{"as_of":"2026-08-15T03:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b94a99cd4895c802c866dc8eb9350bfa065c170c63d4dae76f2c8f6e04739811","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T21:11:05.907279Z","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":"2026-06-30T03:04:14.850159Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-08-11T21:11:05.907279Z","title":"Malik, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.04946","last_updated":"2024-12-06T11:06:01Z","snapshot_observed_at":"2026-08-14T05:46:02.265506Z","submitted_at":"2024-12-06T11:06:01Z","title":"Impact of the Scalar Isovector $\\delta$-meson on the description of nuclear matter and neutron star properties","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T21:11:05.907279Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2412.04946"},"observation_digest":"sha256:f250dea3b5c0d9b8daff9c84cc826bb68a012e3f95e345887d67e562ee3db98d","observation_id":"b9431d03-d995-4992-837b-b1a18bbc81e9","resolution":{"observed_at":"2026-08-11T21:11:05.907279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-08-11T10:36:09.970400Z","title":"Malik, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.16513","last_updated":"2025-04-28T02:09:34Z","snapshot_observed_at":"2026-08-14T09:58:44.401775Z","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":35,"source":"pdf_text","source_observed_at":"2026-08-11T10:36:09.970400Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2412.16513"},"observation_digest":"sha256:3c7aa38fa5cecb22c8fc06118cc4e17d712548b6d8737f79346d919c81c797f0","observation_id":"1057b993-6541-4da4-85be-f3b84c2e8b1e","resolution":{"observed_at":"2026-08-11T10:36:09.970400Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-08-08T23:14:27.536088Z","title":"Malik, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04211","last_updated":"2025-02-06T16:51:15Z","snapshot_observed_at":"2026-08-14T04:34:31.267743Z","submitted_at":"2025-02-06T16:51:15Z","title":"Exploring the limits of nucleonic metamodelling using different relativistic density functionals","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-08T23:14:27.536088Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2502.04211"},"observation_digest":"sha256:042f51c9a830d7feb17769181a9ea6625c46359012b38a80d02fe56620b768b6","observation_id":"610774bf-d680-43ce-bebc-33ee2e85a10f","resolution":{"observed_at":"2026-08-08T23:14:27.536088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-08-07T14:28:09.474408Z","title":"Malik, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.18888","last_updated":"2025-05-24T22:16:54Z","snapshot_observed_at":"2026-08-14T04:25:22.251818Z","submitted_at":"2025-05-24T22:16:54Z","title":"Constraints on maximum neutron star mass from proto-neutron star evolution","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T14:28:09.474408Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2505.18888"},"observation_digest":"sha256:d6ccea14877ff609a093ab0feba3f8b200806872bc647b816b04e188556532d0","observation_id":"6bb3abe3-441b-45df-94e1-d9819824b6f8","resolution":{"observed_at":"2026-08-07T14:28:09.474408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-08-06T16:35:48.078167Z","title":"Malik, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.13227","last_updated":"2025-08-21T13:29:55Z","snapshot_observed_at":"2026-08-10T22:01:48.115042Z","submitted_at":"2025-07-17T15:39:44Z","title":"Effect of Dark matter and $\\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars","version":2},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-06T16:35:48.078167Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2507.13227"},"observation_digest":"sha256:9aeaed40e7fdd6389fe229998ebcdf46ce4ea6a661232c96bece7a35fce9d9fd","observation_id":"09e04d0b-eb95-4f7b-bcb8-b50cd5023844","resolution":{"observed_at":"2026-08-06T16:35:48.078167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":"2301.08169","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-06-30T03:04:14.850159Z","title":"Malik, M","venue":null,"work_id":"d52a46ca-cde6-4017-ae60-121bb5230c94","year":2023},"citing_paper":{"arxiv_id":"2512.01503","last_updated":"2026-05-13T01:30:52Z","snapshot_observed_at":"2026-08-02T18:04:54.038553Z","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":55,"source":"pdf_text","source_observed_at":"2026-05-17T03:09:32.415798Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2512.01503"},"observation_digest":"sha256:512795968319f12ecb0d9f45f6481f3c081bd180d117f35e84612df8d365aa8f","observation_id":"f55d9db6-a2e8-4346-81ad-922adbb0108c","resolution":{"observed_at":"2026-05-17T03:11:29.758032Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":"2301.08169","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-06-30T03:04:14.850159Z","title":"Malik, M","venue":null,"work_id":"d52a46ca-cde6-4017-ae60-121bb5230c94","year":2023},"citing_paper":{"arxiv_id":"2606.29576","last_updated":"2026-06-28T19:42:10Z","snapshot_observed_at":"2026-08-05T14:46:57.158272Z","submitted_at":"2026-06-28T19:42:10Z","title":"Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-06-30T01:49:38.961950Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2606.29576"},"observation_digest":"sha256:d7c667b20191de8d261fdb4a0bc5257ffa0de8eaff6c7a2d6ac3149022f4b59d","observation_id":"a830281d-629f-48ff-877b-652cbfe50b37","resolution":{"observed_at":"2026-06-30T03:04:14.852954Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08169","snapshot_observed_at":"2026-08-02T05:44:17.889600Z","title":"Malik, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.13268","last_updated":"2026-07-14T21:03:17Z","snapshot_observed_at":"2026-08-12T13:08:46.506949Z","submitted_at":"2026-07-14T21:03:17Z","title":"Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-02T05:44:17.889600Z"},"links":{"cited_paper":"/paper/2301.08169","citing_paper":"/paper/2607.13268"},"observation_digest":"sha256:477f0350750681aa028045da824c0645d63fef501eacb033b2cd251623bcbb25","observation_id":"d937d67b-1807-4b1c-a07f-f370914fed3f","resolution":{"observed_at":"2026-08-02T05:44:17.889600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2301.08169/citation-record","integrity":"/paper/2301.08169/integrity","json":"/paper/2301.08169/citation-record.json","paper":"/paper/2301.08169"},"outbound":[],"paper":{"arxiv_id":"2301.08169","last_updated":"2023-06-08T09:28:54Z","latest_version":4,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-13T13:01:06.221029Z","submitted_at":"2023-01-19T16:59:37Z","title":"Spanning the full range of neutron star properties within a microscopic description"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2301.08169."}