{"as_of":"2026-08-16T15:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cfb7154a19a0377dd3ee35c81984d292be594785f1e380c8ad2fc7d2ecbddc90","coverage":[{"denominator":171,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T17:26:49.814438Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"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/2508.12963/citation-record","integrity":"/paper/2508.12963/integrity","json":"/paper/2508.12963/citation-record.json","paper":"/paper/2508.12963"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201425314","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:28:46.259735Z","title":"V., 2015, @doi [ ] 10.1051/0004-6361/201425314 , https://ui.adsabs.harvard.edu/abs/2015A&A...576A..34A 576, A34","venue":null,"work_id":"2186cccb-24da-4be5-98a8-4eacbe401f1f","year":2015},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.361167Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:f5054cd250a6e5c7a405fd15bd6dc4b9fc27375d35ec337202c3e69bb7bc5887","observation_id":"98cdea94-eee5-466b-bd38-76d3964846f5","resolution":{"observed_at":"2026-08-15T17:28:46.264510Z","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":{"arxiv_id":"2209.08940","last_updated":"2022-11-10T15:33:49Z","snapshot_observed_at":"2026-08-16T00:37:07.834861Z","submitted_at":"2022-09-19T11:49:41Z","title":"Gaussian Process regression for astronomical time-series","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.08940","snapshot_observed_at":"2026-08-15T17:26:49.366834Z","title":"arXiv:2209.08940","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.366834Z"},"links":{"cited_paper":"/paper/2209.08940","citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:822595cdb4f963c1863b2dad9cd57c770d49e4d7094827b6b38e9c5e11471d5b","observation_id":"59cb8a44-e7ec-4669-a557-a943476f424f","resolution":{"observed_at":"2026-08-15T17:26:49.366834Z","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":"2026-08-15T17:26:49.371800Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.371800Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:97cbe1973cca0417ef45b30b20cd4b40d1639b488f9b868d17071463fd086bf2","observation_id":"6d578c74-5247-4d7f-8ab3-d67bc9b76ef4","resolution":{"observed_at":"2026-08-15T17:26:49.371800Z","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":"2026-08-15T17:26:49.376569Z","title":"A., 2022, @doi [ ] 10.1051/0004-6361/202243276 , https://ui.adsabs.harvard.edu/abs/2022A&A...664A..34A 664, A34","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.376569Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:acd770d1a47e938877bb6b70aa13e6cf25dee5500c9da2f6c9880b74b776b3ed","observation_id":"93d7822e-2ef9-45d6-aa7d-4bcdf58eab59","resolution":{"observed_at":"2026-08-15T17:26:49.376569Z","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":"2026-08-15T17:26:49.381564Z","title":"C., Wildi F., 2023, @doi [ ] 10.1051/0004-6361/202244663 , https://ui.adsabs.harvard.edu/abs/2023A&A...669A..39A 669, A39","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.381564Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:e457d40819d836a81b2ad801f711cec6666cc847cc6b9d8f8285f147f3005ffa","observation_id":"342b4d61-8e95-4281-b55e-ab6eaf99c6a4","resolution":{"observed_at":"2026-08-15T17:26:49.381564Z","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":"2026-08-15T17:26:49.386386Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.386386Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:be7aafbb0a50b54d8374f5b387f8603750693ffdd1ac55fd48db493bc8c0dde7","observation_id":"221e750e-4c11-4a50-be82-78f5011d9042","resolution":{"observed_at":"2026-08-15T17:26:49.386386Z","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":"10.1051/0004-6361/202142027","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:28:46.218030Z","title":"J., Kochukhov O., 2022, @doi [ ] 10.1051/0004-6361/202142027 , https://ui.adsabs.harvard.edu/abs/2022A&A...658A.162A 658, A162","venue":null,"work_id":"36f2e158-e678-42bf-8384-36c2099529c9","year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.391693Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:3a5d9fb256ef8ee2dcf06e48e89797774a1108b593d0b2e0fb99464bbe10956f","observation_id":"787365f4-2a33-4f71-b2ae-f3d5c1aa98a1","resolution":{"observed_at":"2026-08-15T17:28:46.222732Z","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":"2026-08-15T17:26:49.396130Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.396130Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:b7e8752bfe828120c9b646cb90239202cc9c3d36a9fcbafac86b67dacea71343","observation_id":"c6c069b1-3900-4fbe-8e7a-58ce180e1da2","resolution":{"observed_at":"2026-08-15T17:26:49.396130Z","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":"2026-08-15T17:26:49.401396Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.401396Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:0229876ce001db755d5ce91a6c197f33f1b682b9808ea3b5cd5ed2b13700c4c7","observation_id":"0be012dc-b186-4e38-838d-20436188a574","resolution":{"observed_at":"2026-08-15T17:26:49.401396Z","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":"2026-08-15T17:26:49.405936Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.405936Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:82cf0f8d80d67ea7a76e160c899d9809ab64f285e882a2f25a7debd01ec9f2f8","observation_id":"ea09edf8-e559-4511-9d11-5f15c068833d","resolution":{"observed_at":"2026-08-15T17:26:49.405936Z","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":"2026-08-15T17:26:49.410290Z","title":"A., Landstreet J","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.410290Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:c90133311609de3a4bf898cd77c601f1c0aa919a4e3095ac0dd51c46eca41f1b","observation_id":"7dc85ea3-ad28-486e-b545-c843807615cb","resolution":{"observed_at":"2026-08-15T17:26:49.410290Z","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":"2026-08-15T17:26:49.418363Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.418363Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:ec69edbc543feac1136c937ef0e65196ce24496f94945d5fcdb0af15cc0db37d","observation_id":"eb0e8e1c-fceb-43b2-bb45-b9bdee558ab6","resolution":{"observed_at":"2026-08-15T17:26:49.418363Z","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":"2026-08-15T17:26:49.422745Z","title":"M., Zicher