{"as_of":"2026-08-11T05:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:98a3db2d83820f317c23ab8ccc770bbaadacb4eab6e3cb9b95c28497d5fda3ca","coverage":[{"denominator":47,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":47,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T11:57:57.023960Z","state":"measured"},{"denominator":47,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":47,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.22297/citation-record","integrity":"/paper/2507.22297/integrity","json":"/paper/2507.22297/citation-record.json","paper":"/paper/2507.22297"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1902.10103","last_updated":"2019-02-26T18:31:17Z","snapshot_observed_at":"2026-08-03T18:23:59.553463Z","submitted_at":"2019-02-26T18:31:17Z","title":"The Planet Nine Hypothesis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10103","snapshot_observed_at":"2026-08-06T11:57:56.763579Z","title":"Batygin, K., Brown M.,","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.763579Z"},"links":{"cited_paper":"/paper/1902.10103","citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:84dc5d937a1a37cf2775409b603e3478e73cfebbeaf17249f109b5831f813d23","observation_id":"55644519-e806-4b1b-98e0-91cf2d35afe9","resolution":{"observed_at":"2026-08-06T11:57:56.763579Z","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":"2026-08-06T11:57:56.887556Z","title":"Lopez, E., Fortney, J.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.887556Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:4f016058489fda87d0d85f5014e2e8d0760e60826be6d7e6d6985f66ed82a1f7","observation_id":"9604c028-d6d8-4223-bf30-9a041c23e6a5","resolution":{"observed_at":"2026-08-06T11:57:56.887556Z","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":"2026-08-06T11:57:56.774879Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.774879Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:209d28034a250c0d31ee6d4ea04c4e2f9342e00b467a1d0d80f0ae6607c6846c","observation_id":"e8372d60-3728-489e-8d31-cfec89736afe","resolution":{"observed_at":"2026-08-06T11:57:56.774879Z","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":"2026-08-06T11:57:56.790126Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.790126Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:e8c099edffc076787d434c959f7220e1430f94802643f0ecbac493694aeab316","observation_id":"205f7dce-4510-4301-a73e-d43480baae4b","resolution":{"observed_at":"2026-08-06T11:57:56.790126Z","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":"2026-08-06T11:57:56.816670Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.816670Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:37b8c53437fb4e6c205a189c037c91d362294b5ebce81c268206ce1d579f88c4","observation_id":"8ee6c6ca-8503-4e51-9104-dacca15ba6cd","resolution":{"observed_at":"2026-08-06T11:57:56.816670Z","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":"2026-08-06T11:57:56.821206Z","title":"https://doi.org/10.1051/0004-6361/202244056","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.821206Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:94c0d113322916b7914590ea46fcc011f988faaf4fbf331240b0f46dacf36cf6","observation_id":"fcdd8e32-2c72-410b-880d-eadeee40f494","resolution":{"observed_at":"2026-08-06T11:57:56.821206Z","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":"10.1016/j.icarus.2016.09.023","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Mallorquín et al.,","venue":"Icarus","work_id":"abed9834-3e75-411a-a447-04aad8bc1943","year":2016},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.904233Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:d08c6d374c4667d9069683ec26ff35b5fa0be3290e97e145586946be03460fe6","observation_id":"a0dfdee2-e6c4-4b59-bcc9-30eb4ee973b0","resolution":{"observed_at":"2026-08-06T11:57:57.278372Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-06T11:57:56.769938Z","title":"Batygin, K., Morbidelli, A., Brown, M., Nesvorný, D.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.769938Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:26ca7db68037e4f2a90ca32b604c1e1804af96bb98516591efffc39ca7ad393c","observation_id":"6a91021f-4a16-4b6d-b6d1-c2dbd784b8ca","resolution":{"observed_at":"2026-08-06T11:57:56.769938Z","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":"2026-08-06T11:57:56.878462Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.878462Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:35a86ff2a6d0de627fef2495ee9162874ecd87a0af9f9f0a7368ff69de34800a","observation_id":"0763652e-01a5-4501-ab5e-c4d5b4239b1e","resolution":{"observed_at":"2026-08-06T11:57:56.878462Z","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":"2026-08-06T11:57:56.882995Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.882995Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:b75139391df0515b93954df02844055cbf8c19ecf009e9427a867b99946b4328","observation_id":"75893d0e-79dd-44df-b94b-7912e4ff0c63","resolution":{"observed_at":"2026-08-06T11:57:56.882995Z","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":"2026-08-06T11:57:56.892663Z","title":"Mahajan, Eastman