{"as_of":"2026-08-15T15:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0e5d9e5b30b19fd053c91d9c9effb6dcb5fe567cd4fe394d8ead8c94cc787af9","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":"2026-08-15T06:32:42.880941+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":"2026-08-14T11:35:56.377518Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-14T11:35:57.669196Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1704.05851","last_updated":"2017-08-01T15:16:53Z","snapshot_observed_at":"2026-08-14T21:05:58.003220Z","submitted_at":"2017-04-19T18:00:02Z","title":"Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models","version":3},"cited_work":{"arxiv_id":"1704.05851","doi":null,"metadata_source":"pith","pith_arxiv_id":"1704.05851","snapshot_observed_at":"2026-08-14T11:35:57.669196Z","title":"Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models","venue":"astro-ph.HE","work_id":"cb2ef82e-d451-470e-abae-b8157ba72cc9","year":2017},"citing_paper":{"arxiv_id":"1908.08822","last_updated":"2019-12-09T07:53:33Z","snapshot_observed_at":"2026-08-15T12:42:26.082822Z","submitted_at":"2019-08-23T13:39:38Z","title":"Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T11:35:56.377518Z"},"links":{"cited_paper":"/paper/1704.05851","citing_paper":"/paper/1908.08822"},"observation_digest":"sha256:0fe265d9cd4a0ec9f7716eafe889b0a75891872343501a34001b83fdd72b0ec2","observation_id":"08b1cca8-5d6a-4857-b697-48e4f1251ec2","resolution":{"observed_at":"2026-08-14T11:35:57.674031Z","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":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1704.05851","last_updated":"2017-08-01T15:16:53Z","snapshot_observed_at":"2026-08-14T21:05:58.003220Z","submitted_at":"2017-04-19T18:00:02Z","title":"Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.05851","snapshot_observed_at":"2026-07-31T07:22:46.099216Z","title":"Where and When: Optimal Scheduling of the Electromagnetic Follow-up of Gravitational-wave Events Based on Counterpart Light-curve Models","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.28438","last_updated":"2026-07-30T16:13:33Z","snapshot_observed_at":"2026-08-13T12:07:24.939195Z","submitted_at":"2026-07-30T16:13:33Z","title":"Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology","version":1},"reference_index":228,"source":"arxiv_source","source_observed_at":"2026-07-31T07:22:46.099216Z"},"links":{"cited_paper":"/paper/1704.05851","citing_paper":"/paper/2607.28438"},"observation_digest":"sha256:bc3b2aae6750141847a2661f613d7224229f6ff3a321080fdbc6ca3b51e60d87","observation_id":"5b341eca-f98e-448a-bd6c-fa8195df4814","resolution":{"observed_at":"2026-07-31T07:22:46.099216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1704.05851/citation-record","integrity":"/paper/1704.05851/integrity","json":"/paper/1704.05851/citation-record.json","paper":"/paper/1704.05851"},"outbound":[],"paper":{"arxiv_id":"1704.05851","last_updated":"2017-08-01T15:16:53Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T21:05:58.003220Z","submitted_at":"2017-04-19T18:00:02Z","title":"Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models"},"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 2 inbound Pith citation observations for arXiv:1704.05851."}