N., 2022a, @doi [ ] 10.1093/mnras/stab2889 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.509..866B 509, 866","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.422745Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:7aaea76ce19053036d5b956c83c7189a1b52c0b1cda64b0534050f38c8291ea8","observation_id":"245b0ebd-7b0e-42f8-a167-7707a17ff762","resolution":{"observed_at":"2026-08-15T17:26:49.422745Z","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":"10.1093/mnras/stac638","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:28:46.160692Z","title":null,"venue":null,"work_id":"79e1709d-6d0b-41cb-8c8c-449b2537656b","year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.427288Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:3332b7b33a7b2e40b7d1987afbcf0fa523f7462f0ecda71d68768bcaf6f8b1d6","observation_id":"bfe71696-88d4-4a60-abee-923199f4be29","resolution":{"observed_at":"2026-08-15T17:28:46.166352Z","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":"2026-08-15T17:26:49.431734Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.431734Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:518b235b157d7b7b29071865e67b7f06d8fb781a66cd131a8be8c4b14f946a57","observation_id":"2025a26f-f14c-4795-85a5-e1a2fe225636","resolution":{"observed_at":"2026-08-15T17:26:49.431734Z","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":"10.1051/0004-6361/202141812","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:28:46.141942Z","title":null,"venue":null,"work_id":"b5b2d711-9f69-4e19-8dce-2def7e8870a9","year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.436156Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:9a6d55964fd2b6969dfaa82bcde59b842aaad81a49f16f111b91f51a235626fc","observation_id":"ef858fa0-1da3-45d3-82d2-2e5c99a2b669","resolution":{"observed_at":"2026-08-15T17:28:46.145883Z","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":"2026-08-15T17:26:49.440715Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.440715Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:70063699d5c615b8520480fcd785d622d47b61a170f34ee6de1f07466aed4bce","observation_id":"2e55d9d1-e78d-4265-80ad-a01e9e25904f","resolution":{"observed_at":"2026-08-15T17:26:49.440715Z","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":"2026-08-15T17:26:49.444923Z","title":"V., 2005, @doi [Living Reviews in Solar Physics] 10.12942/lrsp-2005-8 , https://ui.adsabs.harvard.edu/abs/2005LRSP....2....8B 2, 8","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.444923Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:ee612741268c6edf47a2775f5a5abdae304e6e4f067b599c1aad2df81ba754ba","observation_id":"aea06a2f-85e5-4f86-bb4d-f29de8efe53d","resolution":{"observed_at":"2026-08-15T17:26:49.444923Z","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":"2026-08-15T17:26:49.448961Z","title":"T., et al., 2020, @doi [ ] 10.3847/1538-3881/ab811d , https://ui.adsabs.harvard.edu/abs/2020AJ....159..238B 159, 238","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.448961Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:78cf90345ea66e515237f547b5eb72130a750a6ec34d10441c1f103f6c0656c3","observation_id":"de6e96e6-6ec7-4d06-a25f-75196a591050","resolution":{"observed_at":"2026-08-15T17:26:49.448961Z","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":"2026-08-15T17:26:49.453576Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.453576Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:1a1d7836c53e2d6ee4f3d35af7ccb3390232a47f80572dfb6ff2f141ec633af7","observation_id":"4fd1ccd4-4e04-41f1-8e13-a0a5d89c5700","resolution":{"observed_at":"2026-08-15T17:26:49.453576Z","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":"2026-08-15T17:26:49.457967Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.457967Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:13c22cf606c4281bc90a83fa5b5c02154188a25da333171b96a04408248b1dea","observation_id":"490916cc-295f-4642-aff4-95f9c135bff5","resolution":{"observed_at":"2026-08-15T17:26:49.457967Z","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":"2026-08-15T17:26:49.462180Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.462180Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:4e74bcc942f5c2d5c7a666847d6793f939e34c6054c508c58b11ce833d7bd9a6","observation_id":"d56d927a-d7f4-4444-8ca1-ba26cb0fa2c2","resolution":{"observed_at":"2026-08-15T17:26:49.462180Z","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":"2026-08-15T17:26:49.466713Z","title":"M., et al., 2020, @doi [ ] 10.3847/1538-3881/ab99c9 , https://ui.adsabs.harvard.edu/abs/2020AJ....160...67B 160, 67","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.466713Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:b9622cfc1178d19f8a5470b98ed5155158e502914b2a197ad24acad9c1df20e8","observation_id":"993b1c0d-9f75-4261-a655-9e90f59a11cb","resolution":{"observed_at":"2026-08-15T17:26:49.466713Z","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":"2026-08-15T17:26:49.471101Z","title":"F., Donati J","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.471101Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:8bcbe3463eef40e4ec055abe8a1f0149716e9ca9550c76cc5a06059dc30ce617","observation_id":"2d5cf8cb-1677-42c0-b515-c50ca32d9273","resolution":{"observed_at":"2026-08-15T17:26:49.471101Z","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":"2026-08-15T17:26:49.475557Z","title":"S., Browning