{"as_of":"2026-08-09T22:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:193266bc9032b801e71fe8571c65c8512e08ba0b58fc2efe176a6f4e2d8b4ac9","coverage":[{"denominator":88,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":88,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T11:59:09.563802Z","state":"measured"},{"denominator":88,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":88,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+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/2608.05500/citation-record","integrity":"/paper/2608.05500/integrity","json":"/paper/2608.05500/citation-record.json","paper":"/paper/2608.05500"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1407.2608","last_updated":"2014-07-09T20:00:07Z","snapshot_observed_at":"2026-07-06T03:48:33.625107Z","submitted_at":"2014-07-09T20:00:07Z","title":"Determining stellar atmospheric parameters and chemical abundances of FGK stars with iSpec","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2608","snapshot_observed_at":"2026-08-08T11:59:09.316077Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.316077Z"},"links":{"cited_paper":"/paper/1407.2608","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:9ba418092d0149666c8e372b6b0d186330e1c9741a91f6d44cc32b12042366f7","observation_id":"1d33ae0a-7a8d-4f3d-8f12-98ce967abded","resolution":{"observed_at":"2026-08-08T11:59:09.316077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.03769","last_updated":"2022-04-07T22:49:35Z","snapshot_observed_at":"2026-07-06T12:58:06.068351Z","submitted_at":"2022-04-07T22:49:35Z","title":"ARIADNE: Measuring accurate and precise stellar parameters through SED fitting","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03769","snapshot_observed_at":"2026-08-08T11:59:09.319937Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.319937Z"},"links":{"cited_paper":"/paper/2204.03769","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:c10c57e05230fbdc6cc23200457eac2d41e4311b9694a13119a0cbe16638007d","observation_id":"f23573cd-a964-410f-b727-660995df41fe","resolution":{"observed_at":"2026-08-08T11:59:09.319937Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.2624","last_updated":"2009-08-18T20:00:01Z","snapshot_observed_at":"2026-07-06T02:00:37.399439Z","submitted_at":"2009-08-18T20:00:01Z","title":"Accurate masses and radii of normal stars: modern results and applications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.2624","snapshot_observed_at":"2026-08-08T11:59:09.323201Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.323201Z"},"links":{"cited_paper":"/paper/0908.2624","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:d9df8e2760aaa80d1e4ebd4c55ec24122272a4617463041edcd8de5d38134c5e","observation_id":"a45f26b2-07ca-4805-8204-fc8a993d8382","resolution":{"observed_at":"2026-08-08T11:59:09.323201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.07834","last_updated":"2018-01-24T02:00:37Z","snapshot_observed_at":"2026-07-06T06:19:58.980832Z","submitted_at":"2018-01-24T02:00:37Z","title":"SkyMapper Southern Survey: First Data Release (DR1)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.07834","snapshot_observed_at":"2026-08-08T11:59:09.326390Z","title":", keywords =","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.326390Z"},"links":{"cited_paper":"/paper/1801.07834","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:4adcb9764a0e35a5b7b702f92baf3869a54eb42bcf415de5cf0f7a11c9ad68e3","observation_id":"bd0b5490-d4d9-4cb4-9123-b8c24e647998","resolution":{"observed_at":"2026-08-08T11:59:09.326390Z","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":"2026-08-08T11:59:09.329701Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.329701Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:74705654cfcbc8898240e130875b58fdd854c65b3ccb2ad059b6f2fbc9b47193","observation_id":"e2276c41-cfb2-4b04-b88a-735a2ba0d2af","resolution":{"observed_at":"2026-08-08T11:59:09.329701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.0031","last_updated":"2010-11-09T23:11:37Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2010-07-30T23:13:19Z","title":"The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.0031","snapshot_observed_at":"2026-08-08T11:59:09.332816Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.332816Z"},"links":{"cited_paper":"/paper/1008.0031","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:3a9bfbf09f6cfc03ece7e7dae800e56f68fe4d048a0f4bf8cfe1b380f8fdcfc5","observation_id":"b3396f6e-c28d-45a2-ac81-ec495dad8403","resolution":{"observed_at":"2026-08-08T11:59:09.332816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.0554","last_updated":"2008-05-05T15:34:05Z","snapshot_observed_at":"2026-07-06T01:37:52.705734Z","submitted_at":"2008-05-05T15:34:05Z","title":"A grid of MARCS model atmospheres for late-type stars I. Methods and general properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.0554","snapshot_observed_at":"2026-08-08T11:59:09.335933Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.335933Z"},"links":{"cited_paper":"/paper/0805.0554","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:967518a63b95afde6b915117975d86bb2d630ca2f17fc0e5fea9f013bd9502ef","observation_id":"489dacf7-1d2e-47f2-a518-80dbd7e5b332","resolution":{"observed_at":"2026-08-08T11:59:09.335933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405087","last_updated":"2004-05-05T15:30:48Z","snapshot_observed_at":"2026-07-07T00:42:19.442022Z","submitted_at":"2004-05-05T15:30:48Z","title":"New Grids of ATLAS9 Model Atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405087","snapshot_observed_at":"2026-08-08T11:59:09.339195Z","title":"Modelling of Stellar Atmospheres , year = 2003, editor =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.339195Z"},"links":{"cited_paper":"/paper/astro-ph/0405087","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:1153c2e489afbe518d0a531ec480eb3c726026ae7784da4f04bc93255cd60fe8","observation_id":"ca5c2795-ee86-43d9-bcee-935f484fad8f","resolution":{"observed_at":"2026-08-08T11:59:09.339195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5632","last_updated":"2013-04-24T11:04:19Z","snapshot_observed_at":"2026-07-06T03:09:25.962992Z","submitted_at":"2013-03-22T14:48:27Z","title":"A new extensive library of PHOENIX stellar atmospheres and synthetic spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5632","snapshot_observed_at":"2026-08-08T11:59:09.342560Z","title":"Astronomy and Astrophysics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.342560Z"},"links":{"cited_paper":"/paper/1303.5632","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:3309bfc5d12fed54d32869342cb6ab626ddf90397950f4e0466c9b31607cf66c","observation_id":"1f1d2f4d-08df-463c-b763-9175761b46bf","resolution":{"observed_at":"2026-08-08T11:59:09.342560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.5405","last_updated":"2010-11-24T15:57:46Z","snapshot_observed_at":"2026-07-06T02:19:40.798677Z","submitted_at":"2010-11-24T15:57:46Z","title":"Model Atmospheres From Very Low Mass Stars to Brown Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.5405","snapshot_observed_at":"2026-08-08T11:59:09.345681Z","title":"16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun , year = 2011, editor =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.345681Z"},"links":{"cited_paper":"/paper/1011.5405","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:5a0a80619ad2f9bd73c172673f089f5dbfa31b7424d1c9e9d1394d26d093f788","observation_id":"56a3540f-de7f-4611-aa17-8e89ccd95094","resolution":{"observed_at":"2026-08-08T11:59:09.345681Z","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":"2026-08-08T11:59:09.349136Z","title":"Astronomy and