{"as_of":"2026-08-15T21:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:22d549dff179cbb2233366d6fd484b21c6cdfbacefad4497a61c51a172a2d760","coverage":[{"denominator":122,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T17:19:05.905003Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.11379/citation-record","integrity":"/paper/2507.11379/integrity","json":"/paper/2507.11379/citation-record.json","paper":"/paper/2507.11379"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.568416Z","title":"Haensel, A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.568416Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:5b4c319c21e063cfb0245ab0a6afb438beb1358f376120edff7048cbfcc999f7","observation_id":"8e42fbb0-b579-42e3-96a5-283292cd8a28","resolution":{"observed_at":"2026-08-06T17:18:56.568416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.548366Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.548366Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:4bb0db2321146f8997feba352a4450f9465a879a190a25d555cdc1516342dfb0","observation_id":"0a09aa17-c013-41e5-9fdf-46851618d49e","resolution":{"observed_at":"2026-08-06T17:18:56.548366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.596296Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.596296Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:5c066c73da0dc2db1d7036ab3b9b4b759973b6264b948fc50fd1d113c99db2da","observation_id":"7eb62c08-e743-47be-970d-3a9533902e63","resolution":{"observed_at":"2026-08-06T17:18:56.596296Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.623442Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.623442Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:888a9764d960f3ede6d2504a3504b6483508ae562441fefec6bf8b10f5709641","observation_id":"8d0572ef-b3bd-4695-8655-bee8d31b3983","resolution":{"observed_at":"2026-08-06T17:18:56.623442Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.651675Z","title":"Cutter, T","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.651675Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1ece4d025e87baeea77c37cb3e0cb64f12aef7188e4377574240dab274734ac1","observation_id":"f1d21bf7-5302-431c-b5b4-7ea9451d67a2","resolution":{"observed_at":"2026-08-06T17:18:56.651675Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.747273Z","title":"Malik, N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.747273Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:463183d1265fd05c64b0887d63868f5f335164149465a2fcd024becaf2275d3b","observation_id":"43273cee-6f43-471a-945a-b17aa33055e4","resolution":{"observed_at":"2026-08-06T17:18:56.747273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.843496Z","title":"Faber, Classical Quantum Gravity 26, 114004 (2009)","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.843496Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:850aaed445f0fa85465f47a7ea3eed2ac32bf4c1e1b5864d038abc23825600f6","observation_id":"f23cb34d-0e59-4ad3-9b93-b5c24ab2ad54","resolution":{"observed_at":"2026-08-06T17:18:56.843496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:56.966553Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:56.966553Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:5765177d337df0411d172fa4c5c327cfe84b18d81ffa188cb2ca2eb4d7fe43fd","observation_id":"f75cb5c3-f877-4221-82cf-7dd7376c0cc2","resolution":{"observed_at":"2026-08-06T17:18:56.966553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.079871Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.079871Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:ca9ea20984bcb3f67ac598156be9d8870499e66e64096e0f190ce9d8d3dcc927","observation_id":"604b1e8b-bebc-4e7b-99e5-fd65296c25c7","resolution":{"observed_at":"2026-08-06T17:18:57.079871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.250485Z","title":"Piekarewicz and F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.250485Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:ffd7e644a4edfe3ea3ad695a9cbf60430b395f63b9319e6cdec8f4a79df4ad37","observation_id":"32193dc2-c43d-4418-8060-f1528e902c58","resolution":{"observed_at":"2026-08-06T17:18:57.250485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.374535Z","title":"Annala, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.374535Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1cf2f047e01dc4ace4570d9c5552274f8d5282cc088425f3fa58d16fae99bcfd","observation_id":"e6a5fcc5-e9e9-4df2-a246-8bfd50353730","resolution":{"observed_at":"2026-08-06T17:18:57.374535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.501148Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.501148Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:ec06b4cd0e5484ab17ac3659fbd4309787242817516f35ff0c3887c1ee7de85b","observation_id":"f96929ee-da3e-41a2-9fcb-8aa77d343782","resolution":{"observed_at":"2026-08-06T17:18:57.501148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.589635Z","title":"Binnington and