M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.475557Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:b49e72ee92e47cae09081e91cf65545e86d2044a6669d392e4fea633783142d6","observation_id":"59a81c45-5597-4ed9-a615-634b226b578e","resolution":{"observed_at":"2026-08-15T17:26:49.475557Z","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":"2026-08-15T17:26:49.480080Z","title":"R., et al., 2024, @doi [Nature Astronomy] 10.1038/s41550-024-02405-6 , https://ui.adsabs.harvard.edu/abs/2024NatAs...8.1359C 8, 1359","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.480080Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:96d0b46bfaee697784860b9078d66278d99a52fd043190fc2a034555daf8738c","observation_id":"528977fa-e22c-42dd-a900-19aaa2e22142","resolution":{"observed_at":"2026-08-15T17:26:49.480080Z","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":"2026-08-15T17:26:49.484473Z","title":"J., Cegla H","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.484473Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:fa8b6ebe639b37e9f3dc06c6aba782f087c56808541267d39d339fc85fc75768","observation_id":"926434d0-eb4e-410f-96e3-f92a62ddc869","resolution":{"observed_at":"2026-08-15T17:26:49.484473Z","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":"2026-08-15T17:26:49.488833Z","title":"H., Witte S., 2013, @doi [ ] 10.1051/0004-6361/201220942 , https://ui.adsabs.harvard.edu/abs/2013A&A...552A..16C 552, A16","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.488833Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:c2a07cd71053666cbde347fc38a9ee56afacc3ba162a6c3648808b1e9623b937","observation_id":"253c3641-2e49-47e2-919c-5b619dbb270d","resolution":{"observed_at":"2026-08-15T17:26:49.488833Z","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":"2026-08-15T17:26:49.493231Z","title":"C., 1994, @doi [ ] 10.1093/mnras/269.3.814 , https://ui.adsabs.harvard.edu/abs/1994MNRAS.269..814C 269, 814","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.493231Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:970d04fa9b0e21a9a3e6bf25f8bb5912619f1cbb163f4a73b35e390549a0dfee","observation_id":"4926e777-77be-436f-8b56-10567b8cc2be","resolution":{"observed_at":"2026-08-15T17:26:49.493231Z","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":"2026-08-15T17:26:49.497537Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.497537Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:621a0a128effc662cdbcc46b51ebefada59dc8aa6f65ab703b4ee3fbc5c8f8d8","observation_id":"ce3a0a9a-9341-4c9b-9a54-6b7699abaabc","resolution":{"observed_at":"2026-08-15T17:26:49.497537Z","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":"2026-08-15T17:26:49.501878Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.501878Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:49e72079cea9abaf81cf73ed01b552ac1249be8da97a14dbb09c954b69a5dd15","observation_id":"836e44df-5768-452f-92cd-df9f10a77356","resolution":{"observed_at":"2026-08-15T17:26:49.501878Z","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":"2026-08-15T17:26:49.506105Z","title":"S., Ramsay S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.506105Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:fdda4a6dbab8143f1f0312e2fe07bb46704172d1dbfa428afb2cf20ea106d1bc","observation_id":"3fb7787e-14ba-454a-bb57-ccae32b6b3f4","resolution":{"observed_at":"2026-08-15T17:26:49.506105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.14291","last_updated":"2021-07-29T19:29:59Z","snapshot_observed_at":"2026-08-09T07:29:42.262804Z","submitted_at":"2021-07-29T19:29:59Z","title":"Extreme Precision Radial Velocity Working Group Final Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.14291","snapshot_observed_at":"2026-08-15T17:26:49.510670Z","title":"arXiv:2107.14291","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.510670Z"},"links":{"cited_paper":"/paper/2107.14291","citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:83b742f06df17338f7c73cb0992b0c8fe0166fa855fc56d83a4c781a14712257","observation_id":"abda74f5-af82-47b5-8c86-e2588199d93f","resolution":{"observed_at":"2026-08-15T17:26:49.510670Z","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":"2026-08-15T17:26:49.515224Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.515224Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:de7255d72937079c310470c61d5b55c9b2c89823a2ac8a7f809f51d2fe8b5f0d","observation_id":"33561a37-59be-48f3-a8bd-a5d2b778b322","resolution":{"observed_at":"2026-08-15T17:26:49.515224Z","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":"2026-08-15T17:26:49.519372Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.519372Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:140c73e5999f95fe4d8261616315aecda5c335ddbb4b34505c2b1f63deb21dd1","observation_id":"115ab60a-4130-4e59-ba14-747fab154b6c","resolution":{"observed_at":"2026-08-15T17:26:49.519372Z","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":"2026-08-15T17:26:49.523855Z","title":"C., Pepe F., 2021, @doi [ ] 10.1051/0004-6361/202140986 , https://ui.adsabs.harvard.edu/abs/2021A&A...653A..43C 653, A43","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.523855Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:e3570bf01ade666f0bdcfffa8eb407523d17cbd664e91c565c04f9a223648653","observation_id":"671b9faa-e5ba-4556-b869-95bc86ea2ecb","resolution":{"observed_at":"2026-08-15T17:26:49.523855Z","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":"2026-08-15T17:26:49.528052Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.528052Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:0d5c1090f66ac1b0335bf73621c8fe5f37d088e20f7cc59a0c6fe45e4fc13101","observation_id":"2c8c6dbb-722b-4239-8647-5ef48da71014","resolution":{"observed_at":"2026-08-15T17:26:49.528052Z","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":"2026-08-15T17:26:49.531988Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.531988Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:5adfb4772f6cc868605770e44a5c997fa8a3fda991722e2e016075f81deee626","observation_id":"2969910e-9a49-4458-9b92-d3b62b0e955f","resolution":{"observed_at":"2026-08-15T17:26:49.531988Z","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":"2026-08-15T17:26:49.536115Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.536115Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:317e4cc8a8d7896b6a980e27fe00ba6484a4acd8693965cbff1b3c388b5bb149","observation_id":"3a9eff57-f50b-40d9-8f69-1556c6650bbd","resolution":{"observed_at":"2026-08-15T17:26:49.536115Z","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":"2026-08-15T17:26:49.540316Z","title":"B., Unger