and Kirk,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.892663Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:4d09a2944267772e575e10bcafee128deea15477f25231dfa619e278b2bcfb96","observation_id":"09a2906a-4455-4eb0-80fd-b8b4aa2d5acf","resolution":{"observed_at":"2026-08-06T11:57:56.892663Z","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":"2026-08-06T11:57:56.898809Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.898809Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:05b6a1cba8ae413328c4293076e60c135b465a230081e6b455d8acbcf9cf1cdd","observation_id":"073d8d30-74cf-40d6-9d85-6d7a68bc68be","resolution":{"observed_at":"2026-08-06T11:57:56.898809Z","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":"2026-08-06T11:57:56.910092Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.910092Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:359fdceede4565a2320517e56b65e5ac0f95ab782d7c739fcc06587cf0f75cfd","observation_id":"04a36782-4b1e-475a-8bcc-1efd4e181bb4","resolution":{"observed_at":"2026-08-06T11:57:56.910092Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-06T11:57:56.920995Z","title":"An inner eccentric sub-Neptune and an outer sub-Neptune-mass candidate around BD+00 444 (TOI-2443)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.920995Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:1c221daba2129e0cfef3c8a75ddb1799dd6d21f6ca2223e5d6509f2499b933d7","observation_id":"dbe1be0b-04cc-41da-85c8-53db4693e20f","resolution":{"observed_at":"2026-08-06T11:57:56.920995Z","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":"2026-08-06T11:57:56.937689Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.937689Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:eebf9a00b6124bf929c730d97dab3e33c79e4f8a3b5b5d4d2cfa7469ee5b43bc","observation_id":"ea0deadc-8a1c-4284-a159-20c70b8e2e8a","resolution":{"observed_at":"2026-08-06T11:57:56.937689Z","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":"2026-08-06T11:57:56.932323Z","title":"Orell-Miquel et al.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.932323Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:5082bce8d610b2ce0454a890d0e8ccb1169ee07e6b7a8b4f515a794c5d60d6f4","observation_id":"485afb2c-f0d9-4096-900c-ca7b8d3beb46","resolution":{"observed_at":"2026-08-06T11:57:56.932323Z","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":"2026-08-06T11:57:56.944173Z","title":"https://doi.org/10.1051/0004-6361/201936482","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.944173Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:fa6de9410fa383b8c2614b62962e9dbfb96d2a167ec252dd7333206cb23b2e82","observation_id":"9a405326-486f-4f50-8c28-879a73b5e35b","resolution":{"observed_at":"2026-08-06T11:57:56.944173Z","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":"2026-08-06T11:57:56.950135Z","title":"https://doi.org/10.1051/0004-6361/202449911","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.950135Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:be76443d847062378a467a581ab1c67ca793c5ea233c7c254596b133ef3ed16b","observation_id":"0ec9d7a5-bdf5-4749-96fe-328cfef184b7","resolution":{"observed_at":"2026-08-06T11:57:56.950135Z","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":"2026-08-06T11:57:56.973101Z","title":"https://doi.org/10.2458/azu_uapress_9780816540068","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.973101Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:b776c4d78ee363798c2529269e4773b7d472422379ec4cc5e37810ecfaea6345","observation_id":"43d47aa0-d727-482d-a478-0384b5a627ae","resolution":{"observed_at":"2026-08-06T11:57:56.973101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.06214","last_updated":"2023-03-10T21:28:53Z","snapshot_observed_at":"2026-07-06T15:01:30.019542Z","submitted_at":"2023-03-10T21:28:53Z","title":"A Catalog of Exoplanets with Equilibrium Temperature less than 600 K","version":1},"cited_work":{"arxiv_id":"2303.06214","doi":"10.48550/arxiv.2303.06214","metadata_source":"pith","pith_arxiv_id":"2303.06214","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"A Catalog of Exoplanets with Equilibrium Temperature less than 600 K","venue":"astro-ph.EP","work_id":"eafaef1c-60fd-45fc-95f7-ed4139fe0a00","year":2023},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.978912Z"},"links":{"cited_paper":"/paper/2303.06214","citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:386fe325a0210abaf7c8381af096c738eb6b3cf4e4a96fb9f9321e342965826c","observation_id":"bfd52b4b-ea5d-4363-87c2-e3fafdb71ca4","resolution":{"observed_at":"2026-08-06T11:57:57.146932Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-3881/ac8553","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Goffo et al.,","venue":"The Astronomical