{"as_of":"2026-08-16T06:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8bca4c80c3f0382179eeb6a9c8bf6526fdb93346e8d3a58cad0268f3621cbab5","coverage":[{"denominator":67,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":67,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T15:26:35.761897Z","state":"measured"},{"denominator":67,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":67,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/1908.01191/citation-record","integrity":"/paper/1908.01191/integrity","json":"/paper/1908.01191/citation-record.json","paper":"/paper/1908.01191"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.493480Z","title":"Chromospheric variations in main-sequence stars","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.493480Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:33d5190a8b7092c281368594043ccbf0e9db642654ed40ba2276d231b4d9a783","observation_id":"e17e31cd-e32a-44ca-b4e2-a569705b0b6e","resolution":{"observed_at":"2026-08-14T15:26:35.493480Z","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":"2026-08-14T15:26:35.497976Z","title":"Time Evolution of the Magnetic Activity Cycle Period","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.497976Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:dc87c24325b2d33e447de9c671b18ada5bddded65cd62edf2d3020d841dc9742","observation_id":"10489704-be2c-4733-9e6e-efddd43282dd","resolution":{"observed_at":"2026-08-14T15:26:35.497976Z","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/stu760","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.144056Z","title":"Looking for activity cycles in late-type Kepler stars using time-frequency analysis","venue":null,"work_id":"92057c8a-8820-406c-85ea-c466cf2eac4a","year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.502303Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:0a60873c893e41b5c8efd97d1343285037900dc33e44d9e5969ae81361d0d81c","observation_id":"7ca9e676-a2a4-499e-a32f-8f2ff7a230ca","resolution":{"observed_at":"2026-08-14T15:26:36.148153Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.605690Z","title":"Solar activity cycle frequency shifts of low-degree p-modes","venue":null,"work_id":"64782d61-6303-484d-989b-7adc6e0f180a","year":1998},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.506419Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c3cfb3a47bf879d65b83a4dde0114e8e1988aca967c90ddea2d189eae5f4ca58","observation_id":"641a1f38-addf-47f8-a774-cf97ebce5ddf","resolution":{"observed_at":"2026-08-14T15:26:36.609836Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.510498Z","title":"A Helioseismic Perspective on the Depth of the Minimum Between Solar Cycles 23 and 24","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.510498Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:1d42d95b2d73ae172afe62eba071e5da2642689cc57930af355e3165bd451d95","observation_id":"9de69986-c433-4914-82d2-9eb59c18a833","resolution":{"observed_at":"2026-08-14T15:26:35.510498Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.593658Z","title":"A Comparison Between Global Proxies of the Sun’s Magnetic Activity Cycle: Inferences from Helioseismology","venue":null,"work_id":"a77d5117-212d-44df-86c9-12ed3c119291","year":2015},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.515821Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:9fb08e533adfdca360cdae750a4dfa56ada7140d37d10db4bc822a3c0ca8f6f4","observation_id":"e4fb6522-2872-4cdb-aeae-c3d865330f87","resolution":{"observed_at":"2026-08-14T15:26:36.597771Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.582140Z","title":"Scientific Objectives for a Minisat: CoRoT","venue":null,"work_id":"66c95098-76f1-415b-8512-44818b305a57","year":2006},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.519817Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:a81da8a595718352076972c359e0e49f3166169e835eececbd42cdbee8a5d0d3","observation_id":"cde563b3-aa43-4018-aef8-9be4b610a274","resolution":{"observed_at":"2026-08-14T15:26:36.586311Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.527290Z","title":"CoRoT Reveals a Magnetic Activity Cycle in a Sun-Like Star","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.527290Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:6771268c5f5f128326adc7760999c56bccbfcd9360531262d9c5736bc1ddb43a","observation_id":"387278bd-2e63-44de-8bb0-a8f73dd07aa0","resolution":{"observed_at":"2026-08-14T15:26:35.527290Z","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":"2026-08-14T15:26:35.531178Z","title":"The spectrum of solar p-modes and the solar activity cycle","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.531178Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c919c3f6691674c7e7e649ded0527796a99068254a2897b4d36e1333572aefda","observation_id":"ad1e63f1-d4bb-4bcd-84c5-e1ee4e51a44e","resolution":{"observed_at":"2026-08-14T15:26:35.531178Z","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":"2026-08-14T15:26:35.534965Z","title":"Width