Astrophysics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.349136Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:621b440056bf57726481442c1eeff09c80d7358ad841da96c062aa5c1a0681e0","observation_id":"a8113f15-3a76-42e9-b69e-fbb203590352","resolution":{"observed_at":"2026-08-08T11:59:09.349136Z","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":"2026-08-08T11:59:09.351621Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.351621Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:7f2a3bd4b828eef95218998b450918de71cbfe8cf909229468e73bb151a1f8d4","observation_id":"5aae4eb3-24b5-4250-9742-475b7fc75dbe","resolution":{"observed_at":"2026-08-08T11:59:09.351621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00211","last_updated":"2022-07-30T13:18:15Z","snapshot_observed_at":"2026-08-08T06:26:45.516905Z","submitted_at":"2022-07-30T13:18:15Z","title":"Gaia Data Release 3: Summary of the content and survey properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.00211","snapshot_observed_at":"2026-08-08T11:59:09.354190Z","title":"Summary of the content and survey properties","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.354190Z"},"links":{"cited_paper":"/paper/2208.00211","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:8628c93e5cb1dec77eb1564a369f041ad84936b7a96f26fabec16be0c81c0e62","observation_id":"bfbbac0b-4b14-433b-9a1d-03e180529d08","resolution":{"observed_at":"2026-08-08T11:59:09.354190Z","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":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T11:59:10.613062Z","title":"Local standard of rest","venue":null,"work_id":"6c2e8c26-ca82-4928-965b-65865012ef01","year":2010},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.357063Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:89a09fa7ce9cd857cc33d46366828e9b58835576b7af04fa631ffef5fad3c69a","observation_id":"0a9a2ba8-53fa-4173-a86b-304fe9ea50d2","resolution":{"observed_at":"2026-08-08T11:59:10.615703Z","resolver_source":"arxiv_id_nonexistent","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.09051","last_updated":"2018-02-03T05:50:41Z","snapshot_observed_at":"2026-07-06T06:20:30.991203Z","submitted_at":"2018-01-27T08:23:31Z","title":"BANYAN. XI. The BANYAN $\\Sigma$ multivariate Bayesian algorithm to identify members of young associations within 150 pc","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.09051","snapshot_observed_at":"2026-08-08T11:59:09.359511Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.359511Z"},"links":{"cited_paper":"/paper/1801.09051","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:5aade1e6716d7661ba0967294c11134244625c43d0de27f96d84ddd5c043fcaa","observation_id":"5a80b4e1-f0a9-415d-a70a-f4527a5faf61","resolution":{"observed_at":"2026-08-08T11:59:09.359511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.00691","last_updated":"2020-11-20T06:04:18Z","snapshot_observed_at":"2026-08-08T21:11:38.251304Z","submitted_at":"2020-02-03T12:59:13Z","title":"Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.00691","snapshot_observed_at":"2026-08-08T11:59:09.362196Z","title":", keywords =","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.362196Z"},"links":{"cited_paper":"/paper/2002.00691","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:87dea39049c0051b25bd6c8c1230b871c5d9e218f24f18d5ee84f5a8edc9e598","observation_id":"2985034f-db8d-468c-aebf-1ed69d83631c","resolution":{"observed_at":"2026-08-08T11:59:09.362196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.05467","last_updated":"2020-03-11T18:09:44Z","snapshot_observed_at":"2026-07-06T09:04:04.935134Z","submitted_at":"2020-03-11T18:09:44Z","title":"Unresolved stellar companions with Gaia DR2 astrometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.05467","snapshot_observed_at":"2026-08-08T11:59:09.365359Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.365359Z"},"links":{"cited_paper":"/paper/2003.05467","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:20e9198c1f79e13b3cfd1f18b9f572cd58cac6577b787e594e9bcfa5b837c11a","observation_id":"49657604-092d-4546-889a-e42dec719b03","resolution":{"observed_at":"2026-08-08T11:59:09.365359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.1051","last_updated":"2012-11-05T22:03:45Z","snapshot_observed_at":"2026-07-06T02:59:12.334357Z","submitted_at":"2012-11-05T22:03:45Z","title":"Opening the 100-Year Window for Time Domain Astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.1051","snapshot_observed_at":"2026-08-08T11:59:09.368486Z","title":"New Horizons in Time Domain Astronomy , year = 2012, editor =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.368486Z"},"links":{"cited_paper":"/paper/1211.1051","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:6a5cd8e9f974f62458771244ce238b6e5239acbfb13c667b44de3b84643486a6","observation_id":"532d2719-6f37-4cc9-af81-593a40f00e0b","resolution":{"observed_at":"2026-08-08T11:59:09.368486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.00879","last_updated":"2018-03-28T21:20:09Z","snapshot_observed_at":"2026-07-06T06:21:33.612777Z","submitted_at":"2018-02-02T23:56:41Z","title":"ATLAS: A High-Cadence All-Sky Survey System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.00879","snapshot_observed_at":"2026-08-08T11:59:09.371283Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.371283Z"},"links":{"cited_paper":"/paper/1802.00879","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:0056752853e919a11a3e5bc7dd33e4095cc81b76bd79b07ae517cce9b9daa6e4","observation_id":"343c44ba-166b-41a3-b5e1-eb45e3674fb8","resolution":{"observed_at":"2026-08-08T11:59:09.371283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.07060","last_updated":"2017-06-21T18:00:08Z","snapshot_observed_at":"2026-07-06T05:47:54.334362Z","submitted_at":"2017-06-21T18:00:08Z","title":"The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.07060","snapshot_observed_at":"2026-08-08T11:59:09.374218Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.374218Z"},"links":{"cited_paper":"/paper/1706.07060","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e9ff181424b7ac436c3309c7b7dcba30bcbffe9593645d8d3e455ef62f53add5","observation_id":"f987d515-3383-40cd-9099-61148c26ba79","resolution":{"observed_at":"2026-08-08T11:59:09.374218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.0287","last_updated":"2007-05-02T13:47:18Z","snapshot_observed_at":"2026-08-09T17:25:09.143453Z","submitted_at":"2007-05-02T13:47:18Z","title":"The Wide Field Spectrograph (WiFeS)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.0287","snapshot_observed_at":"2026-08-08T11:59:09.377192Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.377192Z"},"links":{"cited_paper":"/paper/0705.0287","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:60361b2b25abb7b42116258debf8a852a66b091ce30b23b783890edc53c0f613","observation_id":"7ec15a51-8590-4750-a314-e86466401baf","resolution":{"observed_at":"2026-08-08T11:59:09.377192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.2666","last_updated":"2013-11-12T03:43:09Z","snapshot_observed_at":"2026-08-03T17:50:36.585587Z","submitted_at":"2013-11-12T03:43:09Z","title":"PyWiFeS: A Rapid Data Reduction Pipeline for the Wide Field Spectrograph (WiFeS)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.2666","snapshot_observed_at":"2026-08-08T11:59:09.380253Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.380253Z"},"links":{"cited_paper":"/paper/1311.2666","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:43daf1a26c6d2d6c80170dac4c550bcacdec3f8463c4149a5e95bb7fc18872c2","observation_id":"491e47bf-9ce6-4e5a-9253-1301cb90d56b","resolution":{"observed_at":"2026-08-08T11:59:09.380253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05144","last_updated":"2016-01-20T01:05:05Z","snapshot_observed_at":"2026-08-01T16:27:33.353696Z","submitted_at":"2016-01-20T01:05:05Z","title":"MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05144","snapshot_observed_at":"2026-08-08T11:59:09.382976Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.382976Z"},"links":{"cited_paper":"/paper/1601.05144","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:bc30086e4cbb6f0e1229503f05e34123bd9de9a7cd3384efd95b536461382cd6","observation_id":"9e53ab28-7aa6-40ad-9bb3-9f4c19da4859","resolution":{"observed_at":"2026-08-08T11:59:09.382976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04772","last_updated":"2018-01-15T12:36:00Z","snapshot_observed_at":"2026-08-04T10:26:52.692323Z","submitted_at":"2018-01-15T12:36:00Z","title":"Ten years of speckle interferometry at SOAR","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04772","snapshot_observed_at":"2026-08-08T11:59:09.385685Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.385685Z"},"links":{"cited_paper":"/paper/1801.04772","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:53368beee57768b3c26296bd806576c3a58de98fee552897d4acdd22d1a6b1de","observation_id":"c254092e-8be3-48e9-b5b4-38f895ac7c8a","resolution":{"observed_at":"2026-08-08T11:59:09.385685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10871","last_updated":"2019-11-11T14:46:43Z","snapshot_observed_at":"2026-08-06T01:51:02.780809Z","submitted_at":"2019-08-28T18:00:04Z","title":"SOAR TESS Survey. I: Sculpting of TESS planetary systems by stellar companions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.10871","snapshot_observed_at":"2026-08-08T11:59:09.388318Z","title":null,"venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.388318Z"},"links":{"cited_paper":"/paper/1908.10871","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:60d193ff6d05d5c44cef10d95ce67d520989858945fdb5073576b1ec037f91f7","observation_id":"fd8529f7-f03b-4a38-996d-7cabd60294cd","resolution":{"observed_at":"2026-08-08T11:59:09.388318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.08549","last_updated":"2019-11-04T22:06:08Z","snapshot_observed_at":"2026-08-05T08:42:32.184744Z","submitted_at":"2018-12-20T13:29:28Z","title":"Juliet: a versatile modelling tool for transiting and non-transiting exoplanetary systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.08549","snapshot_observed_at":"2026-08-08T11:59:09.391141Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.391141Z"},"links":{"cited_paper":"/paper/1812.08549","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:0c01798043f1612b550e9a4454481702e7daa27a1558abdd14a3eef2b8628bc8","observation_id":"abbdbcf4-5ea4-4d1c-99a7-3134644b7877","resolution":{"observed_at":"2026-08-08T11:59:09.391141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.02176","last_updated":"2021-12-03T22:20:02Z","snapshot_observed_at":"2026-07-06T12:15:13.803759Z","submitted_at":"2021-12-03T22:20:02Z","title":"The TESS Faint Star Search: 1,617 TOIs from the TESS Primary Mission","version":1},"cited_work":{"arxiv_id":"2112.02176","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.02176","snapshot_observed_at":"2026-08-08T11:59:10.488317Z","title":"The TESS Faint Star Search: 1,617 TOIs from the TESS Primary Mission","venue":"astro-ph.EP","work_id":"7e8a13ef-5989-4084-ac3d-386ce1644a39","year":2021},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.393871Z"},"links":{"cited_paper":"/paper/2112.02176","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:273841f7095be6ce249eabdc7288671c8a5c74a0f3a2b270c7a67979b8188aa1","observation_id":"6bb1a56b-0604-4985-81c2-a06415c2bb0c","resolution":{"observed_at":"2026-08-08T11:59:10.491193Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.06459","last_updated":"2020-11-12T16:00:58Z","snapshot_observed_at":"2026-08-05T01:43:29.600748Z","submitted_at":"2020-11-12T16:00:58Z","title":"Photometry of 10 Million Stars from the First Two Years of TESS Full Frame Images","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.06459","snapshot_observed_at":"2026-08-08T11:59:09.396619Z","title":"Research Notes of the American Astronomical Society , keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.396619Z"},"links":{"cited_paper":"/paper/2011.06459","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:519708a0ee681d1c31fd8b52b3e2ab1b52a76db854188ba1f08b0c6e6be90daa","observation_id":"fa63fc37-a73c-4683-b4ce-14ab09029a5f","resolution":{"observed_at":"2026-08-08T11:59:09.396619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0206099","last_updated":"2002-06-06T15:28:53Z","snapshot_observed_at":"2026-07-07T00:26:50.187441Z","submitted_at":"2002-06-06T15:28:53Z","title":"A box-fitting algorithm in the search for periodic transits","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0206099","snapshot_observed_at":"2026-08-08T11:59:09.399346Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.399346Z"},"links":{"cited_paper":"/paper/astro-ph/0206099","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:f4b225572370e9b63913cc6aa02ab89e0fb274e775c13a5e666651b5028449c7","observation_id":"1e6f2249-fd37-4411-b7a9-d6796bdf4dfa","resolution":{"observed_at":"2026-08-08T11:59:09.399346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02814","last_updated":"2021-11-08T10:02:34Z","snapshot_observed_at":"2026-07-06T12:05:25.336577Z","submitted_at":"2021-11-04T12:27:52Z","title":"prose: A Python framework for modular astronomical images processing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02814","snapshot_observed_at":"2026-08-08T11:59:09.402328Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.402328Z"},"links":{"cited_paper":"/paper/2111.02814","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:ff5403f09d9c63972b5101da16c67b1c5228d831d6bb3809d0627495276a4f49","observation_id":"76d9cb5a-3dc9-4ba3-9d92-0cf552b2abc4","resolution":{"observed_at":"2026-08-08T11:59:09.402328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.2437","last_updated":"2013-07-29T20:31:18Z","snapshot_observed_at":"2026-07-06T03:13:08.675100Z","submitted_at":"2013-05-10T20:47:54Z","title":"Las Cumbres Observatory Global Telescope Network","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.2437","snapshot_observed_at":"2026-08-08T11:59:09.405209Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.405209Z"},"links":{"cited_paper":"/paper/1305.2437","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:8cebda6778a1ceaaf29f1c9a4fc94b81ea13bfbad55bf00784d7ab94288d224d","observation_id":"d2756368-41dd-42ca-8d2b-8537deedb96f","resolution":{"observed_at":"2026-08-08T11:59:09.405209Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.03516","last_updated":"2016-10-22T17:40:09Z","snapshot_observed_at":"2026-07-06T04:11:45.635345Z","submitted_at":"2015-03-11T21:57:13Z","title":"Understanding The Effects Of Stellar Multiplicity On The Derived Planet Radii From Transit Surveys: Implications for Kepler, K2, and TESS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.03516","snapshot_observed_at":"2026-08-08T11:59:09.408051Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.408051Z"},"links":{"cited_paper":"/paper/1503.03516","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:53a4686f2b30b970edbc0217ba6621971cd0f7d22fd69d736c8708e8e7ea2e29","observation_id":"9bcb0d4f-72af-493b-99bd-bc7c146f7444","resolution":{"observed_at":"2026-08-08T11:59:09.408051Z","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":"2026-08-08T11:59:09.410989Z","title":"Publications of the Astronomical Society of Australia , author=","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.410989Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:9e36e6b1c5164b9e3c9805efb0e40c61b4ac2b9ae958741e034e10b0badd305d","observation_id":"621d6d89-0e72-40da-83fe-868b451f886d","resolution":{"observed_at":"2026-08-08T11:59:09.410989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5072","last_updated":"2013-07-18T20:19:59Z","snapshot_observed_at":"2026-07-06T03:18:35.692259Z","submitted_at":"2013-07-18T20:19:59Z","title":"Reanalysis