{"as_of":"2026-08-14T19:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cef639dfba7512db535b74e8f6d5c0d818a0581a1f65f217d6a77790f5fb8096","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":"2026-08-14T06:32:32.682623+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":"sha256:68a2c3ff09dff86a4af1330aa5772d85ae2f8417e95f017d647a1d9c6e6b6ad0","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:a85aa5a6c4458d1e6e2bc0895dc49a419b8668a990954e2e3e50347e2765459d","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:0f6a121bda377c7ec6b9e3e6368402fabbbfc3e3f31c7805d6e32d19e097e775","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:1fca8a191e511e8b3e8b7d956e18dcc6b4238e9bbb3755fb7729c59eeea3ac12","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:2dc464f2caf1cdbae0a7689c324d4932b85fe485789f62d6dcd17ab0110bb4b1","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:c28af4ce6dbf8f4496687263fc6c845bd0f8ee0b7132b7148ccb105b9dda1e84","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:93f24bae306ed9ac9588c051092bd0fe1cd1199886dd496bb506f49be821fb18","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:4282ba212bb3efb391932deb362735190b965b50f3ebee907587fbc682be61a0","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:d04da804689e442e24a7a231f64908bd56bc01fc39d5dba0f279437c4b4135a9","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:c0a681a74f9a38c816c89563a81a74288ffbea6564aec8325be615fd3af1b97e","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:543503929fdc33d0df6f3ea7b05abe952f1094cb8b4191ca8a71bea7a6a24450","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:554b5b653698235d7798d2ccdf7b70d19583e619760b0cbf269fe08d37f8f61e","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:324915c2af8246bec8fafb1f215b69eda38df3ca4e643d663dcd7c1f9c8010f6","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:f384d91b305ba504899ffbe98f34fda1b4d68a9b7e13436e886f533bb38cd0cc","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:7b25494bfd9b7ad7c1dd82e473ff1984679774d743527cbc8ec98e0d218ab786","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:531680d6bf722b9c1ade181e66917c474c325bf8068ccee922199b920b5d7613","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:530ca5720ab5f42df359bc15276fc7a61e773102703a1eb59373e4e6c1fa6451","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":"sha256:85097778981e63a62ef4875741c17c86f69e2d251b1ceed62468d0c461711ab6","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:594ade89bab2b8745ad170d265da0c472041a6b8147488079d4855c9e24b258b","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:bbc1ac673a8bc5388df0a67ddba8de1f9061460727daaaeee46a7dd92368e8f7","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:5da9550d2d040e45dadc95ad573d5e5a9c853409bade2c877d6cf687e5664527","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:23d0a597b6e34bf877ad60416475cca416e604f67a5f26d58c8c6a889885062d","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:f668aae08c13b6f66ef13f60a8cff636d31c894ceb8aeb0c4d7cd041c25f615a","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:83fb231926c8f7263c17c57ebae1d34e9ec74e9899673c667a0ebdd2476c9664","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:ad189e9e80d9ffa78eba7a0e91af3d835f22bb4b87390c2ea09284961ebbf22f","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:cf616c9fe101dbc2f833b7de7c998cf6d26b3c58bd5ce754a9ba7c553c822d3a","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:5c0c700ca7d6bfb1365d13f8d91a60f91d59c45c63e8fb2013f85049bd47e40e","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:f7993bc907718cfee297df394b6e684cb365c3b7ff3f5a87e895521ddabbb670","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:4d867a1077f549b00057ae08d7fbe1bfbdeb8ca0a4e0380789b548d7913ae592","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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":"sha256:288a2084de2a6ec594fa333a85d15b4b5b276a8310c6f1e0138ac594b92fe983","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:ca7bccdc31ca2fcc8c22c219fb7678bcf42321cf6e31d18cc1c402f8502cd182","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:e453ccd58360c4937600d4fc6415a0fa38868d755169205806bd65c99c4de439","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":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:e75b95ed4cc76320c58c1b1075c53ccd39d0603135ee8b54ad84481f9a4a9e17","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 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 38 of 38 outbound references and 0 inbound Pith citation observations for arXiv:2608.04967."}