and Energy of Solar p-Modes Observed by Global Oscillation Network Group","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.534965Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:99b71ab519ccee8526907c4c6210ce36988361c0c47188d39c31b68b6c32b934","observation_id":"570c950a-ea7e-4809-bede-e6e45ccd6604","resolution":{"observed_at":"2026-08-14T15:26:35.534965Z","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":"10.1051/0004-6361/201116633","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.097078Z","title":"About the p-mode frequency shifts in HD 49933","venue":null,"work_id":"1125cd61-f3ce-4357-833e-3a9f61f4f4bb","year":2011},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.539026Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:ea1a159a5c79ead66699488fa2d297ccb9f308753ceb77432d06e4cb7be224b8","observation_id":"22b53a9e-9175-46ff-956b-2a636848de30","resolution":{"observed_at":"2026-08-14T15:26:36.101327Z","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":"2026-08-14T15:26:35.542711Z","title":"Solar-cycle effects on solar oscillation frequencies","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.542711Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:731f2e02b018fb8dd39200881edc394593d36ee863595ee060df88a3761d372d","observation_id":"f224050f-1839-4b8b-801c-2b8f0085c3ad","resolution":{"observed_at":"2026-08-14T15:26:35.542711Z","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":"10.1051/0004-6361:20031541","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.077201Z","title":"Solar p modes in 10 years of the IRIS network","venue":null,"work_id":"b22b41a9-9a9d-47fb-ad9d-86919ad9bd02","year":2004},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.546843Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:bbe98386360be027d0d1db0b98021c64b6695489f6767e737292acf66ae3fd5b","observation_id":"fb917c00-d24a-4040-adc9-c3e7b9723fe2","resolution":{"observed_at":"2026-08-14T15:26:36.081090Z","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":"2026-08-14T15:26:35.550837Z","title":"Kepler planet-detection mission: Introduction and first results","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.550837Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c4f93bd648fc4fce6293e14009723a8197b08084ef241309f97e9066ef7a537f","observation_id":"c7a28196-f72b-41c7-a850-9c14eb71fc38","resolution":{"observed_at":"2026-08-14T15:26:35.550837Z","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":"2026-08-14T15:26:35.554792Z","title":"Kepler Mission Design, Realized Photometric Performance, and Early Science","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.554792Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:ee9315180d6373f28872f62b5f28fef5313f9c668f86362a0d1a427c50c88e42","observation_id":"7dc69669-9bca-4b33-9967-9e9d09f21f1b","resolution":{"observed_at":"2026-08-14T15:26:35.554792Z","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":"2026-08-14T15:26:35.558602Z","title":"Magnetic variability in the young solar analog KIC 10644253","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.558602Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c0b409eacdc1b9f10426cbf5ecb355057e62f17177e555530bcdca62fb7523b3","observation_id":"c35aab1f-6da0-4ad3-9df7-f58421651e8b","resolution":{"observed_at":"2026-08-14T15:26:35.558602Z","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":"2026-08-14T15:26:35.566667Z","title":"Stellar magnetic activity and variability of oscillation parameters: An investigation of 24 solar-like stars observed by Kepler","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.566667Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:36b9b6e977478ff9640224043745e411db479ba362e159d543062e99ba7dffed","observation_id":"b768fa62-3e86-4ac4-903c-7b0023394b9e","resolution":{"observed_at":"2026-08-14T15:26:35.566667Z","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":"2026-08-14T15:26:35.570434Z","title":"Frequency dependence of p-mode frequency shifts induced by magnetic activity in Kepler solar-like stars","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.570434Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:8927cc2ca3b8962e016c530c017aefff6596678538c964a10c21d78913cf49b5","observation_id":"422ddb71-0281-458a-b870-6f089f0e5ac4","resolution":{"observed_at":"2026-08-14T15:26:35.570434Z","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":"2026-08-14T15:26:35.574238Z","title":"Signatures of Magnetic Activity in the Seismic Data of Solar-type Stars Observed by Kepler","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.574238Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:e2c324488f6e62e85010d02e2345f1cde5198dac8809da19baff642c212e4fce","observation_id":"53d2d344-0985-4edd-8458-5b1441503c11","resolution":{"observed_at":"2026-08-14T15:26:35.574238Z","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":"2026-08-14T15:26:35.578088Z","title":"Evidence