of the FEROS observations of HIP 11952","version":1},"cited_work":{"arxiv_id":"1307.5072","doi":null,"metadata_source":"pith","pith_arxiv_id":"1307.5072","snapshot_observed_at":"2026-08-08T11:59:10.435985Z","title":"Reanalysis of the FEROS observations of HIP 11952","venue":"astro-ph.SR","work_id":"bb7270c7-e464-4f45-8fcb-3090b80bba04","year":2013},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.414189Z"},"links":{"cited_paper":"/paper/1307.5072","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:5db251fa5d513eee168c39aec50d5648e17bb35636eb960b3ac7110dbf0cdf3e","observation_id":"d322cdde-a1a9-40dc-a0f6-e3077162afdc","resolution":{"observed_at":"2026-08-08T11:59:10.438856Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.02279","last_updated":"2016-12-16T02:43:11Z","snapshot_observed_at":"2026-07-06T05:10:02.139648Z","submitted_at":"2016-09-08T05:26:20Z","title":"CERES: A Set of Automated Routines for Echelle Spectra","version":2},"cited_work":{"arxiv_id":"1609.02279","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.02279","snapshot_observed_at":"2026-08-08T11:59:10.424521Z","title":"CERES: A Set of Automated Routines for Echelle Spectra","venue":"astro-ph.IM","work_id":"0ad360e1-4829-49b1-b082-8d736d6eadce","year":2016},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.417360Z"},"links":{"cited_paper":"/paper/1609.02279","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:a63364e6d72494c1711b36e3521c66be6cfebd97a46b023def8ecb3893e52a6e","observation_id":"119536e9-fbb6-4f7c-a3d6-69079f106905","resolution":{"observed_at":"2026-08-08T11:59:10.427523Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:59:09.420118Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.420118Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:69e0971f3a58762222d6c376a6827becde35c376d01587c42fe1734955e3a856","observation_id":"eab87357-788d-4e96-a0fc-a92f002127e7","resolution":{"observed_at":"2026-08-08T11:59:09.420118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.01199","last_updated":"2020-07-01T16:50:12Z","snapshot_observed_at":"2026-08-05T20:51:25.853117Z","submitted_at":"2020-06-01T18:52:46Z","title":"Classifying Single Stars and Spectroscopic Binaries Using Optical Stellar Templates","version":2},"cited_work":{"arxiv_id":"2006.01199","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.01199","snapshot_observed_at":"2026-08-08T11:59:10.412766Z","title":"Classifying Single Stars and Spectroscopic Binaries Using Optical Stellar Templates","venue":"astro-ph.SR","work_id":"1e352ced-7340-4b0f-8f2f-d598dbb9a135","year":2020},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.422766Z"},"links":{"cited_paper":"/paper/2006.01199","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:418d838915a0ea0dd10c0925df1e11c1137c277e361957a3d3ba2b69d89a42a4","observation_id":"d96e097e-a3c1-40e4-836b-1c1ab4903b3d","resolution":{"observed_at":"2026-08-08T11:59:10.415825Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1307.2657","last_updated":"2013-07-10T02:42:52Z","snapshot_observed_at":"2026-07-06T03:17:51.662650Z","submitted_at":"2013-07-10T02:42:52Z","title":"Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-Main Sequence Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2657","snapshot_observed_at":"2026-08-08T11:59:09.425565Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.425565Z"},"links":{"cited_paper":"/paper/1307.2657","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e71f2f2d41cbe90267c647cf79cbeb788f79b3c8c54bf2b669275e66894f7826","observation_id":"f0f37e4a-5dbf-4c86-882f-8bc45ac050cb","resolution":{"observed_at":"2026-08-08T11:59:09.425565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.2573","last_updated":"2009-01-16T21:21:15Z","snapshot_observed_at":"2026-07-06T01:52:43.589353Z","submitted_at":"2009-01-16T21:21:15Z","title":"The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.2573","snapshot_observed_at":"2026-08-08T11:59:09.428366Z","title":"A new formalism for the floating-mean and Keplerian periodograms","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.428366Z"},"links":{"cited_paper":"/paper/0901.2573","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:eb5a243c07906e4943f4c771a1696a34a5ee2c536cbd9d384f59a59fa6fdadb5","observation_id":"e157b2cb-dd61-4252-a0a8-65eca17454e1","resolution":{"observed_at":"2026-08-08T11:59:09.428366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09710","last_updated":"2017-07-19T16:09:05Z","snapshot_observed_at":"2026-07-06T05:35:35.581300Z","submitted_at":"2017-03-28T18:00:02Z","title":"Fast and scalable Gaussian process modeling with applications to astronomical time series","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.09710","snapshot_observed_at":"2026-08-08T11:59:09.431235Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.431235Z"},"links":{"cited_paper":"/paper/1703.09710","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:391ed6d1dbf19a286daaa6708b087c7a91723855baeae272659701f7c6379b6c","observation_id":"fb845aae-1e94-447f-8b15-5146c7df7142","resolution":{"observed_at":"2026-08-08T11:59:09.431235Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.1391","last_updated":"2012-06-07T03:54:17Z","snapshot_observed_at":"2026-07-06T02:49:29.847162Z","submitted_at":"2012-06-07T03:54:17Z","title":"HATSouth: a global network of fully automated identical wide-field telescopes","version":1},"cited_work":{"arxiv_id":"1206.1391","doi":null,"metadata_source":"pith","pith_arxiv_id":"1206.1391","snapshot_observed_at":"2026-08-08T11:59:10.374785Z","title":"HATSouth: a global network of fully automated identical wide-field telescopes","venue":"astro-ph.EP","work_id":"83d07684-8433-430b-bc70-7a926e7d0fc9","year":2012},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.434040Z"},"links":{"cited_paper":"/paper/1206.1391","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:517d95c59e3ed0aa24b5db5829bb3b27b79afab11e40356c647e77b8f7d698e5","observation_id":"d283f53f-0c85-4bae-bc10-a3739ef1354d","resolution":{"observed_at":"2026-08-08T11:59:10.377812Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:59:09.436869Z","title":", year = 1995, month = nov, volume =","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.436869Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:849eaee1fcc706960eb3ff65cb174ed80104cd608dc46469bf2b4856f85128f7","observation_id":"f20163ea-0329-40df-9014-99d514304596","resolution":{"observed_at":"2026-08-08T11:59:09.436869Z","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":"2301.03704","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T11:59:10.361737Z","title":", keywords =","venue":null,"work_id":"6d7ae848-15e0-4049-a7cf-d41eadb11988","year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.439426Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:6426345bec7813952762cf64b56cc4f7724ca0e88dbc2dd7899e8da4d1377266","observation_id":"a881d289-d97b-4022-9c95-42352b31e9ce","resolution":{"observed_at":"2026-08-08T11:59:10.366142Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.11605","last_updated":"2022-09-23T14:18:48Z","snapshot_observed_at":"2026-08-02T14:48:18.340400Z","submitted_at":"2022-09-23T14:18:48Z","title":"The ESO Science Archive","version":1},"cited_work":{"arxiv_id":"2209.11605","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.11605","snapshot_observed_at":"2026-08-08T11:59:10.174956Z","title":"The ESO Science