{"as_of":"2026-08-05T21:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fad0cb1ccac889b6a40c1ab8a97ceede3a8aec841e99387cb1fadd6f22ee4cae","coverage":[{"denominator":89,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":89,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T12:49:06.247397Z","state":"measured"},{"denominator":89,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":89,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+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/2607.19325/citation-record","integrity":"/paper/2607.19325/integrity","json":"/paper/2607.19325/citation-record.json","paper":"/paper/2607.19325"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.00026","last_updated":"2017-09-29T18:43:06Z","snapshot_observed_at":"2026-07-06T06:02:02.014789Z","submitted_at":"2017-09-29T18:43:06Z","title":"Precise Masses in the WASP-47 System","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.00026","snapshot_observed_at":"2026-08-01T12:48:54.032730Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.032730Z"},"links":{"cited_paper":"/paper/1710.00026","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:08820d77061ee714bc6189f7460cc3cf8c5072f4834d00c0b2e20343c2b69df9","observation_id":"b45e7ce4-6d0c-42c3-a844-15de858b48dd","resolution":{"observed_at":"2026-08-01T12:48:54.032730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.07820","last_updated":"2017-09-15T18:16:43Z","snapshot_observed_at":"2026-08-05T13:00:50.699671Z","submitted_at":"2015-11-24T17:47:57Z","title":"Planetary Candidates from the First Year of the K2 Mission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.07820","snapshot_observed_at":"2026-08-01T12:48:54.145915Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.145915Z"},"links":{"cited_paper":"/paper/1511.07820","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:2cb93a6cdcf78208d7418c2686da6e506cd57071da3d53fa334edfb2d3992702","observation_id":"7126703e-637d-4602-80a7-7e21757d1095","resolution":{"observed_at":"2026-08-01T12:48:54.145915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00071","last_updated":"2024-01-05T18:53:03Z","snapshot_observed_at":"2026-07-06T15:10:45.160875Z","submitted_at":"2023-03-31T18:39:39Z","title":"The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00071","snapshot_observed_at":"2026-08-01T12:48:54.195096Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.195096Z"},"links":{"cited_paper":"/paper/2304.00071","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:01fb58ffaf25559193082073d4e5c123b5df66491795766330f0e7b96d071dc4","observation_id":"00808844-583d-4863-8f20-87f7d120d274","resolution":{"observed_at":"2026-08-01T12:48:54.195096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.01748","last_updated":"2025-02-03T19:00:10Z","snapshot_observed_at":"2026-07-06T20:30:31.588538Z","submitted_at":"2025-02-03T19:00:10Z","title":"Resolving the Super-Earth/Gas Giant Connection in Stellar Mass and Metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.01748","snapshot_observed_at":"2026-08-01T12:48:54.341613Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.341613Z"},"links":{"cited_paper":"/paper/2502.01748","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:4737c28eea922ea2b242dbe76f6d35943a8eca112f1418c668e2f9328302bf3d","observation_id":"fa23a7f0-819a-42f7-baac-e9681fa07827","resolution":{"observed_at":"2026-08-01T12:48:54.341613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20035","last_updated":"2025-07-13T14:41:23Z","snapshot_observed_at":"2026-08-05T14:30:29.284965Z","submitted_at":"2025-05-26T14:22:38Z","title":"Cold Jupiters and small planets: Friends, foes, or indifferent? A search for correlations with the largest exoplanet samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20035","snapshot_observed_at":"2026-08-01T12:48:54.500880Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.500880Z"},"links":{"cited_paper":"/paper/2505.20035","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:1c2709536fc4201893f17ee1a93a42f4f3122a76161a6fb91f8f5150d07f04d1","observation_id":"9a5b9d9b-3017-43cf-9a36-7be375123b24","resolution":{"observed_at":"2026-08-01T12:48:54.500880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.03303","last_updated":"2020-02-15T16:21:27Z","snapshot_observed_at":"2026-08-05T13:30:19.305847Z","submitted_at":"2018-03-08T21:00:02Z","title":"Kepler-78 and the Ultra-Short-Period Planets","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.03303","snapshot_observed_at":"2026-08-01T12:48:54.681093Z","title":", keywords =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.681093Z"},"links":{"cited_paper":"/paper/1803.03303","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:604b30fa11347003b496d16276dbd593dc9a9c697013bba27808acb79c3a7dca","observation_id":"c9007f7e-00bb-4574-a7f9-516c6e059d41","resolution":{"observed_at":"2026-08-01T12:48:54.681093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09533","last_updated":"2016-10-29T15:44:05Z","snapshot_observed_at":"2026-07-06T05:16:39.176458Z","submitted_at":"2016-10-29T15:44:05Z","title":"Absolute densities, masses, and radii of the WASP-47 system determined dynamically","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09533","snapshot_observed_at":"2026-08-01T12:48:54.767443Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.767443Z"},"links":{"cited_paper":"/paper/1610.09533","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:cd31feb4601f55502e3b50dd238e31d8410392e1a22ca1f27e37b0cce00b4233","observation_id":"bd446b5c-a41d-4edb-ad1a-da5b44f1e1b1","resolution":{"observed_at":"2026-08-01T12:48:54.767443Z","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":"2026-08-01T12:48:54.911157Z","title":"Ground-based and Airborne Instrumentation for Astronomy IV , year = 2012, editor =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.911157Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:024e2030881ce0c3da092ba531889f9a1021c85450cfd16b384f0be6f0c9f8a0","observation_id":"f18a1ef3-5c94-4980-ab3d-421059d36bef","resolution":{"observed_at":"2026-08-01T12:48:54.911157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.2379","last_updated":"2014-03-10T20:00:09Z","snapshot_observed_at":"2026-07-06T03:38:06.024393Z","submitted_at":"2014-03-10T20:00:09Z","title":"A Study of the Shortest-Period Planets Found With Kepler","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.2379","snapshot_observed_at":"2026-08-01T12:48:54.966995Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:54.966995Z"},"links":{"cited_paper":"/paper/1403.2379","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:60cf6fc16849792d6e0336de04ea596e24195123ed0b15956ec927a4150c98f2","observation_id":"c203620a-5e7e-444a-8d88-52bf284d9c95","resolution":{"observed_at":"2026-08-01T12:48:54.966995Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.03146","last_updated":"2017-01-08T05:04:31Z","snapshot_observed_at":"2026-07-31T05:08:16.974200Z","submitted_at":"2015-06-10T02:23:18Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.03146","snapshot_observed_at":"2026-08-01T12:48:55.048153Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.048153Z"},"links":{"cited_paper":"/paper/1506.03146","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:251419775fbad2da36dd5c6bc47dfb8a03c1f7f4c0d897cd65546f6ad3ca635a","observation_id":"82d121de-6ec9-4f4f-828f-6e8ae14cf82e","resolution":{"observed_at":"2026-08-01T12:48:55.048153Z","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":"2026-08-01T12:48:55.166188Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.166188Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:c9e29a5c4672b10eccca23878f389d60a2ab4da338cd6802b15d9b2753165a1a","observation_id":"e7597c9d-a4d0-4ca7-8e41-2bc0f6d91e1a","resolution":{"observed_at":"2026-08-01T12:48:55.166188Z","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":"2026-08-01T12:48:55.250453Z","title":"Ricker