for the Impact of Stellar Activity on the Detectability of Solar-like Oscillations Observed by Kepler","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.578088Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:92f7c07e12d5e5120865386b2d2128d0a10a366ce43d1006d7fa31bc5a46a6ce","observation_id":"f67a8631-30e0-4e88-b30e-81db55c299e5","resolution":{"observed_at":"2026-08-14T15:26:35.578088Z","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":"2026-08-14T15:26:35.581825Z","title":"Chromospheric Activity in G and K Main-Sequence Stars, and What It Tells Us about Stellar Dynamos","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.581825Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:0f610de89ff4befcf9dc65e1c40a1b01c5f4424db98556c69c14a6db50ab793a","observation_id":"c80c0bdf-bdd5-4a30-b8a4-6c1552553d9b","resolution":{"observed_at":"2026-08-14T15:26:35.581825Z","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":"2026-08-14T15:26:35.585671Z","title":"Improved Age Estimation for Solar-Type Dwarfs Using Activity- Rotation Diagnostics","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.585671Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:f78b5c3e9ad04bd46e75aefcc570d74d730c17485de4ae9290cb246f3c772a82","observation_id":"09cd409b-fc1f-426c-9b35-3bc8ec7d99ce","resolution":{"observed_at":"2026-08-14T15:26:35.585671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.570347Z","title":"Magnetic cycles and rotation periods of late-type stars from photometric time series","venue":null,"work_id":"ebbf040a-06cf-4a52-a3f8-a210b9bf7d64","year":2016},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.589352Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c109d3eab56d962156c6ac29240ab835043c855bae235fb971a99b740cf5388e","observation_id":"97c473d1-c555-4770-a0de-be4f43f85472","resolution":{"observed_at":"2026-08-14T15:26:36.574396Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2026-08-14T15:26:35.592816Z","title":"Magnetic Evolution and the Disappearance of Sun-Like Activity Cycles","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.592816Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:3f49885405c27cd8a79ded636e579cbb44f1d56c9ebe37cad7cce9b5ef84c972","observation_id":"cefc7f5a-a446-4dfc-be2c-3c82e53a3f02","resolution":{"observed_at":"2026-08-14T15:26:35.592816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.558314Z","title":"Reconciling solar and stellar magnetic cycles with nonlinear dynamo simulations","venue":null,"work_id":"4a76365b-2cf2-4467-8843-9b499517da1c","year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.596441Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:2a2d526cea2285f8c3ff2936ecae04f4f52f9536bba05db9df11d83fdd22bb11","observation_id":"ba99d81b-a6d3-43cf-8013-8ad7e0f5fee6","resolution":{"observed_at":"2026-08-14T15:26:36.562546Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2026-08-14T15:26:35.600248Z","title":"Dynamo cycles in global convection simulations of solar-like stars","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.600248Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:f2c88a04943d2036c09e569905ee5ccbfcb682346814fb9fe6ac8521123ab98c","observation_id":"0d36db83-9a92-41ce-9877-de0796bd41ad","resolution":{"observed_at":"2026-08-14T15:26:35.600248Z","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":"2026-08-14T15:26:35.604016Z","title":"On the Sensitivity of Magnetic Cycles in Global Simulations of Solar-like Stars","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.604016Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:5840d1f2f1bb9b59d0c3697274e1752c527e767e7878bc6e12dc8e4dc8a34695","observation_id":"bf5dcedc-6f8a-4087-9712-9b6ba1781fc4","resolution":{"observed_at":"2026-08-14T15:26:35.604016Z","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":"2026-08-14T15:26:35.608861Z","title":"Inferences on Stellar Activity and Stellar Cycles from Asteroseismology","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.608861Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c14f7302b61b1bec088b665f2d64a5923e7c121d6f18ed73b8625b5f39cb892d","observation_id":"fb498c62-732d-4c54-a91a-57c251c95471","resolution":{"observed_at":"2026-08-14T15:26:35.608861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.547290Z","title":"The variability of magnetic activity in solar-type stars","venue":null,"work_id":"3c46bbd1-0041-4c6e-89f9-d36567c4e1db","year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.613321Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:973df6b26fe0f2c76f16ed665cbafff1c0267bca3ab93046bf7b7682a9825b06","observation_id":"381ed0ac-8d1b-4941-a61e-d9ff57ed2f94","resolution":{"observed_at":"2026-08-14T15:26:36.551099Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"10.1007/s11214-011-9780-1","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.971574Z","title":"Total