{"as_of":"2026-08-12T16:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:84da46e7d3296cbf958d327d54cba55712f11e1bc9c408e637a0508dae63ce9b","coverage":[{"denominator":38,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":38,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T12:45:54.139325Z","state":"measured"},{"denominator":38,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":38,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+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/2608.04967/citation-record","integrity":"/paper/2608.04967/integrity","json":"/paper/2608.04967/citation-record.json","paper":"/paper/2608.04967"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T12:45:58.372422Z","title":"Abbottet al., Phys","venue":null,"work_id":"5aaaee7f-420f-48b0-a614-971f69fad323","year":2018},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.032593Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:cd280ee6dec7506898ebb130e0a8740ac142f7c1fc847db0fc9ffa8994e7fc82","observation_id":"36ca16cc-c939-44c8-be1f-6958c2a6d99a","resolution":{"observed_at":"2026-08-06T12:45:58.437642Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:58.217706Z","title":"Riley,et al.Astrophys","venue":null,"work_id":"79bbe0f2-6ecd-4a3c-bb8e-cf6f849315ff","year":2019},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.041866Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:0acf8095f14399d87ae7390cd7c67bf1268f93516768c6755ba7bf6d40eceb03","observation_id":"75876001-f48f-4854-9d4b-c882ec282b2f","resolution":{"observed_at":"2026-08-06T12:45:58.301621Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:58.052338Z","title":"Miller,et al., Astrophys","venue":null,"work_id":"79a0e34c-518b-4b47-88fc-01de356344b0","year":2019},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.048472Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:a8d7e9b4873eddf8d1b1191664ce696ea89002e035f2781a8d7e31247ba1a49b","observation_id":"a949affa-2bf2-493d-9c36-8fd9a63027c6","resolution":{"observed_at":"2026-08-06T12:45:58.135601Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:53.056144Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.056144Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:97595add634d7fef9ea2f0a2a47dadcc50d89905bcf73ba45e3be8fd095f28cf","observation_id":"536d47f9-1d0d-46b0-8338-3562fe31e257","resolution":{"observed_at":"2026-08-06T12:45:53.056144Z","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":"2026-08-06T12:45:57.912800Z","title":null,"venue":null,"work_id":"71dfbe35-d74a-4977-b380-7126e4fc6da2","year":2024},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.063271Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:b09af64e1ba245f34410e43f4fce941925e1029635d1075739f6c25468d26c77","observation_id":"aabaaf4e-738c-44ee-8752-618691f3a6e3","resolution":{"observed_at":"2026-08-06T12:45:57.951044Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:57.787508Z","title":"Zhao and J","venue":null,"work_id":"1ae846eb-5e3a-4e70-8daf-e8916be4fa4c","year":2020},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.070987Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:1c0aae09e8803f3b3e55d27b07c596b16cd126b966b86cfda20d403c89b08d42","observation_id":"8a56aa53-402b-45b7-8bb3-2486e2ab851e","resolution":{"observed_at":"2026-08-06T12:45:57.829093Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:57.674071Z","title":"Han and M","venue":null,"work_id":"8c3356cf-2277-416e-b388-34066488c16b","year":2020},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.081647Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:c21b20949237a151b72f973dac12d0c4b61f68065065cbe9f3792b4e0ce13392","observation_id":"0cff5731-8886-4419-84f4-7248ed1bd043","resolution":{"observed_at":"2026-08-06T12:45:57.715246Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:57.556672Z","title":"Ferreira and C","venue":null,"work_id":"7233480e-a6f0-456a-9925-4cdf5373041a","year":2024},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.091345Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:a6df08f504486e2a701e065cdac9da6796f810549914a89a68becc6bd81cb875","observation_id":"5ed13849-d17e-49af-9315-24cd90f84605","resolution":{"observed_at":"2026-08-06T12:45:57.603339Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:57.432237Z","title":null,"venue":null,"work_id":"3b19e8c6-8fad-410c-8a5e-09c7b7a3b8b0","year":2025},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.099680Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:42297d4b9ccb454b33bb67067adae28b6c5096decc2f099e4887df230992e458","observation_id":"42106871-711b-4a13-b161-3c0fed21a86d","resolution":{"observed_at":"2026-08-06T12:45:57.478977Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:53.111681Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.111681Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:6f4530b9866a9d5abd1a9f6fc9e292db34ec6493cc783dcde054d8f6756c0f78","observation_id":"9e9121d9-1f63-4586-902e-e0634f2cb076","resolution":{"observed_at":"2026-08-06T12:45:53.111681Z","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":"2026-08-06T12:45:57.246759Z","title":"Grundler