Archive","venue":"astro-ph.IM","work_id":"d64932e1-d649-4be3-8baa-7ff5fa4d3783","year":2022},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.442023Z"},"links":{"cited_paper":"/paper/2209.11605","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:da8df5216e693ba48e1a5d13dc62b1ca470dab39c67f743eca0766594edecc99","observation_id":"c8341139-9458-44db-a538-51dd5b002e8c","resolution":{"observed_at":"2026-08-08T11:59:10.177736Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.00012","last_updated":"2018-06-29T18:00:07Z","snapshot_observed_at":"2026-07-06T06:47:37.855343Z","submitted_at":"2018-06-29T18:00:07Z","title":"Photoevaporation and High-Eccentricity Migration Created the Sub-Jovian Desert","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.00012","snapshot_observed_at":"2026-08-08T11:59:09.444913Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.444913Z"},"links":{"cited_paper":"/paper/1807.00012","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:96f7d2475afd4223f15befb5fa27911d03dc1b7412349a99639bec00a59ac412","observation_id":"132b074d-1d8b-453b-b537-74fe5c249432","resolution":{"observed_at":"2026-08-08T11:59:09.444913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.06117","last_updated":"2018-01-18T16:44:09Z","snapshot_observed_at":"2026-07-06T06:19:14.564337Z","submitted_at":"2018-01-18T16:44:09Z","title":"Origins of Hot Jupiters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.06117","snapshot_observed_at":"2026-08-08T11:59:09.447838Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.447838Z"},"links":{"cited_paper":"/paper/1801.06117","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:576b887e01e4de1c585443393722c1d07abe1fca395dd8c4d12226485c943a70","observation_id":"739837be-60ba-4605-a0b7-be5800924206","resolution":{"observed_at":"2026-08-08T11:59:09.447838Z","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":"2026-08-08T11:59:09.450602Z","title":"Journal of Astronomical Telescopes, Instruments, and Systems , year = 2015, month = jan, volume =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.450602Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:cd4bc50714e1c3a606bf8f0ee5bdad9a5d3053da3d27082d9c744036bef02092","observation_id":"3943a247-c217-4ee5-805b-92cf7ff9d73a","resolution":{"observed_at":"2026-08-08T11:59:09.450602Z","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":"2026-08-08T11:59:09.453180Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.453180Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:37c695af66b43acf998f75abb8217a38196d7bde6e5ef6d5cd74aa7764f930e2","observation_id":"2e4a06d2-04ac-474c-bbeb-ee771e6fe4e8","resolution":{"observed_at":"2026-08-08T11:59:09.453180Z","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":"2026-08-08T11:59:09.455748Z","title":"Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave , year = 2016, editor =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.455748Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:affaa54ce1d9ff955765d98e687439023e016dc38a86c3bec432f5a89d3495ca","observation_id":"9354aa65-bd7d-452a-92f7-6d47dfd65d54","resolution":{"observed_at":"2026-08-08T11:59:09.455748Z","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":"2026-08-08T11:59:09.458417Z","title":"Optical and Infrared Spectroscopy of Circumstellar Matter , year = 1999, editor =","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.458417Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:0c0dc4c2101c4d58edfe8db04de4e3d1295688be69c532a8d0f2499018867acb","observation_id":"37690453-50e4-48ea-81d9-fdb55dd0c68c","resolution":{"observed_at":"2026-08-08T11:59:09.458417Z","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":"2026-08-08T11:59:09.461056Z","title":"Optical and IR Telescope Instrumentation and Detectors , year = 2000, editor =","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.461056Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:928e78ce3b33dbeef6083b483fb0dfb2fd820ec8b154664678af40ae8d8166d4","observation_id":"33f3a64f-29ea-4d9a-aeec-0917ecc9e100","resolution":{"observed_at":"2026-08-08T11:59:09.461056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.00373","last_updated":"2017-06-28T10:50:14Z","snapshot_observed_at":"2026-08-06T23:23:30.917463Z","submitted_at":"2017-04-02T21:53:57Z","title":"The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.00373","snapshot_observed_at":"2026-08-08T11:59:09.463693Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.463693Z"},"links":{"cited_paper":"/paper/1704.00373","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:100ee4e44b07416f3861947679251f163f2abeb8a39ba3aa5da1ad0d2a32c998","observation_id":"bf621d5b-2669-4899-9845-7dbf9a58ee6d","resolution":{"observed_at":"2026-08-08T11:59:09.463693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4293","last_updated":"2013-12-16T10:23:26Z","snapshot_observed_at":"2026-07-06T03:30:57.897408Z","submitted_at":"2013-12-16T10:23:26Z","title":"Planet-Disc Interactions and Early Evolution of Planetary Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4293","snapshot_observed_at":"2026-08-08T11:59:09.466416Z","title":"Protostars and Planets VI , year = 2014, editor =","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.466416Z"},"links":{"cited_paper":"/paper/1312.4293","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e2210af8e6db3e1370badcc67729ed37c112b7cac7fde4676c050aaaa0160e8c","observation_id":"37dff2c1-1d60-46a1-8622-adf7a207dc7f","resolution":{"observed_at":"2026-08-08T11:59:09.466416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.14694","last_updated":"2024-08-28T01:13:26Z","snapshot_observed_at":"2026-08-03T01:41:23.987752Z","submitted_at":"2024-08-26T23:47:24Z","title":"Searching for GEMS: Characterizing Six Giant Planets around Cool Dwarfs","version":2},"cited_work":{"arxiv_id":"2408.14694","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.14694","snapshot_observed_at":"2026-08-08T11:59:10.129950Z","title":"Searching for GEMS: Characterizing Six Giant Planets around Cool Dwarfs","venue":"astro-ph.EP","work_id":"409a922d-ffe8-41ee-a04c-882c3c7686b5","year":2024},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.469385Z"},"links":{"cited_paper":"/paper/2408.14694","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:a2d2e40a420f59c92354e87f7f2a96108a81d4f880a787366514e8f6e9bd0a3a","observation_id":"2d9d1476-faab-4f4d-8e0c-dc1e7501f0c5","resolution":{"observed_at":"2026-08-08T11:59:10.132952Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.10703","last_updated":"2019-06-25T18:00:07Z","snapshot_observed_at":"2026-07-06T08:02:45.611767Z","submitted_at":"2019-06-25T18:00:07Z","title":"TESS Hunt for Young and Maturing Exoplanets (THYME): A planet in the 45 Myr Tucana-Horologium association","version":1},"cited_work":{"arxiv_id":"1906.10703","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.10703","snapshot_observed_at":"2026-08-08T11:59:10.118418Z","title":"TESS Hunt for Young and Maturing Exoplanets (THYME): A planet in the 45 Myr Tucana-Horologium association","venue":"astro-ph.EP","work_id":"f582a446-21a0-4883-ad30-cc6946f25087","year":2019},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.472265Z"},"links":{"cited_paper":"/paper/1906.10703","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:f27b29d22a6827a7da8baccd1b8ce9b2b57615539f08d23f6ffc8062c5c7a28e","observation_id":"dcdf7dd9-a5fb-4812-86c0-4a8af6a73381","resolution":{"observed_at":"2026-08-08T11:59:10.121396Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:59:09.475167Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.475167Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:d44e0f475e89dbbf66b30707f6be04f7e9be22294b99e0dcdef8e968d0a294b2","observation_id":"c39c4a58-a25d-4042-ad5d-c74c3456694e","resolution":{"observed_at":"2026-08-08T11:59:09.475167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.03019","last_updated":"2016-09-10T09:44:34Z","snapshot_observed_at":"2026-07-06T05:10:18.891650Z","submitted_at":"2016-09-10T09:44:34Z","title":"The