Journal","work_id":"249d6c3c-4ac8-49ae-ba95-1c47460771fe","year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.857382Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:f96219e30c295af1f973d60881120950814cca73c6924fed7d307b2e87149450","observation_id":"6f45fc05-5152-4a67-a2fa-0ec5a32287f1","resolution":{"observed_at":"2026-08-06T11:57:57.406486Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-06T11:57:57.012121Z","title":"https://doi.org/10.3847/0004-637X/819/2/127","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:57.012121Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:2c7a5c7b5ed1c69a2ebc175c3472df8b29c80324b2f68ca5d03d18293bf33152","observation_id":"ec75c0f0-0085-44c6-95cb-8f0634bbde85","resolution":{"observed_at":"2026-08-06T11:57:57.012121Z","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":"2026-08-06T11:57:57.018441Z","title":"https://doi.org/10.1073/pnas.1812905116","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:57.018441Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:81fff61b71f0f1fe46ed6464d1b515b05564d01ef255d4dc0bf0ed55bbf54e6e","observation_id":"4e33bad5-867b-43fa-a4ba-cff37c0ea871","resolution":{"observed_at":"2026-08-06T11:57:57.018441Z","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":"2026-08-06T11:57:57.023960Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:57.023960Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:62dd4fca3686a85170ea31be7f63ac9ab07ac650e2c7cd6517ef131c063f1369","observation_id":"a37641c0-1bf0-42d9-8875-861cd0c1790b","resolution":{"observed_at":"2026-08-06T11:57:57.023960Z","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":"10.3847/psj/ad2201","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Raymond S., Izidoro, A., Morbidelli, A.,","venue":"The Planetary Science Journal","work_id":"0fee440f-2546-40d6-a414-d4af4b4382dd","year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.967499Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:4ad4f44dacf2e9147e9f46663ad6c0382b5ef45487d5b22f74daf55536dcae7c","observation_id":"5c9251ad-2c4d-481f-b070-2f3fba529568","resolution":{"observed_at":"2026-08-06T11:57:57.181056Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-06T11:57:56.842473Z","title":"Delraz et al.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.842473Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:ab6eff5ecd95643df0eb290479116aba0e7a0f089cbbc69fa627658a77c84cd3","observation_id":"7a9c4cf5-735f-402d-87af-c404c8dea647","resolution":{"observed_at":"2026-08-06T11:57:56.842473Z","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":"10.3847/1538-3881/ac32ddhttps://doi.org/10.3847/1538-3881/ac32dd","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T11:57:57.601902Z","title":"Brown, M.,","venue":null,"work_id":"8dd729e3-0839-4e00-ae0e-3fe98fe00638","year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.802241Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:adb2bea7cf4858a8526ae30bfc5253113b0d91e92b83233d9324291f3d925bc4","observation_id":"5eef24a6-0784-4f54-86ee-4ffbb20738e3","resolution":{"observed_at":"2026-08-06T11:57:57.606842Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abc87a","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Zeng, L., Sasselov, D., Jacobsen, S.,","venue":"The Astrophysical Journal","work_id":"8e37d47c-82ba-4097-9289-58e07aecc9f3","year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.998312Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:169014c3b07926258697b4f37550867c1aac522017c6ed9dcc06f6c9d7d9efc4","observation_id":"7790f60b-5407-4c3f-82ef-29d8a4425a7f","resolution":{"observed_at":"2026-08-06T11:57:57.105771Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-06T11:57:56.865656Z","title":"Hasegawa, Y.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.865656Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:d0ffb15d852eaa0ca503bec5844cccfe4bc7e631b3627d75dbe149193929a67f","observation_id":"49568bd7-d415-4bde-939e-a1674d5524f6","resolution":{"observed_at":"2026-08-06T11:57:56.865656Z","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":"2026-08-06T11:57:56.812365Z","title":"Cadieux et al.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":146,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.812365Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:53b985b2315c051cd53f48aa7e7212ed50d3ecec2d14d912e945cd27c4bf8060","observation_id":"ef4abae1-c1c3-4910-baf5-f8cb4df7a07a","resolution":{"observed_at":"2026-08-06T11:57:56.812365Z","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":"2026-08-06T11:57:56.853127Z","title":"Greklek-McKeon et al.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":172,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.853127Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:d6a559e9452957b245b5579c5eab77174e8c13e7b731b4b6acd0455e5c76ce99","observation_id":"2794c2ca-9981-448e-9e22-4b88c09d8ec5","resolution":{"observed_at":"2026-08-06T11:57:56.853127Z","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":"2026-08-06T11:57:56.779763Z","title":"Benneke et al.