and Joshua N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.250453Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:0ffcace57b4088bf808d4cb8140515e007d898f75ff2447e309f6288c65604de","observation_id":"7f21e534-a093-4218-a3d9-262ff42be71b","resolution":{"observed_at":"2026-08-01T12:48:55.250453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.09480","last_updated":"2019-07-22T18:00:00Z","snapshot_observed_at":"2026-08-02T20:36:01.707573Z","submitted_at":"2019-07-22T18:00:00Z","title":"EXOFASTv2: A public, generalized, publication-quality exoplanet modeling code","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.09480","snapshot_observed_at":"2026-08-01T12:48:55.335055Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.335055Z"},"links":{"cited_paper":"/paper/1907.09480","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:31d45d9cbb23418b97aa5044f161ec413f4891b5962392b6ac63120efbc22b80","observation_id":"e3af28ea-81d9-4281-a9d2-b047eace26df","resolution":{"observed_at":"2026-08-01T12:48:55.335055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.02217","last_updated":"2020-01-07T18:29:53Z","snapshot_observed_at":"2026-07-06T08:49:05.214333Z","submitted_at":"2020-01-07T18:29:53Z","title":"An ultra-short period rocky super-Earth orbiting the G2-star HD 80653","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.02217","snapshot_observed_at":"2026-08-01T12:48:55.443365Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.443365Z"},"links":{"cited_paper":"/paper/2001.02217","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:32df789c13b649d57a624ad3271bd35cf9b07123ee5ceea9c00c1b2fc809f7f0","observation_id":"f4977749-4c05-4c85-984a-d9809198619c","resolution":{"observed_at":"2026-08-01T12:48:55.443365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.05773","last_updated":"2023-09-06T09:27:49Z","snapshot_observed_at":"2026-08-05T02:55:01.347386Z","submitted_at":"2023-04-12T11:31:10Z","title":"Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.05773","snapshot_observed_at":"2026-08-01T12:48:55.604829Z","title":"No excess of cold Jupiters in small planet systems","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.604829Z"},"links":{"cited_paper":"/paper/2304.05773","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:a52bcda5e6925f73ee952f9a35543a84998f91f78e3062a59c66e816500ae985","observation_id":"ef612fd0-a4af-4f04-8b97-468fef5a6b2d","resolution":{"observed_at":"2026-08-01T12:48:55.604829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.3475","last_updated":"2010-12-15T21:22:29Z","snapshot_observed_at":"2026-07-06T02:20:46.794059Z","submitted_at":"2010-12-15T21:22:29Z","title":"Secular Chaos and the Production of Hot Jupiters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.3475","snapshot_observed_at":"2026-08-01T12:48:55.717270Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.717270Z"},"links":{"cited_paper":"/paper/1012.3475","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:6c49a6e55e2c583fb74b045f59f86778b143de90bce23e5270353142b6e90b88","observation_id":"5db7f8eb-e8e8-4b21-899b-a1795b2fa3e5","resolution":{"observed_at":"2026-08-01T12:48:55.717270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.05065","last_updated":"2018-04-13T18:00:00Z","snapshot_observed_at":"2026-08-05T13:10:33.477770Z","submitted_at":"2018-04-13T18:00:00Z","title":"Ultra-short-period planets from secular chaos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.05065","snapshot_observed_at":"2026-08-01T12:48:55.816250Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.816250Z"},"links":{"cited_paper":"/paper/1804.05065","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:7b25fd27eb9cdbbeb563832aff88c9fae0387275b86e496a9ce0289e8ea46287","observation_id":"d839fbf0-b8d2-4c87-901b-e37eb3377599","resolution":{"observed_at":"2026-08-01T12:48:55.816250Z","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":"2026-08-01T12:48:55.938785Z","title":", year = 1996, month = apr, volume =","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:55.938785Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:3a3d01f1ee047e6b960995e0aceb3d548ef080a0e89bd667e1b9a9fdc92ec4cf","observation_id":"995c5692-c71f-4b11-9510-3515c08cbb39","resolution":{"observed_at":"2026-08-01T12:48:55.938785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.06117","last_updated":"2018-01-18T16:44:09Z","snapshot_observed_at":"2026-07-06T06:19:14.564337Z","submitted_at":"2018-01-18T16:44:09Z","title":"Origins of Hot Jupiters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.06117","snapshot_observed_at":"2026-08-01T12:48:56.114339Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.114339Z"},"links":{"cited_paper":"/paper/1801.06117","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:b04ecad2fb0a104b905c917906e80f3169e7aa0390fabf2ca053b7540aa5e652","observation_id":"2f838925-b281-41a0-9be4-58c68c5d2aeb","resolution":{"observed_at":"2026-08-01T12:48:56.114339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02180","last_updated":"2019-04-03T18:04:57Z","snapshot_observed_at":"2026-07-06T07:43:43.696691Z","submitted_at":"2019-04-03T18:04:57Z","title":"dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02180","snapshot_observed_at":"2026-08-01T12:48:56.252556Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.252556Z"},"links":{"cited_paper":"/paper/1904.02180","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:b1fe4762b6651ec65da7cb7aea7b172b938e8fdaf1f38f99e9451d162d319d47","observation_id":"2805cdc8-bd48-4fe1-a399-507324c8c391","resolution":{"observed_at":"2026-08-01T12:48:56.252556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.08549","last_updated":"2019-11-04T22:06:08Z","snapshot_observed_at":"2026-08-05T08:42:32.184744Z","submitted_at":"2018-12-20T13:29:28Z","title":"Juliet: a versatile modelling tool for transiting and non-transiting exoplanetary systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.08549","snapshot_observed_at":"2026-08-01T12:48:56.397310Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.397310Z"},"links":{"cited_paper":"/paper/1812.08549","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:4ec4cc33f806af0405291770f4165fd63d3fb790c4d0492eb1a152591b56e07d","observation_id":"edd7935c-ea9f-476a-9873-73d7fb55718d","resolution":{"observed_at":"2026-08-01T12:48:56.397310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.01527","last_updated":"2024-03-19T09:52:01Z","snapshot_observed_at":"2026-08-04T01:35:32.144989Z","submitted_at":"2024-03-03T14:58:26Z","title":"The