E","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.589635Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:cbeee0fa00e6e0c64cc0523c0c310cee96f2021c626a90fa8db20d7a504e9d7b","observation_id":"f84d0eda-7761-4a84-8239-3d32fd1f2070","resolution":{"observed_at":"2026-08-06T17:18:57.589635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.640632Z","title":"Damour, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.640632Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1ffb38b4d6e3838752a2aacf04602be3d2ca06e7a0e5cdae5d30a24608650551","observation_id":"b90a8d90-a09c-4df6-9802-79ea1b46bdda","resolution":{"observed_at":"2026-08-06T17:18:57.640632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.721288Z","title":"Hinderer, B","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.721288Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:354398166a94b098ec2d9db8901bc449cf1f7e039df1486b139691414cfc6252","observation_id":"6d9a5125-3ce5-4583-9f96-5373c29d23dc","resolution":{"observed_at":"2026-08-06T17:18:57.721288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.810208Z","title":"Hinderer, Astrophys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.810208Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1cb2e5fe162423a1a9f646e671fce7071f5b65f940e62df99d10e4cc5afa539a","observation_id":"78b2fedd-25ff-4408-80f1-31cc73d578cd","resolution":{"observed_at":"2026-08-06T17:18:57.810208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.879923Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.879923Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:5c1a74833fa59a6bc83f7c8fb445a2db70a344e3533df067c936f7e8aed3ab89","observation_id":"32e27ef9-cf96-4336-bbdf-0104d356a84a","resolution":{"observed_at":"2026-08-06T17:18:57.879923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:57.963694Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:57.963694Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:802bc9593a5f0f4606cb4efc17b028f7ca8c70e1eb12da44f36b931dadc614e0","observation_id":"45a0aed3-e0f7-4cf1-ab36-5b824083f9a5","resolution":{"observed_at":"2026-08-06T17:18:57.963694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.040835Z","title":"Goldstein et al ., Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.040835Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:4af9d94e8db0f45fc45bcb3f16286a1f4fca3a60470a47d32fe8c7391dbc6c67","observation_id":"f1565d47-6498-4eed-a338-2de8197dfe34","resolution":{"observed_at":"2026-08-06T17:18:58.040835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.124245Z","title":"Savchenko et al ., Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.124245Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:501a2f3eef848b0245b13a8bf2abe82fd28ce2c5cc99f3352dfbfa3cbb502b0d","observation_id":"cf1d33af-e554-44a1-b512-d1df1eb95722","resolution":{"observed_at":"2026-08-06T17:18:58.124245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.213889Z","title":"Postnikov, M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.213889Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1d81547cf5c7c3b8b980e88fcd5d67d30638f9a30a9f908a2d3be262d9413804","observation_id":"ef640d8d-e23c-47b3-a6d3-5c4745427275","resolution":{"observed_at":"2026-08-06T17:18:58.213889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.289013Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.289013Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:d3cbaa9b35a2110764303260659aa8fb61d4ec19da254f5cd5f42a4da3e04d2c","observation_id":"2b65ee1e-2d31-45c7-81be-2dcdf6b96680","resolution":{"observed_at":"2026-08-06T17:18:58.289013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.390365Z","title":"Kumar, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.390365Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:159541161ae01062241291b6fdc55e29f30e5cea2a9686209067b8d7c6dbd6c6","observation_id":"a2716f8e-f5e4-4935-b8ac-dcfed460c5d2","resolution":{"observed_at":"2026-08-06T17:18:58.390365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.470731Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.470731Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:9f8e6567356743d7a44bde27f775a848ee3f4f344c94a991b465db84e162f38d","observation_id":"e2bce6aa-a552-4909-a10a-36e4974e8891","resolution":{"observed_at":"2026-08-06T17:18:58.470731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.535620Z","title":"Damour and A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.535620Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:42ab8ececa2c334ee43f916c94774e4a849c9abcd80310cd51f585e53145d182","observation_id":"2f9e9f4a-1b86-466a-b72d-767436ed4e3e","resolution":{"observed_at":"2026-08-06T17:18:58.535620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.628967Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.628967Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:921979d195f273c03a738443e927da0efdfcbb909bbe08c66d751a8f505176b1","observation_id":"c941d8bb-824f-45bc-b019-b7f0bab64c4c","resolution":{"observed_at":"2026-08-06T17:18:58.628967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.714919Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.714919Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:016d4f9d66679453060b0d1a428c6e8d4aceb83abab28d1e9128af9c579412bf","observation_id":"fc02491c-1e58-4846-a2bf-afdca07a45b4","resolution":{"observed_at":"2026-08-06T17:18:58.714919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.766139Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.766139Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