{"as_of":"2026-08-11T22:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7c848f50138b543f8a7e8ed4f3cbc4ded5cda86f30213480be684c5276cf4b5d","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T19:21:20.401980Z","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":"2026-07-02T00:36:25.272217Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-08-10T19:21:20.401980Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10272","last_updated":"2025-05-14T10:53:06Z","snapshot_observed_at":"2026-08-10T23:28:55.106348Z","submitted_at":"2025-01-17T15:59:21Z","title":"Data-driven approach for extracting tidal information from neutron star binary mergers observed with the Einstein Telescope","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T19:21:20.401980Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2501.10272"},"observation_digest":"sha256:dd8d5f064781f25b6ab7bb759c4d8abdc4fecdd4c886ef26b746b81ebefa291f","observation_id":"4e4fa45a-8215-4545-8b0a-6d79fded1eab","resolution":{"observed_at":"2026-08-10T19:21:20.401980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-08-07T14:28:46.274269Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.18921","last_updated":"2026-06-08T18:10:09Z","snapshot_observed_at":"2026-08-08T20:36:44.978874Z","submitted_at":"2025-05-25T01:04:40Z","title":"Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T14:28:46.274269Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2505.18921"},"observation_digest":"sha256:d99463819285f52ca27dac8b744b322be51f793604c6ba19610556e4dfada89e","observation_id":"e3b1d1a5-cc90-4052-8c12-ca0501831328","resolution":{"observed_at":"2026-08-07T14:28:46.274269Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-08-05T19:46:32.508457Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.11872","last_updated":"2026-05-23T02:23:15Z","snapshot_observed_at":"2026-08-11T01:55:31.847999Z","submitted_at":"2025-08-16T02:12:39Z","title":"Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-05T19:46:32.508457Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2508.11872"},"observation_digest":"sha256:8ce8c79ee52f333d6a4aeb44e101a63f53deaa3f40bb110572ce85d8f42a34a8","observation_id":"823e8ca0-5e21-413d-b42f-d6de827fbb6a","resolution":{"observed_at":"2026-08-05T19:46:32.508457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":"2205.10283","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-07-02T00:36:25.272217Z","title":null,"venue":null,"work_id":"d10ee9d1-cc69-40aa-a178-088a1cb7f31a","year":2022},"citing_paper":{"arxiv_id":"2510.09104","last_updated":"2026-05-21T12:53:58Z","snapshot_observed_at":"2026-08-02T16:10:55.190085Z","submitted_at":"2025-10-10T07:58:38Z","title":"Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-22T12:52:58.423553Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2510.09104"},"observation_digest":"sha256:cd5e83b7ee8466b7cb5e3f53bd61613be0a4cd3a4ab0f60389b76a069de35d2c","observation_id":"55a7c69f-dc25-46be-afe5-7acd99f7d127","resolution":{"observed_at":"2026-05-22T12:54:52.581136Z","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":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":"2205.10283","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-07-02T00:36:25.272217Z","title":null,"venue":null,"work_id":"d10ee9d1-cc69-40aa-a178-088a1cb7f31a","year":2022},"citing_paper":{"arxiv_id":"2606.02690","last_updated":"2026-06-01T18:00:00Z","snapshot_observed_at":"2026-08-02T08:48:27.840816Z","submitted_at":"2026-06-01T18:00:00Z","title":"Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-28T13:18:38.984279Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2606.02690"},"observation_digest":"sha256:1c5bb03c8e0ee876211242c7ba7028a4e9b5ad341f52cdfab245eb5ee814a21f","observation_id":"71c0a15a-896b-4bc2-b28d-5f81ff1f56a1","resolution":{"observed_at":"2026-07-02T00:36:25.274273Z","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":"2205.10283","last_updated":"2022-11-21T21:18:21Z","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10283","snapshot_observed_at":"2026-07-31T07:22:45.404319Z","title":"and Brodie, Liam and Haber, Alexander and Tews, Ingo","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28438","last_updated":"2026-07-30T16:13:33Z","snapshot_observed_at":"2026-08-03T00:12:06.425303Z","submitted_at":"2026-07-30T16:13:33Z","title":"Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-31T07:22:45.404319Z"},"links":{"cited_paper":"/paper/2205.10283","citing_paper":"/paper/2607.28438"},"observation_digest":"sha256:c7853d3ab6db93d70859457e18da89922b2c64d0926e0e242034e208ae4a6baf","observation_id":"a3f73532-b1ba-49e9-a10b-3e3c5f57fc4e","resolution":{"observed_at":"2026-07-31T07:22:45.404319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2205.10283/citation-record","integrity":"/paper/2205.10283/integrity","json":"/paper/2205.10283/citation-record.json","paper":"/paper/2205.10283"},"outbound":[],"paper":{"arxiv_id":"2205.10283","last_updated":"2022-11-21T21:18:21Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T13:12:09.513050Z","submitted_at":"2022-05-20T16:28:37Z","title":"Relativistic mean-field theories for neutron-star physics based on chiral effective field theory"},"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 6 inbound Pith citation observations for arXiv:2205.10283."}