{"as_of":"2026-08-08T17:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:57e2db9b64aa43bc79ef493df19a263ab7da68af090653c8fd41b23d309c1c3a","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T11:32:34.343963Z","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":"2026-07-04T16:19:57.226048Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1802.09710","last_updated":"2018-02-27T04:02:22Z","snapshot_observed_at":"2026-07-06T06:25:33.709663Z","submitted_at":"2018-02-27T04:02:22Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09710","snapshot_observed_at":"2026-08-08T11:32:34.343963Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07902","last_updated":"2025-02-11T19:17:15Z","snapshot_observed_at":"2026-08-08T11:25:45.621408Z","submitted_at":"2025-02-11T19:17:15Z","title":"Building Neutron Stars with the MUSES Calculation Engine","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T11:32:34.343963Z"},"links":{"cited_paper":"/paper/1802.09710","citing_paper":"/paper/2502.07902"},"observation_digest":"sha256:ef26edc5877a6b6abc56d99681f0ed847f924a889a789ad06653abda3fa91433","observation_id":"47a2a629-57ff-41ea-810e-97db2b86c69b","resolution":{"observed_at":"2026-08-08T11:32:34.343963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09710","last_updated":"2018-02-27T04:02:22Z","snapshot_observed_at":"2026-07-06T06:25:33.709663Z","submitted_at":"2018-02-27T04:02:22Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09710","snapshot_observed_at":"2026-08-07T15:31:32.525042Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.14921","last_updated":"2025-05-20T21:15:29Z","snapshot_observed_at":"2026-08-08T07:38:50.103324Z","submitted_at":"2025-05-20T21:15:29Z","title":"An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T15:31:32.525042Z"},"links":{"cited_paper":"/paper/1802.09710","citing_paper":"/paper/2505.14921"},"observation_digest":"sha256:7f7cd25bc0935512420d5d25e2007aea175b019f8756994b3384f48a15ea272a","observation_id":"667db487-b389-4a7f-996f-f153c46c29b1","resolution":{"observed_at":"2026-08-07T15:31:32.525042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09710","last_updated":"2018-02-27T04:02:22Z","snapshot_observed_at":"2026-07-06T06:25:33.709663Z","submitted_at":"2018-02-27T04:02:22Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09710","snapshot_observed_at":"2026-08-03T20:20:20.289217Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.20378","last_updated":"2026-06-28T03:18:05Z","snapshot_observed_at":"2026-08-06T06:55:09.797555Z","submitted_at":"2025-11-25T14:59:28Z","title":"Toward a Unified Understanding of the Dense Matter Equation of State","version":2},"reference_index":296,"source":"pdf_text","source_observed_at":"2026-08-03T20:20:20.289217Z"},"links":{"cited_paper":"/paper/1802.09710","citing_paper":"/paper/2511.20378"},"observation_digest":"sha256:4c70ebfb3afd625990edf0ae6d3ad013857cf984a9fbe4ffc7b4e5fe5bbde168","observation_id":"135931da-351f-441e-b205-83aa2fc38f1b","resolution":{"observed_at":"2026-08-03T20:20:20.289217Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09710","last_updated":"2018-02-27T04:02:22Z","snapshot_observed_at":"2026-07-06T06:25:33.709663Z","submitted_at":"2018-02-27T04:02:22Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","version":1},"cited_work":{"arxiv_id":"1802.09710","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.09710","snapshot_observed_at":"2026-07-04T16:19:57.226048Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","venue":"nucl-th","work_id":"43165dbc-ec7a-44eb-a8a5-809f5412c979","year":2018},"citing_paper":{"arxiv_id":"2606.07742","last_updated":"2026-06-05T18:00:04Z","snapshot_observed_at":"2026-07-06T23:47:19.773490Z","submitted_at":"2026-06-05T18:00:04Z","title":"Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-06-27T21:37:55.919953Z"},"links":{"cited_paper":"/paper/1802.09710","citing_paper":"/paper/2606.07742"},"observation_digest":"sha256:758001e0ce0d7c16df34f43c0ee31dc328001ee1694cc67fa3249658c22974b2","observation_id":"1181ee4f-7737-4dc6-9827-802d646b5901","resolution":{"observed_at":"2026-07-02T19:07:18.393503Z","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":"1802.09710","last_updated":"2018-02-27T04:02:22Z","snapshot_observed_at":"2026-07-06T06:25:33.709663Z","submitted_at":"2018-02-27T04:02:22Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","version":1},"cited_work":{"arxiv_id":"1802.09710","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.09710","snapshot_observed_at":"2026-07-04T16:19:57.226048Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory","venue":"nucl-th","work_id":"43165dbc-ec7a-44eb-a8a5-809f5412c979","year":2018},"citing_paper":{"arxiv_id":"2606.26326","last_updated":"2026-06-24T19:12:40Z","snapshot_observed_at":"2026-08-03T00:30:24.951043Z","submitted_at":"2026-06-24T19:12:40Z","title":"Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine","version":1},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-06-26T00:47:21.247516Z"},"links":{"cited_paper":"/paper/1802.09710","citing_paper":"/paper/2606.26326"},"observation_digest":"sha256:5becb2e4b501a3738450edfcce09d030f879ed3e902c36811c08cd5d336f3361","observation_id":"dc01320c-42b6-4806-a3a6-787c943a05dc","resolution":{"observed_at":"2026-07-04T16:19:57.228968Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/1802.09710/citation-record","integrity":"/paper/1802.09710/integrity","json":"/paper/1802.09710/citation-record.json","paper":"/paper/1802.09710"},"outbound":[],"paper":{"arxiv_id":"1802.09710","last_updated":"2018-02-27T04:02:22Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T06:25:33.709663Z","submitted_at":"2018-02-27T04:02:22Z","title":"Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and 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":"2026-08-08T06:32:00.761636+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 5 inbound Pith citation observations for arXiv:1802.09710."}