{"as_of":"2026-08-16T01:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a5d888efc0661146513b8521f48c84bde7c7be4e1f37202f883313af52272ccb","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":"2026-08-11T04:39:37.228040Z","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":"2026-07-10T13:17:05.705076Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-08-11T04:39:37.228040Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.18681","last_updated":"2024-12-24T21:05:34Z","snapshot_observed_at":"2026-08-12T15:13:28.374358Z","submitted_at":"2024-12-24T21:05:34Z","title":"Gamma-ray bursts: what do we know today that we did not know 10 years ago?","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-11T04:39:37.228040Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2412.18681"},"observation_digest":"sha256:d1c5f4efbd2d86e1b4ab336f100f5e22b346e40bee3c96bbf1a5f914412e38e4","observation_id":"a5dfc7d0-0eb6-4bd0-bc94-b6f9e1d49d0f","resolution":{"observed_at":"2026-08-11T04:39:37.228040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-08-05T15:52:56.311653Z","title":"Arcavi et al., Nature 551, 64 (2017), arXiv:1710.05843 [astro-ph.HE]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.19342","last_updated":"2025-08-26T18:00:29Z","snapshot_observed_at":"2026-08-12T21:48:50.124546Z","submitted_at":"2025-08-26T18:00:29Z","title":"Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-05T15:52:56.311653Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2508.19342"},"observation_digest":"sha256:18dcee9aad5fdf89c2f6a6c3e29518150714e607a1eee91b8bb1a5d621d1e21f","observation_id":"422ec523-c605-40c1-8afb-e4e4380af585","resolution":{"observed_at":"2026-08-05T15:52:56.311653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":"1710.05843","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-07-10T13:17:05.705076Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","venue":"astro-ph.HE","work_id":"408ec39f-99c9-48cf-940f-b5bba8fbe773","year":2017},"citing_paper":{"arxiv_id":"2605.13719","last_updated":"2026-05-13T16:04:26Z","snapshot_observed_at":"2026-08-11T13:32:22.320156Z","submitted_at":"2026-05-13T16:04:26Z","title":"The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-14T17:44:05.459557Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2605.13719"},"observation_digest":"sha256:1a6ac90de6b826797e6645e34c2518ef2e480a69aa7d8d38dff49b01dbb3ff30","observation_id":"c29f1400-766f-4f97-a151-da6c9b692a36","resolution":{"observed_at":"2026-05-14T17:49:23.369851Z","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":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":"1710.05843","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-07-10T13:17:05.705076Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","venue":"astro-ph.HE","work_id":"408ec39f-99c9-48cf-940f-b5bba8fbe773","year":2017},"citing_paper":{"arxiv_id":"2605.16132","last_updated":"2026-05-15T16:15:03Z","snapshot_observed_at":"2026-08-15T00:44:35.831307Z","submitted_at":"2026-05-15T16:15:03Z","title":"Nucleosynthesis in the fast ejecta of a neutron star merger","version":1},"reference_index":135,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2605.16132"},"observation_digest":"sha256:a2e2889700780aec0b6772b2e08af2b2b9b5ae6b2ca13fca1ae91c806be112a0","observation_id":"7168698b-5533-4d02-9d57-c545a79e1cf2","resolution":{"observed_at":"2026-05-20T16:23:35.133249Z","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":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":"1710.05843","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-07-10T13:17:05.705076Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","venue":"astro-ph.HE","work_id":"408ec39f-99c9-48cf-940f-b5bba8fbe773","year":2017},"citing_paper":{"arxiv_id":"2606.11299","last_updated":"2026-06-09T18:00:02Z","snapshot_observed_at":"2026-08-12T15:48:11.069118Z","submitted_at":"2026-06-09T18:00:02Z","title":"A magnetar formation in binary neutron star merger","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:f056dab2aba668ebe5cd636d60ebe6f75064bba9769e7b62931509573e8394f2","observation_id":"1eeb9e04-4d02-4ba3-a18c-21678c9ce8aa","resolution":{"observed_at":"2026-07-03T07:37:44.743963Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":"1710.05843","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-07-10T13:17:05.705076Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","venue":"astro-ph.HE","work_id":"408ec39f-99c9-48cf-940f-b5bba8fbe773","year":2017},"citing_paper":{"arxiv_id":"2607.08090","last_updated":"2026-07-09T03:55:45Z","snapshot_observed_at":"2026-08-02T13:57:46.281635Z","submitted_at":"2026-07-09T03:55:45Z","title":"Multi-wavelength Constraints on the Transient EP250905a","version":1},"reference_index":247,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2607.08090"},"observation_digest":"sha256:8ffc4a01e818f89d44d8673be5bc62d66c0e882faff9ad0bc581a5716d24ca71","observation_id":"95305275-9305-487a-9554-1203d17168ac","resolution":{"observed_at":"2026-07-10T13:17:05.706435Z","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":"1710.05843","last_updated":"2017-10-16T16:57:49Z","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05843","snapshot_observed_at":"2026-07-14T03:58:52.342855Z","title":"Arcaviet al., Nature551, 64 (2017), arXiv:1710.05843 [astro-ph.HE]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.11670","last_updated":"2026-07-13T15:12:18Z","snapshot_observed_at":"2026-08-14T14:33:00.164595Z","submitted_at":"2026-07-13T15:12:18Z","title":"Extending the infrastructure of the BAM code towards resistive general-relativistic magnetohydrodynamics: tests and first applications","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-14T03:58:52.342855Z"},"links":{"cited_paper":"/paper/1710.05843","citing_paper":"/paper/2607.11670"},"observation_digest":"sha256:e8dc77a02b2c58f30128f0bbc1b9183ad5ce108864665032d80848e7d3260643","observation_id":"91bf83d4-ef79-477f-8662-d82109537978","resolution":{"observed_at":"2026-07-14T03:58:52.342855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1710.05843/citation-record","integrity":"/paper/1710.05843/integrity","json":"/paper/1710.05843/citation-record.json","paper":"/paper/1710.05843"},"outbound":[],"paper":{"arxiv_id":"1710.05843","last_updated":"2017-10-16T16:57:49Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T20:23:18.635927Z","submitted_at":"2017-10-16T16:57:49Z","title":"Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger"},"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 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1710.05843."}