imprint of exoplanet formation history on observable present-day spectra of hot Jupiters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.03019","snapshot_observed_at":"2026-08-08T11:59:09.477748Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.477748Z"},"links":{"cited_paper":"/paper/1609.03019","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:0421a7ec9dc4b9e188c69c2a0f07d443863ddde1d6b552f4984b0d8702a86275","observation_id":"c8bf7350-2cc1-40be-b645-18e499208f44","resolution":{"observed_at":"2026-08-08T11:59:09.477748Z","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":"2026-08-08T11:59:09.480668Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.480668Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:fb317e40d2e1dbbc214e2dda0363659247b3ae5bdc1a9ea378c400dbfc4ca054","observation_id":"e0384163-66e8-4e60-983f-339d01c8856c","resolution":{"observed_at":"2026-08-08T11:59:09.480668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.00010","last_updated":"2016-07-05T09:57:17Z","snapshot_observed_at":"2026-07-06T04:51:21.601945Z","submitted_at":"2016-03-31T20:00:01Z","title":"Warm Jupiters from secular planet-planet interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.00010","snapshot_observed_at":"2026-08-08T11:59:09.483654Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.483654Z"},"links":{"cited_paper":"/paper/1604.00010","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:a6ab11a66881a1f5fe4d24d702fdc62a75a703605bd23ad1601cdc9a313a3aec","observation_id":"dc2f78c4-4dbf-499d-8cbd-64351118eb20","resolution":{"observed_at":"2026-08-08T11:59:09.483654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0807.1686","last_updated":"2008-07-10T18:24:46Z","snapshot_observed_at":"2026-07-06T01:41:41.210998Z","submitted_at":"2008-07-10T18:24:46Z","title":"Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0807.1686","snapshot_observed_at":"2026-08-08T11:59:09.486887Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.486887Z"},"links":{"cited_paper":"/paper/0807.1686","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:17a4277bf8350858482b65c347e45ca58ff7899797c0da304bdfaebc2d8a5636","observation_id":"5f8d2987-db8b-4595-8d44-201555514e06","resolution":{"observed_at":"2026-08-08T11:59:09.486887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.07175","last_updated":"2016-01-26T21:00:01Z","snapshot_observed_at":"2026-08-07T07:47:36.198038Z","submitted_at":"2016-01-26T21:00:01Z","title":"The Eccentric Kozai-Lidov Effect and Its Applications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.07175","snapshot_observed_at":"2026-08-08T11:59:09.489794Z","title":"Annual Review of Astronomy and Astrophysics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.489794Z"},"links":{"cited_paper":"/paper/1601.07175","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:49f755d6b06e5459b6ec408f3416090ed226201778ac418a00e4f5920018ef55","observation_id":"90a7fa2b-61aa-456d-9e30-f3e0b9833fb2","resolution":{"observed_at":"2026-08-08T11:59:09.489794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0606346","last_updated":"2006-06-14T16:48:23Z","snapshot_observed_at":"2026-08-09T19:06:05.137123Z","submitted_at":"2006-06-14T16:48:23Z","title":"Effects of Secular Interactions in Extrasolar Planetary Systems","version":1},"cited_work":{"arxiv_id":"astro-ph/0606346","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0606346","snapshot_observed_at":"2026-08-08T11:59:10.073695Z","title":"Effects of Secular Interactions in Extrasolar Planetary Systems","venue":"astro-ph","work_id":"e7901dbd-64ee-407e-b04a-520d1c4f6b2f","year":2006},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.492485Z"},"links":{"cited_paper":"/paper/astro-ph/0606346","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:c54462b3bd8fa51996c91e0448f3bf39039e0da5e493e321627efa0a65b44559","observation_id":"a5148be6-8adc-4b54-87fb-81d5ca9b51c1","resolution":{"observed_at":"2026-08-08T11:59:10.076797Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703163","last_updated":"2008-06-06T03:04:03Z","snapshot_observed_at":"2026-07-07T01:07:50.296173Z","submitted_at":"2007-03-07T23:49:20Z","title":"Origins of Eccentric Extrasolar Planets: Testing the Planet-Planet Scattering Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703163","snapshot_observed_at":"2026-08-08T11:59:09.495216Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.495216Z"},"links":{"cited_paper":"/paper/astro-ph/0703163","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e6a0e4023e8f284e5d1a88fe372c0e6b14649ce8095419e30ef52e5b75b6f055","observation_id":"31a2be86-2c99-4899-b6ad-fd906a1335db","resolution":{"observed_at":"2026-08-08T11:59:09.495216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.16204","last_updated":"2023-08-25T16:01:31Z","snapshot_observed_at":"2026-08-07T06:12:13.376053Z","submitted_at":"2023-05-25T16:06:52Z","title":"Transiting Exoplanet Yields for the Roman Galactic Bulge Time Domain Survey Predicted from Pixel-Level Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.16204","snapshot_observed_at":"2026-08-08T11:59:09.498068Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.498068Z"},"links":{"cited_paper":"/paper/2305.16204","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:9aa86e82b8db1495ba6b66e408a4cc6ebd22857c1a9e4ae9e3a0183a69fb7620","observation_id":"28abe0ab-23c1-47ec-bf46-e92f56f876ac","resolution":{"observed_at":"2026-08-08T11:59:09.498068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.05569","last_updated":"2019-02-14T19:15:58Z","snapshot_observed_at":"2026-07-06T07:33:12.016548Z","submitted_at":"2019-02-14T19:15:58Z","title":"The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.05569","snapshot_observed_at":"2026-08-08T11:59:09.500748Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.500748Z"},"links":{"cited_paper":"/paper/1902.05569","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:2ef6cdcbb28601229df3ef713eb22e0c77dac437bbf55038ebb2cabb658b1904","observation_id":"409986dd-69c5-4b1c-bfa7-dbdda2955415","resolution":{"observed_at":"2026-08-08T11:59:09.500748Z","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":"2511.04673","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T11:59:10.043187Z","title":", keywords =","venue":null,"work_id":"baebf943-a3a6-41e2-b3dd-cf342e623d4a","year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.503664Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:0026baac26ffbcb91753c801d07e1c4f200f1ade6eee635c7f6f927eae1c2fbd","observation_id":"3689577a-c9b4-495a-8816-19aa66beb7ba","resolution":{"observed_at":"2026-08-08T11:59:10.047719Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:59:09.506174Z","title":"Research Notes of the American Astronomical Society , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.506174Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:2fdd069bea31e75d1cfdde765ba8ca25bdc421d5ffbae5be4da29d6967625498","observation_id":"bd280044-a99f-4ebb-8ce3-a80a3530b7ae","resolution":{"observed_at":"2026-08-08T11:59:09.506174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.2150","last_updated":"2013-03-09T00:00:13Z","snapshot_observed_at":"2026-07-06T03:08:18.252982Z","submitted_at":"2013-03-09T00:00:13Z","title":"The Mass of KOI-94d and a Relation for Planet Radius, Mass, and Incident Flux","version":1},"cited_work":{"arxiv_id":"1303.2150","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.2150","snapshot_observed_at":"2026-08-08T11:59:09.850576Z","title":"The Mass of KOI-94d and a Relation for Planet Radius, Mass, and Incident