N., Hara N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.540316Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:884d087008558e660d10fb62fb2a8c9cf90d559d29eadd692b9d05ba36b013b2","observation_id":"cff4d86c-7f41-41f9-8582-05aedd3d2c08","resolution":{"observed_at":"2026-08-15T17:26:49.540316Z","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":"2026-08-15T17:26:49.544563Z","title":"M., Galland F., Udry S., Mayor M., 2007, @doi [ ] 10.1051/0004-6361:20078144 , https://ui.adsabs.harvard.edu/abs/2007A&A...473..983D 473, 983","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.544563Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:0730d3dae145300f3418483d53b9d6b7e5f86cbe379fe12e0667ae73ab7a544d","observation_id":"62d6207b-6c92-42e4-a6cc-59e135f6ced7","resolution":{"observed_at":"2026-08-15T17:26:49.544563Z","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":"2026-08-15T17:26:49.548935Z","title":"F., 1999, @doi [ ] 10.1046/j.1365-8711.1999.02096.x , https://ui.adsabs.harvard.edu/abs/1999MNRAS.302..457D 302, 457","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.548935Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:4eec3d2677ff9247e2cb07ce7da5a894a571e6cd09d1204be68401e8dbdca798","observation_id":"b0c1f98f-6e49-49f3-a13e-fc5c586d6f94","resolution":{"observed_at":"2026-08-15T17:26:49.548935Z","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":"2026-08-15T17:26:49.553102Z","title":"F., Brown S","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.553102Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:37117fb3ba2a87b28bd0d3cf0a4ccafd92ebe960e857ad5ef0818ca0e8f74eff","observation_id":"4b540b03-909a-4414-a828-24fe09118845","resolution":{"observed_at":"2026-08-15T17:26:49.553102Z","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":"2026-08-15T17:26:49.557529Z","title":"F., Landstreet J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.557529Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:cccc479be6f7c9a1a82a3dc3cfddef5377aeeeb642b63a6395791b2714af2808","observation_id":"9a9216a3-fd14-4b0d-bb1c-aa0829905c70","resolution":{"observed_at":"2026-08-15T17:26:49.557529Z","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":"2026-08-15T17:26:49.561761Z","title":"F., Semel M., Praderie F., 1989, , https://ui.adsabs.harvard.edu/abs/1989A&A...225..467D 225, 467","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.561761Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:6fe8d82ee59ffaa68c00015ff8e1ba3420a16c52cb16e0b0ffe4b00c55a676e9","observation_id":"be7f6e7c-9355-466f-91ea-78ef822d9b60","resolution":{"observed_at":"2026-08-15T17:26:49.561761Z","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":"2026-08-15T17:26:49.565946Z","title":"F., Henry G","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.565946Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:70a64311a3f2da07855b48348ebefcb65b3fd8cf0151f4a1fc848fc62bed45f4","observation_id":"0e50ee28-41bd-4c87-8136-4333bbccbd30","resolution":{"observed_at":"2026-08-15T17:26:49.565946Z","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":"2026-08-15T17:26:49.570141Z","title":"F., Semel M., Carter B","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.570141Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:9f067fe1b3e93b09e662296932dffa0d35130fdcde03f4e72ede580891c07f9f","observation_id":"2cadde91-697b-4c42-8e86-29294d10c885","resolution":{"observed_at":"2026-08-15T17:26:49.570141Z","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":"2026-08-15T17:26:49.574624Z","title":"F., Mengel M., Carter B","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.574624Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:477ffbc9fc62e7d28b6c889e607231dae25d3d0ab69edc3517dcdd02428614d3","observation_id":"8a09647c-53f4-4767-8195-3b694e3b84da","resolution":{"observed_at":"2026-08-15T17:26:49.574624Z","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":"2026-08-15T17:26:49.584124Z","title":"F., et al., 2003, @doi [ ] 10.1046/j.1365-2966.2003.07031.x , https://ui.adsabs.harvard.edu/abs/2003MNRAS.345.1145D 345, 1145","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.584124Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:4c65b6ccb578ee6df2ce2003fcb9c180d25f48527ef71693a380d28440937edf","observation_id":"40458051-5528-4ca3-90f5-798a07fa9fab","resolution":{"observed_at":"2026-08-15T17:26:49.584124Z","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":"2026-08-15T17:26:49.588481Z","title":"F., Howarth I","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.588481Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:da678eff5cb3de2c97ea212d3e8ef51b5b5960672b4f9c1472d7e94089078895","observation_id":"d85c0c48-5d5f-4d1d-8ef6-f327a2588db2","resolution":{"observed_at":"2026-08-15T17:26:49.588481Z","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":"2026-08-15T17:26:49.592762Z","title":"F., et al., 2006b, @doi [ ] 10.1111/j.1365-2966.2006.10558.x , https://ui.adsabs.harvard.edu/abs/2006MNRAS.370..629D 370, 629","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.592762Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:113ac1606faed969456107e8d4f076706dd94fbc153b69ecb62f4dda22142a58","observation_id":"8945428b-6ac1-4197-a68a-83233ea01574","resolution":{"observed_at":"2026-08-15T17:26:49.592762Z","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":"2026-08-15T17:26:49.601123Z","title":"F., et al., 2012, @doi [ ] 10.1111/j.1365-2966.2012.21482.x , https://ui.adsabs.harvard.edu/abs/2012MNRAS.425.2948D 