{"as_of":"2026-08-12T12:20:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f47f05a85c40e959df8dd8d8568faf1d5eb67107411c8fe50b0f10c932a671ed","coverage":[{"denominator":35,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":35,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:59:59.095067Z","state":"measured"},{"denominator":35,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":35,"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/2608.06944/citation-record","integrity":"/paper/2608.06944/integrity","json":"/paper/2608.06944/citation-record.json","paper":"/paper/2608.06944"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:59:59.546380Z","title":null,"venue":null,"work_id":"bed262dc-13ff-45d0-8c3c-e2aae4e7c40d","year":null},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.961348Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:affed6975d17cede0ae5b3aff4a6bbaeb9193d1873cc2cd222e9650afb5c7b05","observation_id":"ade624d7-5b70-4b30-b127-cd2a28ffd6d9","resolution":{"observed_at":"2026-08-10T17:59:59.549670Z","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":"2026-08-10T17:59:59.534935Z","title":"The first is the computation ofCij(τ )from Eq","venue":null,"work_id":"21180aaf-4589-4525-b446-99567bbb5a1c","year":null},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.965963Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:334497c7d879ab875d4997c512b1425cbdc0c80e7a592c76855e289810d507d7","observation_id":"9410eecb-67b9-46bf-952b-e2d13b92c11a","resolution":{"observed_at":"2026-08-10T17:59:59.538889Z","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":"2026-08-10T17:59:59.522197Z","title":"The prior distribution of these parameters is given byπ(Θ, λ|Ma), andp(δt|Ma) is evidence for the modelMa","venue":null,"work_id":"e5e9f9e1-3ff3-41c3-9919-fc4235dd4ab6","year":null},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.970016Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:d5379e2c64049ca3d85873935fabbf2c07680d70be065f7f0f97ed4168be7cf9","observation_id":"441a03ad-5454-48ea-b9f1-4f27a00c1bac","resolution":{"observed_at":"2026-08-10T17:59:59.526915Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"1602.03640","last_updated":"2016-02-11T08:15:32Z","snapshot_observed_at":"2026-07-06T04:45:49.467632Z","submitted_at":"2016-02-11T08:15:32Z","title":"The International Pulsar Timing Array: First Data Release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03640","snapshot_observed_at":"2026-08-10T17:59:58.995822Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.995822Z"},"links":{"cited_paper":"/paper/1602.03640","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:f3de96ccafc1f0b9f107379a8e389c356307daa0822f5806edde161415071bf2","observation_id":"47c43835-8daf-40e0-927e-337b62d2317d","resolution":{"observed_at":"2026-08-10T17:59:58.995822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.02138","last_updated":"2018-12-06T22:50:49Z","snapshot_observed_at":"2026-08-12T12:19:25.369073Z","submitted_at":"2018-09-06T18:00:01Z","title":"Massive BH Binaries as Periodically-Variable AGN","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.02138","snapshot_observed_at":"2026-08-10T17:59:58.999747Z","title":"Z.Kelley, Z.Haiman, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.999747Z"},"links":{"cited_paper":"/paper/1809.02138","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:95fd04bc1b80003dba91265f4296a18538ceee98a3a5200c14e8d976015933d0","observation_id":"3f64a13a-eae3-4d6c-a1a6-512fa9a98fe8","resolution":{"observed_at":"2026-08-10T17:59:58.999747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16214","last_updated":"2023-06-28T13:51:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-06-28T13:51:02Z","title":"The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16214","snapshot_observed_at":"2026-08-10T17:59:58.983533Z","title":"Antoniadiset al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.983533Z"},"links":{"cited_paper":"/paper/2306.16214","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:237a14f03e53638ba3b5cf285c6a18d7de3ed72382ed076da8d0467c70b7a6f7","observation_id":"0a39991a-efe1-484a-a087-6521ce6914b5","resolution":{"observed_at":"2026-08-10T17:59:58.983533Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16213","last_updated":"2023-06-28T13:51:01Z","snapshot_observed_at":"2026-08-06T22:50:08.228581Z","submitted_at":"2023-06-28T13:51:01Z","title":"The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16213","snapshot_observed_at":"2026-08-10T17:59:58.987797Z","title":"Agazieet al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.987797Z"},"links":{"cited_paper":"/paper/2306.16213","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:b24e6201e30cfa407794bcd3a7cdadc1dc532283a51da9b684bbf37abfae31c6","observation_id":"d68985dd-5cb4-41a2-b8ac-7350940e341a","resolution":{"observed_at":"2026-08-10T17:59:58.987797Z","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":"2026-08-10T17:59:59.510367Z","title":"curse