GAPS Programme at TNG LV. Multiple molecular species in the atmosphere of HAT-P-11 b and review of the HAT-P-11 planetary system","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.01527","snapshot_observed_at":"2026-08-01T12:48:56.529192Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.529192Z"},"links":{"cited_paper":"/paper/2403.01527","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:d645353ba5f6c247deb2b1d7f9b1f9a50ea9c47f789cef0d14168852fcc66d1b","observation_id":"d7dfc968-d32f-4704-a5b9-7843d6760dcd","resolution":{"observed_at":"2026-08-01T12:48:56.529192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.07304","last_updated":"2015-06-24T10:20:23Z","snapshot_observed_at":"2026-07-06T04:21:52.011550Z","submitted_at":"2015-06-24T10:20:23Z","title":"A Gaussian process framework for modelling stellar activity signals in radial velocity data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.07304","snapshot_observed_at":"2026-08-01T12:48:56.664743Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.664743Z"},"links":{"cited_paper":"/paper/1506.07304","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:c3d4b1dffd978fda957edd565bab775ced6b46771f7a3f5a1e825d42c33079a7","observation_id":"55470871-f8e2-4e38-926e-59c7e1a283b4","resolution":{"observed_at":"2026-08-01T12:48:56.664743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.12538","last_updated":"2021-03-24T16:04:32Z","snapshot_observed_at":"2026-08-05T03:02:47.236391Z","submitted_at":"2021-03-23T13:47:05Z","title":"The TESS Objects of Interest Catalog from the TESS Prime Mission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.12538","snapshot_observed_at":"2026-08-01T12:48:56.854575Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.854575Z"},"links":{"cited_paper":"/paper/2103.12538","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:b943c5e3bf66701e10bf06df0d2ad6ec954da1ffe3d05e30190e995afa0116d3","observation_id":"86bb0524-58b1-40af-a2a1-cf50d25b4cc0","resolution":{"observed_at":"2026-08-01T12:48:56.854575Z","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":"2026-08-01T12:48:56.931353Z","title":"Cannon and Edward C","venue":null,"work_id":null,"year":1918},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:56.931353Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:dfb484121f23eae806538e423a2b4b0e6264fd0c902a2a0f14bcd31baea96dda","observation_id":"0c9d83d9-0bb6-4034-bcb2-ea1b63b9b5c2","resolution":{"observed_at":"2026-08-01T12:48:56.931353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00211","last_updated":"2022-07-30T13:18:15Z","snapshot_observed_at":"2026-07-06T13:36:58.879342Z","submitted_at":"2022-07-30T13:18:15Z","title":"Gaia Data Release 3: Summary of the content and survey properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.00211","snapshot_observed_at":"2026-08-01T12:48:57.126586Z","title":"Summary of the content and survey properties","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:57.126586Z"},"links":{"cited_paper":"/paper/2208.00211","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:f8098e0893c5fab807754aecdde2c9749aee6e2bf7f975f8cc2b228c525aab9e","observation_id":"28c9313a-da39-4f90-9dd4-fa685643de47","resolution":{"observed_at":"2026-08-01T12:48:57.126586Z","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":"2026-08-01T12:48:57.255041Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:57.255041Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:7078feccf48553f6e862155d8f125d2ab6fc5da1d0d5f4d76de13e7225660ec3","observation_id":"a7e65e18-a1f3-4e1a-b161-60943f1c36ae","resolution":{"observed_at":"2026-08-01T12:48:57.255041Z","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":"2026-08-01T12:48:57.408183Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:57.408183Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:f7987d07eae525199d09d91bb8781b75c693c7ac088cc7d41825f7411fbb92d3","observation_id":"4af585ca-7715-450d-ad80-c3986745cce3","resolution":{"observed_at":"2026-08-01T12:48:57.408183Z","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":"2026-08-01T12:48:57.634744Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:57.634744Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:68e7917e665967a81caa485a72f7d0e1699774bdc1d54e9fe258fa8804c1d794","observation_id":"33525743-4a8e-45ca-b4cd-c34650c7c5fa","resolution":{"observed_at":"2026-08-01T12:48:57.634744Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.2657","last_updated":"2013-07-10T02:42:52Z","snapshot_observed_at":"2026-07-06T03:17:51.662650Z","submitted_at":"2013-07-10T02:42:52Z","title":"Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-Main Sequence Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2657","snapshot_observed_at":"2026-08-01T12:48:57.844749Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:57.844749Z"},"links":{"cited_paper":"/paper/1307.2657","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:d4022713ebef91135625176c5d299df84628d132aa7d759bea769f857024750d","observation_id":"b1aacbc7-ae5a-4232-95ef-6527cfc4df77","resolution":{"observed_at":"2026-08-01T12:48:57.844749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09417","last_updated":"2024-11-14T13:10:29Z","snapshot_observed_at":"2026-08-01T00:17:32.111328Z","submitted_at":"2024-11-14T13:10:29Z","title":"The GAPS programme at TNG LXIV: An inner eccentric sub-Neptune and an outer sub-Neptune-mass candidate around BD+00 444 (TOI-2443)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09417","snapshot_observed_at":"2026-08-01T12:48:58.054819Z","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":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:58.054819Z"},"links":{"cited_paper":"/paper/2411.09417","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:e1484094a8e093123ea0e9e78480fb28e06a90f7e0fffb75c4a9809988a670fa","observation_id":"92548021-0b98-4337-940e-3bd043c3baf6","resolution":{"observed_at":"2026-08-01T12:48:58.054819Z","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":"2026-08-01T12:48:58.254743Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:58.254743Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:dae46cf306b7447605d52d5f75529d513b52f50e70edf4d5a814cfba2081be32","observation_id":"59cebacc-c0a5-472f-ad50-c73f07c52612","resolution":{"observed_at":"2026-08-01T12:48:58.254743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.03304","last_updated":"2015-02-24T10:18:06Z","snapshot_observed_at":"2026-07-06T04:06:10.070072Z","submitted_at":"2015-01-14T10:44:09Z","title":"Can Kozai-Lidov cycles explain Kepler-78b?