Flux","venue":"astro-ph.EP","work_id":"3befec80-4686-4a78-9162-c74bd86d27d1","year":2013},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.508759Z"},"links":{"cited_paper":"/paper/1303.2150","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e740ebfdadd7ee889007807e6cc0a5bd8d658ee01f42b0073db009186847154e","observation_id":"7c7168c9-5aad-4dc8-a37a-3566be5324c6","resolution":{"observed_at":"2026-08-08T11:59:09.853739Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.03671","last_updated":"2018-09-14T21:54:27Z","snapshot_observed_at":"2026-07-06T06:38:17.165138Z","submitted_at":"2018-05-09T18:01:28Z","title":"A Framework for Prioritizing the TESS Planetary Candidates Most Amenable to Atmospheric Characterization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.03671","snapshot_observed_at":"2026-08-08T11:59:09.511562Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.511562Z"},"links":{"cited_paper":"/paper/1805.03671","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:5b1a5c1e7ae1b005df1ec164118640c282eb12461b88b14d214b0d300b8078c5","observation_id":"f3f0adce-5361-4b9c-97a1-ee8a23bc2a44","resolution":{"observed_at":"2026-08-08T11:59:09.511562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.04291","last_updated":"2020-09-09T13:26:33Z","snapshot_observed_at":"2026-08-09T20:13:23.211144Z","submitted_at":"2020-09-09T13:26:33Z","title":"Evidence of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.04291","snapshot_observed_at":"2026-08-08T11:59:09.515077Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.515077Z"},"links":{"cited_paper":"/paper/2009.04291","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e649a69c3a8fd80022d14c0a41665ea086fa562e9a4162ac7d19469d5196744f","observation_id":"6c16fee9-551d-4e38-a97e-e71062dd660e","resolution":{"observed_at":"2026-08-08T11:59:09.515077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2142","last_updated":"2008-02-15T11:47:30Z","snapshot_observed_at":"2026-07-06T01:31:38.281359Z","submitted_at":"2007-11-14T10:02:48Z","title":"Primary transit of the planet HD189733b at 3.6 and 5.8 microns","version":2},"cited_work":{"arxiv_id":"0711.2142","doi":null,"metadata_source":"pith","pith_arxiv_id":"0711.2142","snapshot_observed_at":"2026-08-08T11:59:09.820420Z","title":"Primary transit of the planet HD189733b at 3.6 and 5.8 microns","venue":"astro-ph","work_id":"340d6cb8-3c6b-461b-a388-78cbdc881c75","year":2007},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.517950Z"},"links":{"cited_paper":"/paper/0711.2142","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:c7f9999d9a8acb989e710795470288e9c86c171a44521c3250b8fb5a439719d9","observation_id":"a3c862cc-3023-4fac-8359-33ba68ece477","resolution":{"observed_at":"2026-08-08T11:59:09.823791Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.07595","last_updated":"2016-01-29T01:35:05Z","snapshot_observed_at":"2026-07-06T04:44:19.147136Z","submitted_at":"2016-01-27T23:30:43Z","title":"Statistics of Long Period Gas Giant Planets in Known Planetary Systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.07595","snapshot_observed_at":"2026-08-08T11:59:09.520722Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.520722Z"},"links":{"cited_paper":"/paper/1601.07595","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:e197510040dfdf1e140857767db085a8cf96ce79ce6b8e4cf12a3d9d6a2104d5","observation_id":"ffc0d335-2b05-45f8-ad80-1f96a8a89962","resolution":{"observed_at":"2026-08-08T11:59:09.520722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.2954","last_updated":"2014-03-13T22:18:17Z","snapshot_observed_at":"2026-07-06T03:30:31.888709Z","submitted_at":"2013-12-10T21:00:03Z","title":"Friends of Hot Jupiters I: A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.2954","snapshot_observed_at":"2026-08-08T11:59:09.523775Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.523775Z"},"links":{"cited_paper":"/paper/1312.2954","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:3fe6f861eaf26374a971f34167e5ec299545fb42280262d7377e538f13ba32b4","observation_id":"1f7f747a-2da3-47f4-a79b-ff808e364095","resolution":{"observed_at":"2026-08-08T11:59:09.523775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.10852","last_updated":"2020-03-24T13:56:11Z","snapshot_observed_at":"2026-07-06T09:06:58.966574Z","submitted_at":"2020-03-24T13:56:11Z","title":"TESS spots a hot Jupiter with an inner transiting Neptune","version":1},"cited_work":{"arxiv_id":"2003.10852","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.10852","snapshot_observed_at":"2026-08-08T11:59:09.790941Z","title":"TESS spots a hot Jupiter with an inner transiting Neptune","venue":"astro-ph.EP","work_id":"cbaf6e9c-6fc0-4068-af7e-c601ffa1067c","year":2020},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.526425Z"},"links":{"cited_paper":"/paper/2003.10852","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:d442a57bac561788609884543e2eebc056c313b36b0c33558d8704360a558803","observation_id":"2a6b932b-9040-4100-a5c4-7a12136570a6","resolution":{"observed_at":"2026-08-08T11:59:09.794503Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1508.02411","last_updated":"2021-11-15T21:46:00Z","snapshot_observed_at":"2026-07-06T04:26:19.776042Z","submitted_at":"2015-08-10T20:12:23Z","title":"WASP-47: A Hot Jupiter System with Two Additional Planets Discovered by K2","version":3},"cited_work":{"arxiv_id":"1508.02411","doi":null,"metadata_source":"pith","pith_arxiv_id":"1508.02411","snapshot_observed_at":"2026-08-08T11:59:09.775633Z","title":"WASP-47: A Hot Jupiter System with Two Additional Planets Discovered by K2","venue":"astro-ph.EP","work_id":"29235199-112d-4731-a2cc-bb6aa04d8e38","year":2015},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.529085Z"},"links":{"cited_paper":"/paper/1508.02411","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:bf31fb2b0d94e3f68983f65f1e45dd743f66741153e35062d81a7d0d36b83191","observation_id":"7baa7991-7148-4f91-a98d-398220616594","resolution":{"observed_at":"2026-08-08T11:59:09.780701Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0606175","last_updated":"2006-06-07T21:05:29Z","snapshot_observed_at":"2026-08-02T11:43:56.221088Z","submitted_at":"2006-06-07T21:05:29Z","title":"The James Webb Space Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0606175","snapshot_observed_at":"2026-08-08T11:59:09.531743Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.531743Z"},"links":{"cited_paper":"/paper/astro-ph/0606175","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:c7893319b519a42f725af8d9531e2c2207acb071c20c916e16e5ce03e2eb5c87","observation_id":"9b025bd5-30d6-4d98-b6be-f1fab47ce54f","resolution":{"observed_at":"2026-08-08T11:59:09.531743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.4804","last_updated":"2011-09-22T21:24:18Z","snapshot_observed_at":"2026-07-06T02:21:05.525174Z","submitted_at":"2010-12-21T21:00:01Z","title":"Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.4804","snapshot_observed_at":"2026-08-08T11:59:09.534433Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.534433Z"},"links":{"cited_paper":"/paper/1012.4804","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:d49498a57d06ae2789197f94572b1e561c88ab0463400ce99400a81bb99e0699","observation_id":"04f2546d-e724-45cf-bdf1-94b6696d3baf","resolution":{"observed_at":"2026-08-08T11:59:09.534433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.04163","last_updated":"2018-11-10T00:08:13Z","snapshot_observed_at":"2026-07-06T07:13:49.181221Z","submitted_at":"2018-11-10T00:08:13Z","title":"Real-time processing of the imaging data from the network of Las Cumbres Observatory Telescopes using BANZAI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.04163","snapshot_observed_at":"2026-08-08T11:59:09.537329Z","title":"Software and Cyberinfrastructure for Astronomy V , year = 2018, editor =","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.537329Z"},"links":{"cited_paper":"/paper/1811.04163","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:afd5ab4e1467e17726079883ef486a720840d75bfc9c87a6d799ff96d73479b7","observation_id":"3102bfc1-4b2f-4787-bea6-5b2afde905fd","resolution":{"observed_at":"2026-08-08T11:59:09.537329Z","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":"2026-08-08T11:59:09.540028Z","title":"American Astronomical Society Meeting Abstracts \\#233 , year = 2019, series =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.540028Z"},"links":{"citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:9646b6a9ea6aa1d2bbd0352932b03c4a0629bc58cb1b3654bb82ac0ef332f6fa","observation_id":"51490aaa-acb3-4ecb-b482-e0ff1a0a83ce","resolution":{"observed_at":"2026-08-08T11:59:09.540028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.3971","last_updated":"2013-09-16T14:18:10Z","snapshot_observed_at":"2026-08-04T16:48:13.726945Z","submitted_at":"2013-09-16T14:18:10Z","title":"CHIRON - A Fiber Fed Spectrometer for Precise Radial Velocities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.3971","snapshot_observed_at":"2026-08-08T11:59:09.542392Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.542392Z"},"links":{"cited_paper":"/paper/1309.3971","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:0352ee0d9f22635e3be87f85c0f112d58c48f580d5d5b6d6514b7b38259f28b6","observation_id":"cae29978-652e-43e5-ac46-af78b1a6dcae","resolution":{"observed_at":"2026-08-08T11:59:09.542392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08285","last_updated":"2015-08-19T03:48:44Z","snapshot_observed_at":"2026-07-06T04:25:16.554761Z","submitted_at":"2015-07-29T20:10:41Z","title":"batman: BAsic Transit Model cAlculatioN in Python","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.08285","snapshot_observed_at":"2026-08-08T11:59:09.545062Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.545062Z"},"links":{"cited_paper":"/paper/1507.08285","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:7440b9ec84b66a583f841fb539374daeb896afa218201b638ad5038576ccc362","observation_id":"c6cfb661-7472-4e08-86e0-33ff9015bc0e","resolution":{"observed_at":"2026-08-08T11:59:09.545062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.01947","last_updated":"2018-01-06T00:37:42Z","snapshot_observed_at":"2026-07-06T06:17:24.959986Z","submitted_at":"2018-01-06T00:37:42Z","title":"RadVel: The Radial Velocity Modeling Toolkit","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.01947","snapshot_observed_at":"2026-08-08T11:59:09.547575Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.547575Z"},"links":{"cited_paper":"/paper/1801.01947","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:f844a0f154ba7d48535c6812865159d9b89981705d2cd1335b16408cca7a5272","observation_id":"5680d7cd-754d-495a-abec-a6b4c205f81a","resolution":{"observed_at":"2026-08-08T11:59:09.547575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.0009","last_updated":"2013-08-14T16:30:16Z","snapshot_observed_at":"2026-07-06T03:19:41.818517Z","submitted_at":"2013-07-31T20:00:00Z","title":"Efficient, uninformative sampling of limb darkening coefficients for two-parameter laws","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.0009","snapshot_observed_at":"2026-08-08T11:59:09.550289Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.550289Z"},"links":{"cited_paper":"/paper/1308.0009","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:2809e5e20e59fb50278835791a1de3b706486a5ad44e53e3144a34f207dac489","observation_id":"c113b3d9-864b-42d6-906e-760db103b617","resolution":{"observed_at":"2026-08-08T11:59:09.550289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02180","last_updated":"2019-04-03T18:04:57Z","snapshot_observed_at":"2026-07-06T07:43:43.696691Z","submitted_at":"2019-04-03T18:04:57Z","title":"dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02180","snapshot_observed_at":"2026-08-08T11:59:09.552808Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.552808Z"},"links":{"cited_paper":"/paper/1904.02180","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:3934887e1d6dfc0dbc37c9c767be03626f5387addaf5914b3c8f16c37040627f","observation_id":"628f3b24-977e-437a-ad10-e88d8e84d6a2","resolution":{"observed_at":"2026-08-08T11:59:09.552808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20588","last_updated":"2025-05-26T23:45:44Z","snapshot_observed_at":"2026-08-08T11:35:05.695585Z","submitted_at":"2025-05-26T23:45:44Z","title":"Continuous helium absorption from the leading and trailing tails of WASP-107b","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20588","snapshot_observed_at":"2026-08-08T11:59:09.555607Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.555607Z"},"links":{"cited_paper":"/paper/2505.20588","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:fcc1b5edd53ed5ca55d2719e25c2121fbabaf9558e1d91024c8d80ba9acf54e5","observation_id":"e29d42c7-fa15-40db-b707-f9df7aa9e4f8","resolution":{"observed_at":"2026-08-08T11:59:09.555607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.10919","last_updated":"2021-05-24T20:33:19Z","snapshot_observed_at":"2026-08-07T22:23:26.115765Z","submitted_at":"2021-01-26T16:40:51Z","title":"Identifying Planetary Transit Candidates in TESS Full-Frame Image Light Curves via Convolutional Neural Networks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.10919","snapshot_observed_at":"2026-08-08T11:59:09.558430Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.558430Z"},"links":{"cited_paper":"/paper/2101.10919","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:b4260b5115fbc67c71dbdac182759fbb84fce53e63dc4393a02a752612536e3f","observation_id":"ef878d96-a01e-41f2-ba4e-cdf1ebee5db3","resolution":{"observed_at":"2026-08-08T11:59:09.558430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.04817","last_updated":"2017-01-17T10:02:03Z","snapshot_observed_at":"2026-08-08T08:09:52.266405Z","submitted_at":"2017-01-17T10:02:03Z","title":"AstroImageJ: Image Processing and Photometric Extraction for Ultra-Precise Astronomical Light Curves (Expanded Edition)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.04817","snapshot_observed_at":"2026-08-08T11:59:09.561043Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.561043Z"},"links":{"cited_paper":"/paper/1701.04817","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:2daf3c97f67edd5246823f5bd5844a62db27e5051591fe66e7da8a9b605155ba","observation_id":"0403df15-cff1-4a0d-ab99-4dec24c50859","resolution":{"observed_at":"2026-08-08T11:59:09.561043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.6182","last_updated":"2012-12-26T14:11:13Z","snapshot_observed_at":"2026-07-06T03:02:51.507561Z","submitted_at":"2012-12-26T14:11:13Z","title":"The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.6182","snapshot_observed_at":"2026-08-08T11:59:09.563802Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-08T11:59:09.563802Z"},"links":{"cited_paper":"/paper/1212.6182","citing_paper":"/paper/2608.05500"},"observation_digest":"sha256:9e1e1d58dac41a83179f181392404f34608cf9ca5744bca8a899e31176652970","observation_id":"71221248-45a4-4a69-a5fd-5981be738336","resolution":{"observed_at":"2026-08-08T11:59:09.563802Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.05500","last_updated":"2026-08-06T01:10:52Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-09T21:10:37.618128Z","submitted_at":"2026-08-06T01:10:52Z","title":"The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars"},"reference_resolution":{"displayed":88,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":72,"verified_exact":14,"verified_fuzzy":0},"total_outbound_references":88},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 88 of 88 outbound references and 0 inbound Pith citation observations for arXiv:2608.05500."}