{"as_of":"2026-08-15T16:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5a3d2949890d46d5ac8ceaa49ba08f13e68b570008bf7962471a889332a1aa52","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:48:03.464682Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":206,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-08-14T11:46:09.565930Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08364","last_updated":"2019-08-22T13:35:44Z","snapshot_observed_at":"2026-08-15T05:44:29.806404Z","submitted_at":"2019-08-22T13:35:44Z","title":"H.E.S.S. searches for TeV gamma rays associated to high-energy neutrinos","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:46:09.565930Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/1908.08364"},"observation_digest":"sha256:943b904de7068921c149466d9687f898bceb237991d07dbe658c4a9d76870f0b","observation_id":"34e15cf3-bbad-48de-96de-424a50f44f54","resolution":{"observed_at":"2026-08-14T11:46:09.565930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-08-14T11:48:03.464682Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08421","last_updated":"2019-12-02T02:26:09Z","snapshot_observed_at":"2026-08-15T15:06:05.190906Z","submitted_at":"2019-08-22T14:58:14Z","title":"Multi-messenger tests of cosmic-ray acceleration in radiatively inefficient accretion flows","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T11:48:03.464682Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/1908.08421"},"observation_digest":"sha256:bbe8b8c3739e83c8b389b26e80e998a65cbab2596354eac4ef78aa88cf2a130d","observation_id":"6bd5af95-01b8-432b-a75d-e6e23d5e8c0f","resolution":{"observed_at":"2026-08-14T11:48:03.464682Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-08-14T04:42:38.070831Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.02798","last_updated":"2019-09-06T10:00:43Z","snapshot_observed_at":"2026-08-15T12:39:57.322245Z","submitted_at":"2019-09-06T10:00:43Z","title":"Following up Transient Sources at Very High Energies with MAGIC","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:38.070831Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/1909.02798"},"observation_digest":"sha256:938a0e52b67a75d9a4cca586c536c73af2ac966b579be205023a2857c2a49687","observation_id":"6f8abfda-312a-4560-9427-175f643126e4","resolution":{"observed_at":"2026-08-14T04:42:38.070831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-08-12T14:29:06.756841Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.15329","last_updated":"2024-11-22T19:50:49Z","snapshot_observed_at":"2026-08-13T18:41:37.122331Z","submitted_at":"2024-11-22T19:50:49Z","title":"Transforming Antarctic Ice into a Cherenkov Neutrino Detector","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T14:29:06.756841Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/2411.15329"},"observation_digest":"sha256:487439837c9a3a5a2e7c826488d017344396286e7e08fd89a25bc0500ce4bad2","observation_id":"4c0ac188-0a24-4cd2-83dd-99f1d90fd472","resolution":{"observed_at":"2026-08-12T14:29:06.756841Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":"1612.06028","doi":"10.1016/j.astropartphys.2017.05.002","metadata_source":"pith","pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The IceCube Realtime Alert System","venue":"astro-ph.HE","work_id":"aedcfaf1-d531-42a6-ad38-42dcb309fffb","year":2016},"citing_paper":{"arxiv_id":"2606.01158","last_updated":"2026-05-31T11:03:43Z","snapshot_observed_at":"2026-07-06T23:41:43.820102Z","submitted_at":"2026-05-31T11:03:43Z","title":"Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/2606.01158"},"observation_digest":"sha256:6703318c18b4cb5edca9d268016bd1166cf37b527d772959828a663ebcd8bfd7","observation_id":"5a9854fe-cb03-4ad5-a688-3487feeee33f","resolution":{"observed_at":"2026-06-28T16:42:23.523373Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-03T19:38:35.974681+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T19:38:35.974681+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":"1612.06028","doi":"10.1016/j.astropartphys.2017.05.002","metadata_source":"pith","pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The IceCube Realtime Alert System","venue":"astro-ph.HE","work_id":"aedcfaf1-d531-42a6-ad38-42dcb309fffb","year":2016},"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":1},"reference_index":168,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/2606.30764"},"observation_digest":"sha256:3881eb99b1c9fe56a5ed6cdab0a78c2031c7648beedf155ea284f280982b20e2","observation_id":"4ae54911-65e4-4ef0-9337-ebc2364794aa","resolution":{"observed_at":"2026-07-01T02:05:14.038864Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-03T19:38:35.974681+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T19:38:35.974681+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06028","snapshot_observed_at":"2026-07-14T16:57:50.370612Z","title":"Astropart Phys 92:30--41","venue":null,"work_id":null,"year":2017},"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":2,"source":"arxiv_source","source_observed_at":"2026-07-14T16:57:50.370612Z"},"links":{"cited_paper":"/paper/1612.06028","citing_paper":"/paper/2606.30764"},"observation_digest":"sha256:d54880a83bf3a38ba4fb7ef8c3aefb1abd3d313593c912168feb53a943dda562","observation_id":"5a768ccf-a5f6-4fde-b30f-6a0e384771f3","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"}}],"links":{"evidence":"/evidence","html":"/paper/1612.06028/citation-record","integrity":"/paper/1612.06028/integrity","json":"/paper/1612.06028/citation-record.json","paper":"/paper/1612.06028"},"outbound":[],"paper":{"arxiv_id":"1612.06028","last_updated":"2017-05-23T15:03:43Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T21:24:50.790244Z","submitted_at":"2016-12-19T02:25:44Z","title":"The IceCube Realtime Alert System"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1612.06028."}