10:19:33.47462+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T10:19:33.47462+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stae273","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Monthly Notices of the Royal Astronomical Society , volume =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"0b83dab0-bd79-4b0a-8085-ee81fc85f04b","year":2024},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:e3e0d6e12a2ad3b8f40140035c3d182ec48229dbd1abe76ee37f18e04ad03cb9","observation_id":"698382f1-ec78-4d9a-b311-8538a47eec41","resolution":{"observed_at":"2026-06-30T19:55:00.430530Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-05-24T06:53:52.550792+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T06:53:52.550792+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0008425","last_updated":"2000-08-28T14:30:56Z","snapshot_observed_at":"2026-07-07T00:12:42.550606Z","submitted_at":"2000-08-28T14:30:56Z","title":"On the Absorption of X-rays in the Interstellar Medium","version":1},"cited_work":{"arxiv_id":"astro-ph/0008425","doi":"10.1086/317016","metadata_source":"pith","pith_arxiv_id":"astro-ph/0008425","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"2000, ApJ, 542, 914, doi: 10.1086/317016","venue":"astro-ph","work_id":"11a9d7b2-27c5-47ad-9632-8957164bc632","year":2000},"citing_paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-06-30T19:52:33.605384Z"},"links":{"cited_paper":"/paper/astro-ph/0008425","citing_paper":"/paper/2605.15360"},"observation_digest":"sha256:9ddea10580c19128a911a2880c9014f008dbf666d1dd0af1266e93c0619b8805","observation_id":"d80bb792-ec81-441b-8e78-01563a9e56b8","resolution":{"observed_at":"2026-06-30T19:55:00.382631Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-22T04:08:12.544124+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-22T04:08:12.544124+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.15360","last_updated":"2026-06-28T17:16:58Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-19T19:13:53.042356Z","submitted_at":"2026-05-14T19:39:45Z","title":"Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars"},"reference_resolution":{"displayed":36,"state_counts":{"malformed_identifier":0,"metadata_mismatch":8,"parse_uncertain":0,"unresolved":0,"verified_exact":27,"verified_fuzzy":1},"total_outbound_references":36},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 36 of 36 outbound references and 0 inbound Pith citation observations for arXiv:2605.15360."}