Solar Irradiance: What Have We Learned from the Last Three Cycles and the Recent Minimum? Space Sci","venue":null,"work_id":"4a312449-f1cb-4b71-a8de-2417dce7991a","year":2013},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.616939Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:463f76b0559106f4527faf66f430f5ef17746e78776a434697be0bac7fce9b91","observation_id":"0b0a18fd-5f40-46d0-bcaa-9ab1109bccac","resolution":{"observed_at":"2026-08-14T15:26:35.976092Z","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":"2026-08-14T15:26:35.620957Z","title":"The nature of solar brightness variations","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.620957Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:cd206c703993d69c3606531014bc6f03c5b711f6d3bdc183c49810a57cca1d3f","observation_id":"23ea2844-711c-475a-af7a-5c06f042a37d","resolution":{"observed_at":"2026-08-14T15:26:35.620957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.535519Z","title":"Variability of Sun-like stars: reproducing observed photometric trends","venue":null,"work_id":"96817a98-cd8c-46fd-a2c6-280063647add","year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.625564Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:4d4894ef8124a430f70ebba45e3c8d653ae38cd8e0df2dab3288dfbea330ebe1","observation_id":"109d0994-5972-464b-9a22-1d1de5072217","resolution":{"observed_at":"2026-08-14T15:26:36.539620Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2026-08-14T15:26:35.629136Z","title":"Photometric magnetic-activity metrics tested with the Sun: application to Kepler M dwarfs","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.629136Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:ee18691bbce0c518b45f21e0db0467abf4477cad5bf1bdd3aab69c7d0e59f62a","observation_id":"260715e5-6166-4f6f-a913-3389a51ee939","resolution":{"observed_at":"2026-08-14T15:26:35.629136Z","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":"2026-08-14T15:26:35.633068Z","title":"Photospheric and chromospheric magnetic activity of seismic solar analogs","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.633068Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:466562d3ccf5c41d810e08d6c066fa3f87aa7be9bb354188d907a95a3d08c411","observation_id":"a8548397-5c43-40a6-b57f-acb9ca0cd07b","resolution":{"observed_at":"2026-08-14T15:26:35.633068Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.636741Z","title":"Photospheric activity of the Sun with VIRGO and GOLF","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.636741Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:0e850e4b186c939cb48bc480174fd66fcbb57209d43b1e18d47f1280fcd8fb93","observation_id":"7785ad97-8186-4721-8528-a471d9bf9278","resolution":{"observed_at":"2026-08-14T15:26:35.636741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.523186Z","title":"Stellar cycles from photometric data: CoRoT stars","venue":null,"work_id":"26579772-794a-4d04-bf49-d29bfe45cb81","year":2015},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.640534Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:8f6a48884273c546878ca3c48fbc872f1016d93a454a510766d15d766c0e1c8e","observation_id":"e7ef7f0d-df23-4e7c-b372-0c84d90fa14f","resolution":{"observed_at":"2026-08-14T15:26:36.527494Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2026-08-14T15:26:35.644094Z","title":"Long-term Photometric Variability in Kepler Full-frame Images: Magnetic Cycles of Sun-like Stars","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.644094Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:03e91d97d786e4d2cdbfd2e6984203c6bdf27262fab145252bf6889b6d4efd95","observation_id":"4c28c2bd-7cd5-4f94-b968-2a7626c463ab","resolution":{"observed_at":"2026-08-14T15:26:35.644094Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.647980Z","title":"Sounding stellar cycles with Kepler - III","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.647980Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:886963b5593251b6435591e02bca5a21c3f5dc4a43fc8fd03e742f25037904ac","observation_id":"df2b3b21-80d7-44bb-b922-52d82ea101e2","resolution":{"observed_at":"2026-08-14T15:26:35.647980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.509844Z","title":"A Synthetic Sample of Short-cadence Solar-like Oscillators for TESS","venue":null,"work_id":"e3a81813-fa02-41cc-a4b4-fd8b42b6cd9b","year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.651804Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:0aa177c745d860c0c68c9b26b75621f033f4089147b6a7e32b010ccc5a6270b5","observation_id":"26971635-4a1b-4dd9-afb9-eedbcbf5d1ad","resolution":{"observed_at":"2026-08-14T15:26:36.515019Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.655792Z","title":"Transiting