of dimensionality","venue":null,"work_id":"6a402881-31df-4b48-aa6a-98be940c96e5","year":null},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.974937Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:6907d42cb9a55e65ae280139a0fb8095aa2830326f35296cc22d7f83e1544f70","observation_id":"c3c955ac-c399-4cc6-9492-6579ed3f0a84","resolution":{"observed_at":"2026-08-10T17:59:59.514355Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2306.16215","last_updated":"2023-06-28T13:51:03Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-06-28T13:51:03Z","title":"Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16215","snapshot_observed_at":"2026-08-10T17:59:58.991925Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.991925Z"},"links":{"cited_paper":"/paper/2306.16215","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:26c08b7f4c8fdad5b27d888bf458bd972918e9190d3d6ff0c2e11225b7a70009","observation_id":"cdafdfc7-5517-4082-a004-9640eda4a1ff","resolution":{"observed_at":"2026-08-10T17:59:58.991925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.08857","last_updated":"2024-05-14T18:00:00Z","snapshot_observed_at":"2026-07-06T18:14:20.889736Z","submitted_at":"2024-05-14T18:00:00Z","title":"Rapid parameter estimation for pulsar-timing-array datasets with variational inference and normalizing flows","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.08857","snapshot_observed_at":"2026-08-10T17:59:59.017396Z","title":"Vallisneri, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.017396Z"},"links":{"cited_paper":"/paper/2405.08857","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:e493b754fd72315c71eea54616d7be086ff4b6f687ab94fae1027ff2cbc1bbc2","observation_id":"b2a660d6-5e62-4fd7-b67c-6e1e9f4c6cad","resolution":{"observed_at":"2026-08-10T17:59:59.017396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.04803","last_updated":"2015-06-22T13:00:29Z","snapshot_observed_at":"2026-08-06T01:44:53.092111Z","submitted_at":"2015-03-16T20:00:12Z","title":"Expected properties of the first gravitational wave signal detected with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.04803","snapshot_observed_at":"2026-08-10T17:59:59.003082Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.003082Z"},"links":{"cited_paper":"/paper/1503.04803","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:51abfc98bd06f0104325532a0ac2624d2ace74bcc9678751baf8a0e85aa0e90f","observation_id":"011e6758-9789-48d1-9098-87cd1b49dc3b","resolution":{"observed_at":"2026-08-10T17:59:59.003082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.12078","last_updated":"2024-07-16T18:00:00Z","snapshot_observed_at":"2026-07-06T18:47:25.751118Z","submitted_at":"2024-07-16T18:00:00Z","title":"Resolving the nano-Hz gravitational wave sky: the detectability of eccentric binaries with PTA experiments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.12078","snapshot_observed_at":"2026-08-10T17:59:59.006968Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.006968Z"},"links":{"cited_paper":"/paper/2407.12078","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:293d3bfc2f971fbeb424b09d57e5c4bd01ffde2ebc356b4ef552e3eaff6d646f","observation_id":"c29f2cc3-9e84-4786-9e09-774a5e02e741","resolution":{"observed_at":"2026-08-10T17:59:59.006968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01074","last_updated":"2025-04-01T18:00:02Z","snapshot_observed_at":"2026-08-12T10:13:43.668860Z","submitted_at":"2025-04-01T18:00:02Z","title":"Lighting up the nano-hertz gravitational wave sky: opportunities and challenges of multimessenger astronomy with PTA experiments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01074","snapshot_observed_at":"2026-08-10T17:59:59.010343Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.010343Z"},"links":{"cited_paper":"/paper/2504.01074","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:db9d78f522cee76ff866bf70eee033293e6b3a6d1e263ddb9dd75af4ada943e3","observation_id":"b098f40d-3a59-48e0-bbde-a67122730f62","resolution":{"observed_at":"2026-08-10T17:59:59.010343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:59:59.013764Z","title":"Manzini and S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.013764Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:721b688f5eba9148d1cdf42497c253fb648a9a5f491a69a77ea3bf0f3c5b930d","observation_id":"285551b9-5047-4d06-b575-e32b124630cf","resolution":{"observed_at":"2026-08-10T17:59:59.013764Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.05570","last_updated":"2016-02-16T21:17:21Z","snapshot_observed_at":"2026-07-06T04:46:31.221295Z","submitted_at":"2016-02-16T21:17:21Z","title":"From