and B","venue":null,"work_id":"3a7a9007-dba0-4d9a-a887-177e49754fd2","year":2025},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.123250Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:b0903917a43ea75a9d8f461aef5f2374423bc048227f6c5e9e976499e9daf572","observation_id":"7fdee509-4da9-4a73-b205-483391512af3","resolution":{"observed_at":"2026-08-06T12:45:57.332081Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:57.125006Z","title":"Chen, Nucl","venue":null,"work_id":"3bdf2119-4d3d-406b-a32f-d0f3c1f93e2e","year":2014},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.133340Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:2dd98838e6c4db5b995f7532e76e459b40254f489f5f578d61054a62d037bf4f","observation_id":"00c2b201-a9df-4e2a-b02d-0e91dfbe170d","resolution":{"observed_at":"2026-08-06T12:45:57.195488Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:56.992940Z","title":"Zhang and B.A","venue":null,"work_id":"19231212-7d7f-4240-aadd-ff846b680221","year":2019},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.143511Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:722b59bf63b84d135f089e44fb76dff8bb50d243437ad9f21439fd352673815d","observation_id":"f4772731-469e-47fa-a7dc-23cd529bb35b","resolution":{"observed_at":"2026-08-06T12:45:57.078426Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:56.856155Z","title":"Xie and B.A","venue":null,"work_id":"1e8516e0-071f-47aa-8b3a-8dddb108cc11","year":2019},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.152716Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:dd224a42d17a89125f3818062468bd68f938a743ccf9d9d98545fb2760791d45","observation_id":"ec852c70-5a9a-40bc-ad6a-6d388fee4a18","resolution":{"observed_at":"2026-08-06T12:45:56.928219Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:56.726713Z","title":"Zhang and B.A","venue":null,"work_id":"3e7986d9-f248-45dd-abca-c0c753f13da2","year":2019},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.164312Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:f5f33ca3bfea8f2b950f5d42debffe42df2153de2391a2a790d2a6de1f6af7bc","observation_id":"068733ce-6868-41e0-b5a7-f1b8727efa24","resolution":{"observed_at":"2026-08-06T12:45:56.781526Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:56.608595Z","title":"Li,et al.Sci","venue":null,"work_id":"f8ce9cc2-944b-4612-bd57-1779cfec181b","year":2025},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.175077Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:37f21e530dcbb4c5b90aeab915c5bd686d37996480d2e0f2cc08f6ef64d2a8d8","observation_id":"671332ae-3b5d-4e05-830a-ae72940e023a","resolution":{"observed_at":"2026-08-06T12:45:56.670881Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:56.485538Z","title":"Cruise,et al., Nature Astron.9, 36 (2025)","venue":null,"work_id":"7f40c3e4-54d5-40d7-91aa-c4943248d84f","year":2025},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.183043Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:3958e89553de068389e158441707149902f6404bd55ba4206bbcd3ee53cdaabc","observation_id":"c38f7ba6-b721-4840-994b-2e41af361df5","resolution":{"observed_at":"2026-08-06T12:45:56.546497Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:56.363492Z","title":"Hild, et al., Class","venue":null,"work_id":"70dc9473-0030-427e-9680-19d6195f89ad","year":2010},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.194048Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:760349388d472f97909f4a7f36d7a6de0c00437c620a04e8f40182d75f5a2b11","observation_id":"34e0b770-c813-470a-af02-c3dc9014d92d","resolution":{"observed_at":"2026-08-06T12:45:56.425244Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:53.203560Z","title":"Abbott, et al., Astrophys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.203560Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:c3b74f91845ecb237ed6c58d858a7bcfac9d88c5b9503a42ca4c853c1e011d3d","observation_id":"816f99fa-461d-4793-a299-5fd25b879c24","resolution":{"observed_at":"2026-08-06T12:45:53.203560Z","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":"2026-08-06T12:45:56.201866Z","title":"Sathyaprakash, et