425, 2948","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.601123Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:78b9844a6590e8787cf266a6e7c2620f6f8a5db59dea4f4b0439ab315e72a5eb","observation_id":"5558d3c3-ab6e-459d-af3c-6ae8a7475e62","resolution":{"observed_at":"2026-08-15T17:26:49.601123Z","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":"2026-08-15T17:26:49.605396Z","title":"F., et al., 2014, @doi [ ] 10.1093/mnras/stu1679 , https://ui.adsabs.harvard.edu/abs/2014MNRAS.444.3220D 444, 3220","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.605396Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:c0aa5d56d25a82fe36d60ccf51035a79ff49e9002f60b688ac384ab0f27cacb7","observation_id":"90916399-d7b2-453a-89ef-4bc3c096eb3c","resolution":{"observed_at":"2026-08-15T17:26:49.605396Z","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":"2026-08-15T17:26:49.609602Z","title":"F., et al., 2017, @doi [ ] 10.1093/mnras/stw2904 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.465.3343D 465, 3343","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.609602Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:12a77c13b37c24db79f0c64ce335bf884a3c14dbdf987c6fff6295339f854381","observation_id":"3d306b43-f58b-4b32-98d8-7315f7210467","resolution":{"observed_at":"2026-08-15T17:26:49.609602Z","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":"2026-08-15T17:26:49.614126Z","title":"F., et al., 2023, @doi [ ] 10.1093/mnras/stad1193 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525..455D 525, 455","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.614126Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:965f9d02f64fbac29ed49edd54f2761e42ccdae84b67ad758ec961455a803a72","observation_id":"83458952-0ae1-4034-b52e-a7088e5a311f","resolution":{"observed_at":"2026-08-15T17:26:49.614126Z","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":"2026-08-15T17:26:49.618313Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.618313Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:e4098021f6847e0bf77adbcd62c0b18a4594d52cd4f63dc8a299ba8bb2fa8c56","observation_id":"0d9418eb-0465-4d4c-af52-9c699abb2ebc","resolution":{"observed_at":"2026-08-15T17:26:49.618313Z","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":"2026-08-15T17:26:49.622767Z","title":"C., Monteiro M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.622767Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:1c8083df044a618383f28940c04f75b6bab1d770f58f3bfd718543e969ae06d4","observation_id":"100072dc-82e1-4aaf-ba2c-2f350d2fdd03","resolution":{"observed_at":"2026-08-15T17:26:49.622767Z","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":"2026-08-15T17:26:49.627240Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.627240Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:14dc6e8edc8cc5228868490eeeb2a110b788e00a69878b65c3eb149a70bcf233","observation_id":"ec2ae642-38fd-4191-b7d1-011a56eb8ef7","resolution":{"observed_at":"2026-08-15T17:26:49.627240Z","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":"2026-08-15T17:26:49.632012Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.632012Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:89e6bec212cb8bd1e3d4244422421cd74111868e90d3dcda0554e23879d33520","observation_id":"5a9fa401-22df-4f8a-b977-35e59068d26d","resolution":{"observed_at":"2026-08-15T17:26:49.632012Z","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":"2026-08-15T17:26:49.636233Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.636233Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:f5d21daca714e3d3dca696e7cd899911f449dba8f3c0b997a8d3f84cce4d9919","observation_id":"00b0c13c-7b18-4931-9d72-0cd5c20715c7","resolution":{"observed_at":"2026-08-15T17:26:49.636233Z","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":"10.1103/physrevd.83.105014","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:28:45.848734Z","title":"A., Frommert M., 2011, @doi [ ] 10.1103/PhysRevD.83.105014 , https://ui.adsabs.harvard.edu/abs/2011PhRvD..83j5014E 83, 105014","venue":null,"work_id":"f547f174-0d04-43e0-92fb-bc1fc72c29ed","year":2011},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.640353Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:8f1805cb4233b52eecda37093f958808c1989169e974a62ab41cf67570febcc3","observation_id":"e1b8d58f-7ae9-47b1-9e25-6c5cdb655e7d","resolution":{"observed_at":"2026-08-15T17:28:45.855967Z","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":"2026-08-15T17:26:49.644909Z","title":"A., Frommert M., Kitaura F","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.644909Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:da6c981a4d76fcefc9b6223c5d72a66f33429e036924c7f69e652481ec480fd0","observation_id":"bec9f36a-4291-4ca7-9023-9af1c82325a8","resolution":{"observed_at":"2026-08-15T17:26:49.644909Z","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":"2026-08-15T17:26:49.649549Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.649549Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:99e7b91d97c0bf43a29d2c814c34e8a508722b40f8effba9eda9a998f11bb099","observation_id":"2e4fa305-14ba-4e9f-86dd-7c96c89174f0","resolution":{"observed_at":"2026-08-15T17:26:49.649549Z","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":"2026-08-15T17:26:49.654100Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.654100Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:14d0ed6aa131add1faefc869f8c63b4335f60e55a45fcfa47e1d132ceb3c4e25","observation_id":"8f51ed1f-2650-41d5-bdd6-e26016d6b84f","resolution":{"observed_at":"2026-08-15T17:26:49.654100Z","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":"2026-08-15T17:26:49.658422Z","title":"P., et al., 2022, @doi [ ] 10.1051/0004-6361/202142337 , https://ui.adsabs.harvard.edu/abs/2022A&A...658A.115F 