{"as_of":"2026-08-18T22:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fcf54d47d5d1746333b3b6368bef3c7a5f4b44a3b28f66f06ef7ff8318e8ef31","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":"2026-08-18T06:34:40.430872+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":"2026-08-08T10:10:48.437906Z","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":"2026-05-11T10:11:15.575445Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.18739","last_updated":"2025-02-14T13:46:35Z","snapshot_observed_at":"2026-08-16T23:35:36.194000Z","submitted_at":"2024-07-26T13:51:05Z","title":"Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars","version":2},"cited_work":{"arxiv_id":"2407.18739","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.18739","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"f1ecaa96-4909-4743-8421-7c1fbce650ad","year":2025},"citing_paper":{"arxiv_id":"2604.11431","last_updated":"2026-04-13T13:18:06Z","snapshot_observed_at":"2026-08-14T20:30:10.195503Z","submitted_at":"2026-04-13T13:18:06Z","title":"Impact of Effective Nucleon Mass and Multineutron States on the Equation of State for Core-Collapse Supernovae","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-10T15:34:47.069340Z"},"links":{"cited_paper":"/paper/2407.18739","citing_paper":"/paper/2604.11431"},"observation_digest":"sha256:6b0a7f17e09774ff9393ba2a26759bc174ca59c7b4cfb444aeaac5be3e177764","observation_id":"c4175281-6737-4521-8c32-1d403140bfc8","resolution":{"observed_at":"2026-05-11T10:11:15.657376Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18739","last_updated":"2025-02-14T13:46:35Z","snapshot_observed_at":"2026-08-16T23:35:36.194000Z","submitted_at":"2024-07-26T13:51:05Z","title":"Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18739","snapshot_observed_at":"2026-08-01T00:06:07.708214Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.23253","last_updated":"2026-07-25T15:28:48Z","snapshot_observed_at":"2026-08-14T19:21:49.964038Z","submitted_at":"2026-07-25T15:28:48Z","title":"On the Nucleon Effective Mass in Neutron Stars Cooling","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-01T00:06:07.708214Z"},"links":{"cited_paper":"/paper/2407.18739","citing_paper":"/paper/2607.23253"},"observation_digest":"sha256:bdfdf5c292854bdd1eed5afc007f4c59c21604706b0ea4df8776fd037869f1da","observation_id":"e05915fa-0c24-493d-9dcc-3c18abe2b561","resolution":{"observed_at":"2026-08-01T00:06:07.708214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18739","last_updated":"2025-02-14T13:46:35Z","snapshot_observed_at":"2026-08-16T23:35:36.194000Z","submitted_at":"2024-07-26T13:51:05Z","title":"Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18739","snapshot_observed_at":"2026-08-08T10:10:48.437906Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05582","last_updated":"2026-08-06T04:10:03Z","snapshot_observed_at":"2026-08-12T12:06:26.690294Z","submitted_at":"2026-08-06T04:10:03Z","title":"Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-08T10:10:48.437906Z"},"links":{"cited_paper":"/paper/2407.18739","citing_paper":"/paper/2608.05582"},"observation_digest":"sha256:2446648f7f3071502906c79c6c5be742b2b6bf5e77148bc641a3513da544a685","observation_id":"191392c5-bab0-42f7-9eb7-ee8cbb5288f8","resolution":{"observed_at":"2026-08-08T10:10:48.437906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.18739/citation-record","integrity":"/paper/2407.18739/integrity","json":"/paper/2407.18739/citation-record.json","paper":"/paper/2407.18739"},"outbound":[],"paper":{"arxiv_id":"2407.18739","last_updated":"2025-02-14T13:46:35Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-16T23:35:36.194000Z","submitted_at":"2024-07-26T13:51:05Z","title":"Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.18739."}