{"as_of":"2026-08-16T14:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f56a86e8a28ef383f57dcc3b516d6068f3853d3d6b5a62af937b730bfcbf5084","coverage":[{"denominator":51,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":51,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T14:56:01.811776Z","state":"measured"},{"denominator":51,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":51,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+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/1908.02217/citation-record","integrity":"/paper/1908.02217/integrity","json":"/paper/1908.02217/citation-record.json","paper":"/paper/1908.02217"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:01.183738Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.183738Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:c6f4bcf138e1a9ec21f41789d132e0aa1dc277060b227f7ab18732a486c5c983","observation_id":"07e721e5-5adf-4d22-a01e-1800aa603b2c","resolution":{"observed_at":"2026-08-14T14:56:01.183738Z","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":"10.1007/978-3-319-30648-3_7-1","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:02.807695Z","title":"C., 2017, Transit-Timing and Duration Variations for the Discovery and Characterization of Exoplanets","venue":null,"work_id":"ec20575f-a1ab-47d8-9933-8df3c686573e","year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.191493Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:7c7b788a1e14208357b0602ef0662da28e9db4a8f508ed1ace2daca0191623c8","observation_id":"27c1d7da-780c-496f-8163-02608b146894","resolution":{"observed_at":"2026-08-14T14:56:02.813646Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:03.497589Z","title":"W., O'Neil M., 2014","venue":null,"work_id":"17e8ddb2-7367-4963-a81f-4aa759346447","year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.209551Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:6faac64f3633a2e7386f5be15553de8ec39743df8ebb55a9c15217cc5bdb566b","observation_id":"d108c1b5-8831-4d19-a991-6f27f1e2cdca","resolution":{"observed_at":"2026-08-14T14:56:03.504334Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.6992","last_updated":"2014-06-26T19:44:34Z","snapshot_observed_at":"2026-08-14T23:28:55.678799Z","submitted_at":"2014-06-26T19:44:34Z","title":"SPIRou: the near-infrared spectropolarimeter/high-precision velocimeter for the Canada-France-Hawaii telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.6992","snapshot_observed_at":"2026-08-14T14:56:01.219951Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.219951Z"},"links":{"cited_paper":"/paper/1406.6992","citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:24b71edb7992c321789c27c9f04a1065d98a6d8b8e5f2600ac53b5f8e69f0c81","observation_id":"b971b8b5-0eea-49a6-b7e0-528578c53fde","resolution":{"observed_at":"2026-08-14T14:56:01.219951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.ascom.2013.11.003","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:02.775061Z","title":"V., 2013, @doi [Astronomy and Computing] 10.1016/j.ascom.2013.11.003 , http://adsabs.harvard.edu/abs/2013A","venue":null,"work_id":"41076dbf-eff1-4158-bc7c-20881d72611b","year":2013},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.236978Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:d3016d56239b81a6f029e63dbc82dbad3c98805fa790a7dba59e51d1324b38e8","observation_id":"98e2a8b7-0261-4f97-9fa5-e5cc9fa95209","resolution":{"observed_at":"2026-08-14T14:56:02.790903Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-14T14:56:01.248300Z","title":"V., 2018, @doi [ ] 10.3847/1538-4365/aae3e9 , https://ui.adsabs.harvard.edu/abs/2018ApJS..239....2B 239, 2","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.248300Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:4ddcb75488acfbd7fe69ed223f5f35d2638c83b02d499191516a44ee69eb4be9","observation_id":"1de6854e-00ec-43b0-bc6e-bc5bad8467fb","resolution":{"observed_at":"2026-08-14T14:56:01.248300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:03.456153Z","title":"Online at <A