:7c665f3a5f6d79c4b28d35e60d46ee9fa4013af24b3c5409ca4f8a63336eaeaf","observation_id":"5cad9ab2-1813-4fa9-89f2-5d10b578db70","resolution":{"observed_at":"2026-08-06T17:18:58.766139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.867861Z","title":"Kubis, Phys","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.867861Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:193009529b761d5669c24645d46a1443f1ea2790d46181518a70bf2620e09e25","observation_id":"feb02c9c-43e4-46e6-bbbc-123e97db49ab","resolution":{"observed_at":"2026-08-06T17:18:58.867861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:58.953230Z","title":"Worley, P","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:58.953230Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:77e8317b24686187c73be0618e383eeb47ebfaf93e9c19c72cd141b53fa02328","observation_id":"5f5823cb-713c-4b9a-8f2f-6435ae2267bf","resolution":{"observed_at":"2026-08-06T17:18:58.953230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.017115Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.017115Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:eaaf7fbf63bdd9d57949b6581718ea303c37e8f9137f71c9c1a944a4c2738cfb","observation_id":"7df47848-fb0d-40dd-9746-c49badc62b1d","resolution":{"observed_at":"2026-08-06T17:18:59.017115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.090587Z","title":"Atta and D","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.090587Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:afa8b4ae75771bf34f113a55f1f96524989f902dd008e99445c0fa0b857f7dc5","observation_id":"c1efdd63-0857-43bd-aac4-e389511304a6","resolution":{"observed_at":"2026-08-06T17:18:59.090587Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.176287Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.176287Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:cb9599ab3cf0c8f2193360ed49e624414b4f337bfe5eef8cfcd218dfb6013182","observation_id":"6bc787db-4e17-4b9d-ae7f-905d6d6e2a73","resolution":{"observed_at":"2026-08-06T17:18:59.176287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.278288Z","title":"Douchin and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.278288Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:e8e3719a4dd28a64de5d3f9e86349f3fa052aad80c837ab37c8271cab6a56054","observation_id":"5c8b82d8-d065-44ef-9e08-8905c465f015","resolution":{"observed_at":"2026-08-06T17:18:59.278288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.380817Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.380817Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:6953e9a56019e37520c0504806a911857e7a2ce498a1d053ecaec0f743c23e20","observation_id":"dd0812d1-dd3a-45dc-a016-239b0a2f16b5","resolution":{"observed_at":"2026-08-06T17:18:59.380817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.449200Z","title":"Lim and J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.449200Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:0888b0f8eca7a84d5209c231a5fd21513805afebcd5f945f8cb658e08621977b","observation_id":"e46659e5-beab-4d1d-93b9-9e17fba221e2","resolution":{"observed_at":"2026-08-06T17:18:59.449200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.527095Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.527095Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:9aa54de82149ce2552d769fc5f8bd7e7127d358ee08fd191c2057a98c11221cb","observation_id":"ddf2e202-ca88-49ca-8821-78213bffd3df","resolution":{"observed_at":"2026-08-06T17:18:59.527095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.621248Z","title":"¨Ozel and P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.621248Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:c78c8cab63671e0a521f079ae12aa7139034261cf9f6cadb0439d5df37d55459","observation_id":"91e72943-206a-43da-91bf-21cb2cbe6dd1","resolution":{"observed_at":"2026-08-06T17:18:59.621248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.698539Z","title":"Arzoumanian et al ., Astrophys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.698539Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:aef9d937812afdc032c91583339699df700baac4394531b3d01de2ec36728d27","observation_id":"7fcdebf9-6a59-44e7-afd2-d30873e491a2","resolution":{"observed_at":"2026-08-06T17:18:59.698539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.823139Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.823139Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:d3aa292c99e39cd93af5fa2c584cea4f736a9acd2f699144e0c447e2520e257b","observation_id":"70ca4dbf-e6a0-4b62-a216-2cb47e0da0eb","resolution":{"observed_at":"2026-08-06T17:18:59.823139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:18:59.913220Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T17:18:59.913220Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:d296a12e899c6b247e1f662cd46a1367d21d77f6494dfb2fd1dbdad6df546f27","observation_id":"f91c23cc-fd9b-40cf-a9d1-fe26d7ca224e","resolution":{"observed_at":"2026-08-06T17:18:59.913220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:00.016757Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.016757Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:6b15aed455270d6fdead39829d860490c29e82033ef5e87aa935b73c611001cd","observation_id":"b9c21fc6