{"as_of":"2026-08-17T01:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ad3bee8a5f0373f01023c68bf8adefba81d48759eb82ae98a3d72928df6abfe9","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:23:57.141488Z","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":"2026-05-11T00:05:50.373187Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1609.06328","last_updated":"2016-10-25T10:26:22Z","snapshot_observed_at":"2026-08-14T21:38:57.473464Z","submitted_at":"2016-09-20T20:01:06Z","title":"Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.06328","snapshot_observed_at":"2026-08-14T13:23:57.141488Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.05325","last_updated":"2019-08-14T19:46:21Z","snapshot_observed_at":"2026-08-16T18:56:49.682696Z","submitted_at":"2019-08-14T19:46:21Z","title":"Highlights of Galactic Physics with VERITAS","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T13:23:57.141488Z"},"links":{"cited_paper":"/paper/1609.06328","citing_paper":"/paper/1908.05325"},"observation_digest":"sha256:67b84ba62e7e105bac07b22d4ab970ce6d46e3807be567913a8f05c3a9f41596","observation_id":"575434ce-4d64-4060-a8e5-b9b5149e744e","resolution":{"observed_at":"2026-08-14T13:23:57.141488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.06328","last_updated":"2016-10-25T10:26:22Z","snapshot_observed_at":"2026-08-14T21:38:57.473464Z","submitted_at":"2016-09-20T20:01:06Z","title":"Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron","version":2},"cited_work":{"arxiv_id":"1609.06328","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1609.06328","snapshot_observed_at":"2026-07-04T21:29:43.791435Z","title":null,"venue":null,"work_id":"1c14da4e-fa53-4993-92b2-5d46ab54b7e1","year":2017},"citing_paper":{"arxiv_id":"2604.08175","last_updated":"2026-04-09T12:32:10Z","snapshot_observed_at":"2026-08-14T03:12:46.146347Z","submitted_at":"2026-04-09T12:32:10Z","title":"How many VHE gamma-ray binaries with young pulsars can be observed?","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-10T18:42:16.317215Z"},"links":{"cited_paper":"/paper/1609.06328","citing_paper":"/paper/2604.08175"},"observation_digest":"sha256:bd5f5abeea8438ef4851bc88e31b47bc39149c9c0f4f788c776f5398513a376e","observation_id":"8b74d881-e905-4ca4-97bc-0adc129829eb","resolution":{"observed_at":"2026-07-04T21:29:43.791435Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1609.06328/citation-record","integrity":"/paper/1609.06328/integrity","json":"/paper/1609.06328/citation-record.json","paper":"/paper/1609.06328"},"outbound":[],"paper":{"arxiv_id":"1609.06328","last_updated":"2016-10-25T10:26:22Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-14T21:38:57.473464Z","submitted_at":"2016-09-20T20:01:06Z","title":"Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.06328."}