{"as_of":"2026-08-11T16:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:88504b5ecc3fbd9712e96c831e6c80e722cb4d87db35c8e6040c2b12c819aeac","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":"2026-08-11T06:34:44.6726+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":"2026-08-06T13:05:34.712486Z","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":"2026-07-10T23:57:49.607414Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1811.05515","last_updated":"2018-11-13T20:00:36Z","snapshot_observed_at":"2026-07-06T07:14:31.358596Z","submitted_at":"2018-11-13T20:00:36Z","title":"On the importance of progenitor asymmetry to shock revival in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.05515","snapshot_observed_at":"2026-08-04T19:19:17.420034Z","title":"MNRAS483(1), 208–222 (2019) https://doi.org/10.1093/mnras/sty3114 arXiv:1811.05515 [astro-ph.HE]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.09419","last_updated":"2025-09-11T13:01:45Z","snapshot_observed_at":"2026-08-09T10:40:14.038903Z","submitted_at":"2025-09-11T13:01:45Z","title":"Impact of rotation on the accretion of entropy perturbations in collapsing massive stars","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-04T19:19:17.420034Z"},"links":{"cited_paper":"/paper/1811.05515","citing_paper":"/paper/2509.09419"},"observation_digest":"sha256:dc81b6b2a012bff5fe85b42b69e804d2bd38f8da48f87231262ed24350f352e3","observation_id":"e6113f25-d556-4ee7-90f1-67d8b497da1f","resolution":{"observed_at":"2026-08-04T19:19:17.420034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.05515","last_updated":"2018-11-13T20:00:36Z","snapshot_observed_at":"2026-07-06T07:14:31.358596Z","submitted_at":"2018-11-13T20:00:36Z","title":"On the importance of progenitor asymmetry to shock revival in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":"1811.05515","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.05515","snapshot_observed_at":"2026-07-10T23:57:49.607414Z","title":"Nagakura, K","venue":"astro-ph.HE","work_id":"e5f1d204-e0a0-41df-897d-deb69374bcd1","year":2018},"citing_paper":{"arxiv_id":"2605.04896","last_updated":"2026-05-06T13:27:04Z","snapshot_observed_at":"2026-08-11T12:23:54.516230Z","submitted_at":"2026-05-06T13:27:04Z","title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-08T15:59:11.556246Z"},"links":{"cited_paper":"/paper/1811.05515","citing_paper":"/paper/2605.04896"},"observation_digest":"sha256:09ae5faeff84da64476e5998e9effa4d36d1e07ba251039ed4a50a996fe1f497","observation_id":"1b5fdea2-3e9a-47a1-98e7-2650e99bdbab","resolution":{"observed_at":"2026-07-04T23:13:37.590880Z","resolver_source":"arxiv_id","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"}},{"citation":{"cited_paper":{"arxiv_id":"1811.05515","last_updated":"2018-11-13T20:00:36Z","snapshot_observed_at":"2026-07-06T07:14:31.358596Z","submitted_at":"2018-11-13T20:00:36Z","title":"On the importance of progenitor asymmetry to shock revival in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":"1811.05515","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.05515","snapshot_observed_at":"2026-07-10T23:57:49.607414Z","title":"Nagakura, K","venue":"astro-ph.HE","work_id":"e5f1d204-e0a0-41df-897d-deb69374bcd1","year":2018},"citing_paper":{"arxiv_id":"2607.06664","last_updated":"2026-07-07T18:00:01Z","snapshot_observed_at":"2026-08-07T09:00:48.980402Z","submitted_at":"2026-07-07T18:00:01Z","title":"Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors","version":1},"reference_index":246,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1811.05515","citing_paper":"/paper/2607.06664"},"observation_digest":"sha256:1b0f285ea6dbc5265df6e0652b82b2e35090d476a642f26641080234ca9bd602","observation_id":"1a0becce-f035-497c-8bab-35cbb8d7305f","resolution":{"observed_at":"2026-07-10T23:57:49.622481Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"1811.05515","last_updated":"2018-11-13T20:00:36Z","snapshot_observed_at":"2026-07-06T07:14:31.358596Z","submitted_at":"2018-11-13T20:00:36Z","title":"On the importance of progenitor asymmetry to shock revival in core-collapse supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.05515","snapshot_observed_at":"2026-08-06T13:05:34.712486Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04954","last_updated":"2026-08-05T15:24:33Z","snapshot_observed_at":"2026-08-08T23:13:39.548028Z","submitted_at":"2026-08-05T15:24:33Z","title":"3D simulations of a complete convective silicon shell burning phase","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-06T13:05:34.712486Z"},"links":{"cited_paper":"/paper/1811.05515","citing_paper":"/paper/2608.04954"},"observation_digest":"sha256:4a363ecef5e71d3e09a0da52fbe12a0d9e6bfc601a2d4febc3b31b90de656bda","observation_id":"88a0fabc-e483-4962-8e0a-d5531e47b501","resolution":{"observed_at":"2026-08-06T13:05:34.712486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1811.05515/citation-record","integrity":"/paper/1811.05515/integrity","json":"/paper/1811.05515/citation-record.json","paper":"/paper/1811.05515"},"outbound":[],"paper":{"arxiv_id":"1811.05515","last_updated":"2018-11-13T20:00:36Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T07:14:31.358596Z","submitted_at":"2018-11-13T20:00:36Z","title":"On the importance of progenitor asymmetry to shock revival in core-collapse supernovae"},"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 4 inbound Pith citation observations for arXiv:1811.05515."}