-e096-4ba7-a537-ae56010f27d7","resolution":{"observed_at":"2026-08-06T17:19:00.016757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:20.087921Z","title":null,"venue":null,"work_id":"a69e475a-ebf6-419f-ad10-0082f72a7af9","year":2015},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.085578Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:bf4c8d846433fecc68a0a01c667bcb694c72ddfc2bae97facd17f47872cb1819","observation_id":"53ca7f59-caa0-4c02-bda4-17c1387fdb82","resolution":{"observed_at":"2026-08-06T17:19:20.124633Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:19.961962Z","title":null,"venue":null,"work_id":"5a1f3cfd-3b88-4388-b811-bd12150a49c0","year":2020},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.167250Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:6dff52267e36b6016954d9fa39d1c71f89f7f53905f55afe69f0978af927960a","observation_id":"293620be-1e9b-4380-ac32-6bec9f35c2d0","resolution":{"observed_at":"2026-08-06T17:19:20.019581Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:19.758987Z","title":"Ni and Z","venue":null,"work_id":"4194df87-0405-4e90-b561-a922df7f679a","year":2011},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.252968Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:3f0f36cbdd8f2b24a321733efda89776bcc0f83c6cef3ea7c639856e32c511e4","observation_id":"9cc35144-da33-49e3-8e7a-049b443c2e30","resolution":{"observed_at":"2026-08-06T17:19:19.872868Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:19.525531Z","title":null,"venue":null,"work_id":"cec47e98-7813-4137-9366-73a79250f13e","year":2019},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.338228Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:71352c752264bbd55eed4abf7b06bd25fdf6ccd30588add5569b3e9778a00f30","observation_id":"50794c83-f215-4ca8-9d46-ea5327f64f2b","resolution":{"observed_at":"2026-08-06T17:19:19.638131Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:19.329817Z","title":"Furumoto, Y","venue":null,"work_id":"201d2eec-98b8-475a-b657-55875af8abea","year":2009},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.443622Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:a5b3370e0408aed0e0d29d9fd3e9f5139f312f141e4fe06e0188b063533f7421","observation_id":"fb4e3cfd-d725-4927-955f-6a2be6bfc008","resolution":{"observed_at":"2026-08-06T17:19:19.414965Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:19.135193Z","title":null,"venue":null,"work_id":"fe75d7d7-de84-44b1-9b1b-c1bf3bc371ba","year":2008},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.541311Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:69f3ba387768967b5a0a2910b2951bf980e03362a1fcd38558d707619f489c1b","observation_id":"7c8380c4-9a5e-4ac5-893e-cca10e38aaf5","resolution":{"observed_at":"2026-08-06T17:19:19.216482Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:18.970440Z","title":null,"venue":null,"work_id":"3be6aa4f-a074-42c8-82b9-06c4aa980baa","year":2007},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.676228Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:c6bf92609ddcb97315998a1b243cbb761422729e1aa1af54b6a3f455a386b167","observation_id":"bea376eb-5620-450a-8f3d-b5a5d497666a","resolution":{"observed_at":"2026-08-06T17:19:19.045933Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:00.782121Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.782121Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:f4aad6ef21ebfd877aa0cf6ec829d579c8602d280b2a80def35d667323bd1afa","observation_id":"fd3cb699-ad49-42ff-81c6-591739816467","resolution":{"observed_at":"2026-08-06T17:19:00.782121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:18.783472Z","title":null,"venue":null,"work_id":"44f1f6c3-2373-428c-9084-44742886aa14","year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.860681Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:e8faa81cab9bde6f1ba3cbbea574563e99eae3c555d30463e737d1de2a7fa7a4","observation_id":"d53b23e8-104b-47c8-a279-78bf32fa09ff","resolution":{"observed_at":"2026-08-06T17:19:18.879232Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:18.600928Z","title":null,"venue":null,"work_id":"682fd0cb-0c08-44be-a4c7-20d8364a2e87","year":2016},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:00.996238Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:cd5aa320220d8deb2779dd28b306b8a06d654ff3f20c0153e4c9b8f475b6a874","observation_id":"eba14113-e07d-4918-b161-57f7e77a6a18","resolution":{"observed_at":"2026-08-06T17:19:18.687938Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:18.457760Z","title":null,"venue":null,"work_id":"1f798517-46a3-46ca-aa17-c6fd9eb4c6da","year":2012},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.074082Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1d95aa1dd8d1983d017ee9cbecd9a9105413d195b88fea7831ed2eb5f49ba6f5","observation_id":"8d3f42a3-1ddb-4486-8b09-943c2d22f20f","resolution":{"observed_at":"2026-08-06T17:19:18.536904Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:18.241712Z","title":null,"venue":null,"work_id":"4a9e7c0b-7152-4b11-9512-8376c5d846c5","year":2023},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.144586Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:1b4c4271f73e2617af22fccf7eb7955050bf077410815571a29460b7ceb55634","observation