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.03304","snapshot_observed_at":"2026-08-01T12:48:58.434745Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:58.434745Z"},"links":{"cited_paper":"/paper/1501.03304","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:16463362b78a2479f1c37458ea0410556ad40f1fc4d9bbbe68b54eda54c762c3","observation_id":"fa23ecba-094b-4e24-9ffa-8359e317bf35","resolution":{"observed_at":"2026-08-01T12:48:58.434745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0104126","last_updated":"2001-04-06T23:38:19Z","snapshot_observed_at":"2026-07-07T00:17:41.659524Z","submitted_at":"2001-04-06T23:38:19Z","title":"Evolution in Binary and Triple Stars, with an application to SS Lac","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0104126","snapshot_observed_at":"2026-08-01T12:48:58.614745Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:58.614745Z"},"links":{"cited_paper":"/paper/astro-ph/0104126","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:a0dd5c779460b7c0209afb760725cba9ef11809a028a1d8baf60744b0599ff26","observation_id":"a06d9cb6-83d6-411d-aa60-eecf7c066cfb","resolution":{"observed_at":"2026-08-01T12:48:58.614745Z","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":"2026-08-01T12:48:58.814752Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:58.814752Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:d4ec412dfc3d100742fece216602f708b432eeb720b8873304d5366f38f30eb5","observation_id":"e0f67971-32e0-42f4-bb0f-a7543f556135","resolution":{"observed_at":"2026-08-01T12:48:58.814752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.1382","last_updated":"2012-03-07T05:35:25Z","snapshot_observed_at":"2026-07-06T02:44:08.056463Z","submitted_at":"2012-03-07T05:35:25Z","title":"Kepler Presearch Data Conditioning I - Architecture and Algorithms for Error Correction in Kepler Light Curves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.1382","snapshot_observed_at":"2026-08-01T12:48:58.974746Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:58.974746Z"},"links":{"cited_paper":"/paper/1203.1382","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:86d3d2bcff9f04baf0fd8415623b982dba0a2fc00b65ce45d32e6cd77ba1150a","observation_id":"b9ec1806-9302-4888-af4f-8baf453ff4ab","resolution":{"observed_at":"2026-08-01T12:48:58.974746Z","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":"2026-08-01T12:48:59.144750Z","title":", year = 2014, month = jan, volume =","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:59.144750Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:2fd86e64c0ff281477e24806e786b23980ab5fc3d45f9e13b76ee366a5849be5","observation_id":"1723d0f0-9ba7-4e42-93f2-cc831ee802ec","resolution":{"observed_at":"2026-08-01T12:48:59.144750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.1383","last_updated":"2012-03-07T05:35:37Z","snapshot_observed_at":"2026-08-02T10:31:52.545012Z","submitted_at":"2012-03-07T05:35:37Z","title":"Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.1383","snapshot_observed_at":"2026-08-01T12:48:59.384746Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:59.384746Z"},"links":{"cited_paper":"/paper/1203.1383","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:43293a1c2a5be0547be70d7ff8598ea58fa9d0c2dab262db41b15e0749598fe0","observation_id":"64baa859-a33f-4110-9427-f614444d91c3","resolution":{"observed_at":"2026-08-01T12:48:59.384746Z","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":"2026-08-01T12:48:59.699073Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:59.699073Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:33acb3f1d26e87f426e5f6dcb431a463d13259d74d0fd8f16aafdcde8bd72e3e","observation_id":"ba913d0b-ec51-4f08-9ee4-5dfcff077231","resolution":{"observed_at":"2026-08-01T12:48:59.699073Z","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":"10.1117/12.857625","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Software and Cyberinfrastructure for Astronomy , year = 2010, editor =","venue":"Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE","work_id":"4de30d81-b2e7-4d1d-b7d9-92b024a3c74d","year":2010},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-01T12:48:59.944322Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:9eb25e57607f29d61c05df91be1360ae23f5c87bd33e942dfc00c1da5b3dbc5c","observation_id":"1335dacb-1d48-4f6c-83c4-e845c270f4ea","resolution":{"observed_at":"2026-08-01T12:53:42.422886Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-01T12:49:00.042471Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.042471Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:0fe8a9a777639f818e0ef5b731b286f5aa6ee33eec5a7177fcadfab32bc5d8c6","observation_id":"fa8d0fce-2eee-448b-8f78-8587c964767b","resolution":{"observed_at":"2026-08-01T12:49:00.042471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0407318","last_updated":"2004-11-15T15:46:02Z","snapshot_observed_at":"2026-07-07T00:43:38.895035Z","submitted_at":"2004-07-15T20:45:15Z","title":"Tidal Interactions and Disruptions of Giant Planets on Highly Eccentric Orbits","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0407318","snapshot_observed_at":"2026-08-01T12:49:00.144746Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.144746Z"},"links":{"cited_paper":"/paper/astro-ph/0407318","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:b8063db4210ccf8fd1b0bf2bb84991399bb854c7e23bcef98cbe87e4580550aa","observation_id":"f53fbf44-64be-4080-86b8-f8b07c0f06a2","resolution":{"observed_at":"2026-08-01T12:49:00.144746Z","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":"2026-08-01T12:49:00.254745Z","title":"Lindstedt \\`a l' \\'e tude du mouvement des com \\`e tes p \\'e riodiques","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.254745Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:42b1ebea0ad9398e44aba980237cb6294c89428cfe24c3234689677ea310dcab","observation_id":"63f35308-73a2-48de-8d20-4a7d203d4f90","resolution":{"observed_at":"2026-08-01T12:49:00.254745Z","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":"2026-08-01T12:49:00.384765Z","title":", volume=","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.384765Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:8df99313dbe7ba850ab6de697f7d6e336bc563a7f6facf60deeb92bc82d4e2be","observation_id":"dfc25c58-b292-4684-997e-9b440a5a9777","resolution":{"observed_at":"2026-08-01T12:49:00.384765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0303010","last_updated":"2003-03-01T19:02:04Z","snapshot_observed_at":"2026-07-07T00:31:35.668551Z","submitted_at":"2003-03-01T19:02:04Z","title":"Planet Migration and Binary Companions: the case of HD 80606b","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0303010","snapshot_observed_at":"2026-08-01T12:49:00.544745Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.544745Z"},"links":{"cited_paper":"/paper/astro-ph/0303010","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:c5edd91b4138810b4aed68d40ff9e245553abaefd72ccb6b1cec1b086ae5f010","observation_id":"1c7f80e5-070d-4cc9-8200-8cfbb4d47b78","resolution":{"observed_at":"2026-08-01T12:49:00.544745Z","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":"2026-08-01T12:49:00.661907Z","title":"Planetary and Space Science , volume=","venue":null,"work_id":null,"year":1962},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.661907Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:efd471cfedc485d83a87c912ea1a80adbe81267a599e973c488b9ac8913ef146","observation_id":"062f1ba7-f9f6-4bfa-9e2e-c9f461b02858","resolution":{"observed_at":"2026-08-01T12:49:00.661907Z","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":"2026-08-01T12:49:00.744738Z","title":", volume=","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.744738Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:e0901c82f45595ce8384a3f96223c75ff54b90b1ce23e685fad30cbe150dc9c5","observation_id":"97c9c918-350d-4950-861f-a50178778360","resolution":{"observed_at":"2026-08-01T12:49:00.744738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3853","last_updated":"2014-08-17T20:01:10Z","snapshot_observed_at":"2026-07-06T03:51:55.171820Z","submitted_at":"2014-08-17T20:01:10Z","title":"A Technique for Extracting Highly Precise Photometry for the Two-Wheeled Kepler Mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3853","snapshot_observed_at":"2026-08-01T12:49:00.868667Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:00.868667Z"},"links":{"cited_paper":"/paper/1408.3853","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:1fc4521eccc5ad417c9c242c641cc232b61030a072f3eaa4e5c0424db587dea0","observation_id":"7b60e6ef-ee93-46e7-98f5-ca872b6783ed","resolution":{"observed_at":"2026-08-01T12:49:00.868667Z","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":"2026-08-01T12:49:01.040236Z","title":", keywords =","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:01.040236Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:46122da9026788acf58b5861bd27da91b3a3de389219698cdab400a6e57a3352","observation_id":"aac6711f-2765-45c3-babf-78488b61db20","resolution":{"observed_at":"2026-08-01T12:49:01.040236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.05716","last_updated":"2021-11-23T21:44:30Z","snapshot_observed_at":"2026-08-04T22:28:55.400994Z","submitted_at":"2021-11-10T14:53:47Z","title":"Probing Kepler's hottest small planets via homogeneous search and analysis of optical secondary eclipses and phase variations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.05716","snapshot_observed_at":"2026-08-01T12:49:01.152599Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:01.152599Z"},"links":{"cited_paper":"/paper/2111.05716","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:0aafd4f5cdad754e3b9b3d3851e94b291eb8103f538c64235250e6e0f6add9e0","observation_id":"0208a4c3-900c-4207-ae45-a3e6dc611f7b","resolution":{"observed_at":"2026-08-01T12:49:01.152599Z","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":"2026-08-01T12:49:01.444745Z","title":"IEEE Transactions on Pattern Analysis and Machine Intelligence , keywords =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:01.444745Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:361f34d4fcbd0a91f89cc1174ad0aa876f434459a1365ae62b81f53619a33a31","observation_id":"3ea545a6-5e41-469c-997e-51ee4c8c6034","resolution":{"observed_at":"2026-08-01T12:49:01.444745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202462","last_updated":"2002-02-25T19:31:27Z","snapshot_observed_at":"2026-07-07T00:25:13.180226Z","submitted_at":"2002-02-25T19:31:27Z","title":"Eccentricity Evolution for Planets in Gaseous Disks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0202462","snapshot_observed_at":"2026-08-01T12:49:01.575142Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:01.575142Z"},"links":{"cited_paper":"/paper/astro-ph/0202462","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:81da0b6a2b3df047860d6fbe74e1c4e454b814970b1f1ef3e2bf0dd7e5ee6bd8","observation_id":"57b0fb29-2d0b-47d1-9705-32e850f2c806","resolution":{"observed_at":"2026-08-01T12:49:01.575142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08667","last_updated":"2015-09-03T16:01:08Z","snapshot_observed_at":"2026-07-06T04:25:24.625762Z","submitted_at":"2015-07-30T20:08:45Z","title":"Eccentric Jupiters via Disk-Planet Interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.08667","snapshot_observed_at":"2026-08-01T12:49:01.695326Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:01.695326Z"},"links":{"cited_paper":"/paper/1507.08667","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:93d5e2a578d7982cdfb249a97de03be1cbb71fbd1c26d4c8c51ba81aa8a86856","observation_id":"3b664ed3-7141-46f2-8e65-34af0feca37b","resolution":{"observed_at":"2026-08-01T12:49:01.695326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703163","last_updated":"2008-06-06T03:04:03Z","snapshot_observed_at":"2026-07-07T01:07:50.296173Z","submitted_at":"2007-03-07T23:49:20Z","title":"Origins of Eccentric Extrasolar Planets: Testing the Planet-Planet Scattering Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703163","snapshot_observed_at":"2026-08-01T12:49:01.839661Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:01.839661Z"},"links":{"cited_paper":"/paper/astro-ph/0703163","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:ab6703611684502c6daecaaecd417a4fe23fd3ffc8031c58cb23c41f2e47bdca","observation_id":"8a358e5f-8fd3-49f3-b89d-f1283f05c21f","resolution":{"observed_at":"2026-08-01T12:49:01.839661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.19511","last_updated":"2024-12-05T18:33:19Z","snapshot_observed_at":"2026-08-05T16:45:42.734421Z","submitted_at":"2024-05-29T20:48:24Z","title":"Planet-Planet Scattering and ZLK Migration -- The Dynamical History of HAT-P-11","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.19511","snapshot_observed_at":"2026-08-01T12:49:02.034494Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.034494Z"},"links":{"cited_paper":"/paper/2405.19511","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:5490b29679153d9e6be08043d6829b3e93a89a3c77dfbd4685781d4626b4830f","observation_id":"ad1148e7-7cda-48fb-8545-2eedac343b86","resolution":{"observed_at":"2026-08-01T12:49:02.034494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.02564","last_updated":"2019-09-09T19:35:05Z","snapshot_observed_at":"2026-08-04T16:02:22.508413Z","submitted_at":"2019-03-06T19:00:02Z","title":"Planet-planet scattering as the source of the highest eccentricity exoplanets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.02564","snapshot_observed_at":"2026-08-01T12:49:02.064826Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.064826Z"},"links":{"cited_paper":"/paper/1903.02564","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:933abe34d66f201fa256314067adb26c53227333c5734f1a23b6e808a6256b1c","observation_id":"6b34f0b1-8c68-4970-a59c-5e73000a2096","resolution":{"observed_at":"2026-08-01T12:49:02.064826Z","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":"2026-08-01T12:49:02.146337Z","title":", keywords =","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.146337Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:0418fe6cbedb44966576a704b05060f295bf2f4a535b25e63ac7edafecea9b13","observation_id":"2d79875b-2df6-4337-ac1d-fd0222dba1bd","resolution":{"observed_at":"2026-08-01T12:49:02.146337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.11837","last_updated":"2021-10-22T15:14:06Z","snapshot_observed_at":"2026-08-04T20:58:08.325908Z","submitted_at":"2021-10-22T15:14:06Z","title":"Physically-motivated basis functions for temperature maps of