al., Class","venue":null,"work_id":"bb7e5754-e715-4f2b-8857-cd0e1b391592","year":2012},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.213777Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:dc760fafbd8fbc463cc0b712b04922b8fd687dabeeeba27b28408bd29385406f","observation_id":"d9884826-ca90-42c7-9da0-08a02de00c3f","resolution":{"observed_at":"2026-08-06T12:45:56.252520Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09882","last_updated":"2021-10-06T14:54:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-09-20T23:34:33Z","title":"A Horizon Study for Cosmic Explorer: Science, Observatories, and Community","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.09882","snapshot_observed_at":"2026-08-06T12:45:53.225859Z","title":"Evans,et al., [arXiv:2109.09882 [astro-ph.IM]]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.225859Z"},"links":{"cited_paper":"/paper/2109.09882","citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:1fdac07e5e9a302234acf771ce32a51d669de76159d9a9946979421add6d1fd8","observation_id":"40b643f6-0110-4adc-ac74-dacfb2df8f68","resolution":{"observed_at":"2026-08-06T12:45:53.225859Z","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":"2026-08-06T12:45:56.091231Z","title":"Chatziioannou, Phys","venue":null,"work_id":"c0212dc8-05af-49a0-a8df-a9b033386dad","year":2022},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.240393Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:17956cca9356debac1c38480083480804d73029610366124b1ea1b160a1064b2","observation_id":"d1300f79-ea07-4cb1-9283-1d01b59a0e56","resolution":{"observed_at":"2026-08-06T12:45:56.143365Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.995699Z","title":"Pacilio, et al., Phys","venue":null,"work_id":"4bf05985-e320-4e36-8eb7-e49c22c81f49","year":2022},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.252482Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:d10202ab411e11842dcbb55d8419a747d136da64b6087b43017bd662679ec644","observation_id":"d27b2440-93d0-47fc-96dd-7242320b52cc","resolution":{"observed_at":"2026-08-06T12:45:56.035066Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.868264Z","title":"Bandopadhyay, et al., Class","venue":null,"work_id":"b05d730e-f49e-42e2-82d6-1591c9349b2b","year":2024},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.284299Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:737ab453b82867c6207b0051e4233f0552221e1c614e420bc4d35c226ab56ca9","observation_id":"2635deba-5ff5-4811-aaa9-45d031afb655","resolution":{"observed_at":"2026-08-06T12:45:55.914854Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.730350Z","title":"Finstad, L.V","venue":null,"work_id":"593f15d6-8fdd-4996-a8a7-21161cfb9c2a","year":2023},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.335342Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:ab6d8d71a8882cf977d026864544b5da7b0a4660b3516ed37e327ce5bbd59a48","observation_id":"fa67384c-28ad-406b-9377-3832492b4596","resolution":{"observed_at":"2026-08-06T12:45:55.792828Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.597623Z","title":"Walker,et al., Phys","venue":null,"work_id":"6a93dbf4-5895-43fc-aec1-729fa5392aee","year":2024},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.379714Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:157af39727ed7a23b2a169d62a57f39d088a248308c511346ae650d7cea1e85f","observation_id":"f442b154-454f-44d5-a620-d96088868603","resolution":{"observed_at":"2026-08-06T12:45:55.658247Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.437364Z","title":null,"venue":null,"work_id":"0f4133f5-eb3e-4a44-80c9-f60e6f12f146","year":2026},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.447922Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:50fff79634824683ce77715c3dd14239468c488051365550a227770ae9a4e2de","observation_id":"0b057a87-30a4-4979-b6cf-65b5af5e6527","resolution":{"observed_at":"2026-08-06T12:45:55.510604Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.343387Z","title":"Zhang, B.A","venue":null,"work_id":"419b2c1b-b961-4df6-80cd-930b6091c26d","year":2018},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.504379Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:5cbd74ebe0adba826565f515ca01be060dc128927a4cc4ea41b29379d80fd21c","observation_id":"4da01869-9484-4a09-816a-89e7f7dedca0","resolution":{"observed_at":"2026-08-06T12:45:55.366359Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.191227Z","title":"Xie and