Spin Noise to Systematics: Stochastic Processes in the First International Pulsar Timing Array Data Release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.05570","snapshot_observed_at":"2026-08-10T17:59:59.034385Z","title":"Lentatiet al., Mon","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.034385Z"},"links":{"cited_paper":"/paper/1602.05570","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:8afaa2ebc5ac74d7cbb77583d0191fb716a7ddc4b157cca7250746d161b6c224","observation_id":"7340276a-e783-4b4c-b9e6-261b5da1d5c9","resolution":{"observed_at":"2026-08-10T17:59:59.034385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.5932","last_updated":"2012-10-02T19:41:12Z","snapshot_observed_at":"2026-08-10T08:25:18.158483Z","submitted_at":"2012-02-27T13:38:37Z","title":"Understanding and analysing time-correlated stochastic signals in pulsar timing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.5932","snapshot_observed_at":"2026-08-10T17:59:59.021435Z","title":"van Haasteren and Y","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.021435Z"},"links":{"cited_paper":"/paper/1202.5932","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:2568f04c7f938181d60f4c1dac17926af50bd77429c4ccd3ab59d2b5a0403c91","observation_id":"adfedf6d-9ca1-416a-a8af-b7f63acce5a7","resolution":{"observed_at":"2026-08-10T17:59:59.021435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.05186","last_updated":"2021-11-09T14:55:37Z","snapshot_observed_at":"2026-07-06T12:06:55.554120Z","submitted_at":"2021-11-09T14:55:37Z","title":"Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search","version":1},"cited_work":{"arxiv_id":"2111.05186","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.05186","snapshot_observed_at":"2026-08-10T17:59:59.252000Z","title":"Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search","venue":"astro-ph.HE","work_id":"fd123352-d96f-4e82-85b5-db9896217385","year":2021},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.025434Z"},"links":{"cited_paper":"/paper/2111.05186","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:5d125730451c7394740c786ed5bc179eef66fe6741ae2d9659d06e88850dec25","observation_id":"c629d1ac-c6b4-4310-aad2-62e55308379b","resolution":{"observed_at":"2026-08-10T17:59:59.256364Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2026-08-10T17:59:59.030145Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.030145Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:ab599252c3016958e4d63e7cfe88b970a9c1331f482d87a142b3cf58cc0806f2","observation_id":"7e5c80c0-24e1-4249-ada8-9a8feb3567ad","resolution":{"observed_at":"2026-08-10T17:59:59.030145Z","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":"2026-08-10T17:59:59.480146Z","title":null,"venue":null,"work_id":"64e83be9-3d36-40f4-a7b4-c78285681dbe","year":2025},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.050183Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:1c818578cb9319981a2a764a1b2c836982bfe9701320953e6cf041a0a196b33c","observation_id":"c88a32ff-c98b-4f02-ac39-3facbf8bd7ec","resolution":{"observed_at":"2026-08-10T17:59:59.483819Z","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":{"arxiv_id":"1210.3578","last_updated":"2013-06-25T17:37:17Z","snapshot_observed_at":"2026-07-06T02:57:32.294251Z","submitted_at":"2012-10-12T17:14:19Z","title":"Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.3578","snapshot_observed_at":"2026-08-10T17:59:59.038401Z","title":"Lentati, P","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.038401Z"},"links":{"cited_paper":"/paper/1210.3578","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:b35561194c0cf5afb93834ffcfcdd793c49c80fe37cff9757856b2a4b3aa7933","observation_id":"efe9cc4a-4296-43ce-ac4c-d067cf6a2166","resolution":{"observed_at":"2026-08-10T17:59:59.038401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.1838","last_updated":"2014-07-07T20:00:02Z","snapshot_observed_at":"2026-08-02T07:31:17.236153Z","submitted_at":"2014-07-07T20:00:02Z","title":"New advances in the Gaussian-process approach to pulsar-timing data analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.1838","snapshot_observed_at":"2026-08-10T17:59:59.042121Z","title":"van Haasteren and