658, A115","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.658422Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:8bd64bb7ab728a05ff38e3ee533904222b499d6c4e96e4fbabc3222abce9df62","observation_id":"c38ba758-7718-4bf7-b2b3-65c15079be36","resolution":{"observed_at":"2026-08-15T17:26:49.658422Z","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":"2026-08-15T17:26:49.662647Z","title":"F., 2022, @doi [ ] 10.1093/mnras/stac2682 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.5887F 516, 5887","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.662647Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:121307005a91147ea1fe920f6f7eae5bf06baf8de13ec3d4b7b425372f847ff1","observation_id":"b49c6c9c-ee27-48a0-bb78-231338d02106","resolution":{"observed_at":"2026-08-15T17:26:49.662647Z","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":"2026-08-15T17:26:49.666920Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.666920Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:c51bacd7e12f3071ecc61bf1a2144e1b4fb8d11913463fdd2d940d4a0ff6cc84","observation_id":"d47b1453-514b-4f1f-ad73-3233a975ef3e","resolution":{"observed_at":"2026-08-15T17:26:49.666920Z","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":"2026-08-15T17:26:49.671441Z","title":"A., et al., 2016, @doi [ ] 10.1088/1538-3873/128/964/066001 , https://ui.adsabs.harvard.edu/abs/2016PASP..128f6001F 128, 066001","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.671441Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:18fcb788cebbd9859bc3c1d3c8c3c8400f73034e748054cd95dda7afacec7a82","observation_id":"a4e6a90a-aa53-4e9c-91ab-3e10799151c5","resolution":{"observed_at":"2026-08-15T17:26:49.671441Z","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":"2026-08-15T17:26:49.675831Z","title":"P., et al., 2016, @doi [ ] 10.1093/mnras/stv2924 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.457..580F 457, 580","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.675831Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:6c2aa2959a9ad1b5a1c27260b9f6f552eee572577649b6e09f7aaf8ce5c9caaa","observation_id":"3ea659d9-3897-46f9-8572-58038f88fd7a","resolution":{"observed_at":"2026-08-15T17:26:49.675831Z","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":"2026-08-15T17:26:49.680132Z","title":"P., \\'O Fionnag \\'a in D., Fossati L., Vidotto A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.680132Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:459c98cfd0922569ef7485e849d92905f34bfff3e056e59b0309ac3a5689e012","observation_id":"e67c7516-dcbd-4747-b1a9-a5a2c21c2469","resolution":{"observed_at":"2026-08-15T17:26:49.680132Z","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":"2026-08-15T17:26:49.684941Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.684941Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:a2fd06de8df6193226827c11c01f105beb551dbfc4037b4bcab0df75764e635e","observation_id":"333c43c7-6110-4afa-aa64-1c64dec97336","resolution":{"observed_at":"2026-08-15T17:26:49.684941Z","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":"2026-08-15T17:26:49.689331Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.689331Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:946315dcbbd9969444e52d61a8805042da56a86c5c00e81313b9be424122d4f2","observation_id":"03bfc47d-c975-47cc-b312-8118571540f0","resolution":{"observed_at":"2026-08-15T17:26:49.689331Z","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":"2026-08-15T17:26:49.693835Z","title":"R., Wicht J., 2013, @doi [ ] 10.1051/0004-6361/201220317 , https://ui.adsabs.harvard.edu/abs/2013A&A...549L...5G 549, L5","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.693835Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:3d2099abb34c285f916bb6dd6c0287449d0e73b377dfee68c4c71b70f1df63d5","observation_id":"59e59e0b-48cf-4631-ad29-b95a238a0229","resolution":{"observed_at":"2026-08-15T17:26:49.693835Z","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":"2026-08-15T17:26:49.698320Z","title":"V., Ryabchikova T","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.698320Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:87e8054d849e4d05eed5370bf77a8bc9ad8ced6806e25c54b77f844ab4a97fcd","observation_id":"17ee091e-232c-4182-9994-d79a0a993a1d","resolution":{"observed_at":"2026-08-15T17:26:49.698320Z","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":"2026-08-15T17:26:49.702524Z","title":"F., et al., 2021, @doi [ ] 10.3847/1538-3881/abd79e , https://ui.adsabs.harvard.edu/abs/2021AJ....161..130G 161, 130","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.702524Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:76d8e72e4fd7b2ae05d8b99735b65d7a89c1a52fcab447415bbf052fb61ea5ba","observation_id":"ed247b86-8b46-4874-9d2f-1bcf75935de3","resolution":{"observed_at":"2026-08-15T17:26:49.702524Z","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":"2026-08-15T17:26:49.706700Z","title":"F., et al., 2025, @doi [ ] 10.3847/1538-3881/ad89bf , https://ui.adsabs.harvard.edu/abs/2025AJ....169....1G 169, 1","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.706700Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:199c6cfd76a46c93e609a57a103d6b512407e9d70b855b02628b283bc7778c84","observation_id":"b304b2f4-db3c-4578-8e71-023e776d4668","resolution":{"observed_at":"2026-08-15T17:26:49.706700Z","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":"2026-08-15T17:26:49.711117Z","title":"D., Thompson S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.711117Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:a29532a773c7eccd61f4317e2f025419c3b5653f02fc13a3647df88c9491f059","observation_id":"56a32496-e69c-4de9-8ee9-7d57746d0330","resolution":{"observed_at":"2026-08-15T17:26:49.711117Z","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":"2026-08-15T17:26:49.715582Z","title":"C., Delisle J.