{"as_of":"2026-08-08T05:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ddb3d2d731a5c34935ca61022de8b92ece2ad57bbeb373b1c5dfd464f12c5cba","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":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T10:19:42.450063Z","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":"2026-07-03T08:37:46.382668Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":"1903.04981","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-03T08:37:46.382668Z","title":"Unified equations of state for cold non-accreting neutron stars with Brus- sels–Montreal functionals – I. Role of symmetry energy","venue":null,"work_id":"8fd8b4d5-3949-4514-ba06-6a4c2cc31757","year":2018},"citing_paper":{"arxiv_id":"2505.16929","last_updated":"2026-04-14T09:24:59Z","snapshot_observed_at":"2026-07-06T21:28:43.610849Z","submitted_at":"2025-05-22T17:22:16Z","title":"Properties of the neutron star crust informed by nuclear structure data","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-22T01:36:22.187463Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2505.16929"},"observation_digest":"sha256:991eab0defb748f5cafbb174d6da6d0dcda1839bd39cd6e725f6e9b01ab12252","observation_id":"db40a06f-e796-457c-8f8d-85002ab82fae","resolution":{"observed_at":"2026-05-22T01:40:54.076401Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-08-07T10:19:42.450063Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.05603","last_updated":"2025-08-13T15:01:01Z","snapshot_observed_at":"2026-08-08T03:45:39.693103Z","submitted_at":"2025-06-05T21:33:31Z","title":"Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-07T10:19:42.450063Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2506.05603"},"observation_digest":"sha256:b940541eb99127913169d09624928b1051b2338de8a55ff3e84b3caced3055d9","observation_id":"d545d3f4-e192-446a-8006-64d394fc7732","resolution":{"observed_at":"2026-08-07T10:19:42.450063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-08-07T05:14:55.116509Z","title":"Role of symmetry energy","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.08658","last_updated":"2025-06-10T10:19:43Z","snapshot_observed_at":"2026-08-07T10:37:26.398774Z","submitted_at":"2025-06-10T10:19:43Z","title":"Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-07T05:14:55.116509Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2506.08658"},"observation_digest":"sha256:a6e3b5f2395c56db7ee9f77f3dc93b2b851d08dde2a898b21a0d2a9297255630","observation_id":"eb21e006-b815-4b92-b966-071a19015c5d","resolution":{"observed_at":"2026-08-07T05:14:55.116509Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-08-03T23:37:04.896699Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.05651","last_updated":"2026-07-23T15:06:21Z","snapshot_observed_at":"2026-08-07T14:25:25.561667Z","submitted_at":"2025-11-07T19:00:01Z","title":"Neutron stars can shine a light on elusive lepton-flavor-violating dark matter","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-03T23:37:04.896699Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2511.05651"},"observation_digest":"sha256:f5456d2f399fda75952d566410061236b1b74f8b8c4675481ee8d77ceea0a86c","observation_id":"a3af2e44-6dda-4fae-a34d-5a53303058a5","resolution":{"observed_at":"2026-08-03T23:37:04.896699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":"1903.04981","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-03T08:37:46.382668Z","title":"Unified equations of state for cold non-accreting neutron stars with Brus- sels–Montreal functionals – I. Role of symmetry energy","venue":null,"work_id":"8fd8b4d5-3949-4514-ba06-6a4c2cc31757","year":2018},"citing_paper":{"arxiv_id":"2602.02272","last_updated":"2026-05-13T22:56:08Z","snapshot_observed_at":"2026-08-02T12:03:08.214304Z","submitted_at":"2026-02-02T16:13:48Z","title":"Radial Oscillations of Neutron Stars with Vector-Induced Scalar Hair","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-16T08:15:27.979441Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2602.02272"},"observation_digest":"sha256:62f13e7efde32c960f0ca65850c6d373f11f9eedb1d8853ce69ae53f2b5eaf05","observation_id":"b0c1a18f-756d-4b11-93a0-6e18450a6476","resolution":{"observed_at":"2026-05-16T08:17:36.410527Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-08-03T04:14:51.986484Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.06111","last_updated":"2026-06-24T08:31:42Z","snapshot_observed_at":"2026-08-06T14:38:27.293620Z","submitted_at":"2026-02-05T19:00:00Z","title":"Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams","version":3},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-08-03T04:14:51.986484Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2602.06111"},"observation_digest":"sha256:eccfb07f138889625a59862487ff6e65ac852c0538c3fa87ddba3565e60bb13c","observation_id":"0fa2a440-eeba-4a90-8106-107b3051514f","resolution":{"observed_at":"2026-08-03T04:14:51.986484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":"1903.04981","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-03T08:37:46.382668Z","title":"Unified