_id":"d43c944b-82d9-48d6-b3c4-5ef5292b0387","resolution":{"observed_at":"2026-08-06T17:19:18.343215Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:18.029325Z","title":null,"venue":null,"work_id":"dcedf420-54ba-4c02-830b-6725d8db9f6a","year":2011},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.224316Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:341a84d9355d19a271fab081de9a61ce64dbdaf9de547b99e6eb8344fa93384a","observation_id":"4526dd44-8093-4e6e-a204-f824830ccde9","resolution":{"observed_at":"2026-08-06T17:19:18.113116Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:17.804148Z","title":null,"venue":null,"work_id":"271c0410-a9f7-4c4f-b356-38d716ef527b","year":1996},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.320117Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:e21af829302e48565f9c4dfbf0722e383719196df653513fc699ae4353efc25b","observation_id":"bbf20816-40d4-4e80-86b7-8ffd3cec3b30","resolution":{"observed_at":"2026-08-06T17:19:17.919302Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:17.653555Z","title":null,"venue":null,"work_id":"e1e70cd3-b3e2-4bfb-93a8-f463ec8ddd34","year":2021},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.433331Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:a26d2c7b56c0383ac512406504d773c7edca945b41b497a8dfff65c2f7f31ada","observation_id":"5eb06a7d-7064-4086-a650-5b46305cf70a","resolution":{"observed_at":"2026-08-06T17:19:17.744719Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:17.501169Z","title":null,"venue":null,"work_id":"ebc9fc68-a920-469d-b8ff-e9232fb63f9d","year":2011},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.577140Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:672ed2b394ac6d5ef0719eb3fc624225dfac7773a2ccbc5348e5bc1fc81e2fed","observation_id":"1a75280a-5b1f-4722-b3e0-b0b14e37b4b8","resolution":{"observed_at":"2026-08-06T17:19:17.593119Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:17.345140Z","title":null,"venue":null,"work_id":"d971fc3c-e54c-4add-b5c5-f458f40f56d4","year":2014},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.691623Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:f4d80ae1503da00c1d175b95af54f41150d7205a09acc0bb512b03bf1f08ad02","observation_id":"32731583-022d-4d1c-b603-d28007af62e6","resolution":{"observed_at":"2026-08-06T17:19:17.426923Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:17.175493Z","title":"Mukhopadhyay, J","venue":null,"work_id":"e3ea0210-552b-42ce-91cd-fdc54b1b4e2b","year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.851478Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:56f4fe629e50b22f5b725f2267d03215a713607a3e54d25c7fa73d8ac333d144","observation_id":"36892081-d3bd-48ac-9f32-52281314b63b","resolution":{"observed_at":"2026-08-06T17:19:17.257198Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:16.957567Z","title":"Sabatucci and O","venue":null,"work_id":"2a73cb4c-d696-4b19-9f79-98e2955a1e26","year":2020},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:01.983917Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:e24656eb579c7acbbe4b7ea8223ba74a89d7476d8f55d5366d427390c25a93d2","observation_id":"dcec5032-598d-4803-ad1d-ec9686936b12","resolution":{"observed_at":"2026-08-06T17:19:17.054520Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:16.721459Z","title":null,"venue":null,"work_id":"fe738052-5a9f-40d1-9a1e-447b658aaf68","year":1998},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.119960Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:a8e153901251cfbbe06a63b732b057f4e75298cf881f506842fd3e91ce460bb9","observation_id":"1792b80c-0dd0-4cef-81f6-872fa8c022da","resolution":{"observed_at":"2026-08-06T17:19:16.843839Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:16.508839Z","title":null,"venue":null,"work_id":"b768bead-7202-4060-9029-ab9de4fa11fb","year":2022},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.246446Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:66ac7b1e257214566c14918dc0ad33d55dc473212575ee3161f22dc00280f287","observation_id":"b9cf13c9-e0e1-4726-bd2d-bed42ec6e559","resolution":{"observed_at":"2026-08-06T17:19:16.621829Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:16.277154Z","title":null,"venue":null,"work_id":"217a2adb-56c0-49f2-bb7a-b85540b4de7b","year":2000},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.371081Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:d0bf8da8f73e16dcf46277942943ebfdc27206d3165a688637dab93a5567183f","observation_id":"9d810b27-79bb-41c0-9c22-a9ad444383cb","resolution":{"observed_at":"2026-08-06T17:19:16.410025Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:16.096706Z","title":null,"venue":null,"work_id":"df63dba7-bf5e-4809-b84a-e77212c1b48f","year":2010},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.488105Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:fdb8ce7c39015530d27ef1a44a13cdb9350cfc88a7bc5f05c7fbd68a983a4b64","observation_id":"98b444d4-debc-4f5f-83d3-9ce7939247d9","resolution":{"observed_at":"2026-08-06T17:19:16.193371Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:15.925532Z","title":"Baldo and