B.A","venue":null,"work_id":"048db743-77c0-4f28-ade7-00676df861de","year":2020},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.584357Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:21d2080b52ecc3f914d4cc47b4bab32379b91e1da86d3b75415084c3b95d0b57","observation_id":"aa9a35e2-4c2d-4cbc-a85b-6edc2878c108","resolution":{"observed_at":"2026-08-06T12:45:55.279832Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.121576Z","title":null,"venue":null,"work_id":"1afd0871-fa5c-4c96-b311-021386d47cee","year":2021},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.620109Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:d1ebdf3ecf76a2d8c1761151ea9ebb9d3c4ff40a895f9377ab92eda86db5e313","observation_id":"dc1d7ada-39f8-4124-8a5d-4e7eadc090c6","resolution":{"observed_at":"2026-08-06T12:45:55.137483Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:55.048747Z","title":null,"venue":null,"work_id":"09b5f48b-e396-4b0e-9164-da12611646c3","year":2019},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.667727Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:4bc8e09b3d58106824487def1711d96816aa0fb49fe19d4a720a48c771c73074","observation_id":"a8998591-765f-4dfa-97f4-cae89f7cdef8","resolution":{"observed_at":"2026-08-06T12:45:55.070828Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:53.749595Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.749595Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:e70d98088d340c524a2e464aada5848fc30979661a46c7570a8f2d0c881cfe0a","observation_id":"bd744ab6-af79-4b4e-91fe-f57bc2ff5af0","resolution":{"observed_at":"2026-08-06T12:45:53.749595Z","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":"2026-08-06T12:45:54.968191Z","title":"Margueron, R.H","venue":null,"work_id":"378dfdb8-4a55-4f6d-92e7-a193eeb3c799","year":2018},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.846113Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:7c276828c4ed5c5c7ec126103e82ef442cbfb3783638946985ed070f005df243","observation_id":"127d647e-4123-4082-ae92-82b51a56fafc","resolution":{"observed_at":"2026-08-06T12:45:55.007470Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:54.833109Z","title":null,"venue":null,"work_id":"f6526063-b0d6-4827-b8ef-8111bf9eea39","year":1970},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.886471Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:e57c484b37d56e6026c41c875d010d091e8f62139dc0e32f360051d0072ac267","observation_id":"58ccc1e1-071b-491a-aee0-c48dcab95c63","resolution":{"observed_at":"2026-08-06T12:45:54.871030Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:54.690013Z","title":"Alford, S","venue":null,"work_id":"ce1e4828-992f-4638-bf99-a23bf2960c8c","year":2013},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:53.924962Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:206b972135a711d4349df507b347da6cb9ef5d0cf0e1c335d7764e53d5a1e10d","observation_id":"b8b98b33-943f-4240-9107-7e300e018d6e","resolution":{"observed_at":"2026-08-06T12:45:54.771667Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:54.556137Z","title":"Richter and B","venue":null,"work_id":"8ee70fed-a1cc-40f0-98c6-c21ae5dc738c","year":2023},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:54.023785Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:9c6723d870f2280eb57444f0f2b1399734eb0b8430eb441238a70c67348822ec","observation_id":"2523db6a-6ab7-441d-bdd2-06d18f4368ae","resolution":{"observed_at":"2026-08-06T12:45:54.615497Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:54.456489Z","title":"Lattimer, M","venue":null,"work_id":"ad19e168-68cb-442d-8f28-bc047c87a8f2","year":2007},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:54.093274Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:a7bb2c53efc3ba32743661a61de2b7d0fd16d2b6dacca95b4599382573d38ca0","observation_id":"86e1d1d7-e5b5-43e5-8cbb-c29835083901","resolution":{"observed_at":"2026-08-06T12:45:54.503136Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-06T12:45:54.343399Z","title":null,"venue":null,"work_id":"6a673c77-8e69-45b5-8dae-0f137841b977","year":2025},"citing_paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T12:45:54.139325Z"},"links":{"citing_paper":"/paper/2608.04967"},"observation_digest":"sha256:e3ddc72c6e764e35360f195948b966af02844b89aa69915746820dad102ba1c4","observation_id":"8d82301a-52d2-4a01-b946-140457dc455e","resolution":{"observed_at":"2026-08-06T12:45:54.385704Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.04967","last_updated":"2026-08-05T15:36:56Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T11:10:39.646191Z","submitted_at":"2026-08-05T15:36:56Z","title":"Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii"},"reference_resolution":{"displayed":38,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":12,"verified_exact":0,"verified_fuzzy":26},"total_outbound_references":38},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 38 of 38 outbound references and 0 inbound Pith citation observations for arXiv:2608.04967."}