exoplanets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.11837","snapshot_observed_at":"2026-08-01T12:49:02.285271Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.285271Z"},"links":{"cited_paper":"/paper/2110.11837","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:551364821d76e5a8bfacd2db7ff4ebc7f029736e1386dd6cfe296e329473f40a","observation_id":"48aa34ef-10f3-47c4-918f-cf660064dad7","resolution":{"observed_at":"2026-08-01T12:49:02.285271Z","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":"2026-08-01T12:49:02.395006Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.395006Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:5fea6119bebb248db7708b6cdd00aa054d80b28e7ea170d68baf5fdd41eca091","observation_id":"b56e211a-bafa-46bc-8b0d-685cdb4f6548","resolution":{"observed_at":"2026-08-01T12:49:02.395006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15087","last_updated":"2020-10-28T17:01:22Z","snapshot_observed_at":"2026-08-05T06:12:43.863565Z","submitted_at":"2020-10-28T17:01:22Z","title":"Formation of Ultra-Short-Period Planets by Obliquity-Driven Tidal Runaway","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15087","snapshot_observed_at":"2026-08-01T12:49:02.534750Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.534750Z"},"links":{"cited_paper":"/paper/2010.15087","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:73b9ffaa4025a62e08d2653b72114e7dadc7650a07629a1a452380cd4be72b90","observation_id":"69e9ff0f-9987-4e44-a054-dd7ef73f7a4f","resolution":{"observed_at":"2026-08-01T12:49:02.534750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.00009","last_updated":"2016-03-29T12:14:27Z","snapshot_observed_at":"2026-08-04T07:17:32.646705Z","submitted_at":"2016-01-29T21:00:11Z","title":"The GAPS programme with HARPS-N at TNG XI. Pr~0211 in M~44: the first multi-planet system in an open cluster","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.00009","snapshot_observed_at":"2026-08-01T12:49:02.638080Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.638080Z"},"links":{"cited_paper":"/paper/1602.00009","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:193ad71d80c4d8b3448911b278a5d1c4e3d84c99014e730b536525fb376500dd","observation_id":"c6f186e8-b029-41e7-a025-cddcefde98e5","resolution":{"observed_at":"2026-08-01T12:49:02.638080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.03502","last_updated":"2018-01-10T19:00:04Z","snapshot_observed_at":"2026-07-06T06:18:04.975530Z","submitted_at":"2018-01-10T19:00:04Z","title":"An ultra-short period rocky super-Earth with a secondary eclipse and a Neptune-like companion around K2-141","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.03502","snapshot_observed_at":"2026-08-01T12:49:02.791338Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.791338Z"},"links":{"cited_paper":"/paper/1801.03502","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:cab6849e7d3cdcfbc7bdea10c036137b34f41f1339ca76be8df2f03ba682e67f","observation_id":"6fa3d201-eb1b-4aad-ad68-090ffc0e42d3","resolution":{"observed_at":"2026-08-01T12:49:02.791338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16888","last_updated":"2023-10-25T18:00:02Z","snapshot_observed_at":"2026-07-06T16:38:33.021861Z","submitted_at":"2023-10-25T18:00:02Z","title":"The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16888","snapshot_observed_at":"2026-08-01T12:49:02.887213Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.887213Z"},"links":{"cited_paper":"/paper/2310.16888","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:57597b7a67d6e94513b76db3b2b855e5547e46a9392e6fe2f36f123a3f49bfd8","observation_id":"02243123-f9e6-455b-8843-60f8b4d0338e","resolution":{"observed_at":"2026-08-01T12:49:02.887213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.03496","last_updated":"2022-06-07T18:00:00Z","snapshot_observed_at":"2026-08-03T22:05:18.189061Z","submitted_at":"2022-06-07T18:00:00Z","title":"The GAPS Programme with HARPS-N at TNG. XXXVII. A precise density measurement of the young ultra-short period planet TOI-1807 b","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.03496","snapshot_observed_at":"2026-08-01T12:49:02.989462Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:02.989462Z"},"links":{"cited_paper":"/paper/2206.03496","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:d290b4828e4815cd666b6208e31af66f5f9034866764dd7fefc1a720fc3d5ac4","observation_id":"6ba946df-c54a-4263-bcec-446ce8863e61","resolution":{"observed_at":"2026-08-01T12:49:02.989462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.13900","last_updated":"2021-07-30T10:08:28Z","snapshot_observed_at":"2026-08-05T17:58:08.016966Z","submitted_at":"2021-07-29T11:22:04Z","title":"A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.13900","snapshot_observed_at":"2026-08-01T12:49:03.072705Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.072705Z"},"links":{"cited_paper":"/paper/2107.13900","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:de933401ecde8ad19c48ba1c814939156a99ae3a332c032fe17e6d5a1ade1fbd","observation_id":"99c0375c-2d40-488e-b603-485a6406da96","resolution":{"observed_at":"2026-08-01T12:49:03.072705Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.0009","last_updated":"2013-08-14T16:30:16Z","snapshot_observed_at":"2026-07-06T03:19:41.818517Z","submitted_at":"2013-07-31T20:00:00Z","title":"Efficient, uninformative sampling of limb darkening coefficients for two-parameter laws","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.0009","snapshot_observed_at":"2026-08-01T12:49:03.168275Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.168275Z"},"links":{"cited_paper":"/paper/1308.0009","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:64887be7a1d4d3a26a34cf2dc6e0230566da744e46d79ae25e7fe3614b518d7e","observation_id":"cfa49c42-5e15-4a1d-ad5b-2d5b3d4eb03f","resolution":{"observed_at":"2026-08-01T12:49:03.168275Z","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":"2026-08-01T12:49:03.246346Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.246346Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:5d62f792b0a322e736fac772c3e8ffb1faccba4f475085003449d368abba9c88","observation_id":"29c8b094-4a53-4825-ba62-f0543901bc29","resolution":{"observed_at":"2026-08-01T12:49:03.246346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08285","last_updated":"2015-08-19T03:48:44Z","snapshot_observed_at":"2026-07-06T04:25:16.554761Z","submitted_at":"2015-07-29T20:10:41Z","title":"batman: BAsic Transit Model cAlculatioN in Python","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.08285","snapshot_observed_at":"2026-08-01T12:49:03.300290Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.300290Z"},"links":{"cited_paper":"/paper/1507.08285","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:c86125267fdad92c5b8c60738439586a98c0961348341cdf99de95605941d47a","observation_id":"23d34783-0b30-4fbc-89da-2699909d73da","resolution":{"observed_at":"2026-08-01T12:49:03.300290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.10678","last_updated":"2020-04-22T16:24:25Z","snapshot_observed_at":"2026-08-05T20:17:10.142460Z","submitted_at":"2020-04-22T16:24:25Z","title":"Efficient modeling of correlated noise II. A flexible noise model with fast and scalable