-B., 2025, @doi [ ] 10.1051/0004-6361/202346391 , https://ui.adsabs.harvard.edu/abs/2025A&A...696A.141H 696, A141","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.715582Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:8136bed77598297463d95f653055dfa02c8fa1a440692d598860472085a90031","observation_id":"1baa09fb-9888-4da8-9983-232d6931d671","resolution":{"observed_at":"2026-08-15T17:26:49.715582Z","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":"10.1093/mnras/248.3.487","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:26:51.046359Z","title":"P., 1991, @doi [ ] 10.1093/mnras/248.3.487 , https://ui.adsabs.harvard.edu/abs/1991MNRAS.248..487H 248, 487","venue":null,"work_id":"e0d1500f-e0b7-4973-a84f-27a4eb1d67be","year":1991},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.720435Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:433e02f22ff15ec99372e59fa31c120e4fa246f4d8eec4cf7412f9fc42a5ad4c","observation_id":"89388cee-23dd-4031-a47a-e894b0140aaf","resolution":{"observed_at":"2026-08-15T17:26:51.050905Z","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":"10.1086/176265","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:26:51.032752Z","title":"P., 1995, @doi [ ] 10.1086/176265 , https://ui.adsabs.harvard.edu/abs/1995ApJ...451..784H 451, 784","venue":null,"work_id":"ba4b6b93-2c14-4eb8-b46f-0d9ebc839cfc","year":1995},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.724961Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:918a096c345df701f989eb620db5f1ded6e80ba82be9e1c02e7e6f33650f76a9","observation_id":"75ba98f3-aec2-42aa-acc2-c3b6980a77f2","resolution":{"observed_at":"2026-08-15T17:26:51.037233Z","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":"2026-08-15T17:26:49.729409Z","title":"M., Donati J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.729409Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:e3c7d7dce1081114c9f83369bd07c576e1c14a46b34bdb763d8ff9af681e81a7","observation_id":"8d74ecff-bd7a-47da-8af3-f9bf5518f403","resolution":{"observed_at":"2026-08-15T17:26:49.729409Z","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":"2026-08-15T17:26:49.733705Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.733705Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:25f6eab0ca4fe1ea5a5a706b0e0828290e77e47a9b4680d6ef7ca2dd5a5dcd57","observation_id":"788a29c2-e7a7-46e3-8aad-fdc143d47148","resolution":{"observed_at":"2026-08-15T17:26:49.733705Z","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":"2026-08-15T17:26:49.737936Z","title":"A., Collier Cameron A., Wilson T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.737936Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:e5cdcd7c8187c4692d3cdfdbf5e11533702f0d04f0cfc4068da65c09d087adfb","observation_id":"bf6606ee-b2f5-43f9-9455-daafe50321e6","resolution":{"observed_at":"2026-08-15T17:26:49.737936Z","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":"2026-08-15T17:26:49.742249Z","title":"A., et al., 2023, @doi [ ] 10.1093/mnras/stad2381 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525.1687J 525, 1687","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.742249Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:bc5967a264b55d3a21143be63e54be911e6aa4404d38c0699ae96edac0c5ac82","observation_id":"d0f22477-7302-4460-b91e-bec35be06116","resolution":{"observed_at":"2026-08-15T17:26:49.742249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.01318","last_updated":"2020-08-25T04:43:40Z","snapshot_observed_at":"2026-08-14T20:17:08.906322Z","submitted_at":"2017-11-03T20:00:59Z","title":"Improving Exoplanet Detection Power: Multivariate Gaussian Process Models for Stellar Activity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.01318","snapshot_observed_at":"2026-08-15T17:26:49.746682Z","title":"E., Stenning D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.746682Z"},"links":{"cited_paper":"/paper/1711.01318","citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:4271f17a899d552788a4aac3bf4efd08c1867297226ea590309175c45d3c1efa","observation_id":"74d13116-ee82-4855-89a3-9083a8eccbca","resolution":{"observed_at":"2026-08-15T17:26:49.746682Z","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":"2026-08-15T17:26:49.751633Z","title":"D., Vidotto A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.751633Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:1c1b7da4863fc422bb0f3f07e57b52eac44dd20b8a43f045d345d0eb6e2bd4a9","observation_id":"dabfcae9-28ea-4fd2-b203-84f06fa39b16","resolution":{"observed_at":"2026-08-15T17:26:49.751633Z","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":"10.1086/164462","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:26:50.975111Z","title":"L., Rice J","venue":null,"work_id":"7debbee3-d5f8-4b56-b06d-6af827581fea","year":1986},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.756419Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:d91cb93965751c438b7739a89e71a7fddfbec8f30f12feb1731797d675b0bf09","observation_id":"e55cc04c-e707-469c-8912-fc0f43b966fa","resolution":{"observed_at":"2026-08-15T17:26:50.979632Z","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":{"arxiv_id":"astro-ph/9403015","last_updated":"1994-03-08T15:57:19Z","snapshot_observed_at":"2026-07-07T01:09:23.319340Z","submitted_at":"1994-03-08T15:57:19Z","title":"Amplitudes of Stellar Oscillations: The Implications for Asteroseismology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9403015","snapshot_observed_at":"2026-08-15T17:26:49.760806Z","title":"R., 1995, @doi [ ] 10.48550/arXiv.astro-ph/9403015 , https://ui.adsabs.harvard.edu/abs/1995A&A...293...87K 293, 87","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.760806Z"},"links":{"cited_paper":"/paper/astro-ph/9403015","citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:0327871954760897a80a9af709bcdb6a0a5c28ca573a7f656919be632767eac9","observation_id":"f6c53c28-92f6-49f4-a165-1aacf5a55bd6","resolution":{"observed_at":"2026-08-15T17:26:49.760806Z","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":"2026-08-15T17:26:49.765643Z","title":"M., Zaire B., Folsom