{"as_of":"2026-08-22T00:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fc1c823dd8ae9a4b0290297a7d3f13fa8eb4ae68a35122aea9e3749d0182ed1a","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:38:47.205337Z","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":"2026-07-04T07:49:39.108515Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-08-11T10:36:09.981514Z","title":"Huang, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.16513","last_updated":"2025-04-28T02:09:34Z","snapshot_observed_at":"2026-08-19T08:35:33.657429Z","submitted_at":"2024-12-21T07:25:36Z","title":"Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T10:36:09.981514Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2412.16513"},"observation_digest":"sha256:cf87aaa922c90ebd60bd9255a39aed517eb4c5795e3421540405794b0746d9c5","observation_id":"ea4807fc-e813-4898-940f-496bf384b165","resolution":{"observed_at":"2026-08-11T10:36:09.981514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-08-08T23:14:27.543275Z","title":"Huang, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04211","last_updated":"2025-02-06T16:51:15Z","snapshot_observed_at":"2026-08-18T16:49:11.921491Z","submitted_at":"2025-02-06T16:51:15Z","title":"Exploring the limits of nucleonic metamodelling using different relativistic density functionals","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-08T23:14:27.543275Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2502.04211"},"observation_digest":"sha256:f1ca249e16a7f17d81a3ab9b86d0f3a7a35a6de84b832f16a09e20b1106d040c","observation_id":"fd911b1f-dd65-42b5-905d-1fae1698627e","resolution":{"observed_at":"2026-08-08T23:14:27.543275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-08-16T04:38:47.205337Z","title":"Huang, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.00911","last_updated":"2025-07-03T08:25:05Z","snapshot_observed_at":"2026-08-18T11:27:06.962442Z","submitted_at":"2025-05-01T23:15:31Z","title":"Bayesian inferences on covariant density functionals from multimessenger astrophysical data: The impacts of likelihood functions of low density matter constraints","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T04:38:47.205337Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2505.00911"},"observation_digest":"sha256:96cd85ee35189225e8aca271cbc7439b43ed07ec58c0a37a0d82d9580cdfca38","observation_id":"a42dc1fd-27f2-4a0f-8409-c018a19af541","resolution":{"observed_at":"2026-08-16T04:38:47.205337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":"2303.17518","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-07-04T07:49:39.108515Z","title":"Huang, G","venue":null,"work_id":"3336aa7b-dc50-470e-8c15-470fc5eb6396","year":2024},"citing_paper":{"arxiv_id":"2505.16929","last_updated":"2026-04-14T09:24:59Z","snapshot_observed_at":"2026-08-14T18:04:59.349679Z","submitted_at":"2025-05-22T17:22:16Z","title":"Properties of the neutron star crust informed by nuclear structure data","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-22T01:36:22.187463Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2505.16929"},"observation_digest":"sha256:5859d518e953ef4ed8d64eb0e6377e82753733ee7f964f897aae987581e38b5a","observation_id":"38470de1-c584-48ba-9f4f-6f6c20302c04","resolution":{"observed_at":"2026-05-22T01:40:54.258808Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-08-07T05:14:55.023019Z","title":"MNRAS529(4), 4650– 4665 (2024) https://doi.org/10.1093/mnras/ stae844 arXiv:2303.17518 [astro-ph.HE]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.08658","last_updated":"2025-06-10T10:19:43Z","snapshot_observed_at":"2026-08-20T04:58:07.595521Z","submitted_at":"2025-06-10T10:19:43Z","title":"Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T05:14:55.023019Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2506.08658"},"observation_digest":"sha256:2e8e5a7ef2ae39a057c9b60bdfadc2ae181cf7cf1909cac4908974b16f1e4ab1","observation_id":"e9616895-19b6-4b9c-ab2f-cf2550700eec","resolution":{"observed_at":"2026-08-07T05:14:55.023019Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-08-03T23:37:06.062394Z","title":"Huang, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.05651","last_updated":"2026-07-23T15:06:21Z","snapshot_observed_at":"2026-08-16T07:49:43.426429Z","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":92,"source":"pdf_text","source_observed_at":"2026-08-03T23:37:06.062394Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2511.05651"},"observation_digest":"sha256:e13d124c7b730fbfc4a138f2510b690bbe6c8294b15bf1e2bd7ea364610ce7ae","observation_id":"0fa8f4a4-4955-4ab8-a302-eb7cbf69052a","resolution":{"observed_at":"2026-08-03T23:37:06.062394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":"2303.17518","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-07-04T07:49:39.108515Z","title":"Huang, G","venue":null,"work_id":"3336aa7b-dc50-470e-8c15-470fc5eb6396","year":2024},"citing_paper":{"arxiv_id":"2512.01503","last_updated":"2026-05-13T01:30:52Z","snapshot_observed_at":"2026-08-19T21:25:00.399731Z","submitted_at":"2025-12-01T10:27:50Z","title":"Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-17T03:09:32.415798Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2512.01503"},"observation_digest":"sha256:8c996f43fbd514cb2652128a05125c90b3184c674c34087e8bf85ab2e100ad90","observation_id":"a39ab2e4-5014-412f-953f-cc242f0c1540","resolution":{"observed_at":"2026-05-17T03:11:29.704668Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-08-03T04:14:54.754768Z","title":"Huang, G","venue":null,"work_id":null,"year":2024},"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":132,"source":"pdf_text","source_observed_at":"2026-08-03T04:14:54.754768Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2602.06111"},"observation_digest":"sha256:4f574015afb289b168de6455c36424255229414db228da72c72b879279ebc76a","observation_id":"d301eb31-5555-46a3-8d14-0b34e0db31c3","resolution":{"observed_at":"2026-08-03T04:14:54.754768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":"2303.17518","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-07-04T07:49:39.108515Z","title":"Huang, G","venue":null,"work_id":"3336aa7b-dc50-470e-8c15-470fc5eb6396","year":2024},"citing_paper":{"arxiv_id":"2606.21435","last_updated":"2026-06-19T13:51:27Z","snapshot_observed_at":"2026-08-06T05:56:14.769876Z","submitted_at":"2026-06-19T13:51:27Z","title":"Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-06-26T12:50:53.032717Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2606.21435"},"observation_digest":"sha256:dee18c3a0093b02903f057938575764073280ee337eef3f9e6aabe1c593ba047","observation_id":"059ee590-373b-4e7c-a21a-c2d1461c19f3","resolution":{"observed_at":"2026-07-04T07:49:39.109755Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.17518","snapshot_observed_at":"2026-07-13T05:17:12.889672Z","title":"Huang, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.09119","last_updated":"2026-07-10T06:16:49Z","snapshot_observed_at":"2026-08-17T03:26:04.600930Z","submitted_at":"2026-07-10T06:16:49Z","title":"Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-13T05:17:12.889672Z"},"links":{"cited_paper":"/paper/2303.17518","citing_paper":"/paper/2607.09119"},"observation_digest":"sha256:601e7f6deadc66a476be953feb428e36fbceeaa15a535237080841022aed5b7a","observation_id":"a93fc9b8-b8da-4bca-ae2e-0d66f930cf00","resolution":{"observed_at":"2026-07-13T05:17:12.889672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2303.17518/citation-record","integrity":"/paper/2303.17518/integrity","json":"/paper/2303.17518/citation-record.json","paper":"/paper/2303.17518"},"outbound":[],"paper":{"arxiv_id":"2303.17518","last_updated":"2024-03-22T15:31:57Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-17T23:54:55.960879Z","submitted_at":"2023-03-30T16:35:36Z","title":"Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models"},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2303.17518."}