{"as_of":"2026-08-19T05:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:271566ba464f4d5ca103656136ce06d4eb7c2a252e5c0815e705fa8246aab766","coverage":[{"denominator":75,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":75,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T10:16:18.752767Z","state":"measured"},{"denominator":75,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":75,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+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/2608.07331/citation-record","integrity":"/paper/2608.07331/integrity","json":"/paper/2608.07331/citation-record.json","paper":"/paper/2608.07331"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.483830Z","title":"L., Chen, X., Ciardi, D., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.483830Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:272285cb012772f15916f02cd59a5bf0698ae719a822c7b2768c7a731e516a7a","observation_id":"70f01be1-367e-4acc-9b97-6d8ccbace470","resolution":{"observed_at":"2026-08-10T10:16:18.483830Z","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":"2026-08-10T10:16:18.487855Z","title":"M., Rosenfeld, K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.487855Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:3f1703028c84a589c96869c5aac564904077e587a18147a06ab4c65216d7cb6e","observation_id":"ac9d2204-9324-4700-bce6-37c7c3632cf3","resolution":{"observed_at":"2026-08-10T10:16:18.487855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/710/2/1596","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.249567Z","title":"J., & Elsworth, Y","venue":null,"work_id":"98c73ea4-d68c-4900-a9f2-e92af8aaa080","year":2010},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.491438Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:5931c1d83cc17bd1c1d7c843575d69b614b3186ccf555b27f36c94c043ef746b","observation_id":"c8be7009-b4fa-4b03-8cec-2b740d9f5313","resolution":{"observed_at":"2026-08-10T10:16:19.253707Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:07.356608+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:07.356608+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.494926Z","title":"A., Huber, D., van Saders, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.494926Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:3ac4277c232ddeeedbbd7bda7e616af2e1aed5b78cf15248f0fa1882d3f88595","observation_id":"98a49e48-5692-4105-a75b-e859beefa00f","resolution":{"observed_at":"2026-08-10T10:16:18.494926Z","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":"2026-08-10T10:16:18.498577Z","title":"M., Christiansen, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.498577Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:1ed25aa311ee3e62dc1e26dc03eacfd81fe243327f803947bf82fabde02a7d42","observation_id":"5e44198f-e157-44a2-93aa-dbc58e911fdf","resolution":{"observed_at":"2026-08-10T10:16:18.498577Z","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":"2026-08-10T10:16:18.501962Z","title":"J., Koch, D., Basri, G., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.501962Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:2b3a2f0aae62da209b564c5e2135306b7a5f7d417bfaccff25f097bf4cb56e6f","observation_id":"8d8523b9-4fad-4765-8904-681b21935c35","resolution":{"observed_at":"2026-08-10T10:16:18.501962Z","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":"2026-08-10T10:16:18.505680Z","title":"M., & Fischer, D","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.505680Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:43373fd8ad5294c283396acd568c7309d22a3a94f169512684029de6017c0635","observation_id":"d625a8ea-3df2-4f71-bbfe-49212b79ca4b","resolution":{"observed_at":"2026-08-10T10:16:18.505680Z","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":"2026-08-10T10:16:18.512214Z","title":"M., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.512214Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:b85ed61d902247bae3cd3bbc9718ee561fde36d90351cbc392db9845c5918c29","observation_id":"07e4f39b-0913-4e86-9cad-db1b70962608","resolution":{"observed_at":"2026-08-10T10:16:18.512214Z","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":"2026-08-10T10:16:18.515606Z","title":"A., Bizzarro, M., Latham, D","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.515606Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:d1b81deacb7a85f0aedd7337928c689489efb9c04a1c8a42f40d5a46794a1faf","observation_id":"3930c2b3-6c96-41ed-9998-1fed307c9892","resolution":{"observed_at":"2026-08-10T10:16:18.515606Z","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":"2026-08-10T10:16:18.518819Z","title":"C., O’Brien, D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.518819Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:9d1901502c9fe6e4637170a00a86543cbc84931a3f49edaf10b3523b9e42756b","observation_id":"920657e6-84a6-45d6-b9ae-5142321eb728","resolution":{"observed_at":"2026-08-10T10:16:18.518819Z","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":"2026-08-10T10:16:19.456203Z","title":"2007, MNRAS, 