methods","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.10678","snapshot_observed_at":"2026-08-01T12:49:03.424749Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.424749Z"},"links":{"cited_paper":"/paper/2004.10678","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:71bd202de9ff1ca0a782c961c98866479797cf8025303e7338a25a44525949a5","observation_id":"ff3150be-48ef-40a4-be5e-d994518878ef","resolution":{"observed_at":"2026-08-01T12:49:03.424749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02440","last_updated":"2022-01-07T13:05:28Z","snapshot_observed_at":"2026-08-05T04:53:24.025051Z","submitted_at":"2022-01-07T13:05:28Z","title":"Efficient modeling of correlated noise. III. Scalable methods for jointly modeling several observables' time series with Gaussian processes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.02440","snapshot_observed_at":"2026-08-01T12:49:03.614754Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.614754Z"},"links":{"cited_paper":"/paper/2201.02440","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:b1812699166e3013dd971d7a0d804347b53df29842f44b90f634769b7f92dd10","observation_id":"3a0795e1-8fbf-4626-a982-b019b73c85cc","resolution":{"observed_at":"2026-08-01T12:49:03.614754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3665","last_updated":"2013-11-25T15:56:48Z","snapshot_observed_at":"2026-07-06T02:43:00.981478Z","submitted_at":"2012-02-16T20:41:19Z","title":"emcee: The MCMC Hammer","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3665","snapshot_observed_at":"2026-08-01T12:49:03.724747Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.724747Z"},"links":{"cited_paper":"/paper/1202.3665","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:e92291357763195c5c7156bfb6f3b5b22130c810375fcac21ec098137cd2cfec","observation_id":"55d846b1-c1d3-4c04-85f1-7a09b90ddc56","resolution":{"observed_at":"2026-08-01T12:49:03.724747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.07433","last_updated":"2015-04-28T11:40:53Z","snapshot_observed_at":"2026-08-05T07:36:07.237752Z","submitted_at":"2015-04-28T11:40:53Z","title":"PyTransit: Fast and Easy Exoplanet Transit Modelling in Python","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.07433","snapshot_observed_at":"2026-08-01T12:49:03.834761Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.834761Z"},"links":{"cited_paper":"/paper/1504.07433","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:a570b5b3481b4ab47b0e67c6868e737938498de236f27422115b6fbcceab8df5","observation_id":"52ce6050-9130-4c63-98bb-cdf2a378da75","resolution":{"observed_at":"2026-08-01T12:49:03.834761Z","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":"2026-08-01T12:49:03.974751Z","title":"doi:10.5281/zenodo.17268284 , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:03.974751Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:5b6c6491f10195112604c27e01191601a24895808ab504d0119d1a62fb24bff8","observation_id":"8dd0b5b4-3da2-4761-8f91-74025837fc9f","resolution":{"observed_at":"2026-08-01T12:49:03.974751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.01862","last_updated":"2020-12-03T12:04:37Z","snapshot_observed_at":"2026-08-05T11:48:40.474394Z","submitted_at":"2020-12-03T12:04:37Z","title":"Auto-correlation functions of astrophysical processes, and their relation to Gaussian processes; Application to radial velocities of different starspot configurations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.01862","snapshot_observed_at":"2026-08-01T12:49:04.145127Z","title":"Application to radial velocities of different starspot configurations","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.145127Z"},"links":{"cited_paper":"/paper/2012.01862","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:bde84bdc758eeb7eb91124f7e276c2bcfcc931a23633b1e9a89cbf244a879810","observation_id":"88ee51e1-1b1b-4f22-ad34-e4049acaa423","resolution":{"observed_at":"2026-08-01T12:49:04.145127Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.5798","last_updated":"2013-01-31T23:50:33Z","snapshot_observed_at":"2026-07-06T02:50:37.363580Z","submitted_at":"2012-06-25T20:00:00Z","title":"EXOFAST: A fast exoplanetary fitting suite in IDL","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.5798","snapshot_observed_at":"2026-08-01T12:49:04.312689Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.312689Z"},"links":{"cited_paper":"/paper/1206.5798","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:8ccbea17392032819958b0c71c21f1f8c055e3e3f7851d2e239f4877dc2fc670","observation_id":"76420911-6c71-4b27-8f9c-bc29d621730f","resolution":{"observed_at":"2026-08-01T12:49:04.312689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.00966","last_updated":"2019-08-07T17:50:27Z","snapshot_observed_at":"2026-07-06T07:57:34.683633Z","submitted_at":"2019-06-03T18:00:00Z","title":"Wotan: Comprehensive time-series de-trending in Python","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.00966","snapshot_observed_at":"2026-08-01T12:49:04.439282Z","title":", keywords =","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.439282Z"},"links":{"cited_paper":"/paper/1906.00966","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:8a530a7b3a057f2f89f8efc97f7b846edea5c83ab5b5c12cc610b1fc8c6e5b21","observation_id":"f7fb98bb-d935-45f2-9aa2-8f958fb889e1","resolution":{"observed_at":"2026-08-01T12:49:04.439282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703166","last_updated":"2008-05-15T00:23:17Z","snapshot_observed_at":"2026-07-07T01:07:50.296173Z","submitted_at":"2007-03-07T21:56:20Z","title":"Dynamical Outcomes of Planet-Planet Scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703166","snapshot_observed_at":"2026-08-01T12:49:04.516754Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.516754Z"},"links":{"cited_paper":"/paper/astro-ph/0703166","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:399ed701cf5651d67c39bb269c4a7a84f4fb9ffb6318f7f03d4fa0aacae2b84b","observation_id":"333f96a4-6046-4cf4-85e7-a8c5228751c1","resolution":{"observed_at":"2026-08-01T12:49:04.516754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703160","last_updated":"2008-05-13T15:17:09Z","snapshot_observed_at":"2026-07-07T01:07:50.296173Z","submitted_at":"2007-03-07T21:00:05Z","title":"Dynamical Origin of Extrasolar Planet Eccentricity Distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703160","snapshot_observed_at":"2026-08-01T12:49:04.668717Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.668717Z"},"links":{"cited_paper":"/paper/astro-ph/0703160","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:fa81c0c346a66d71cf1cab04590d565e991f9c51e4551cc53161a53206f41d11","observation_id":"fb058453-383d-48ed-ac41-65515a4f13cf","resolution":{"observed_at":"2026-08-01T12:49:04.668717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.06971","last_updated":"2015-06-04T08:09:23Z","snapshot_observed_at":"2026-07-06T04:10:10.990919Z","submitted_at":"2015-02-24T21:00:18Z","title":"The destruction of inner planetary systems during high-eccentricity migration of gas