M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.042121Z"},"links":{"cited_paper":"/paper/1407.1838","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:a1f4d457d09d8988e2d18eff60fe3901f55dbea821f33556066f1cb1f82dd620","observation_id":"990cf1d5-2d3e-41d7-94e4-ee9adad8ed76","resolution":{"observed_at":"2026-08-10T17:59:59.042121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.13866","last_updated":"2025-06-16T18:00:02Z","snapshot_observed_at":"2026-08-08T06:40:10.083757Z","submitted_at":"2025-06-16T18:00:02Z","title":"Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.13866","snapshot_observed_at":"2026-08-10T17:59:59.046390Z","title":"Crisostomi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.046390Z"},"links":{"cited_paper":"/paper/2506.13866","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:c00c83410a289c325f1b590cf7d7a2f9528a477a3d1106c687cfa5adba062a8a","observation_id":"aca9b29f-73d7-41de-9391-9dfd0a0d6b77","resolution":{"observed_at":"2026-08-10T17:59:59.046390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.02164","last_updated":"2023-10-10T06:42:20Z","snapshot_observed_at":"2026-07-06T14:58:29.603807Z","submitted_at":"2023-03-03T12:45:03Z","title":"Eryn : A multi-purpose sampler for Bayesian inference","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.02164","snapshot_observed_at":"2026-08-10T17:59:59.065658Z","title":"Karnesis, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.065658Z"},"links":{"cited_paper":"/paper/2303.02164","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:166ab6d8265f14397f7a5acac6fad2e5ccad46e95595664df84d671ae60b75e2","observation_id":"11f02327-31ce-432d-b926-5a043a62d59c","resolution":{"observed_at":"2026-08-10T17:59:59.065658Z","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":"2026-08-10T17:59:59.468536Z","title":"Ivezić, A","venue":null,"work_id":"43921c3d-6a89-441e-9fa3-6a1d59b1f5a4","year":2014},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.054168Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:59453df19f8849a11a9fd54794b11ab39123420b9286895202cd722ac1a7239f","observation_id":"4fb26758-ea21-4dfe-8d53-e9ac1443fca9","resolution":{"observed_at":"2026-08-10T17:59:59.472784Z","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":"2026-08-10T17:59:59.058006Z","title":"Skilling, AIP Conf","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.058006Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:0f9a13edcd142e16bd0158e2f03fd27c9fd61217f8dccf63926ebccf6fc00621","observation_id":"e95f49aa-e161-41c4-9a70-2858e099033c","resolution":{"observed_at":"2026-08-10T17:59:59.058006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03673","last_updated":"2023-01-09T20:48:27Z","snapshot_observed_at":"2026-07-06T14:39:46.284351Z","submitted_at":"2023-01-09T20:48:27Z","title":"Prototype Global Analysis of LISA Data with Multiple Source Types","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03673","snapshot_observed_at":"2026-08-10T17:59:59.061885Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.061885Z"},"links":{"cited_paper":"/paper/2301.03673","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:10b01c491a93f7cb392eeb8a721f9bbed48490e2560de7d48b40a38f10b96274","observation_id":"09fa1c1f-18aa-4e73-9c67-083cea93f9cf","resolution":{"observed_at":"2026-08-10T17:59:59.061885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.03201","last_updated":"2022-11-06T19:00:00Z","snapshot_observed_at":"2026-08-10T20:14:19.092656Z","submitted_at":"2022-11-06T19:00:00Z","title":"Quality over Quantity: Optimizing pulsar timing array analysis for stochastic and continuous gravitational wave signals","version":1},"cited_work":{"arxiv_id":"2211.03201","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.03201","snapshot_observed_at":"2026-08-10T17:59:59.153035Z","title":"Quality over Quantity: Optimizing pulsar timing array analysis for stochastic and continuous gravitational wave signals","venue":"astro-ph.HE","work_id":"6a862756-6249-41ed-9275-cd25c14e91ea","year":2022},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.081164Z"},"links":{"cited_paper":"/paper/2211.03201","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:822b40830b4815f5f0e756efebba9a52defd508dee69f4737789c53c2f7bcf71","observation_id":"c9f8083e-16b1-4c5a-82a7-2170a152d1ed","resolution":{"observed_at":"2026-08-10T17:59:59.158073Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1506.09024","last_updated":"2017-01-25T17:35:26Z","snapshot_observed_at":"2026-07-06T04:22:25.279032Z","submitted_at":"2015-06-30T10:45:24Z","title":"Bayesian model selection without evidences: application to the dark energy equation-of-state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.09024","snapshot_observed_at":"2026-08-10T17:59:59.069699Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.069699Z"},"links":{"cited_paper":"/paper/1506.09024","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:ff50123b2983f5597357fa893166f670f2be3582e4df04c6f27c45faeb66c904","observation_id":"748fa164-28cb-4fef-ac1b-21491aa2f16a","resolution":{"observed_at":"2026-08-10T17:59:59.069699Z","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":"2026-08-10T17:59:59.449802Z","title":"Bartolucci, L","venue":null,"work_id":"6d02afa2-14ba-4e5f-a3b0-19507c0fc5c8","year":2006},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.073421Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:370dace2719582ce6220b539a775752c721f6349b9809f4973975977fc632c97","observation_id":"af9a08f7-0e5c-415b-a9f3-9fb77e8c64b2","resolution":{"observed_at":"2026-08-10T17:59:59.453857Z","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":"2026-08-10T17:59:59.498326Z","title":"We