374, L42, doi: 10.1111/j.1745-3933.2006.00261.x","venue":null,"work_id":"597bc8b1-37e2-4f3b-9f43-7108334f433b","year":2007},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.522184Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:e5d4e2ab2f0bd1d6331c550df8ef2f95db23ec72ea9ae999b54c83d070fdc907","observation_id":"fa5108c6-47bb-48a1-bfa2-b81cd14a0efb","resolution":{"observed_at":"2026-08-10T10:16:19.459593Z","resolver_source":"arxiv_id_nonexistent","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.525801Z","title":"2026, Nature Astronomy, 10, 92, doi: 10.1038/s41550-025-02693-6","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.525801Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:c5e872fd417d2885c9cfdcd9a290466de69bc7d7b39ed813a57ec27570fbcaf3","observation_id":"04387160-5b80-4a12-8628-b68cd5ad0bdf","resolution":{"observed_at":"2026-08-10T10:16:18.525801Z","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":"2026-08-10T10:16:18.529308Z","title":"2021, AJ, 162, 100, doi: 10.3847/1538-3881/ac0f08","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.529308Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:988e5f2ae04ba506cbcf7110497d83f6f85da5cd6b7019f3c7c8754754dcbe79","observation_id":"1dbac2d5-1ee0-46c9-99b1-65bb98c77fd7","resolution":{"observed_at":"2026-08-10T10:16:18.529308Z","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":"2026-08-10T10:16:18.532621Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.532621Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:a57511cc6a73466d91c74dfe96596674664dbb3a3b396fa17724400d2f0e2050","observation_id":"345177c2-a5d2-43e3-92fe-fe34bab4e0ee","resolution":{"observed_at":"2026-08-10T10:16:18.532621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ae5633","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.181267Z","title":"L., Lu, Z., & Ye, L","venue":null,"work_id":"8b15806c-2b65-4484-baa1-381d2eba87e5","year":2026},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.536807Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:3582463032eb1dd427b0991ff123058ea25dbdeacfdbed711a38c35a7493c7b8","observation_id":"0b403c07-89a7-4ef7-bddd-35175b64f690","resolution":{"observed_at":"2026-08-10T10:16:19.184480Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:08.023565+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:08.023565+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ae12a2","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.171664Z","title":"2025, ApJ, 995, 33, doi: 10.3847/1538-4357/ae12a2","venue":null,"work_id":"4cdb557a-9e7d-477d-87fd-a7d368b09314","year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.540229Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:43db8493be5a9cc5c1b0b41970071640b94d731721e70fe11c189d198103dcad","observation_id":"80952b56-e1aa-4173-bf79-0a49a5cddb74","resolution":{"observed_at":"2026-08-10T10:16:19.175010Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:08.07541+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:08.07541+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.543756Z","title":"2012, Research in Astronomy and Astrophysics, 12, 1197, doi: 10.1088/1674-4527/12/9/003","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.543756Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:14febf311d29ddaf1507ef35533666b5016e0c55ff47064b83635a4797b24c37","observation_id":"0ea08d31-1d2f-4a20-aeea-1088b90e611c","resolution":{"observed_at":"2026-08-10T10:16:18.543756Z","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":"2026-08-10T10:16:18.547947Z","title":"J., Contardo, G., Sandoval, A., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.547947Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:5954257ad8def5f4e1dbe64d00af05f9418faca8a6d1db2be5d1e5c5d046acf8","observation_id":"436b8e5a-7df2-4d26-a206-bd4ab3727347","resolution":{"observed_at":"2026-08-10T10:16:18.547947Z","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":"2026-08-10T10:16:18.551202Z","title":"I., & Murray-Clay, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.551202Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:acde993ead66ffb3a7a3a570d9a21530ddf35a596600657dae9867aff0820307","observation_id":"708e42e9-128b-4897-8c9e-5422784044df","resolution":{"observed_at":"2026-08-10T10:16:18.551202Z","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":"2026-08-10T10:16:18.554562Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.554562Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:6fbc14150fa97361318709910af913958af4aa2b41e7a2d6cbd127d2e0d27e1a","observation_id":"7d34dfa2-f669-4074-93ac-af1776394f36","resolution":{"observed_at":"2026-08-10T10:16:18.554562Z","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":"2026-08-10T10:16:18.557767Z","title":"2014, ApJL, 