href=``href=''>https://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=269</A>, id.69","venue":null,"work_id":"a727e358-1fc3-4f65-b756-16620421f952","year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.257119Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:e52287dc07c2f8ae5e0e76368506e3fa06d9ba16b8bbc01b67727e85ecc9e1e9","observation_id":"ab9b8157-c567-46bc-934f-3e962fee863b","resolution":{"observed_at":"2026-08-14T14:56:03.469997Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-14T14:56:01.263791Z","title":"A., Huber D., Gaidos E., van Saders J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.263791Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:92c9beb40d7ddb916629bc097be8bf211469e68265d6ee08ebfd3a46fcf45b20","observation_id":"cd2cb6e8-d5a2-4377-bf85-6336314ae1ed","resolution":{"observed_at":"2026-08-14T14:56:01.263791Z","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":"2026-08-14T14:56:01.270773Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.270773Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:34b414f80a6b41863332709c200ba75c3295c35929b53edcce71e78c94686c49","observation_id":"1f64f8e7-5c91-4f5e-8b23-c10649ec0583","resolution":{"observed_at":"2026-08-14T14:56:01.270773Z","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":"2026-08-14T14:56:01.278288Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.278288Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:43bc7f6a1edd2a1b6d7e07b4219b25af237a6a26270e7cf2c369ac8e8d575a50","observation_id":"7e99c59d-5893-454f-98ea-11c05f5d79b1","resolution":{"observed_at":"2026-08-14T14:56:01.278288Z","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":"10.1051/0004-6361/201732459","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:02.593737Z","title":null,"venue":null,"work_id":"448cc13f-9441-4109-b5a2-1cae04d1af76","year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.285315Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:46a9d0f41c8a080ac2919b77b7f4fba420a803355e7870d9d65b184725ea70da","observation_id":"89c0874e-3f3f-4ebd-ba26-abe907462bd9","resolution":{"observed_at":"2026-08-14T14:56:02.606658Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-14T14:56:01.299314Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.299314Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0e8544c317999848efde11c58ec86abf64084f3db32224a6d3157de67c93464a","observation_id":"01a739d6-0ccb-48fc-8993-285ec98efee9","resolution":{"observed_at":"2026-08-14T14:56:01.299314Z","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":"2026-08-14T14:56:01.307958Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.307958Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:d42a7b174b2e657567b1e4d12f9c3445d354d5fe744ae1e78bffa6392e009e2a","observation_id":"6aea13da-dc7c-41e7-8a7b-e8707794e01a","resolution":{"observed_at":"2026-08-14T14:56:01.307958Z","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":"2026-08-14T14:56:01.316690Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.316690Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:6ce588610c282f91660d81af8653c3e989a005fd9c98306a7b163d380eee2236","observation_id":"7ee0ffeb-385d-486e-9a70-2cb5ba0a4ccd","resolution":{"observed_at":"2026-08-14T14:56:01.316690Z","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":"2026-08-14T14:56:01.325542Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.325542Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:a31a52b074f4c9f5319a66f57ea636156102bc451419aa18d0adcc4405a57109","observation_id":"b4779758-01dd-4f33-bcd5-39afc37849c3","resolution":{"observed_at":"2026-08-14T14:56:01.325542Z","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":"2026-08-14T14:56:01.335413Z","title":"T., Hobson M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.335413Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:ae747f1260f8d329429338e28d25ccf533041c3c8d2bfd104c9c964133dc7c39","observation_id":"33110b7b-6e76-43f4-9a8d-6edabdb49658","resolution":{"observed_at":"2026-08-14T14:56:01.335413Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.2144","last_updated":"2019-11-26T18:54:07Z","snapshot_observed_at":"2026-08-06T09:48:22.577598Z","submitted_at":"2013-06-10T09:22:32Z","title":"Importance Nested Sampling and the MultiNest