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":216,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.779763Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:8ac04cc091328f9e04dc14400d40ce6403e6dc03b3c21b35e6155335842219ea","observation_id":"4c68c390-9389-456c-b309-094d99e2018f","resolution":{"observed_at":"2026-08-06T11:57:56.779763Z","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":"2026-08-06T11:57:56.797746Z","title":"Brown, M., Batygin, K.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":219,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.797746Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:9c3f2ecfeacc464bd17527dbb1b1b24fde58638f3984354d4221f7e7266dbf10","observation_id":"06a28b75-8ee5-4cff-a363-abd90ee50f00","resolution":{"observed_at":"2026-08-06T11:57:56.797746Z","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":"2026-08-06T11:57:56.874097Z","title":"JWST / NIRISS, JWST Near Infrared Imager and Slitless Spectrograph","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":388,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.874097Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:c57bc823b88f32b1433720de1538fb5a692c37c32f47ce3d522c578fd03d9ad5","observation_id":"1d27df79-21ca-4e00-9b52-a5cc381b6151","resolution":{"observed_at":"2026-08-06T11:57:56.874097Z","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":"2026-08-06T11:57:56.955866Z","title":"Pollack, J., Hubickyj, O., Bodenheimer, P., Lissauer, J., Podolak, M., Greenzweig, Y.,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":701,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.955866Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:b33aaf3f1f4940b6d364ba39ca7646b2ddd25a76ac661086f6b48bc37c9866ae","observation_id":"57c975bf-6d82-4371-8d0d-871e3a53ae85","resolution":{"observed_at":"2026-08-06T11:57:56.955866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.14491","last_updated":"2021-06-28T09:12:15Z","snapshot_observed_at":"2026-08-02T01:53:37.897965Z","submitted_at":"2021-06-28T09:12:15Z","title":"Transit detection of the long-period volatile-rich super-Earth $\\nu^2$ Lupi d with $CHEOPS$","version":1},"cited_work":{"arxiv_id":"2106.14491","doi":"10.48550/arxiv.2106.14491","metadata_source":"pith","pith_arxiv_id":"2106.14491","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Transit detection of the long-period volatile-rich super-Earth $\\nu^2$ Lupi d with $CHEOPS$","venue":"astro-ph.EP","work_id":"6a6f935e-e14d-4991-b58d-06265f8fab15","year":2021},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":775,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.848071Z"},"links":{"cited_paper":"/paper/2106.14491","citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:a8068d342079ad44f338f333a8f9e11f4464330e3814dbe3c4eb9e8d5bdb0e81","observation_id":"d379646c-6ad9-4816-b671-18e413b97f77","resolution":{"observed_at":"2026-08-06T11:57:57.442924Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-06T11:57:56.738076Z","title":"Alessi, M., Inglis, J., Pudritz, R., 2020, Formation of Planetary Populations – III","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":989,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.738076Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:452fd511882700a1c57b0ae545809d1f4fc051e8225a80a5522caf04751076ac","observation_id":"a345f99d-30a4-40ce-a11e-4edd4516a5e5","resolution":{"observed_at":"2026-08-06T11:57:56.738076Z","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":"2026-08-06T11:57:56.961817Z","title":"https://doi.org/10.1006/icar.1996.0190","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":1996,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.961817Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:6fffa9a72effe8973c3a6c13b2b25195805bb2880024606594290ada099ab921","observation_id":"07f6fa23-7630-45bd-bc23-16f0a824e831","resolution":{"observed_at":"2026-08-06T11:57:56.961817Z","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":"2026-08-06T11:57:56.926431Z","title":"An extremely low-density super-Earth mass planet around Kepler-87","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2014,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.926431Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:7b023e03886a7d0f470bbbbd1be2c3349e3e9c1767653f5752266b27f7bddf89","observation_id":"51476d3a-961b-49ec-a19e-7d2a74ea9bab","resolution":{"observed_at":"2026-08-06T11:57:56.926431Z","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":"10.3847/0004-637x/832/1/83","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Astrophys","venue":"The Astrophysical