789, L3, doi: 10.1088/2041-8205/789/1/L3","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.557767Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:0a5f94e95e0ab4d4dbbf5cae48e9f2876b99e2ae8bad40a1242a87cf4ab206f5","observation_id":"2e0c3983-5cd7-44b7-9146-f7487aa756f3","resolution":{"observed_at":"2026-08-10T10:16:18.557767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/771/2/107","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.132923Z","title":"E., Howell, S","venue":null,"work_id":"eecbcba2-85ba-488d-94be-240e1c83ed5c","year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.561994Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:d26e6087c79b5891106f89ba472ce24ba29ff343c4905f64ad139e2cd6d31d6c","observation_id":"20c235f8-508a-40f9-bee6-731c1c324f83","resolution":{"observed_at":"2026-08-10T10:16:19.136457Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:08.374302+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:08.374302+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.565273Z","title":"K., Frankel, N., Lind, K., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.565273Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:352fbcf66859ac22189efb7cebc45b1289d58f9183f22ff3a11550481f99ec89","observation_id":"3e071941-09be-4fee-b09d-e9d3db52fbeb","resolution":{"observed_at":"2026-08-10T10:16:18.565273Z","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":"2026-08-10T10:16:18.568536Z","title":"K., Bovy, J., Holtzman, J., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.568536Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:e93c6133e43a109faa1b77350234ad2915ff431a19e3184ae7bc3922c73d5b67","observation_id":"7fc07cc2-158f-4691-a6ed-23a57f10bc47","resolution":{"observed_at":"2026-08-10T10:16:18.568536Z","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":"2026-08-10T10:16:18.572081Z","title":"A., & Valenti, J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.572081Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:43a85dedf650d8ea24295820b8faad8af26e64f1eb933c2bcb02928d81c4ad63","observation_id":"574a2484-485c-4ed1-8492-00f580f45a15","resolution":{"observed_at":"2026-08-10T10:16:18.572081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-6256/149/4/143","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.104355Z","title":"W., Mahadevan, S., Deshpande, R., et al","venue":null,"work_id":"7159a362-d666-49ee-aae4-2c285ce489f0","year":2015},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.575449Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:2f3e17b28c4bb62978464cd7b6afd95ee4b44d381dddf8de64f629adc6f89374","observation_id":"409bdc9d-0e14-460e-9b1c-ae578b1494f9","resolution":{"observed_at":"2026-08-10T10:16:19.107802Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:08.539831+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:08.539831+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.578592Z","title":"J., Petigura, E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.578592Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:a88c7b3c67224c84afd7d1dac0ce1cd93356987ce5e1c827c21e87d831ae8abf","observation_id":"7270a6fa-3ffe-4da1-911b-0d2429f2c8a5","resolution":{"observed_at":"2026-08-10T10:16:18.578592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.660267Z","title":"2013, Physics and Chemistry of Circumstellar Dust Shells","venue":null,"work_id":"fdfd9461-9ef7-4168-a306-cef7a3144166","year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.582250Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:daac8982e22507be789be7cb27a7a215dc37ae5d2d8c03f3aeded1d30f3a182b","observation_id":"7777983a-74ce-4f3a-8211-55e010624351","resolution":{"observed_at":"2026-08-10T10:16:19.663794Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.585557Z","title":"2026, ApJ, 998, 301, doi: 