Exoplanet Survey Satellite (TESS)","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.655792Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:a162360477c8b3630ac55edcdc53d4a152fab3023554777016c3f0f404cebf22","observation_id":"785ef852-94d2-47a8-8f0f-6a3e3452683f","resolution":{"observed_at":"2026-08-14T15:26:35.655792Z","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":"2026-08-14T15:26:35.659706Z","title":"Star counts in the Galaxy","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.659706Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:0d823e7b57c8ec02862f623e7761e46ccc76297cd3a99c42acc6b8d59cf8bf27","observation_id":"b1d7da00-5662-4378-aa68-fd6aebe367f2","resolution":{"observed_at":"2026-08-14T15:26:35.659706Z","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":"2026-08-14T15:26:35.663739Z","title":"The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.663739Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:5d41ee37a953dbf903904459e0c6e947b2557674855bbdd720fffdf6f6abc972","observation_id":"bb77b286-d2f4-4e89-9a3f-b327a50ced09","resolution":{"observed_at":"2026-08-14T15:26:35.663739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.497776Z","title":"Amplitudes of stellar oscillations: the implications for asteroseismology","venue":null,"work_id":"6cedc4a0-a671-480f-bdb8-4546510d19ca","year":1995},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.667436Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:2deb86bd6080cc48b3f737b6ae465ebe351a26514cefd78bbbaa03b59af00771","observation_id":"941dcb4d-6ebd-4450-bcf2-0ef9f549b06a","resolution":{"observed_at":"2026-08-14T15:26:36.501732Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/0004-637x/830/","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.906355Z","title":"The Asteroseismic Potential of TESS: Exoplanet-host Stars","venue":null,"work_id":"8ea47c73-06f7-417c-b7d3-b24ae14927c3","year":2016},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.671099Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:0e5d77a208098be6ebffce1614aafd7ad47db28f19be42f4190547bc78e61803","observation_id":"bfef2148-1e13-41e2-8e8f-471a7a0b8cd4","resolution":{"observed_at":"2026-08-14T15:26:35.910797Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"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":"2007.11581","last_updated":"2020-07-22T11:34:40Z","snapshot_observed_at":"2026-07-06T09:41:00.325073Z","submitted_at":"2020-07-22T11:34:40Z","title":"Minimax-robust forecasting of sequences with periodically stationary long memory multiple seasonal increments","version":1},"cited_work":{"arxiv_id":"2007.11581","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.11581","snapshot_observed_at":"2026-08-14T15:26:36.375979Z","title":"Minimax-robust forecasting of sequences with periodically stationary long memory multiple seasonal increments","venue":"math.ST","work_id":"ab8224cd-1df4-4d66-9fda-b8ec073aa94a","year":2020},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.675069Z"},"links":{"cited_paper":"/paper/2007.11581","citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:56d882e7a8e60c41557610deec27e6bdfc374aed9dbf1f0dc9f0d37f83b78a2c","observation_id":"b73efb98-3c75-4b83-91d8-479552a648f1","resolution":{"observed_at":"2026-08-14T15:26:36.380373Z","resolver_source":"local_arxiv","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":"2026-08-14T15:26:35.680145Z","title":"A new look at dynamo cycle amplitudes","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.680145Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:d73942e0bd480a5fd84013db3a3b2ce3f78d8e41f550ffc3bf1fe5b22507060a","observation_id":"f40ee1b2-ead2-4e47-a121-109763a0ea92","resolution":{"observed_at":"2026-08-14T15:26:35.680145Z","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":"2026-08-14T15:26:35.684879Z","title":"Asteroseismic signatures of stellar magnetic activity cycles","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.684879Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:f22b5694b5f1d437237b2ba054cd3ceaf39520173efe590fbf475b9395f80a63","observation_id":"65c75a16-9bda-4123-803b-e79dc2408ba6","resolution":{"observed_at":"2026-08-14T15:26:35.684879Z","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":"2026-08-14T15:26:35.688537Z","title":"Rotation, convection, and magnetic activity in lower main-sequence stars","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.688537Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:66413acba18019ffc85dd1d415823310e66977a6082d2f90359c88557f0342e5","observation_id":"17aae553-ea49-48b9-b534-defc7eaf1190","resolution":{"observed_at":"2026-08-14T15:26:35.688537Z","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":"2026-08-14T15:26:35.692991Z","title":"Relation of Chromospheric