Algorithm","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.2144","snapshot_observed_at":"2026-08-14T14:56:01.353395Z","title":"P., Cameron E., Pettitt A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.353395Z"},"links":{"cited_paper":"/paper/1306.2144","citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:4cdc4d6f8cb4699e315418dde4279a61a9641bb33c87a4dd4962557534976790","observation_id":"78960491-7134-485d-be4b-03722693d23b","resolution":{"observed_at":"2026-08-14T14:56:01.353395Z","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":"2026-08-14T14:56:01.367456Z","title":"A., et al., 2016, @doi [ ] 10.1088/1538-3873/128/964/066001 , http://adsabs.harvard.edu/abs/2016PASP..128f6001F 128, 066001","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.367456Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:d0d2ed5975e71655ebebd5bb8ab19b685032fe803d14ed261d9d069a6826604a","observation_id":"f478ffae-dc52-4edf-96a9-9aba53a8dc8b","resolution":{"observed_at":"2026-08-14T14:56:01.367456Z","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":"2026-08-14T14:56:01.377465Z","title":"J., Petigura E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.377465Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:00803c17005419b1009a11dad85abaf02b7d83890c497caabcfcb6ae491fa955","observation_id":"e5f54fc3-d9d6-4052-b898-eb4d22e55d92","resolution":{"observed_at":"2026-08-14T14:56:01.377465Z","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":"2026-08-14T14:56:01.384685Z","title":"J., et al., 2017, @doi [ ] 10.3847/1538-3881/aa80eb , http://adsabs.harvard.edu/abs/2017AJ....154..109F 154, 109","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.384685Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:891d44c99d3a031ec21deb352a627bf27939dde3da23cb675b0e43478f47fa29","observation_id":"e66c8e91-3f23-4aec-b4d5-90751db10637","resolution":{"observed_at":"2026-08-14T14:56:01.384685Z","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":"2026-08-14T14:56:01.392428Z","title":"D., et al., 2018, @doi [ ] 10.3847/1538-3881/aab8f3 , http://adsabs.harvard.edu/abs/2018AJ....155..203H 155, 203","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.392428Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:ce03eaa7ca3caa00fc7a0fb3b95f65bb48c1a91f5fea37688aeedde4f94bcc13","observation_id":"79846bd7-9618-4098-90b8-ce99dd5d5bc6","resolution":{"observed_at":"2026-08-14T14:56:01.392428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.04413","last_updated":"2016-06-14T15:10:16Z","snapshot_observed_at":"2026-08-14T21:52:48.614888Z","submitted_at":"2016-06-14T15:10:16Z","title":"EXPRES: A Next Generation RV Spectrograph in the Search for Earth-like Worlds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.04413","snapshot_observed_at":"2026-08-14T14:56:01.406589Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.406589Z"},"links":{"cited_paper":"/paper/1606.04413","citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:384eca979dbef5cb47101add423b409475e77bcb1ca600b6f343a1e1dcdc18de","observation_id":"22547f2d-6e35-498b-ac65-8affed36bd47","resolution":{"observed_at":"2026-08-14T14:56:01.406589Z","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":"2026-08-14T14:56:01.414921Z","title":"D., Fortney J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.414921Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:aa31e7968850889b0f89980866bed686c024c577659c48a3dd4b5e13eab8092a","observation_id":"bab725de-060a-4f5d-8ffe-2edd8253f391","resolution":{"observed_at":"2026-08-14T14:56:01.414921Z","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":"2026-08-14T14:56:01.424740Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.424740Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:1cba57f431326458189373f6539120a2044e3e61892adc62ddc836c535d3dceb","observation_id":"bc1bc6a1-8dc3-412c-bc05-896f3975a2dc","resolution":{"observed_at":"2026-08-14T14:56:01.424740Z","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":"2026-08-14T14:56:01.433399Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.433399Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0487605d47b908bb0e2b29f824580ba4f4d094e2959a7cdbaec003cf83fe9962","observation_id":"b42f11e8-e6fd-41ce-888d-8a6048f564bb","resolution":{"observed_at":"2026-08-14T14:56:01.433399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.00497","last_updated":"2016-09-02T08:13:15Z","snapshot_observed_at":"2026-08-14T21:41:39.609127Z","submitted_at":"2016-09-02T08:13:15Z","title":"EELT-HIRES