10.3847/1538-4357/ae317d","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.585557Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:839f4c69536e1a956a3c7b653a6e2d89a83899e1f468b4e81dc7ed4d244f867e","observation_id":"b182af80-e2b6-4ea0-b623-976c3f5ebbdd","resolution":{"observed_at":"2026-08-10T10:16:18.585557Z","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":"2026-08-10T10:16:18.588838Z","title":"E., & Sari, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.588838Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:452ca7d8e9653b0bb929c9f2a8c94826b797162aaa9670fefe581c6085a510de","observation_id":"d984a130-7844-4643-8a36-123a768ac3a4","resolution":{"observed_at":"2026-08-10T10:16:18.588838Z","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":"2026-08-10T10:16:18.592305Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.592305Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:06dde398cf737c16bba559870805838bb8e2e6b0b9d2179ffc233c531d01148e","observation_id":"25b0dc92-3fa9-4ddc-b8b3-5d1715cc2270","resolution":{"observed_at":"2026-08-10T10:16:18.592305Z","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":"2026-08-10T10:16:18.595623Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.595623Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:c4f52c7201dfd1f9034f33be219b736dd9bd5f69a31ffdde27b88201435b4dd5","observation_id":"7c871f51-4ff4-4108-b7c4-95d77d5c9e76","resolution":{"observed_at":"2026-08-10T10:16:18.595623Z","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":"2026-08-10T10:16:18.598987Z","title":"D., Katz, D., & G´ omez, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.598987Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:4a44d5a0d12944efe8d551bcc052bbc1794ea1c30383e8bf984e0c13314140cf","observation_id":"b1ba4cf0-e0e4-4265-8fdb-1a05b8c4d5bd","resolution":{"observed_at":"2026-08-10T10:16:18.598987Z","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":"2026-08-10T10:16:18.602342Z","title":"2014, ApJ, 795, 65, doi: 10.1088/0004-637X/795/1/65","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.602342Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:3992f1642ecdede33787a0ba95c6bd1c2bb4f8224dd08192c7666b3fa23bc882","observation_id":"b58dcb41-450a-4bb5-9cf7-55cac10ee35d","resolution":{"observed_at":"2026-08-10T10:16:18.602342Z","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":"2026-08-10T10:16:18.609045Z","title":"A., Aller, K","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.609045Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:8b51b0660a4c8a4d9f34bcdc68850dcfa63621f154b2b958bd11dab9c26ea933","observation_id":"fc64abcd-6200-40fd-813d-5f4e7952a9f7","resolution":{"observed_at":"2026-08-10T10:16:18.609045Z","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":"2026-08-10T10:16:18.612390Z","title":"2010, A&A, 522, A1, doi: 10.1051/0004-6361/201015263 Kov´ acs, G., Hartman, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.612390Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:2cfe3a0995093babbf3b0e81d0f0a70c65b4d25b080c7e9bb541bd97ba0f9c23","observation_id":"620e43b2-c8ab-4c5b-8833-8108d2477e70","resolution":{"observed_at":"2026-08-10T10:16:18.612390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504214","last_updated":"2005-05-02T03:44:21Z","snapshot_observed_at":"2026-07-07T00:49:48.159367Z","submitted_at":"2005-04-08T20:12:45Z","title":"Extrasolar Carbon Planets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504214","snapshot_observed_at":"2026-08-10T10:16:18.615570Z","title":"J., & Seager, S","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.615570Z"},"links":{"cited_paper":"/paper/astro-ph/0504214","citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:7ff7315986bc6d6554bb41f1477dd8500fbff06ce017d0961827cd76d35237fd","observation_id":"0ac961c4-5a72-4931-9423-b7dda876e51a","resolution":{"observed_at":"2026-08-10T10:16:18.615570Z","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":"2026-08-10T10:16:18.619238Z","title":"2021, A&A, 649, A4, doi: 10.1051/0004-6361/202039653","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.619238Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:a8d197514503bfe35929eb20d2dd5f555185e03a92db5839a5600a26e667e784","observation_id":"255ee79a-5e09-4067-bb7d-4bf637e73d4e","resolution":{"observed_at":"2026-08-10T10:16:18.619238Z","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":"2026-08-10T10:16:18.622586Z","title":"D., & Fortney, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.622586Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:1045d6ae4029c99ecdfda582146d110d2d49b8363b35027009b0f03ab9d3f36d","observation_id":"eaf33ea6-1c49-41ea-b0bf-9403f0855a93","resolution":{"observed_at":"2026-08-10T10:16:18.622586Z","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":"2026-08-10T10:16:18.626244Z","title":"L