Activity to Convection, Rotation, and Pre–Main-Sequence Evolution","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.692991Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:9499db57628f69d6022cd8a736af0e02b4ffe8b2131246654109d8a8beff8e5b","observation_id":"bcddf41b-92d1-49d3-aa25-da6dbda25619","resolution":{"observed_at":"2026-08-14T15:26:35.692991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.486054Z","title":"Theoretical values of convective turnover times and Rossby numbers for solar-like, pre-main sequence stars","venue":null,"work_id":"8a483115-95c8-4fd9-8f63-5e11896134e8","year":2010},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.696935Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:aeb422eb8e859809f35493cb71766f04feae63aaaa185d8b1aa4bdc6bc18f66c","observation_id":"c4400683-1aaa-4906-8d52-1e6929b26418","resolution":{"observed_at":"2026-08-14T15:26:36.490322Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2026-08-14T15:26:35.700472Z","title":"Time Scales for CaII Emission Decay, Rotational Braking, and Lithium Depletion","venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.700472Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:3e3a2d42eaa07c2c608a7cbeef787a4ffc8f3ea6123f98cfef850bd266e4fe12","observation_id":"b447aef1-d11d-4110-99a2-4e5147a7a145","resolution":{"observed_at":"2026-08-14T15:26:35.700472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.472799Z","title":"Solar cycle induced variations of the low L solar acoustic spectrum","venue":null,"work_id":"79403c1d-4297-4d26-b42e-db8b4c8ecbb5","year":1989},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.704360Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:a62720b8f3e1c24843d3b32db3bb30b27c2ca6b6cc92740480792a3885730d1a","observation_id":"502a40f9-5b48-4f33-afd0-18b0d5c5fe60","resolution":{"observed_at":"2026-08-14T15:26:36.477349Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.708109Z","title":"Solar p-Mode Frequencies over Three Solar Cycles","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.708109Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:eaa160f5b0ab9edc3ea8f22599d44825972cc2e50eb5fe93b63b9a1ed31c4e30","observation_id":"8b2a01ef-3b12-4969-a37d-9b6e4c23966c","resolution":{"observed_at":"2026-08-14T15:26:35.708109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/aab771","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.859831Z","title":"sunstardb: A Database for the Study of Stellar Magnetism and the Solar-stellar Connection","venue":null,"work_id":"8f2fbca6-4ef0-4eb3-9561-0eee9762a6c7","year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.711815Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:dfd93cfa283ef24c37b03d4aec0bf6db5b08ab275fc9d00b364f5e9dbaa336b5","observation_id":"cb053745-4887-4088-949f-4d4e5f967c5f","resolution":{"observed_at":"2026-08-14T15:26:35.864611Z","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":"2026-08-14T15:26:35.715317Z","title":"Sounding stellar cycles with Kepler - I","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.715317Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:cdb5ece90b0f7bf96088cebe5d6fb9a5c10adaebf86c8d0080ea127df779d850","observation_id":"a40ae0b9-39f5-48b5-a4be-7303fe4e4a71","resolution":{"observed_at":"2026-08-14T15:26:35.715317Z","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":"2026-08-14T15:26:35.718862Z","title":"Asteroseismic Fundamental Properties of Solar-type Stars Observed by the NASA Kepler Mission","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.718862Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:36b3d5ee2f1500a2edc59f8b36386230882d58938a410b0c0cb296044db85d2b","observation_id":"97882534-dc3f-4f4f-bb62-d7906c96c8c8","resolution":{"observed_at":"2026-08-14T15:26:35.718862Z","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/stw1326","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.838883Z","title":"Significantly improving stellar mass and radius estimates: a new reference function for the ∆ν scaling relation","venue":null,"work_id":"1fffecdd-be1f-4a13-9598-2966830e1211","year":2016},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.723230Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:fbf7778aa3f8ceb0202c11a04dc19345a12371efc512a5b335e0942979450af5","observation_id":"c6154c39-c148-4042-b5a0-f64cc8d385b8","resolution":{"observed_at":"2026-08-14T15:26:35.844737Z","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":"2026-08-14T15:26:35.727508Z","title":"Testing the Asteroseismic Scaling Relations for Red Giants with Eclipsing Binaries Observed by Kepler","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.727508Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:59c27ff0942620d5355e5a7ed8a780218e10239b0ef2feb5a5db642dd1972f37","observation_id":"6d1a3941-46c8-4730-aada-9796622d38a3","resolution":{"observed_at":"2026-08-14T15:26:35.727508Z","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":"2026-08-14T15:26:35.731398Z","title":"Influence