{"as_of":"2026-08-09T21:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c71ad0faf75b0690c5bfabb0b0939ddb57ee50c0ac0817a02b0cc458d7ede93f","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":29,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":29,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":29,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":29,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T00:43:19.840819Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T19:00:04.479596Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2505.16929","last_updated":"2026-04-14T09:24:59Z","snapshot_observed_at":"2026-07-06T21:28:43.610849Z","submitted_at":"2025-05-22T17:22:16Z","title":"Properties of the neutron star crust informed by nuclear structure data","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-22T01:36:22.187463Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2505.16929"},"observation_digest":"sha256:74da5b7f13a7f96a470a624e5d49fce18a884dce2c7983d41b0b37c3fcf6c3ff","observation_id":"50d0a0aa-600b-4a51-988f-52136af55e8b","resolution":{"observed_at":"2026-05-22T01:40:54.104405Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-07T10:19:36.441993Z","title":"Vinciguerra et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.05603","last_updated":"2025-08-13T15:01:01Z","snapshot_observed_at":"2026-08-09T06:40:16.868328Z","submitted_at":"2025-06-05T21:33:31Z","title":"Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T10:19:36.441993Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2506.05603"},"observation_digest":"sha256:1f154cc80f87bf967d8838cc1a48066ddc8125f89861a07d4d49facf7593bcac","observation_id":"b63dd036-db7c-4597-9ba8-2c96d2c1ff8d","resolution":{"observed_at":"2026-08-07T10:19:36.441993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-07T05:14:54.926616Z","title":"Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.08658","last_updated":"2025-06-10T10:19:43Z","snapshot_observed_at":"2026-08-07T10:37:26.398774Z","submitted_at":"2025-06-10T10:19:43Z","title":"Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T05:14:54.926616Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2506.08658"},"observation_digest":"sha256:5068f348602297ea64afc8155458237c9e4b67932612279e49275f941d9408b6","observation_id":"2432a671-7c86-4c67-9e85-22516c5c775e","resolution":{"observed_at":"2026-08-07T05:14:54.926616Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-06T19:05:26.259517Z","title":"Vinciguerra et al., An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451, Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06577","last_updated":"2025-07-09T06:09:58Z","snapshot_observed_at":"2026-08-09T02:42:27.201027Z","submitted_at":"2025-07-09T06:09:58Z","title":"Ferromagnetic instabilities in quarkyonic matter","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T19:05:26.259517Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2507.06577"},"observation_digest":"sha256:f9127a5c9e4a0642c67b4e2fb52a8995f8ba5819a4e4e3ed244481b2ff960486","observation_id":"a9f24058-43a8-46ca-a1de-49a31b6b32a4","resolution":{"observed_at":"2026-08-06T19:05:26.259517Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-06T16:49:28.917824Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.12540","last_updated":"2025-07-16T18:00:09Z","snapshot_observed_at":"2026-08-08T17:36:40.109662Z","submitted_at":"2025-07-16T18:00:09Z","title":"Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T16:49:28.917824Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2507.12540"},"observation_digest":"sha256:c1db23f2b11d79b980976e56f6eb97034ceb3f241481ffcfdf218012835779ac","observation_id":"41693507-1fc3-435e-9208-63baad01e556","resolution":{"observed_at":"2026-08-06T16:49:28.917824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-06T10:19:15.296773Z","title":"Vinciguerra et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.00236","last_updated":"2026-06-23T06:11:02Z","snapshot_observed_at":"2026-08-08T10:37:43.334314Z","submitted_at":"2025-08-01T00:47:10Z","title":"Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T10:19:15.296773Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2508.00236"},"observation_digest":"sha256:44b7c601e0da7f45510d6697f9e325ed141e7ea09cb1c54593dd4a13a53d0f1d","observation_id":"518a7302-dcbe-42cd-8151-763eb434a2c3","resolution":{"observed_at":"2026-08-06T10:19:15.296773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-05T11:21:41.522403Z","title":"Vinciguerra et al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03008","last_updated":"2025-09-03T04:35:54Z","snapshot_observed_at":"2026-08-09T19:09:00.742011Z","submitted_at":"2025-09-03T04:35:54Z","title":"Origin of nucleon mass in the light of PSR J0614-3329 with quark-hadron