{"as_of":"2026-08-08T08:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ea8b911f16a381fc15efeccdcbc50c76bf1869984e2f5ae703d87690cb669558","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T20:40:57.671882Z","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":"2026-07-08T00:54:20.848078Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1309.0755","last_updated":"2013-09-03T17:39:29Z","snapshot_observed_at":"2026-07-06T03:22:04.722603Z","submitted_at":"2013-09-03T17:39:29Z","title":"The Swift/BAT Hard X-ray Transient Monitor","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.0755","snapshot_observed_at":"2026-08-07T11:52:52.424606Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.03349","last_updated":"2025-06-02T05:32:59Z","snapshot_observed_at":"2026-08-07T11:41:47.279778Z","submitted_at":"2025-06-02T05:32:59Z","title":"Effectiveness of Stacks in the Stacked Hilbert-Huang Transform","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T11:52:52.424606Z"},"links":{"cited_paper":"/paper/1309.0755","citing_paper":"/paper/2506.03349"},"observation_digest":"sha256:25dd4b0c4f6e7596352b0d230f2681501874f5ff0c6ff034cb90b8df6fb2f2b6","observation_id":"2508a2b1-be6f-436b-82f7-777422b5979f","resolution":{"observed_at":"2026-08-07T11:52:52.424606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.0755","last_updated":"2013-09-03T17:39:29Z","snapshot_observed_at":"2026-07-06T03:22:04.722603Z","submitted_at":"2013-09-03T17:39:29Z","title":"The Swift/BAT Hard X-ray Transient Monitor","version":1},"cited_work":{"arxiv_id":"1309.0755","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.0755","snapshot_observed_at":"2026-07-08T00:54:20.848078Z","title":"The Swift/BAT Hard X-ray Transient Monitor","venue":"astro-ph.HE","work_id":"3bd8e5f5-4df1-4510-b57c-1205992bdbff","year":2013},"citing_paper":{"arxiv_id":"2606.09992","last_updated":"2026-06-26T20:15:27Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-08T18:00:03Z","title":"EP260321a/SN 2026gzf: The Faintest Shock Breakout Associated with a Broad-Lined Supernova","version":1},"reference_index":257,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1309.0755","citing_paper":"/paper/2606.09992"},"observation_digest":"sha256:20338531ae5be0f9475f717cf1999e11d8ed0cc22705646aff210cf6b6ce56cb","observation_id":"1d89d57f-8797-4246-af6a-ce8ba032dd1e","resolution":{"observed_at":"2026-06-27T18:41:08.786705Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1309.0755","last_updated":"2013-09-03T17:39:29Z","snapshot_observed_at":"2026-07-06T03:22:04.722603Z","submitted_at":"2013-09-03T17:39:29Z","title":"The Swift/BAT Hard X-ray Transient Monitor","version":1},"cited_work":{"arxiv_id":"1309.0755","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.0755","snapshot_observed_at":"2026-07-08T00:54:20.848078Z","title":"The Swift/BAT Hard X-ray Transient Monitor","venue":"astro-ph.HE","work_id":"3bd8e5f5-4df1-4510-b57c-1205992bdbff","year":2013},"citing_paper":{"arxiv_id":"2607.05182","last_updated":"2026-07-06T15:00:04Z","snapshot_observed_at":"2026-07-09T23:18:22.261215Z","submitted_at":"2026-07-06T15:00:04Z","title":"Spectropolarimetric detection of baryonic mass loading in a transient relativistic jet: application to the black hole X-ray binary Swift J1727.8$-$1613","version":1},"reference_index":286,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1309.0755","citing_paper":"/paper/2607.05182"},"observation_digest":"sha256:af90366055f01ee032d74d3108f35001611adba5c16cf323c4a8b903ee83b894","observation_id":"60a3ef2e-7d7d-4540-a98c-6c6aac8ad230","resolution":{"observed_at":"2026-07-08T00:54:20.849401Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1309.0755","last_updated":"2013-09-03T17:39:29Z","snapshot_observed_at":"2026-07-06T03:22:04.722603Z","submitted_at":"2013-09-03T17:39:29Z","title":"The Swift/BAT Hard X-ray Transient Monitor","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.0755","snapshot_observed_at":"2026-08-07T20:40:57.671882Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05946","last_updated":"2026-08-06T12:13:20Z","snapshot_observed_at":"2026-08-08T08:17:30.619958Z","submitted_at":"2026-08-06T12:13:20Z","title":"Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry","version":1},"reference_index":226,"source":"arxiv_source","source_observed_at":"2026-08-07T20:40:57.671882Z"},"links":{"cited_paper":"/paper/1309.0755","citing_paper":"/paper/2608.05946"},"observation_digest":"sha256:717c40833cad5ac0a4368f5a588975e1e2dca612ce0587d7aeeb8f989c9cc751","observation_id":"60bf9298-c425-4d61-bc96-811b85442053","resolution":{"observed_at":"2026-08-07T20:40:57.671882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1309.0755/citation-record","integrity":"/paper/1309.0755/integrity","json":"/paper/1309.0755/citation-record.json","paper":"/paper/1309.0755"},"outbound":[],"paper":{"arxiv_id":"1309.0755","last_updated":"2013-09-03T17:39:29Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T03:22:04.722603Z","submitted_at":"2013-09-03T17:39:29Z","title":"The Swift/BAT Hard X-ray Transient Monitor"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1309.0755."}