{"as_of":"2026-08-20T19:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:dfde73ed26ebc404652320e7f71419ec656364e1cd83c49f0e0de049be30f477","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T23:49:10.314351Z","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":"2026-07-03T07:37:44.846408Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2204.00737","last_updated":"2022-04-02T01:48:02Z","snapshot_observed_at":"2026-08-16T17:09:49.724576Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.00737","snapshot_observed_at":"2026-08-03T23:49:10.314351Z","title":"515(1):L89--L93","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.04254","last_updated":"2026-05-28T09:50:04Z","snapshot_observed_at":"2026-08-14T17:07:56.525904Z","submitted_at":"2025-11-06T10:42:14Z","title":"3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae","version":2},"reference_index":231,"source":"arxiv_source","source_observed_at":"2026-08-03T23:49:10.314351Z"},"links":{"cited_paper":"/paper/2204.00737","citing_paper":"/paper/2511.04254"},"observation_digest":"sha256:cd1d1a2c807fa3d526d824378f37074b882af5fa642a0252de0472f9032941c9","observation_id":"6826e5d4-aa06-4f84-b0a8-edf50dfd5f33","resolution":{"observed_at":"2026-08-03T23:49:10.314351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.00737","last_updated":"2022-04-02T01:48:02Z","snapshot_observed_at":"2026-08-16T17:09:49.724576Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer","version":1},"cited_work":{"arxiv_id":"2204.00737","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.00737","snapshot_observed_at":"2026-07-03T07:37:44.846408Z","title":"Hotokezaka, M","venue":null,"work_id":"9efd4ecf-7491-4261-9cbd-25d97ee51462","year":2022},"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":54,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/2204.00737","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:efbfaecec3421008b6a441ce58a0732f9c6c0c71aee1f1f159ea7073a10004a1","observation_id":"c076382e-86b7-4e5a-b9c3-1a3d7a5db328","resolution":{"observed_at":"2026-07-03T07:37:44.848187Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.00737","last_updated":"2022-04-02T01:48:02Z","snapshot_observed_at":"2026-08-16T17:09:49.724576Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.00737","snapshot_observed_at":"2026-07-12T05:14:58.841553Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03045","last_updated":"2026-07-03T07:34:46Z","snapshot_observed_at":"2026-08-13T11:34:49.188005Z","submitted_at":"2026-07-03T07:34:46Z","title":"nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-07-12T05:14:58.841553Z"},"links":{"cited_paper":"/paper/2204.00737","citing_paper":"/paper/2607.03045"},"observation_digest":"sha256:bd50a508185f5ba10df27760d90800eb00d6773d270ea9b871a582198ead4c74","observation_id":"2eae86b6-b696-4ac6-87d1-3da67be080c2","resolution":{"observed_at":"2026-07-12T05:14:58.841553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.00737","last_updated":"2022-04-02T01:48:02Z","snapshot_observed_at":"2026-08-16T17:09:49.724576Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.00737","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10818","last_updated":"2026-07-12T16:08:28Z","snapshot_observed_at":"2026-08-19T16:33:40.370245Z","submitted_at":"2026-07-12T16:08:28Z","title":"Late-time emission-line profiles from kilonova models","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2204.00737","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:c7063b90abfab9d9fd05f44da6ea25c4463ba9633c735213c3a32883d3c465f8","observation_id":"74576fd8-f259-4f9f-9b39-3c10d8a01b68","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.00737","last_updated":"2022-04-02T01:48:02Z","snapshot_observed_at":"2026-08-16T17:09:49.724576Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.00737","snapshot_observed_at":"2026-08-01T23:34:10.166185Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15390","last_updated":"2026-07-16T18:41:18Z","snapshot_observed_at":"2026-08-14T17:28:00.498150Z","submitted_at":"2026-07-16T18:41:18Z","title":"Luminous Red Novae as shock-powered transients I: Electron-scattering wings and deviations from Case B","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-01T23:34:10.166185Z"},"links":{"cited_paper":"/paper/2204.00737","citing_paper":"/paper/2607.15390"},"observation_digest":"sha256:825480acea337486696d7bd3225ef8823c485ca82a2241d8fec751e7897374a6","observation_id":"e2a8aafa-74ed-4c8d-b198-96c5441302ea","resolution":{"observed_at":"2026-08-01T23:34:10.166185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2204.00737/citation-record","integrity":"/paper/2204.00737/integrity","json":"/paper/2204.00737/citation-record.json","paper":"/paper/2204.00737"},"outbound":[],"paper":{"arxiv_id":"2204.00737","last_updated":"2022-04-02T01:48:02Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T17:09:49.724576Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2204.00737."}