crossover","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-05T11:21:41.522403Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2509.03008"},"observation_digest":"sha256:e631d6b857ed1775a47d058b1eb4b9140047ebb9df0b36be7e564067fda26a5a","observation_id":"7c70a219-b488-4536-aec2-ded22b28308c","resolution":{"observed_at":"2026-08-05T11:21:41.522403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2509.06145","last_updated":"2026-05-15T10:40:47Z","snapshot_observed_at":"2026-08-05T15:15:32.430472Z","submitted_at":"2025-09-07T17:21:11Z","title":"Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-21T22:56:05.224146Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2509.06145"},"observation_digest":"sha256:808fe373a82c167c4fad4e754cb47341d5e20775163d3d2acabd5bdac672ae01","observation_id":"7dffd9e8-dac6-48cb-8d78-75eac63900b6","resolution":{"observed_at":"2026-05-21T23:00:43.869387Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-03T18:37:51.757564Z","title":"Vinciguerraet al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.04505","last_updated":"2026-07-30T09:21:34Z","snapshot_observed_at":"2026-08-09T11:13:18.516473Z","submitted_at":"2025-12-04T06:24:11Z","title":"Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T18:37:51.757564Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2512.04505"},"observation_digest":"sha256:30afd93c1d173054a4f7d8d603ae2d8b8cf9085925074bf19cd7680dff99db81","observation_id":"1bc9fac4-6443-4b03-886b-642a64161d72","resolution":{"observed_at":"2026-08-03T18:37:51.757564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-03T17:54:34.790126Z","title":"Vinciguerra, et al., An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451, Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2512.07977","last_updated":"2025-12-08T19:10:30Z","snapshot_observed_at":"2026-08-07T20:12:37.930978Z","submitted_at":"2025-12-08T19:10:30Z","title":"Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T17:54:34.790126Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2512.07977"},"observation_digest":"sha256:42f0e339561aae9fc131bcebeeeadd0f7e9fa1e161d7f07e2956a51762dfd84d","observation_id":"99aeddb0-ad3e-419f-8409-569cadf9d6fe","resolution":{"observed_at":"2026-08-03T17:54:34.790126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-04T00:40:09.682873Z","title":"Vinciguerraet al., An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451, Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2601.05999","last_updated":"2026-07-31T19:04:54Z","snapshot_observed_at":"2026-08-06T23:10:54.278432Z","submitted_at":"2026-01-09T18:33:25Z","title":"Constraining Hamiltonians from chiral effective field theory with neutron-star data","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T00:40:09.682873Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2601.05999"},"observation_digest":"sha256:7b8ddd7fe2ec92d4bc5d3f6228ef825f9c1f1eadc6a6ced634d4f0359c548ea2","observation_id":"ebb2b362-98f9-4c14-9c93-9e9d4e7756eb","resolution":{"observed_at":"2026-08-04T00:40:09.682873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2604.04560","last_updated":"2026-07-11T01:33:13Z","snapshot_observed_at":"2026-07-16T23:17:50.080024Z","submitted_at":"2026-04-06T09:40:02Z","title":"Neutron star with dark matter using vector portal","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-10T19:33:30.024439Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2604.04560"},"observation_digest":"sha256:ed3e758b61145cba30f8117a156d6b2756fdbf604023604a44d5366930d0770a","observation_id":"85f1f046-6e5e-4274-a855-020331bb94d6","resolution":{"observed_at":"2026-05-10T22:50:48.441083Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2604.11358","last_updated":"2026-04-13T11:55:17Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-13T11:55:17Z","title":"Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-10T16:04:50.609515Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2604.11358"},"observation_digest":"sha256:f7efe6229312c8f27cd7056a182f89c646cfaa9c66aa7a0bd52bf09ba6fd5566","observation_id":"5b21b5f9-4473-4b4e-abac-c1d20bf73bd6","resolution":{"observed_at":"2026-05-11T09:21:01.551737Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2605.02807","last_updated":"2026-07-30T15:58:12Z","snapshot_observed_at":"2026-08-02T23:57:45.476866Z","submitted_at":"2026-05-04T16:45:38Z","title":"Hadronic lensing","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-08T18:26:45.923519Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2605.02807"},"observation_digest":"sha256:9408c2dad1d5c2b177fe58f225e2318d9a66152947b6ef94f99f3c46be6d3558","observation_id":"aedd8c7d-4ff7-411f-8eff-cd22d8c7b1ef","resolution":{"observed_at":"2026-05-09T06:25:48.118013Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2605.02807","last_updated":"2026-07-30T15:58:12Z","snapshot_observed_at":"2026-08-02T23:57:45.476866Z","submitted_at":"2026-05-04T16:45:38Z","title":"Hadronic