the high-resolution spectrograph for the E-ELT","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.00497","snapshot_observed_at":"2026-08-14T14:56:01.440836Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.440836Z"},"links":{"cited_paper":"/paper/1609.00497","citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:4d40e4a3edc260204b5b2cc14117abdd8e1205b50185032c22ddf6efd22bf15b","observation_id":"e3687b08-0f55-4a0f-bf6c-619319c27030","resolution":{"observed_at":"2026-08-14T14:56:01.440836Z","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":"2026-08-14T14:56:01.465719Z","title":"S., et al., 2018, @doi [ ] 10.1051/0004-6361/201732143 , http://adsabs.harvard.edu/abs/2018A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.465719Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0866c2140fb450e780a80e256fc5bc46777f739d56763f481022d1755da87acc","observation_id":"287bfad7-ae66-4d05-a224-ecfe7ddd6c7d","resolution":{"observed_at":"2026-08-14T14:56:01.465719Z","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":"2026-08-14T14:56:01.475422Z","title":"P., Correia C","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.475422Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:2c21d4d4e4e2696afd8eac5d07d216b0b9849a6da1cc66e7954ad79494c041c8","observation_id":"25798088-e350-4167-a5c7-810397d0569e","resolution":{"observed_at":"2026-08-14T14:56:01.475422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04683","last_updated":"2019-10-28T00:04:52Z","snapshot_observed_at":"2026-08-14T19:04:34.905145Z","submitted_at":"2018-06-12T18:00:02Z","title":"Quantifying the Bayesian Evidence for a Planet in Radial Velocity Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.04683","snapshot_observed_at":"2026-08-14T14:56:01.482802Z","title":"E., Ford E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.482802Z"},"links":{"cited_paper":"/paper/1806.04683","citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:d83c3fd3170278db546b3ded8d6fb53bff289fbd56a188532e5c44ad0405fe9d","observation_id":"d8d1bb43-52dc-4b9a-9a3c-e9bf1ceff744","resolution":{"observed_at":"2026-08-14T14:56:01.482802Z","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":"2026-08-14T14:56:01.491540Z","title":"E., 2019, @doi [Annual Review of Earth and Planetary Sciences] 10.1146/annurev-earth-053018-060246 , https://ui.adsabs.harvard.edu/abs/2019AREPS..47...67O 47, 67","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.491540Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:24a7be0c4bf8ce686c0634192ef1bfade6b347a47d88de34bdfc567e227d3105","observation_id":"9fbdf219-b2df-4f34-a15c-8aa0362caaa6","resolution":{"observed_at":"2026-08-14T14:56:01.491540Z","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":"2026-08-14T14:56:01.498405Z","title":"E., Wu Y., 2013, @doi [ ] 10.1088/0004-637X/775/2/105 , http://adsabs.harvard.edu/abs/2013ApJ...775..105O 775, 105","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.498405Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:edd9ce07c93aad89bb005175b1b0403aecfea7b05cebc00c33c3feff669bd036","observation_id":"1a7b744a-089e-43dc-9e80-426e13814753","resolution":{"observed_at":"2026-08-14T14:56:01.498405Z","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":"2026-08-14T14:56:01.508687Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.508687Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:1a2c20912ea8435e3c03cab51eb77b80186db7fdd33e612f9b4afecf5cdca03c","observation_id":"8e79783e-8adb-4cb4-80dd-bea246d1c9ef","resolution":{"observed_at":"2026-08-14T14:56:01.508687Z","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":"10.1051/0004-6361/201731307","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:02.221766Z","title":null,"venue":null,"work_id":"637a4cc4-d17f-4ebb-91a6-a48721819307","year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.519240Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:66f518297338572ab6efd546164208d72f5e3b93a0f600249afef2939f058291","observation_id":"8826d682-2843-4271-84c4-788bc086b955","resolution":{"observed_at":"2026-08-14T14:56:02.232971Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-14T14:56:01.529757Z","title":"S., Damasso