L","venue":null,"work_id":"b0ffb109-962f-4df6-a1b2-147751bae3c9","year":1999},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.586873Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:431e7f9773b119ad55d0d52eac981cf6ce26b516361f5991d7c62c2aa6f723d5","observation_id":"06b35100-5577-4951-9032-7d39882a6639","resolution":{"observed_at":"2026-08-06T17:19:16.016141Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:15.674468Z","title":null,"venue":null,"work_id":"59aa7747-50fe-4fdc-9aab-3656b6b8732a","year":2020},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.707991Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:5bbeeec8c9973d00a0d9057b698b4740770858f7dc6c963b99bc4f16e38b52e0","observation_id":"ec3444d5-a6c4-4fe3-bdc5-2e9117256f0b","resolution":{"observed_at":"2026-08-06T17:19:15.806888Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:15.510798Z","title":null,"venue":null,"work_id":"3e3af646-54c9-41b2-b18e-b67ffb5ba7de","year":2009},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.816310Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:49050dbf9e7325193caed7f3412c14666b27db0f972232cbb10048db5f025ed6","observation_id":"bb147062-4144-479f-b846-e6d8c59d349f","resolution":{"observed_at":"2026-08-06T17:19:15.605210Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:15.287282Z","title":null,"venue":null,"work_id":"3314fd65-f5fe-4c19-a8a0-ad99c239ec23","year":1997},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:02.915673Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:a9851a64ef64cd67c3dd671522964560d425fdf6481fac52a2a6c108bc081cba","observation_id":"e3dff461-136e-4971-803f-6894637662ba","resolution":{"observed_at":"2026-08-06T17:19:15.401260Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:15.057902Z","title":"Anantaraman, H","venue":null,"work_id":"fd91a24a-b91d-49ea-a85c-f2c69ea8a5f6","year":1983},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.035583Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:6c7354e0c7b2e3d2a223e7eaeacca0c70ee56355c41693c53fad37573582afe1","observation_id":"4c2058ca-400f-4183-932f-9b63e29fb1cc","resolution":{"observed_at":"2026-08-06T17:19:15.157028Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:14.820023Z","title":"Bertsch, J","venue":null,"work_id":"b00683af-fd35-4bbe-9b56-9bd4d9425712","year":1977},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.178476Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:4ef690f2d3693e8cac452538995bbd78d77abe8422422437a9959be219a593b1","observation_id":"6617d356-07e3-4567-a77c-8496cff4fd8f","resolution":{"observed_at":"2026-08-06T17:19:14.939737Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:14.644331Z","title":null,"venue":null,"work_id":"b09dfd41-9358-452a-827d-40a4e288e771","year":1979},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.295603Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:494d98e152cda441a5d119b9918bbf51f7c6f9d32280e845c747e7362c061d67","observation_id":"0e0e8d5c-f17b-4327-8d3c-15e385d78ef7","resolution":{"observed_at":"2026-08-06T17:19:14.700871Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:14.420471Z","title":null,"venue":null,"work_id":"5bf2904c-a0db-4323-9093-0789ba229e32","year":2007},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.404257Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:342da01442d687a4491b82f290016c274ae72d94f0e23d891b29a60060d5c4cd","observation_id":"513b2028-4506-4ef5-9d54-9f8eb84cc938","resolution":{"observed_at":"2026-08-06T17:19:14.514842Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:14.243732Z","title":null,"venue":null,"work_id":"e6c7a270-430b-4738-a8bc-8d84a31b993c","year":1977},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.512791Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:4aabe017786c8047f80b23ef2719841c93f21dd6ad875032a0f6bba1cf4f088e","observation_id":"e1184c6f-4bdd-4bb1-9e14-2f9515ce897d","resolution":{"observed_at":"2026-08-06T17:19:14.344132Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:14.155435Z","title":"Lejeune, Phys","venue":null,"work_id":"9ecf1130-1ab9-4d4b-bbba-de1910b8055f","year":1980},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.660896Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:f9b1fe607cce0f64d39797a87f156ed726a7a04b2a88856244b86c9054347e73","observation_id":"def72ae9-6489-4cb5-bc4c-3b6f5ba1e074","resolution":{"observed_at":"2026-08-06T17:19:14.188443Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:03.803010Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.803010Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:edc9eee50d91606b251a7c9ce33792d7b3dccf326c40a1c42d70fd2ce5dd9f0c","observation_id":"f275c908-9d89-4225-8177-039ab5bd94db","resolution":{"observed_at":"2026-08-06T17:19:03.803010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:03.944843Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:03.944843Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:461bdb3b9cd3e62fb8787bf92dc2a15519c19de03ac018a600bc3cf8907c623e","observation_id":"008cb95f-59ea-4651-9eb9-4dba18960c44","resolution":{"observed_at":"2026-08-06T17:19:03.944843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:13.965500Z","title":"Haensel and