C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.765643Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:1b10ca1094406596140794fb10dec0c7fdd3e4310fa96e2e4a1b8e5131aada61","observation_id":"ee39b663-a667-4269-b68f-942a9f85154b","resolution":{"observed_at":"2026-08-15T17:26:49.765643Z","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":"2026-08-15T17:26:49.770032Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.770032Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:9a6dc57a8b9c9f16dc11a1bf4c4832cea1cd0c39e3f178e8da26d1a74ff0199c","observation_id":"0d8b9adb-ba1e-4268-b0e2-1824f82a8e73","resolution":{"observed_at":"2026-08-15T17:26:49.770032Z","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":"2026-08-15T17:26:49.774611Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.774611Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:9aca10e7c07cd8c31323a4470542fc11ffc1285f582af1570ce4d9cb98faaf70","observation_id":"c26bdbe6-ff58-455b-8c81-64fdce9cd823","resolution":{"observed_at":"2026-08-15T17:26:49.774611Z","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":"2026-08-15T17:26:49.779252Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.779252Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:3d6064df1dcb14af501cc6170f9755744464da49f8339256a3306b8cb95ce10a","observation_id":"b84bb5ee-bf70-4261-9694-652801f06a30","resolution":{"observed_at":"2026-08-15T17:26:49.779252Z","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":"2026-08-15T17:26:49.783541Z","title":"914, Lecture Notes in Physics, Berlin Springer Verlag","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.783541Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:f7636b9ab29f840e79586b1eaa47493232ca0375366936872926d9a3d3ef509e","observation_id":"d662cc9e-ef3c-4835-9f4d-f940c92d3b06","resolution":{"observed_at":"2026-08-15T17:26:49.783541Z","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":"10.1051/0004-6361:20020300","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:26:50.904446Z","title":null,"venue":null,"work_id":"da53a0ba-31ee-45db-bcc0-dd012b9705a4","year":2002},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.787968Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:94bb6437da4cfcf21d1883cbd7a4a95a4cbf8fbc9deb5389cdea4a540ae9cbba","observation_id":"67d1e9ca-ebc8-4cc8-bda1-fed55b39440a","resolution":{"observed_at":"2026-08-15T17:26:50.908862Z","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":"10.1051/0004-6361/200913860","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:26:50.890441Z","title":"A., 2010, @doi [ ] 10.1051/0004-6361/200913860 , https://ui.adsabs.harvard.edu/abs/2010A&A...513A..13K 513, A13","venue":null,"work_id":"63a69035-ead3-4676-aa11-268b73821d64","year":2010},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.792518Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:d68e17f7e5acb961ea3622fe9e09ca91aad2bae8c990cef3dfb962d6f10ac482","observation_id":"87a28ee9-6407-4ed3-8943-6f40ba1d5881","resolution":{"observed_at":"2026-08-15T17:26:50.895017Z","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":"2026-08-15T17:26:49.797610Z","title":"A., Piskunov N., de la Reza R., 2004, @doi [ ] 10.1051/0004-6361:20040517 , https://ui.adsabs.harvard.edu/abs/2004A&A...424..935K 424, 935","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.797610Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:77e1b62f7a229f51b234114e2090e735c581c9eefa1783415904ec52aa8e98ca","observation_id":"13b28bfd-784b-4a7f-997a-a916e4b5a325","resolution":{"observed_at":"2026-08-15T17:26:49.797610Z","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":"2026-08-15T17:26:49.801888Z","title":"W., Landstreet J","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.801888Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:9925de1e5313ab43cd0faea27b541a93c16b4efbb1a4c0e7a78ddbc6592cf011","observation_id":"51f3643e-3c78-461e-bd9b-ac14f1355bb8","resolution":{"observed_at":"2026-08-15T17:26:49.801888Z","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":"10.1051/0004-6361/201220432","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:26:50.867120Z","title":"J., Hackman T., Ilyin I., 2013, @doi [ ] 10.1051/0004-6361/201220432 , https://ui.adsabs.harvard.edu/abs/2013A&A...550A..84K 550, A84","venue":null,"work_id":"96c3531d-89a1-4bf6-845f-7dcb4aefa576","year":2013},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.805836Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:436165c434bcbbe174ade5720b5f95649ab60e78619ebdfdbdeceb01e486c414","observation_id":"53c58769-615a-4787-9974-17bb677346c8","resolution":{"observed_at":"2026-08-15T17:26:50.871627Z","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":"2026-08-15T17:26:49.810219Z","title":"S., et al., 2024, @doi [ ] 10.1093/mnras/stad3723 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.527.7681L 527, 7681","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.810219Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:edc1951ab61d89d4261e518722a527814190d0edc24b8dba45f39130c72a9f7a","observation_id":"78d6dbe8-f1e6-435b-9542-57daa727c683","resolution":{"observed_at":"2026-08-15T17:26:49.810219Z","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":"2026-08-15T17:26:49.814438Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-15T17:26:49.814438Z"},"links":{"citing_paper":"/paper/2508.12963"},"observation_digest":"sha256:8be474815fb6efbba122dbff493a056c5f4ef9212dcfec4161d24a4cc07f4fc7","observation_id":"b63eb18a-e497-4b64-8964-03cbc662e2f3","resolution":{"observed_at":"2026-08-15T17:26:49.814438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2508.12963","last_updated":"2025-08-18T14:37:26Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-16T00:37:48.505693Z","submitted_at":"2025-08-18T14:37:26Z","title":"Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":89,"verified_exact":11,"verified_fuzzy":0},"total_outbound_references":171},"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 100 of 171 outbound references and 0 inbound Pith citation observations for arXiv:2508.12963."}