M., 2017, @doi [ ] 10.1093/mnras/stx664 , http://adsabs.harvard.edu/abs/2017MNRAS.468.3775P 468, 3775","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.529757Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:f53d11c1f4593bf6ed1dfe425724e84d0d39cc6d48f33e82eb3c57156fd0d932","observation_id":"6fffa1e3-beb8-4920-9c30-f24c42fd7529","resolution":{"observed_at":"2026-08-14T14:56:01.529757Z","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":"2026-08-14T14:56:01.543401Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.543401Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:b5657a0d663f36f223aaa9d538cd6ee3e7a47963ba92b55b5bc4822abbcf74a0","observation_id":"30513235-eb13-466f-91cc-db9f67296e27","resolution":{"observed_at":"2026-08-14T14:56:01.543401Z","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":"2026-08-14T14:56:01.565740Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.565740Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:de6feffaebf1465160e4c84ee685967cb9b0cecaebee14a2a3e3f46271b8531e","observation_id":"7e34ccae-23cd-4233-9d82-2d8a11bec79b","resolution":{"observed_at":"2026-08-14T14:56:01.565740Z","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":"2026-08-14T14:56:01.584605Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.584605Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:e63487693ec73aef9985da706edf0e8d2d0fe44fc945ce874d9896e4abed3b8b","observation_id":"cf7b48f0-4675-43cb-8b1d-82727a774f37","resolution":{"observed_at":"2026-08-14T14:56:01.584605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:03.390021Z","title":"C., Mayor M., Naef D., Pepe F., Queloz D., Udry S., Blecha A., 2000, , http://adsabs.harvard.edu/abs/2000A","venue":null,"work_id":"3f747ec8-ac66-4dd5-9206-9fa643d7ce39","year":2000},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.598573Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0fd81c888b391aaa69c2108a471daf6b77febea62fc7dc32d16f24c4f3f7aec6","observation_id":"f047596d-9121-4455-aad9-3b92b7761a1a","resolution":{"observed_at":"2026-08-14T14:56:03.400455Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-14T14:56:01.609728Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.609728Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:212f602805afad50b1ffc8c366226f8b37c0ded535b1bd8d63bd2b0c50187c3c","observation_id":"f35480c4-5755-4af1-ab8b-afce3c57e9e1","resolution":{"observed_at":"2026-08-14T14:56:01.609728Z","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":"2026-08-14T14:56:01.620953Z","title":"P., 2016, @doi [ ] 10.1093/mnras/stw1936 , http://adsabs.harvard.edu/abs/2016MNRAS.463.1844S 463, 1844","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.620953Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:f047c3fe3666134135e6e86171d2a215f39b07e8c9baf544e1c1df0dc51d4408","observation_id":"fb216e0a-e1fc-4645-85f5-383d91bc2c45","resolution":{"observed_at":"2026-08-14T14:56:01.620953Z","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":"2026-08-14T14:56:01.655974Z","title":"I., Esposito M., 2017, @doi [ ] 10.1093/mnras/stx771 , http://adsabs.harvard.edu/abs/2017MNRAS.468.4772S 468, 4772","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.655974Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:b0d7d7f1565d2b90af9de1ec3944e40db84c88ff1cfc3310aa6de66c6af8b665","observation_id":"f27e9886-f490-4c05-8163-cf08dc06b59c","resolution":{"observed_at":"2026-08-14T14:56:01.655974Z","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":"2026-08-14T14:56:01.663832Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.663832Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:e73c7821cb4d76963ec6c7ff230822cf5b5061e679ddea0e229898d514fc1ac2","observation_id":"0bcadbed-8847-4193-884b-c514664f9b13","resolution":{"observed_at":"2026-08-14T14:56:01.663832Z","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":"2026-08-14T14:56:01.675096Z","title":"A., Ciardi