giants","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.06971","snapshot_observed_at":"2026-08-01T12:49:04.801720Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.801720Z"},"links":{"cited_paper":"/paper/1502.06971","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:4b7292a5d24c2d9d6ace80b922be008381e42cc18e5fa43ee045043ff30661a7","observation_id":"59f5a26f-f68a-4896-b0ff-255b27d08bd9","resolution":{"observed_at":"2026-08-01T12:49:04.801720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.4285","last_updated":"2007-05-30T19:18:33Z","snapshot_observed_at":"2026-07-06T01:28:43.938761Z","submitted_at":"2007-05-30T19:18:33Z","title":"Shrinking binary and planetary orbits by Kozai cycles with tidal friction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.4285","snapshot_observed_at":"2026-08-01T12:49:04.966055Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:04.966055Z"},"links":{"cited_paper":"/paper/0705.4285","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:b51c67abb930cd89fc17de19373dfbde5ab3e73407573823a491ac783e32b167","observation_id":"bccdf42a-a01a-49d3-b8a0-5ccf98c3ce77","resolution":{"observed_at":"2026-08-01T12:49:04.966055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.01945","last_updated":"2021-05-06T19:40:28Z","snapshot_observed_at":"2026-07-06T09:52:48.994776Z","submitted_at":"2020-09-03T22:24:47Z","title":"Three Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.01945","snapshot_observed_at":"2026-08-01T12:49:05.140500Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.140500Z"},"links":{"cited_paper":"/paper/2009.01945","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:0b3b4d530148860f42c42338f961169a6aaba96e3103b7d67a793f47c3643ad2","observation_id":"5d36714a-ba29-4d07-bf09-a4c11b14d578","resolution":{"observed_at":"2026-08-01T12:49:05.140500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.08258","last_updated":"2019-04-26T20:39:50Z","snapshot_observed_at":"2026-08-05T06:05:50.389105Z","submitted_at":"2019-01-24T07:18:04Z","title":"Low-Eccentricity Migration of Ultra-Short Period Planets in Multi-Planet Systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.08258","snapshot_observed_at":"2026-08-01T12:49:05.212824Z","title":", keywords =","venue":null,"work_id":null,"year":1901},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.212824Z"},"links":{"cited_paper":"/paper/1901.08258","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:cf664324d07c4e6d520b28f763597b5864d7b0248becc6296ea42251910338e7","observation_id":"c8eaa16e-da97-4b70-8568-3893d8b6e048","resolution":{"observed_at":"2026-08-01T12:49:05.212824Z","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":"2026-08-01T12:49:05.312921Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.312921Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:256fd007a0ecae68c99688adae71b1181fda28b13f48e0d64dc8a294d55ba171","observation_id":"75575ded-757b-48d5-803a-b4ec84ea6d6c","resolution":{"observed_at":"2026-08-01T12:49:05.312921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.5163","last_updated":"2014-03-07T20:42:17Z","snapshot_observed_at":"2026-07-06T03:36:34.006096Z","submitted_at":"2014-02-20T22:34:31Z","title":"The K2 Mission: Characterization and Early results","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.5163","snapshot_observed_at":"2026-08-01T12:49:05.496524Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.496524Z"},"links":{"cited_paper":"/paper/1402.5163","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:22bc7b91885719160b5a3e46fcf2cf4ca17d3181ec649b022552764346be4fda","observation_id":"216a37d0-7c09-4f13-a02d-81825d236886","resolution":{"observed_at":"2026-08-01T12:49:05.496524Z","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":"2026-08-01T12:49:05.641624Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.641624Z"},"links":{"citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:c85613b88e3f5d4a39f33eb99d82f4dfd47db9d9ffb36265cbc923420245554e","observation_id":"9b08f21e-b1ed-47ee-94cd-216e5f25e0b2","resolution":{"observed_at":"2026-08-01T12:49:05.641624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0109491","last_updated":"2001-09-26T18:23:29Z","snapshot_observed_at":"2026-07-07T00:21:47.378879Z","submitted_at":"2001-09-26T18:23:29Z","title":"No planet for HD 166435","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0109491","snapshot_observed_at":"2026-08-01T12:49:05.769372Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.769372Z"},"links":{"cited_paper":"/paper/astro-ph/0109491","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:7e53ccb82e4a6c0f2be5785137fd869a1130cc342eef61d18ea4a4c9a753ae73","observation_id":"49f96867-ad3c-44df-be6c-d4b7cef249ea","resolution":{"observed_at":"2026-08-01T12:49:05.769372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.12186","last_updated":"2019-04-27T17:33:26Z","snapshot_observed_at":"2026-07-06T07:48:54.710107Z","submitted_at":"2019-04-27T17:33:26Z","title":"Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.12186","snapshot_observed_at":"2026-08-01T12:49:05.910471Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:05.910471Z"},"links":{"cited_paper":"/paper/1904.12186","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:d7bf4f076a29546324bac6fcca7216c824f26fa686608d3065e10cb59b1de6d1","observation_id":"bd5172db-a2ad-45bf-96ed-d0b772698cdc","resolution":{"observed_at":"2026-08-01T12:49:05.910471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04772","last_updated":"2018-01-15T12:36:00Z","snapshot_observed_at":"2026-08-04T10:26:52.692323Z","submitted_at":"2018-01-15T12:36:00Z","title":"Ten years of speckle interferometry at SOAR","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04772","snapshot_observed_at":"2026-08-01T12:49:06.124751Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:06.124751Z"},"links":{"cited_paper":"/paper/1801.04772","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:cda35393e3ac6aa4244f9f93d95c3d168ddcbeacf44a309f94a90cb2c4f88928","observation_id":"b0e96d01-d81a-4b96-b908-21b2d5ccc6be","resolution":{"observed_at":"2026-08-01T12:49:06.124751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10871","last_updated":"2019-11-11T14:46:43Z","snapshot_observed_at":"2026-07-06T08:17:29.632392Z","submitted_at":"2019-08-28T18:00:04Z","title":"SOAR TESS Survey. I: Sculpting of TESS planetary systems by stellar companions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.10871","snapshot_observed_at":"2026-08-01T12:49:06.247397Z","title":null,"venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-01T12:49:06.247397Z"},"links":{"cited_paper":"/paper/1908.10871","citing_paper":"/paper/2607.19325"},"observation_digest":"sha256:c7f80851784fd46d84fdd9f21cd7eb840f9776b656c154c8dc62991b9bf7647b","observation_id":"0c808acc-2bd3-4bec-a31d-5a8f79b4e6a2","resolution":{"observed_at":"2026-08-01T12:49:06.247397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.19325","last_updated":"2026-07-21T17:45:09Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-04T18:30:46.862550Z","submitted_at":"2026-07-21T17:45:09Z","title":"Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653"},"reference_resolution":{"displayed":89,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":1,"unresolved":87,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":89},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 89 of 89 outbound references and 0 inbound Pith citation observations for arXiv:2607.19325."}