Journal","work_id":"174875d4-999f-4c96-b610-5fe3a63d5899","year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2016,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.869920Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:253fb300d94f4677b2643728f751c51d30cb2912d05da7145b2fdf0d1b7cfdb6","observation_id":"a6447e7c-dd04-462c-9065-61718cf1a279","resolution":{"observed_at":"2026-08-06T11:57:57.369768Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-06T11:57:56.986718Z","title":"https://doi.org/10.3847/1538- 4357/aa961c","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2018,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.986718Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:86276b615b6c14a8233d696d73a0c47259fd598074b2b76849e6a6953c88344a","observation_id":"2b6dc83e-9665-4876-a6d9-a4865fa5c8aa","resolution":{"observed_at":"2026-08-06T11:57:56.986718Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-06T11:57:56.784516Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2019,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.784516Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:b7bcffbbce67ae2a594b075b75afcecabd828dc2a21a4c25ede8a1bd2ed42c37","observation_id":"8c04ff82-6357-4ee9-b96d-18c42d03d6ee","resolution":{"observed_at":"2026-08-06T11:57:56.784516Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-06T11:57:56.754255Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2022,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.754255Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:7014f0b2c4b997dc21cd3a6f6af664db0f74d95c6856ad7b9dbfe0eaa5715d86","observation_id":"6dea7b9d-23e6-46a7-ba1c-2d2774fce3ee","resolution":{"observed_at":"2026-08-06T11:57:56.754255Z","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":"10.22002/8fjad-x7y61","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"CaltechDATA","venue":"CaltechDATA","work_id":"fd083a5e-d5f1-479f-87e7-79741d0a5663","year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2023,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.807207Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:47a317b759e59db09840d0cd5e3745dd4696ea3a24f051244dd34a63710ded9b","observation_id":"662507b5-377c-48af-a1c5-ad8e97a3d31c","resolution":{"observed_at":"2026-08-06T11:57:57.585172Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.11064","last_updated":"2025-04-11T17:24:11Z","snapshot_observed_at":"2026-08-07T17:50:46.423896Z","submitted_at":"2024-12-15T05:42:30Z","title":"Planet formation theory: an overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.11064","snapshot_observed_at":"2026-08-06T11:57:56.745643Z","title":"submitted to astro-ph.EP","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2024,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.745643Z"},"links":{"cited_paper":"/paper/2412.11064","citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:49a4069a715cbdaec78c70688add6c341b7721a2e23a7689d0fe61b2c4c29998","observation_id":"6925e1bd-a598-43bc-9e4f-9740d479558e","resolution":{"observed_at":"2026-08-06T11:57:56.745643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.03299","last_updated":"2025-06-03T18:36:52Z","snapshot_observed_at":"2026-08-07T11:04:15.900189Z","submitted_at":"2025-06-03T18:36:52Z","title":"The NASA Exoplanet Archive and Exoplanet Follow-up Observing Program: Data, Tools, and Usage","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.03299","snapshot_observed_at":"2026-08-06T11:57:56.825882Z","title":"submitted to Astro- ph.EP, https://doi.org/10.48550/arXiv.2506.03299","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2025,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.825882Z"},"links":{"cited_paper":"/paper/2506.03299","citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:183ea99c7b3fc85b329e1fd1bdd4d1273a971cd586db52358343789c8a911d2c","observation_id":"f7bd7101-8234-45af-b443-db454133e69c","resolution":{"observed_at":"2026-08-06T11:57:56.825882Z","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":"2026-08-06T11:57:56.992738Z","title":"Yoffe, Ofir and Aharonson,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0","version":1},"reference_index":2154,"source":"pdf_text","source_observed_at":"2026-08-06T11:57:56.992738Z"},"links":{"citing_paper":"/paper/2507.22297"},"observation_digest":"sha256:4a9644fd3be0c17314f7ea3c0a82752d2afe1a4ed1b52229c6872f5e5533b2e4","observation_id":"c6d5a124-4dfc-436a-aa66-41580eae7fb7","resolution":{"observed_at":"2026-08-06T11:57:56.992738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.22297","last_updated":"2025-07-30T00:11:20Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-10T05:07:30.213152Z","submitted_at":"2025-07-30T00:11:20Z","title":"The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0"},"reference_resolution":{"displayed":47,"state_counts":{"malformed_identifier":3,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":35,"verified_exact":7,"verified_fuzzy":0},"total_outbound_references":47},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 47 of 47 outbound references and 0 inbound Pith citation observations for arXiv:2507.22297."}