D","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.675096Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:80096fd577925cb1f7da89bcb3739ef3672138b58bae07d5590ece0cca225038","observation_id":"201ca115-3f8e-4831-9a9c-26a566e7e622","resolution":{"observed_at":"2026-08-14T14:56:01.675096Z","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":"2026-08-14T14:56:01.689498Z","title":"M., Marcy G","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.689498Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0ec566e8b912aa3e770227b79c49cd501930ed8463223070522f7e717a05b47b","observation_id":"0168cb3b-b605-4e2d-9226-8c8724ad92bc","resolution":{"observed_at":"2026-08-14T14:56:01.689498Z","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":"2026-08-14T14:56:01.702030Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.702030Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:71d53ad78e2cf3f1d6d8bc3be718b71fdc4bdc6f9ecdc570d2cf4f0ca6d50c79","observation_id":"59b0772a-62d5-4778-9d5e-d57a88ccf019","resolution":{"observed_at":"2026-08-14T14:56:01.702030Z","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":"2026-08-14T14:56:01.708442Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.708442Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:174b1363b75d4e3bc73412a7ca013b9eb0ed5cfd77317f83b6aa3f33a03e6bec","observation_id":"06f05c37-cd8d-4065-a5eb-59ca6739078f","resolution":{"observed_at":"2026-08-14T14:56:01.708442Z","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":"2026-08-14T14:56:01.717365Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.717365Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:112d62a60a25121cd1b3051cc8c4f3c7c0e9fdd9fb32ce4326743ceb1e4484c0","observation_id":"11e5c48a-fc89-4496-80c8-2d40df4fe93e","resolution":{"observed_at":"2026-08-14T14:56:01.717365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:03.359723Z","title":null,"venue":null,"work_id":"8c7a0f75-8f7b-4d14-9b06-4687ef9ca7f2","year":2017},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.766671Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:7015861c86ddd24c107507711aeb1e8e364fc2ed320291265503c8a053f311d0","observation_id":"c839a88d-aa01-4246-8267-88171862b029","resolution":{"observed_at":"2026-08-14T14:56:03.368833Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:03.324661Z","title":null,"venue":null,"work_id":"d79f8b67-0834-4f58-bdb7-d5b53339ddef","year":2019},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.790558Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0eab53954451f464f992a04209822954d892ff925acb9d6299a5d9e7ae55b33f","observation_id":"c43c985e-e420-436f-bc13-205f8e592fa4","resolution":{"observed_at":"2026-08-14T14:56:03.333263Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:56:03.290340Z","title":"B., Sasselov D","venue":null,"work_id":"a5992e77-ac2c-4ea5-8c8f-df3d80ebea25","year":null},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.803254Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:8d2568030feacfd38d9985e4a451f843214d898e7c2a000afef23bf3e0bedcd6","observation_id":"ce29b828-2828-4d4b-8990-8da73774a0d8","resolution":{"observed_at":"2026-08-14T14:56:03.300252Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-14T14:56:01.811776Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-14T14:56:01.811776Z"},"links":{"citing_paper":"/paper/1908.02217"},"observation_digest":"sha256:0dd8be2b31995aded3bffd88768c3f79e93209ecb9f5e5c73c95c014f3f7f22c","observation_id":"74dede57-4d0d-479b-a881-15ec5763c3da","resolution":{"observed_at":"2026-08-14T14:56:01.811776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.02217","last_updated":"2019-08-06T15:38:48Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-16T05:23:00.207689Z","submitted_at":"2019-08-06T15:38:48Z","title":"Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity"},"reference_resolution":{"displayed":51,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":43,"verified_exact":4,"verified_fuzzy":4},"total_outbound_references":51},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 0 inbound Pith citation observations for arXiv:1908.02217."}