equations of state for cold non-accreting neutron stars with Brus- sels–Montreal functionals – I. Role of symmetry energy","venue":null,"work_id":"8fd8b4d5-3949-4514-ba06-6a4c2cc31757","year":2018},"citing_paper":{"arxiv_id":"2605.19731","last_updated":"2026-07-22T00:32:36Z","snapshot_observed_at":"2026-08-02T13:44:04.267230Z","submitted_at":"2026-05-19T12:05:32Z","title":"Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-20T04:20:10.592465Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2605.19731"},"observation_digest":"sha256:e61c1454cbe90a4e5eba21b0b71b6ca7f3af077704178a240ec11cdf423921b6","observation_id":"71cb8c3b-9c90-4a79-a5e1-f1f9895fe3d7","resolution":{"observed_at":"2026-05-20T04:23:03.809575Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-08-02T13:44:08.499830Z","title":"Unified equations of state for cold non-accreting neutron stars with Brus- sels–Montreal functionals – I. Role of symmetry energy,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.19731","last_updated":"2026-07-22T00:32:36Z","snapshot_observed_at":"2026-08-02T13:44:04.267230Z","submitted_at":"2026-05-19T12:05:32Z","title":"Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-02T13:44:08.499830Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2605.19731"},"observation_digest":"sha256:27836a0898b745b1764a3c2d5d6a059192074198bc6b1617551ee55809e2bdd9","observation_id":"b90b963f-a317-400c-a482-9c135cf5787f","resolution":{"observed_at":"2026-08-02T13:44:08.499830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":"1903.04981","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-03T08:37:46.382668Z","title":"Unified equations of state for cold non-accreting neutron stars with Brus- sels–Montreal functionals – I. Role of symmetry energy","venue":null,"work_id":"8fd8b4d5-3949-4514-ba06-6a4c2cc31757","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":70,"source":"pdf_text","source_observed_at":"2026-06-27T21:37:55.919953Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2606.07742"},"observation_digest":"sha256:b0c5a7974a27cbc02875e13b476125a28dfdbfb1a2caa89eed6e0414f2734a30","observation_id":"34622b45-5fe8-4731-8282-70b21dcbdf7f","resolution":{"observed_at":"2026-07-02T19:07:18.420008Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":"1903.04981","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-03T08:37:46.382668Z","title":"Unified equations of state for cold non-accreting neutron stars with Brus- sels–Montreal functionals – I. Role of symmetry energy","venue":null,"work_id":"8fd8b4d5-3949-4514-ba06-6a4c2cc31757","year":2018},"citing_paper":{"arxiv_id":"2607.01937","last_updated":"2026-07-02T09:32:10Z","snapshot_observed_at":"2026-08-03T22:46:45.146654Z","submitted_at":"2026-07-02T09:32:10Z","title":"Neutron stars with primary scalar hair","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-03T08:33:22.475130Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2607.01937"},"observation_digest":"sha256:b0510a34cae175024207e71bebd001be5c55ce2845e8b1464688cc269e83d06b","observation_id":"7e9ff7cc-c25c-47f5-8bce-777e03e5c630","resolution":{"observed_at":"2026-07-03T08:37:46.384067Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-12T09:19:35.429829Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.02597","last_updated":"2026-07-01T09:50:53Z","snapshot_observed_at":"2026-08-07T14:01:28.264782Z","submitted_at":"2026-07-01T09:50:53Z","title":"Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO","version":1},"reference_index":261,"source":"arxiv_source","source_observed_at":"2026-07-12T09:19:35.429829Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2607.02597"},"observation_digest":"sha256:181072a6a69ef2985bc1d4f213126bee32b1cd6762d8573138a989eb481de7d6","observation_id":"5686114c-627c-431e-894c-c1e5fa34a0c2","resolution":{"observed_at":"2026-07-12T09:19:35.429829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04981","snapshot_observed_at":"2026-07-13T02:48:35.465628Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.09468","last_updated":"2026-07-10T14:42:46Z","snapshot_observed_at":"2026-07-15T23:18:16.504690Z","submitted_at":"2026-07-10T14:42:46Z","title":"Neutron contribution to the force on a proton vortex in superconducting neutron-star matter","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-13T02:48:35.465628Z"},"links":{"cited_paper":"/paper/1903.04981","citing_paper":"/paper/2607.09468"},"observation_digest":"sha256:0532446710bc7485c4b2a224672b3b1b7a7b0aac62ab7464d7c1f2f6a861157f","observation_id":"6f8bfd13-6b26-4a32-a319-694e0d64949e","resolution":{"observed_at":"2026-07-13T02:48:35.465628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1903.04981/citation-record","integrity":"/paper/1903.04981/integrity","json":"/paper/1903.04981/citation-record.json","paper":"/paper/1903.04981"},"outbound":[],"paper":{"arxiv_id":"1903.04981","last_updated":"2019-03-12T15:12:44Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-04T10:56:10.618683Z","submitted_at":"2019-03-12T15:12:44Z","title":"Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:1903.04981."}