of magnetic activity on the determination of stellar parameters through asteroseismology","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.731398Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:39972c2d50f61d8e54fffabcac7c88b4bc56dc40783126b8601e3a32da2e8e48","observation_id":"843523aa-dd70-48de-992d-cac6d298ad01","resolution":{"observed_at":"2026-08-14T15:26:35.731398Z","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":"2026-08-14T15:26:35.735514Z","title":"Revised Stellar Properties of Kepler Targets for the Quarter 1-16 Transit Detection Run","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.735514Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c090e8dd7ce16a049f0bf67388df8f05c2d8a54f348d698055b9a796760132ca","observation_id":"99c97a4b-5871-4df1-b857-451025771f1c","resolution":{"observed_at":"2026-08-14T15:26:35.735514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.459572Z","title":"Asteroseismology of 16,000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii","venue":null,"work_id":"72b7021c-9997-4753-acee-f2a619750021","year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.739155Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:4a46b44d973d8e9cc63d77c18daea9b07f4eefea9f3a6ac6603dce36d347a4b6","observation_id":"e861e7ed-0969-40c4-a1cb-d96abc9caf9e","resolution":{"observed_at":"2026-08-14T15:26:36.464675Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:35.742641Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.742641Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:fde680007b8981b308f69210f1e556e257e203f5d4d247c80ea45ba8de3058fb","observation_id":"54244e98-6eda-4429-97b8-6bf343cd28f6","resolution":{"observed_at":"2026-08-14T15:26:35.742641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:26:36.447395Z","title":"Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars","venue":null,"work_id":"58b3faa4-c829-4d29-b75e-bb35af28fe84","year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.746654Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:ea01c9bcc2ee08c23d722a17aa2f0b989eb39df26abb389f3e7b80b9d0c67a64","observation_id":"d11f16ca-55b3-403d-bdae-acb517f20df2","resolution":{"observed_at":"2026-08-14T15:26:36.451988Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"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":"2026-08-14T15:26:35.750632Z","title":"The Influence of Metallicity on Stellar Differential Rotation and Magnetic Activity","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.750632Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:76ebc7adf7acf24e8a5744f3fa585504b1f9b3a27a905a7dff13ab4a094ba8ac","observation_id":"0db24983-45f2-4961-ba5d-29dc3abc0338","resolution":{"observed_at":"2026-08-14T15:26:35.750632Z","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":"2026-08-14T15:26:35.754229Z","title":"Sounding stellar cycles with Kepler - II","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.754229Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:ca69b911b36458ff18a110875fefe6c901fa07883585502c642d556e0e8e8a46","observation_id":"94f9aaa3-6247-4196-9b16-b14c11e64a93","resolution":{"observed_at":"2026-08-14T15:26:35.754229Z","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":"2026-08-14T15:26:35.758279Z","title":"Evidence for photometric activity cycles in 3203 Kepler stars","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.758279Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:c54584267ca4020069a08c888a85a48371a5a2fd141cced97337dd46a14821c6","observation_id":"1162aa00-3f2a-41bc-8334-373326157a7f","resolution":{"observed_at":"2026-08-14T15:26:35.758279Z","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":"2026-08-14T15:26:35.761897Z","title":"The PLATO 2.0 mission","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T15:26:35.761897Z"},"links":{"citing_paper":"/paper/1908.01191"},"observation_digest":"sha256:4ea0af6abe26083f0dd6e1b6416fad1ac64b607cf3ea2e76004cafc6aacad885","observation_id":"d40454c2-ed64-48eb-b752-56b95a043ed5","resolution":{"observed_at":"2026-08-14T15:26:35.761897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.01191","last_updated":"2019-08-03T15:09:53Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-16T03:25:00.535913Z","submitted_at":"2019-08-03T15:09:53Z","title":"Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?"},"reference_resolution":{"displayed":67,"state_counts":{"malformed_identifier":11,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":43,"verified_exact":7,"verified_fuzzy":6},"total_outbound_references":67},"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 67 of 67 outbound references and 0 inbound Pith citation observations for arXiv:1908.01191."}