define these two metrics in the Appendix A","venue":null,"work_id":"03b13a87-f522-40a4-83a7-be39026e7a91","year":null},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:58.979225Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:73eb2e5204bbd4885584c3391a5db0850c1742327ba68cff247b93134b6398ef","observation_id":"b2a54916-8afc-45f5-83d3-9997941bb31e","resolution":{"observed_at":"2026-08-10T17:59:59.502290Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2110.13184","last_updated":"2021-10-25T18:06:21Z","snapshot_observed_at":"2026-08-10T14:04:57.616932Z","submitted_at":"2021-10-25T18:06:21Z","title":"Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: Inferences in the stochastic gravitational-wave background search","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.13184","snapshot_observed_at":"2026-08-10T17:59:59.077347Z","title":"Chenet al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.077347Z"},"links":{"cited_paper":"/paper/2110.13184","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:b8f2cd0e84c576340f389345800a61a1c2b6dbf02c673db47db53cf186242c72","observation_id":"91e2d176-ce0a-4895-afc9-990cc983cd4d","resolution":{"observed_at":"2026-08-10T17:59:59.077347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16224","last_updated":"2023-06-28T13:51:12Z","snapshot_observed_at":"2026-08-10T20:43:56.896435Z","submitted_at":"2023-06-28T13:51:12Z","title":"The second data release from the European Pulsar Timing Array I. The dataset and timing analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16224","snapshot_observed_at":"2026-08-10T17:59:59.085126Z","title":"Antoniadiset al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.085126Z"},"links":{"cited_paper":"/paper/2306.16224","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:f425882fe6f6951ba08a3b3ccc3faca70d11817267597f49aee03fdca1b6b132","observation_id":"ab348652-fc20-4de0-9e8e-b1ca3350e842","resolution":{"observed_at":"2026-08-10T17:59:59.085126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13701","last_updated":"2024-02-21T11:04:30Z","snapshot_observed_at":"2026-08-11T02:00:38.162131Z","submitted_at":"2024-02-21T11:04:30Z","title":"Neural density estimation for Galactic Binaries in LISA data analysis","version":1},"cited_work":{"arxiv_id":"2402.13701","doi":null,"metadata_source":"pith","pith_arxiv_id":"2402.13701","snapshot_observed_at":"2026-08-10T17:59:59.125605Z","title":"Neural density estimation for Galactic Binaries in LISA data analysis","venue":"gr-qc","work_id":"c5c91ae5-f5c6-4471-8023-03bea08556e0","year":2024},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.089020Z"},"links":{"cited_paper":"/paper/2402.13701","citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:4d951de4e648b017eba3e7e473bb47804f98520a75e4a4ef096694910a30d0f0","observation_id":"4ba45537-7718-41c1-ba44-aa91b1013a95","resolution":{"observed_at":"2026-08-10T17:59:59.131597Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2026-08-10T17:59:59.437414Z","title":"Bhattacharyya, Bull","venue":null,"work_id":"0703d416-476f-4a92-b9f9-23ff3e161fad","year":1943},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.092192Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:1dadddcd898513a6e5a88345081c182fed06f475db1cf4abd21410862ce766fe","observation_id":"75d3519d-fee4-4068-b886-d991b110e0e5","resolution":{"observed_at":"2026-08-10T17:59:59.441799Z","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":"2026-08-10T17:59:59.095067Z","title":"Lin, IEEE Trans","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T17:59:59.095067Z"},"links":{"citing_paper":"/paper/2608.06944"},"observation_digest":"sha256:a757f70bd5f26273f89c218b03163604953888245f8b28f612785b77527d2c71","observation_id":"52013348-5197-4444-b5b3-a8ae8e0498cb","resolution":{"observed_at":"2026-08-10T17:59:59.095067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.06944","last_updated":"2026-08-07T08:22:23Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-12T12:12:03.380586Z","submitted_at":"2026-08-07T08:22:23Z","title":"Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays"},"reference_resolution":{"displayed":35,"state_counts":{"malformed_identifier":3,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":25,"verified_exact":3,"verified_fuzzy":4},"total_outbound_references":35},"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 35 of 35 outbound references and 0 inbound Pith citation observations for arXiv:2608.06944."}