{"as_of":"2026-08-11T18:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4b2ab8f71a8d7c69a91b0c0aae3632b929265d972a098b7ebf99ea1e3fe7e601","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T17:27:50.028010Z","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":"2026-08-11T00:33:41.610714Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.18291","last_updated":"2024-07-25T18:00:00Z","snapshot_observed_at":"2026-08-04T17:40:20.331874Z","submitted_at":"2024-07-25T18:00:00Z","title":"The X-ray Luminous Type Ibn SN 2022ablq: Estimates of Pre-explosion Mass Loss and Constraints on Precursor Emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18291","snapshot_observed_at":"2026-08-11T17:27:50.028010Z","title":"2024, arXiv e-prints, arXiv:2407.18291, doi: 10.48550/arXiv.2407.18291","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.09066","last_updated":"2024-12-12T08:53:00Z","snapshot_observed_at":"2026-08-11T17:19:02.105614Z","submitted_at":"2024-12-12T08:53:00Z","title":"Insights into the Properties of Type Ibn/Icn Supernovae and Their Progenitor Channels through X-ray Emission","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T17:27:50.028010Z"},"links":{"cited_paper":"/paper/2407.18291","citing_paper":"/paper/2412.09066"},"observation_digest":"sha256:a0b8710a11157300b649fb1bde32052cc9043d1430b3c0beaf089aa4ab3f2cd5","observation_id":"f5d990d6-7960-4b0a-8329-690c3761cf91","resolution":{"observed_at":"2026-08-11T17:27:50.028010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18291","last_updated":"2024-07-25T18:00:00Z","snapshot_observed_at":"2026-08-04T17:40:20.331874Z","submitted_at":"2024-07-25T18:00:00Z","title":"The X-ray Luminous Type Ibn SN 2022ablq: Estimates of Pre-explosion Mass Loss and Constraints on Precursor Emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18291","snapshot_observed_at":"2026-08-11T16:42:03.568730Z","title":"2024, arXiv e-prints, arXiv:2407.18291","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.09893","last_updated":"2025-01-23T12:55:33Z","snapshot_observed_at":"2026-08-11T16:33:45.073540Z","submitted_at":"2024-12-13T06:26:28Z","title":"Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae","version":2},"reference_index":108,"source":"arxiv_source","source_observed_at":"2026-08-11T16:42:03.568730Z"},"links":{"cited_paper":"/paper/2407.18291","citing_paper":"/paper/2412.09893"},"observation_digest":"sha256:cb1e6bd2c74dbce48ed57459dbedc6d8ba87bcf5049ea8a5a19ac0fcd1490228","observation_id":"452a60e3-c16e-4c57-b92c-b74273ca943b","resolution":{"observed_at":"2026-08-11T16:42:03.568730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18291","last_updated":"2024-07-25T18:00:00Z","snapshot_observed_at":"2026-08-04T17:40:20.331874Z","submitted_at":"2024-07-25T18:00:00Z","title":"The X-ray Luminous Type Ibn SN 2022ablq: Estimates of Pre-explosion Mass Loss and Constraints on Precursor Emission","version":1},"cited_work":{"arxiv_id":"2407.18291","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.18291","snapshot_observed_at":"2026-08-11T00:33:41.610714Z","title":"The X-ray Luminous Type Ibn SN 2022ablq: Estimates of Pre-explosion Mass Loss and Constraints on Precursor Emission","venue":"astro-ph.HE","work_id":"a51c1aea-ca69-4e0d-bedf-82b366bee783","year":2024},"citing_paper":{"arxiv_id":"2608.07661","last_updated":"2026-08-07T18:00:01Z","snapshot_observed_at":"2026-08-11T18:14:04.950476Z","submitted_at":"2026-08-07T18:00:01Z","title":"Wild behaviour near the finish line: the Type Ibn SN 2020able and its stratified environment","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-11T00:33:39.180337Z"},"links":{"cited_paper":"/paper/2407.18291","citing_paper":"/paper/2608.07661"},"observation_digest":"sha256:62f72550a7492a28114e1acbfc39ac0dd054ffe823a297e4c0c4017dd4e4a904","observation_id":"66c5ce1a-b2f6-4c19-9465-d092b52bde57","resolution":{"observed_at":"2026-08-11T00:33:41.616665Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2407.18291/citation-record","integrity":"/paper/2407.18291/integrity","json":"/paper/2407.18291/citation-record.json","paper":"/paper/2407.18291"},"outbound":[],"paper":{"arxiv_id":"2407.18291","last_updated":"2024-07-25T18:00:00Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-04T17:40:20.331874Z","submitted_at":"2024-07-25T18:00:00Z","title":"The X-ray Luminous Type Ibn SN 2022ablq: Estimates of Pre-explosion Mass Loss and Constraints on Precursor Emission"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.18291."}