J","venue":null,"work_id":"6849226c-aeed-478e-ad57-2671c59fe954","year":1989},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.030832Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:b7b386a44ccc338bb2cb4aff1e8222cafe4c83141bbee672ca1931ff97281aa2","observation_id":"be652e4e-2bea-4df3-88ed-bb488726faa0","resolution":{"observed_at":"2026-08-06T17:19:14.069537Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:13.783563Z","title":"P Feynman, N","venue":null,"work_id":"5f6acd37-540e-4aea-9902-69af7607c036","year":1949},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.124506Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:db839a425e48e0ed98b460347b58244b77fc92ddde6bac10fc5b62a986d6c148","observation_id":"5a4ebee0-3c42-4d68-8d01-523f855f9792","resolution":{"observed_at":"2026-08-06T17:19:13.860274Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:13.658574Z","title":"Douchin, P","venue":null,"work_id":"93c94e30-da00-4e98-b363-0bfd8f8d205a","year":2000},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.176067Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:8faa1e8e84fb61b7971ecc0250da21051db26d0b8515a84ef93588e54eccaf90","observation_id":"babf6853-4315-488e-9d0a-77abc462c53e","resolution":{"observed_at":"2026-08-06T17:19:13.703324Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:13.459661Z","title":null,"venue":null,"work_id":"33075f08-bd98-4c6c-8d61-90365a384e8b","year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.305615Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:2e0834922cb484e7c3e465f8690537e4a68b963fcb43184770a818f2035aca5e","observation_id":"73f09d31-8e73-4a51-ab61-942377552902","resolution":{"observed_at":"2026-08-06T17:19:13.559371Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:13.326593Z","title":null,"venue":null,"work_id":"3f188b24-7897-43a4-9bf3-54f9974c248a","year":2020},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.418217Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:dab4437b7cb9907cbd74dd4767bb08b9f7e4b9a137ae2ebfcedd6555dd675d9e","observation_id":"f9257e60-63ae-433d-9f86-86329c207daa","resolution":{"observed_at":"2026-08-06T17:19:13.402813Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:04.482279Z","title":"Landry, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.482279Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:6618e5fb09e7fe1f53fbda9d7eb2aa451d792b01905311e5b7c2546488a90328","observation_id":"7ba85511-a170-4c4b-ae8f-8c303ff1b204","resolution":{"observed_at":"2026-08-06T17:19:04.482279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:13.115201Z","title":"Riley el al ., Astrophys","venue":null,"work_id":"7e017fa7-0c05-4281-8299-1f46e0f1ef8b","year":2021},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.562827Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:86ae0193b4e2419c72fdd71bd8758337b40069db315097df3734a0604804a2b0","observation_id":"db38736c-64bd-49c8-a12c-6a095b4171e4","resolution":{"observed_at":"2026-08-06T17:19:13.196531Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:12.908729Z","title":null,"venue":null,"work_id":"0cc12da8-5a40-437e-ab8b-531885e862b8","year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.627272Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:b3e030028a9c4394b80ced33aae02b4b3d4dff47fc6614124124eb931ca82c7a","observation_id":"5f2e48c0-81cc-462a-9448-f34ad727bbec","resolution":{"observed_at":"2026-08-06T17:19:12.989245Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:12.709787Z","title":"Salmi el al ., Astr","venue":null,"work_id":"91ef54e9-8995-4a2e-8b4c-8219721b9ef8","year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.696297Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:16b28b018eccfc0f79feb4d9355e12abe2c3e24383a2006aff428b1810592e1f","observation_id":"a0c87d16-9ed1-40a3-aae3-b70cb2d36d8f","resolution":{"observed_at":"2026-08-06T17:19:12.800443Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:12.564180Z","title":"Choudhury el al ., Astr","venue":null,"work_id":"90f30cc8-7ba5-4176-a480-1a7f72a66458","year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.801063Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:0380a8059c3e860cc41c58173446b4ef72836af1cb548ba7ef383ca425a754d3","observation_id":"60903d9f-9e61-48f4-b9fe-ca03114dcbca","resolution":{"observed_at":"2026-08-06T17:19:12.645968Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:12.427048Z","title":"Salmi el al ., Astr","venue":null,"work_id":"bc47df1d-d57c-423e-9c26-29821d6d7305","year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:04.880196Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:3b178bafa64aa7d7e47f7a22361d7a05911e325a3eef40e8ac5535704637cc92","observation_id":"c80d5d29-a9c9-481a-8c0b-9055fdea6c75","resolution":{"observed_at":"2026-08-06T17:19:12.497247Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:12.300360Z","title":"Vinciguerra el al ., Astr","venue":null,"work_id":"66c669c8-b850-4690-a85f-1567a9d63dc8","year":2024},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.001957Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:d12718bc0cc657348a482b846c67628eba80d08aa77d9d3877c88b0549f03fd5","observation_id":"4e9ce6ea-5442-4151-a9ff-cb98060bd52b","resolution":{"observed_at":"2026-08-06T17:19:12.357964Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:12.133773Z","title":null,"venue":null,"work_id":"c5ff13c4-ba6e-46a7-986e-879d2555a986","year":2021},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.065588Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:31472fb2cdd3a38f3a2affbc1ab3e4813e430dec5e01bd38c56a691527ed1c39","observation_id":"8cf8b1bd-714d-4e20-a072-2806e38bd1c8","resolution":{"observed_at":"2026-08-06T17:19:12.225413Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.988860Z","title":null,"venue":null,"work_id":"51f87168-fb2c-45df-98a3-640abf0e0d75","year":2019},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.124031Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:809a5b6e6ab5773f6b8c5807474610ac63e380877fdc410a4ef9d465674dbf52","observation_id":"0bea452b-4a65-4a2a-a35b-977eff4847ce","resolution":{"observed_at":"2026-08-06T17:19:12.063578Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.853421Z","title":null,"venue":null,"work_id":"c579187c-98c1-4d7d-8741-ffe546ac34b2","year":2025},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.242654Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:e905e36db5198eba108005c05d3389adffeaf18a6651b2c4e280297d97db767b","observation_id":"6395e0d0-3579-4c39-8d40-2c049b343b1d","resolution":{"observed_at":"2026-08-06T17:19:11.906419Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:05.332951Z","title":"Danielewicz, R","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.332951Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:813e5f0618ab3f199d6595b05ca9f5719e4f6824c50aa29b0efd750cf844bc70","observation_id":"80c8fc4b-5cf2-4289-a144-317ded6e946c","resolution":{"observed_at":"2026-08-06T17:19:05.332951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.694024Z","title":null,"venue":null,"work_id":"511bbe6d-00a7-4808-a0a1-9c8bd54e8c66","year":2021},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.421491Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:b4a607af429e12ccaac616b5fb662d2e4c5097ad635d7d18b68d65a6094a7a58","observation_id":"a776412a-e59e-4a8d-a150-83f90cfdb8f6","resolution":{"observed_at":"2026-08-06T17:19:11.762396Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.575555Z","title":"Garg and G","venue":null,"work_id":"ba68aa25-cc30-4416-b62b-96ae45e79722","year":2018},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.493131Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:4c99c6135e2482cc0955539c9ab9708c56038769a686a7938a2579196ad584be","observation_id":"ce08d915-2836-4d53-8ac4-343d5af6c117","resolution":{"observed_at":"2026-08-06T17:19:11.640293Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.444493Z","title":null,"venue":null,"work_id":"c7051acd-832b-4da2-9099-1ad83d2bbbc4","year":2006},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.555543Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:079125eefb7a953d7e8a36867e0fb2b2cb1e6142d487e33284ac40913ef5cb07","observation_id":"c7fe0c74-9e42-4758-827a-90392943f16a","resolution":{"observed_at":"2026-08-06T17:19:11.517728Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.311153Z","title":null,"venue":null,"work_id":"0fb80040-d10c-4884-b22a-49f437f500ae","year":2020},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.617486Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:69c53954843aa905218acb29781dd14b6365fa6f648cd4b6eddf3845caf0fbc3","observation_id":"ed18e96d-de4a-420f-ad3f-17ae866076df","resolution":{"observed_at":"2026-08-06T17:19:11.370077Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.183497Z","title":"Pagliara and J","venue":null,"work_id":"f84e6520-493e-47c0-a962-20775f323cb5","year":2008},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.679761Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:f477ac1d7fdaf326071b8c5733a59adf212338ef74680c53db138c3f5f31ccb3","observation_id":"d63d3055-1ab1-48d0-b09c-1d5fb49acbef","resolution":{"observed_at":"2026-08-06T17:19:11.252747Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:11.045659Z","title":null,"venue":null,"work_id":"70dd821d-db72-41d9-aeb0-4d0cda9a1a16","year":2008},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.787417Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:8db63a86938cc8733ebd0ebe82c1be1dc8317e0de0334f685436936c4d5a540e","observation_id":"0ab384eb-75de-4328-92dc-eb3ace143373","resolution":{"observed_at":"2026-08-06T17:19:11.105235Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:19:10.920327Z","title":null,"venue":null,"work_id":"14e3bde1-1e95-433a-bdbb-ae6c7a1ef963","year":2013},"citing_paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-06T17:19:05.905003Z"},"links":{"citing_paper":"/paper/2507.11379"},"observation_digest":"sha256:70afe74913c103c55ba25f1c9073753c9c321028e2e36471e5322847fd5e1534","observation_id":"c9ad4230-8aa8-4254-98b3-2bd622295149","resolution":{"observed_at":"2026-08-06T17:19:10.986697Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.11379","last_updated":"2025-07-15T14:49:41Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-13T04:34:07.327525Z","submitted_at":"2025-07-15T14:49:41Z","title":"Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":82,"verified_exact":0,"verified_fuzzy":18},"total_outbound_references":122},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 100 of 122 outbound references and 0 inbound Pith citation observations for arXiv:2507.11379."}