lensing","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-12T04:19:06.681137Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2605.02807"},"observation_digest":"sha256:1064219095b800aeb1e26c58654bc2944ae8a7905775d2192f37fbd028e52c5b","observation_id":"6b85960d-ba4a-44cb-a521-1e856981b7dd","resolution":{"observed_at":"2026-05-12T06:21:28.764860Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-02T15:09:07.261877Z","title":"Vinciguerraet al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.02807","last_updated":"2026-07-30T15:58:12Z","snapshot_observed_at":"2026-08-02T23:57:45.476866Z","submitted_at":"2026-05-04T16:45:38Z","title":"Hadronic lensing","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-02T15:09:07.261877Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2605.02807"},"observation_digest":"sha256:862f2a06e68dd7ce60738ae090d39dd198c6fe877ff369f6a641313fcb00805c","observation_id":"0f183776-65f1-4641-9c7f-2b0118cd57e9","resolution":{"observed_at":"2026-08-02T15:09:07.261877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2605.08584","last_updated":"2026-06-03T18:51:13Z","snapshot_observed_at":"2026-07-06T23:20:47.880233Z","submitted_at":"2026-05-09T01:00:23Z","title":"The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-12T01:12:43.979451Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2605.08584"},"observation_digest":"sha256:6c5e99db3ad217343c7d9445d7d591d8a68a44813681edfa8f06d5ca2864cc32","observation_id":"fa58df0a-430e-4d9c-9db3-f8ac8a7ccbdc","resolution":{"observed_at":"2026-05-12T08:21:25.582941Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2605.08584","last_updated":"2026-06-03T18:51:13Z","snapshot_observed_at":"2026-07-06T23:20:47.880233Z","submitted_at":"2026-05-09T01:00:23Z","title":"The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-30T23:36:07.718605Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2605.08584"},"observation_digest":"sha256:712746671f4ff7101a8cc2c6721056ae4119f1286c82dfeaab4dd980c90ef1d9","observation_id":"192138c2-9955-48bf-b21d-45f6d2fded48","resolution":{"observed_at":"2026-07-01T13:15:46.678115Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2605.14447","last_updated":"2026-05-14T06:41:34Z","snapshot_observed_at":"2026-07-06T23:25:54.070869Z","submitted_at":"2026-05-14T06:41:34Z","title":"Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-15T01:47:28.438537Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2605.14447"},"observation_digest":"sha256:0d0180e1ca2ce8c010fff37c49dd80cf8d39f8db4f7b9e23fa8c7866f07f613e","observation_id":"6621fc00-5f34-4487-b5c5-8cb346d8444e","resolution":{"observed_at":"2026-05-15T01:48:28.250765Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2606.02966","last_updated":"2026-06-02T00:08:57Z","snapshot_observed_at":"2026-07-06T23:43:17.879245Z","submitted_at":"2026-06-02T00:08:57Z","title":"Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-28T09:24:35.059596Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2606.02966"},"observation_digest":"sha256:8273d733eb679d0169ca5e1d7c8dd9056d78339cdf1907d22edb44b9b79dd609","observation_id":"4571fd14-ed53-4a16-a28e-e6db458e838a","resolution":{"observed_at":"2026-07-02T04:06:35.398841Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2606.17875","last_updated":"2026-06-16T12:47:17Z","snapshot_observed_at":"2026-07-06T23:53:25.839293Z","submitted_at":"2026-06-16T12:47:17Z","title":"Hybrid Stars with Post-Merger Rotation Profiles","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-06-26T23:50:12.361235Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2606.17875"},"observation_digest":"sha256:115f0dc5d2b955fae5c4996393be9449c50629350ecf804c354a897439516468","observation_id":"8e8f7919-14ad-446f-8eb4-0e9c7e27824c","resolution":{"observed_at":"2026-07-03T21:58:59.677181Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2606.21435","last_updated":"2026-06-19T13:51:27Z","snapshot_observed_at":"2026-08-06T05:56:14.769876Z","submitted_at":"2026-06-19T13:51:27Z","title":"Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-26T12:50:53.032717Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2606.21435"},"observation_digest":"sha256:a58be7450312f7b1dfa0ea38b9fa2f66672d6a8142c9259298cc53bb37294363","observation_id":"064b47f1-275f-44f1-8bc7-6d9420cd12a1","resolution":{"observed_at":"2026-07-04T07:49:39.049902Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":"2308.09469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-04T19:00:04.479596Z","title":"Vinciguerra, T","venue":null,"work_id":"7c359cdc-875e-4481-9ebf-58c3b73ef03d","year":2024},"citing_paper":{"arxiv_id":"2606.25186","last_updated":"2026-06-23T21:26:31Z","snapshot_observed_at":"2026-08-04T04:10:30.838720Z","submitted_at":"2026-06-23T21:26:31Z","title":"Causality alone bounds the maximum radius difference between different-mass neutron stars","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-25T22:16:36.441357Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2606.25186"},"observation_digest":"sha256:32ebfab249dd2fa38c5c009cefddac8f17785ff585abdfb3263cb7003cd89a33","observation_id":"1007feb0-4309-4869-9c54-6d94327d863a","resolution":{"observed_at":"2026-07-04T19:00:04.480996Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-07-12T00:24:01.284884Z","title":", keywords =","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.03721","last_updated":"2026-07-04T06:04:04Z","snapshot_observed_at":"2026-08-08T10:04:04.593895Z","submitted_at":"2026-07-04T06:04:04Z","title":"A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere","version":1},"reference_index":121,"source":"arxiv_source","source_observed_at":"2026-07-12T00:24:01.284884Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2607.03721"},"observation_digest":"sha256:11ef8d8dc2fa044eeef03e164e36d0f6836795709388aca7106f09feea0ffbc4","observation_id":"107d741b-4e76-408b-b06a-f6b0c79b0fa0","resolution":{"observed_at":"2026-07-12T00:24:01.284884Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-02T03:23:33.802012Z","title":"Vinciguerraet al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.13930","last_updated":"2026-07-15T15:12:43Z","snapshot_observed_at":"2026-08-08T08:44:16.336494Z","submitted_at":"2026-07-15T15:12:43Z","title":"NNStar: An end-to-end AI agent for nuclear matter and neutron star physics","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-02T03:23:33.802012Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2607.13930"},"observation_digest":"sha256:7c260ee4bb50eac9a46efdf37446a0e1ef62d10141f890b0386245dc65b4dfc3","observation_id":"3e625bd7-fe83-44a2-95af-5263afd25ed8","resolution":{"observed_at":"2026-08-02T03:23:33.802012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-01T16:06:33.868444Z","title":"An Updated Mass Radius Analysis of the 2017 2018 NICER Data Set of PSR J0030+0451","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18124","last_updated":"2026-07-20T16:19:21Z","snapshot_observed_at":"2026-08-09T16:14:06.287715Z","submitted_at":"2026-07-20T16:19:21Z","title":"Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars","version":1},"reference_index":135,"source":"arxiv_source","source_observed_at":"2026-08-01T16:06:33.868444Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2607.18124"},"observation_digest":"sha256:4decd427b3cabeb592b102159adfdfd8e947e07aa2742613ee739c4df260e936","observation_id":"5bc52e40-540e-4183-a01f-39a8469419f5","resolution":{"observed_at":"2026-08-01T16:06:33.868444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-01T13:29:49.414450Z","title":"Vinciguerra et al.,An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451,Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.19125","last_updated":"2026-07-21T14:13:04Z","snapshot_observed_at":"2026-08-08T01:44:45.505035Z","submitted_at":"2026-07-21T14:13:04Z","title":"Holographic Soliton Crystals for Dense Nuclear Matter and Neutron Stars","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-01T13:29:49.414450Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2607.19125"},"observation_digest":"sha256:240d13cb42a861fa91615f1993b526c2fe71586d7777e9432cce2d7fcd92a2a4","observation_id":"98142093-2f27-41f4-a6de-5d7ba184697d","resolution":{"observed_at":"2026-08-01T13:29:49.414450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-01T13:16:53.553047Z","title":"Vinciguerraet al., An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451, Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.19220","last_updated":"2026-07-30T14:47:59Z","snapshot_observed_at":"2026-08-07T00:07:35.038667Z","submitted_at":"2026-07-21T15:50:27Z","title":"Quarkyonic Stars with Strangeness","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-01T13:16:53.553047Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2607.19220"},"observation_digest":"sha256:58e5062fa9a11941d7d13a979b3b493d433516a4431276896b78b891591ac87b","observation_id":"25e7b829-bc0b-49d6-ae34-77cab6436025","resolution":{"observed_at":"2026-08-01T13:16:53.553047Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09469","snapshot_observed_at":"2026-08-08T00:43:19.840819Z","title":"Vinciguerra et al., Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-09T02:42:53.548277Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.840819Z"},"links":{"cited_paper":"/paper/2308.09469","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:6c14d5bc57143e79ee06032e40918fa5caaeaad4998872df747b7c1950b0d557","observation_id":"a4cbb7f6-60d8-442f-a5f4-fe4bdea01113","resolution":{"observed_at":"2026-08-08T00:43:19.840819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2308.09469/citation-record","integrity":"/paper/2308.09469/integrity","json":"/paper/2308.09469/citation-record.json","paper":"/paper/2308.09469"},"outbound":[],"paper":{"arxiv_id":"2308.09469","last_updated":"2023-08-18T11:10:46Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T16:07:37.940200Z","submitted_at":"2023-08-18T11:10:46Z","title":"An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 29 inbound Pith citation observations for arXiv:2308.09469."}