., Ness, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.626244Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:89fe65d344db1a70d8679215fc0d7731203e3b6171e3e42cb17a93ee5f65a5fc","observation_id":"df2acf26-3b78-40d6-b1b2-4e649e269f04","resolution":{"observed_at":"2026-08-10T10:16:18.626244Z","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":"2026-08-10T10:16:18.629503Z","title":"L., Minchev, I., Buck, T., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.629503Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:07d534111aa760c1f645bc25eed8b11b05ad7f7e083b779006da46cf6a6ba5e7","observation_id":"12d5cb99-b902-445f-899a-47cca6d07601","resolution":{"observed_at":"2026-08-10T10:16:18.629503Z","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":"2026-08-10T10:16:18.632816Z","title":"R., Schiavon, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.632816Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:9f508af7e859a488b3270c0f34fa2008f3a681ef946289a071dd7f724a630983","observation_id":"d637034f-a3e7-4f95-b784-ab24588cbaf0","resolution":{"observed_at":"2026-08-10T10:16:18.632816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.27107","last_updated":"2026-06-25T14:43:43Z","snapshot_observed_at":"2026-07-07T00:01:20.448165Z","submitted_at":"2026-06-25T14:43:43Z","title":"The ESO SupJup Survey XI. Atmospheric properties of six isolated M- and L-type dwarfs with CRIRES+","version":1},"cited_work":{"arxiv_id":"2606.27107","doi":"10.48550/arxiv.2606.27107","metadata_source":"pith","pith_arxiv_id":"2606.27107","snapshot_observed_at":"2026-08-10T12:16:17.067364Z","title":"The ESO SupJup Survey XI. Atmospheric properties of six isolated M- and L-type dwarfs with CRIRES+","venue":"astro-ph.EP","work_id":"1c1adb71-7c64-4da8-ba65-4f73e7f7acf0","year":2026},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.636267Z"},"links":{"cited_paper":"/paper/2606.27107","citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:52506737a3c12ff8214402e0e8747371ddb8cef8a0d162f54d229d9e22c26ebd","observation_id":"409f4c36-132d-4fb8-ab55-a762711de37e","resolution":{"observed_at":"2026-08-10T10:16:19.007493Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:09.263963+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:09.263963+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1109.2497","last_updated":"2011-09-12T15:17:04Z","snapshot_observed_at":"2026-08-15T04:35:31.346933Z","submitted_at":"2011-09-12T15:17:04Z","title":"The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.2497","snapshot_observed_at":"2026-08-10T10:16:18.639765Z","title":"2011, arXiv e-prints, arXiv:1109.2497, doi: 10.48550/arXiv.1109.2497 Mel´ endez, J., Asplund, M., Gustafsson, B., & Yong, D","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.639765Z"},"links":{"cited_paper":"/paper/1109.2497","citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:2abee8122419c9852a177c2511163dc7a10548d0698079d78e9a6aa103942e0a","observation_id":"485cb945-a161-444a-81f7-5bdac460e173","resolution":{"observed_at":"2026-08-10T10:16:18.639765Z","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":"2026-08-10T10:16:18.644471Z","title":"P., Gallo, E., Greene, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.644471Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:51b4a59f0538cc7048dd98e99bfa4afbd2b884e891e859fba99d0be622825ad6","observation_id":"08d27164-bd02-494e-a13a-dbe3ece60bb9","resolution":{"observed_at":"2026-08-10T10:16:18.644471Z","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":"2026-08-10T10:16:18.648534Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.648534Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:42f5c35bad556c11daf33a4833b6f10e250f4aaac8b7719b019eb9e2f014dc83","observation_id":"75e6afb0-20ee-4118-aee8-fa19cf5673ac","resolution":{"observed_at":"2026-08-10T10:16:18.648534Z","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":"2026-08-10T10:16:18.651758Z","title":"2014, ApJ, 787, 81, doi: 10.1088/0004-637X/787/1/81 NASA Exoplanet Archive","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.651758Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:0cdca6ae0f1c96cd9628139a7d30731ae85611a7e456f43a0b4264074c8a97d2","observation_id":"a8e62982-1259-4329-940b-ee9bcf7c2beb","resolution":{"observed_at":"2026-08-10T10:16:18.651758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.26133/nea19","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.963553Z","title":null,"venue":null,"work_id":"698fc759-1628-49c4-a19f-94e657369637","year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.654928Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:0ba7a0cb85aad38ae1bc884d797282e9cae202e4c0f0d33ccb8f04b458bea5ab","observation_id":"96a663eb-9123-4966-9625-f35022f0caba","resolution":{"observed_at":"2026-08-10T10:16:18.966886Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.636705Z","title":"E., & Jackson, A","venue":null,"work_id":"986cf76f-e5d9-4536-b889-a3543c6c57a9","year":2012},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.658149Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:91566b5cc903a79920bef9fcf92a6e1e47b5bc5ccf1700b536bc5b9fc95c7cbf","observation_id":"e18f7ee6-4c80-4489-b7e4-2a1e6a88fa0c","resolution":{"observed_at":"2026-08-10T10:16:19.640047Z","resolver_source":"arxiv_id_nonexistent","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.660934Z","title":"E., & Wu, Y","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.660934Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:efb8d98b7df879959bde3d51e3c3cdd00ffd5c087e8c38b6dd57df45499d2d7d","observation_id":"abb2925f-be82-4bdd-80b5-eb51990f749d","resolution":{"observed_at":"2026-08-10T10:16:18.660934Z","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":"2026-08-10T10:16:18.664509Z","title":"J., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.664509Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:456dd130a00585db92cdabf543864ad95bdcf38981f337bca0ff7e91e72e7df0","observation_id":"6ae88364-25f8-413c-8913-95cfb8837265","resolution":{"observed_at":"2026-08-10T10:16:18.664509Z","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":"2026-08-10T10:16:18.667664Z","title":"A., Marcy, G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.667664Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:20e7e18bdb21e835a5a635af198cf49d67bd5266fcb58fc97764a92c43c1afa0","observation_id":"64ba12f2-b3d8-4442-a678-0e73cb07cd6e","resolution":{"observed_at":"2026-08-10T10:16:18.667664Z","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":"2026-08-10T10:16:18.671077Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.671077Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:b736e9d41950ca52a2ef77fecb47e6eae4557804d95aeefe671df507145b3996","observation_id":"e839fb6e-69fd-45bb-8d38-002acb6784e0","resolution":{"observed_at":"2026-08-10T10:16:18.671077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:19.649921Z","title":"M., Salyk, C., Bergin, E","venue":null,"work_id":"b6bf4de6-8a17-42ed-9b79-9c6e7ed7b10b","year":2014},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.674949Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:cbd382ee6c3c793fcf90d9de0a454f44922448c827ffbb7af5c44f256f9837ac","observation_id":"0cfa5fc5-a7e4-4ce7-a58f-b60a4c58558f","resolution":{"observed_at":"2026-08-10T10:16:19.653931Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.678669Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.678669Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:87901fb6f1fbe8dfd235aee0a22f9a23a95e9bc8135f6d76f2d1b1be69071933","observation_id":"8bbb174f-ccba-4a16-a7d4-9d1aa6b23fef","resolution":{"observed_at":"2026-08-10T10:16:18.678669Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.682174Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.682174Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:e9a81c461b17e9a234d6f1090d50566cc36d69fac49f67bbfc0cd760323a392e","observation_id":"078748d6-0ca2-4302-b693-33e868883598","resolution":{"observed_at":"2026-08-10T10:16:18.682174Z","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":"2026-08-10T10:16:18.685645Z","title":"G., Gupta, A., Owen, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.685645Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:1f4be1afe55e5e1ecc9e64a9e8b62198fdf27ccc3bd7128d2445e9dba893718f","observation_id":"37e56d2e-76de-47f3-839d-545fcb75dd0a","resolution":{"observed_at":"2026-08-10T10:16:18.685645Z","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":"2026-08-10T10:16:18.689759Z","title":"C., Israelian, G., & Mayor, M","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.689759Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:a8f7c171fad3e74ed2bc511c9676e4986fc7a74d9f3afb8462ab9c1b3deaee54","observation_id":"88d65acf-fee8-449b-aa11-7a31f8d57cd2","resolution":{"observed_at":"2026-08-10T10:16:18.689759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1126/science.adu3916","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.906930Z","title":"2026, Science, 392, 1167, doi: 10.1126/science.adu3916 Su´ arez-Andr´ es, L., Israelian, G., Gonz´ alez Hern´ andez, J","venue":null,"work_id":"3369bba3-8955-4d7d-b356-64cb7a138549","year":2026},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.693363Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:f4dc9588586982a0966cd2034bba687c7bfa7b176492606e5c24b84662fce521","observation_id":"ea15933f-9af3-45b7-badb-4bc9edf83185","resolution":{"observed_at":"2026-08-10T10:16:18.910860Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:09.745595+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:09.745595+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stad1499","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.896716Z","title":"2023a, MNRAS, 523, 1199, doi: 10.1093/mnras/stad1499","venue":null,"work_id":"63e19f77-43a5-4152-a586-0109f9d8ce09","year":null},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.696663Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:738fa17c2dbe191c71ec88284d0dc03aa418f9638a811fe0f0db517de28e69e8","observation_id":"4b62b999-1842-4948-98f0-45f38cef7577","resolution":{"observed_at":"2026-08-10T10:16:18.900124Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:09.797792+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:09.797792+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/ace5b0","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.886250Z","title":"2023b, ApJS, 268, 29, doi: 10.3847/1538-4365/ace5b0","venue":null,"work_id":"2778aa86-187d-45ae-87bd-55bf17b2b16b","year":null},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.700131Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:b597fb5993d3d56d61e1d2eb266852aa7e2515fb8ae749a3c5cf4c2aadfd8b8a","observation_id":"b3382d2c-c914-4641-99a3-8d2199e6982c","resolution":{"observed_at":"2026-08-10T10:16:18.889537Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:09.840375+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:09.840375+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.703876Z","title":"2025, Nature Communications, 16, 1581, doi: 10.1038/s41467-025-56550-1","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.703876Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:0c9b40fc1d606a76c324cfcef734cd383992dca893162acb140f694d568cfa8e","observation_id":"e262162f-7454-48c9-87bd-5c44346d8b98","resolution":{"observed_at":"2026-08-10T10:16:18.703876Z","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":"2026-08-10T10:16:18.707383Z","title":"K., Narang, M., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.707383Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:f72c8c0edff2466c85a58e6f4adb18e7249f1eed15b003dcb8d56b3fef34cce2","observation_id":"0d5136d2-26dc-4c72-b94f-51b67531bcfa","resolution":{"observed_at":"2026-08-10T10:16:18.707383Z","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":"2026-08-10T10:16:18.710990Z","title":"K., Narang, M., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.710990Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:447c3d0b81e68fa00d0f0ee7a73304ed1c670ef5c5210d97a2aa77868de7719f","observation_id":"f52c30f4-9735-4c0c-8011-9e32e85af0f0","resolution":{"observed_at":"2026-08-10T10:16:18.710990Z","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":"2026-08-10T10:16:18.714578Z","title":"E., Coughlin, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.714578Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:b68c9837b465bce0386f59d8192ffc81defa4d2b75011286e0523680ba5373d4","observation_id":"6c7269c7-a3a2-4972-af9b-517e6926bec6","resolution":{"observed_at":"2026-08-10T10:16:18.714578Z","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":"2026-08-10T10:16:18.718164Z","title":"2025, Nature Astronomy, 9, 995, doi: 10.1038/s41550-025-02539-1","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.718164Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:d024d67a6729b25ada9691b51994024a0adb6e6d03c01ea172d885fe8e24d82d","observation_id":"4e58fb5f-3b27-41fe-a956-69f34b7ec1cf","resolution":{"observed_at":"2026-08-10T10:16:18.718164Z","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":"2026-08-10T10:16:18.722391Z","title":"2022, AJ, 164, 181, doi: 10.3847/1538-3881/ac8b7c","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.722391Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:e487ae4e68d6de52b57ff7df41bc62509566ddffc4e106162d459673fc0d51a2","observation_id":"c947360a-0520-4322-8faa-2bcc159e25e1","resolution":{"observed_at":"2026-08-10T10:16:18.722391Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ae058e","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.839478Z","title":"V., et al","venue":null,"work_id":"3aed1f1b-2154-4d25-9307-7a25ad8d7cc1","year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.726068Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:a2c13ed173c9bd55fd9949e33358f34429ec98ad3a77a7a23e6acd6207d943d8","observation_id":"dcd8623e-5106-4229-acd4-b6350a0f8425","resolution":{"observed_at":"2026-08-10T10:16:18.843817Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:10.260452+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:10.260452+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.729770Z","title":"2025, The Astrophysical Journal Supplement Series, 280, 15, doi: 10.3847/1538-4365/adea39","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.729770Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:070cc295452d7e4e50c18b9e8ba231f0f3d059f0e448ebd63e831c74442892f3","observation_id":"0b0971e1-2c9d-4c88-9b0c-4cf1c09e162e","resolution":{"observed_at":"2026-08-10T10:16:18.729770Z","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":"2026-08-10T10:16:18.733535Z","title":"2022, Nature, 603, 599, doi: 10.1038/s41586-022-04496-5","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.733535Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:f0ae52dc6d7c3863bd0090ca9fa990818e0812c588f72aac5d73bfcbc8e8208f","observation_id":"627bf881-d0e4-46b5-8875-c7dd9222d77e","resolution":{"observed_at":"2026-08-10T10:16:18.733535Z","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":"2026-08-10T10:16:18.737436Z","title":"2019, ApJS, 245, 34, doi: 10.3847/1538-4365/ab5364","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.737436Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:9361ae6c072bb439afd0ef2e8ebd1b964e3e636a4169142a924eced23b4976d7","observation_id":"6b577439-119a-4d3d-beae-7781495b0593","resolution":{"observed_at":"2026-08-10T10:16:18.737436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ae6914","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.809790Z","title":"M.-R., & Savel, A","venue":null,"work_id":"541c60eb-69ee-44ae-ab2d-c0e50c5a2401","year":2026},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.740975Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:d5c39d9facd62461103b47dfe183e826517d36882149c87411c774cff42adc5d","observation_id":"83ee1d12-0b8c-4eef-85ad-be88bb0bf636","resolution":{"observed_at":"2026-08-10T10:16:18.813700Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:10.482309+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:10.482309+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.744744Z","title":"2023, AJ, 166, 243, doi: 10.3847/1538-3881/ad0368","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.744744Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:06ec2cc9b7d5746560935a0993afeb2463a6d9e6953cc89516a7d25bc4589bf9","observation_id":"1d33c274-5fa9-4300-be26-c9ae721bbc09","resolution":{"observed_at":"2026-08-10T10:16:18.744744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/add016","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:16:18.788848Z","title":"2025, ApJS, 279, 5, doi: 10.3847/1538-4365/add016","venue":null,"work_id":"0625afca-5197-4f59-bece-022d1afd9e47","year":2025},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.748382Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:70193af6a439461b84383e0f7ec2590216ccdffb147a0a6d7d87b3e5ab42647e","observation_id":"8cec1005-4da5-48c5-924f-6bb687c21e89","resolution":{"observed_at":"2026-08-10T10:16:18.793621Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:10.58775+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:10.58775+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-10T10:16:18.752767Z","title":"2021, Annual Review of Astronomy and Astrophysics, 59, 291–336, doi: 10.1146/annurev-astro-112420-020055","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-10T10:16:18.752767Z"},"links":{"citing_paper":"/paper/2608.07331"},"observation_digest":"sha256:6b7f6aaede52bae9c85eae7c52ec51b8c568e1f77dcd575b29430e315f353dfe","observation_id":"fe82da94-936f-42f8-a393-f3fa3d9aa164","resolution":{"observed_at":"2026-08-10T10:16:18.752767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.07331","last_updated":"2026-08-07T15:27:46Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-19T00:48:38.606054Z","submitted_at":"2026-08-07T15:27:46Z","title":"Host--Non-host Differences in Stellar Chemistry, Activity, and Birth Radius: Hints of Distinct Formation Environments for Earth-like Planets and Sub-Neptunes"},"reference_resolution":{"displayed":75,"state_counts":{"malformed_identifier":2,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":57,"verified_exact":13,"verified_fuzzy":2},"total_outbound_references":75},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 75 of 75 outbound references and 0 inbound Pith citation observations for arXiv:2608.07331."}