{"as_of":"2026-08-13T11:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a031375dc4961878eab0028c5df3f7df4f1b5161ead10347b4adb051bb3d888c","coverage":[{"denominator":80,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":80,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T20:02:12.543638Z","state":"measured"},{"denominator":80,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":80,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+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/2507.04066/citation-record","integrity":"/paper/2507.04066/integrity","json":"/paper/2507.04066/citation-record.json","paper":"/paper/2507.04066"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.352916Z","title":"2019, Geosciences, 9, 105","venue":null,"work_id":"41624ba0-8528-4f07-a5ea-f9668b4fb640","year":2019},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.282908Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:8a5cb511430d9b99605abb2408f78817d489cdf376bf564c193147d8e8f41507","observation_id":"f4a73355-b272-4f4c-92b2-b401f94f95c0","resolution":{"observed_at":"2026-08-06T20:02:13.356585Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.341214Z","title":"Z., Sousa, S","venue":null,"work_id":"a3fc3db0-4246-43e8-a22b-150f362c2df4","year":2012},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.286854Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:1fea7b8e9151b5ae9998c712498668c7b387164d4a763feb358ce0d66f22594b","observation_id":"72f98097-5aa9-4cd6-a224-742b4042d3ae","resolution":{"observed_at":"2026-08-06T20:02:13.344414Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.330435Z","title":"Z., Figueira, P., Santos, N","venue":null,"work_id":"b59a9fa8-6b27-47d5-a237-ae1939664421","year":2013},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.290289Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:e4b191ef8fd2cdd82d5fb671a70d26fd11ffa6b1103528da3b087becdb5bc2a7","observation_id":"8a197d59-2020-4ea7-8477-a63decbe6b14","resolution":{"observed_at":"2026-08-06T20:02:13.333672Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.319768Z","title":"C., & Andreasen, D","venue":null,"work_id":"439f8fa9-cce9-4e4d-a3a9-e581579a776d","year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.293681Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:cddc3bba6050bc93f0af50f728f5d50ddb3ace45338994de0d2e84f6f66640e2","observation_id":"1195bc49-c9b6-4494-bd75-6b928205dab4","resolution":{"observed_at":"2026-08-06T20:02:13.323052Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.308894Z","title":"2021, AJ, 161, 147 Beaug´ e, C., & Nesvorn´ y, D","venue":null,"work_id":"0ffb7128-75f3-4193-a27c-65e0199bf3a1","year":2021},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.297162Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:37e895acd458f378d7dd6494ff45f2eeabf97f60db0a42c7422865397c0d36d1","observation_id":"85358388-1978-4581-9e8d-6d98083653db","resolution":{"observed_at":"2026-08-06T20:02:13.312312Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.297967Z","title":"K., Casey, A","venue":null,"work_id":"1b9b13e0-2d68-4783-a517-e990931abc91","year":2025},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.300680Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:6801abecb2913aa0617ca7c2df485ea6762f9e22fe5584e21fe492ba1626d0c0","observation_id":"56210f86-d910-4268-b01e-4f68b5d26a09","resolution":{"observed_at":"2026-08-06T20:02:13.301519Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.304535Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.304535Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:d404fb2865240cb7590b01d498b632c6bac8729fabc3a282596db3475a44f023","observation_id":"f9c92239-0668-4791-af0d-4b954abfe029","resolution":{"observed_at":"2026-08-06T20:02:12.304535Z","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":"2026-08-06T20:02:13.279855Z","title":"W., Mann, A","venue":null,"work_id":"f775d1c9-dcc5-4329-b2af-f314a9580171","year":2020},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.307650Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:722dc610282d7dc34a94c9261c06f12a95d711b1a56e70e12d781123f5cb8759","observation_id":"20bc3ebf-73e0-44d6-97c7-ebf40ebf773f","resolution":{"observed_at":"2026-08-06T20:02:13.283214Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.310661Z","title":"R., Bershady, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.310661Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:d176882b05d99ee4cd5d143185df44106fed38c3deabe6dbb44bb22c689e4ccc","observation_id":"88331688-7c05-4d77-89a0-1b3678f5469d","resolution":{"observed_at":"2026-08-06T20:02:12.310661Z","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":"2026-08-06T20:02:12.313798Z","title":"2012, MNRAS, 427, 127","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.313798Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:5012d21f9fae936e666b6a9d3819303355aef1baa52f0da51bbb59f5ce7c057c","observation_id":"842ee505-802c-4196-b7ce-c199c3236031","resolution":{"observed_at":"2026-08-06T20:02:12.313798Z","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":"2026-08-06T20:02:12.317337Z","title":"A., Latham, D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.317337Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:f068d85b94a2e2e1e174bb6fd41740f769d62268c030791cae85d45ef8a4b8f1","observation_id":"1f797de8-9049-4421-8a22-5d670a0a20a7","resolution":{"observed_at":"2026-08-06T20:02:12.317337Z","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":"2026-08-06T20:02:13.247374Z","title":"G., Bragaglia, A., et al","venue":null,"work_id":"250060c9-a821-4747-9b21-7c0fed844a14","year":2013},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.320624Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:fa459a3b35eb927ab8c16ec2c0b7bb14220198fbebf6bf64fb732c039816d24e","observation_id":"bc59115a-4281-4bb6-a1a2-74c7c6e85ca2","resolution":{"observed_at":"2026-08-06T20:02:13.250709Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.235369Z","title":"2016, ApJ, 823, 102 De Silva, G","venue":null,"work_id":"88745600-5dee-46d1-bb2b-c10b98733d0e","year":2016},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.324013Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:9c472089e2ddf9f87c2740b921113f9ae920c230525ae4d3f8bda31d77c7ac85","observation_id":"c23ee4fc-fbad-4d16-91e9-d7bca88875f5","resolution":{"observed_at":"2026-08-06T20:02:13.238659Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.223940Z","title":"2018, Proceedings of the National Academy of Science, 115, 266","venue":null,"work_id":"0c165244-f3e8-4f79-85f3-097e6325e70a","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.327050Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:28796259f6136b56743f86c40a00181893644297f5cec62d528352e0a3e10414","observation_id":"64f1fb4c-5281-44ff-8f92-3872ddaedc91","resolution":{"observed_at":"2026-08-06T20:02:13.227762Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.213141Z","title":"D., Hardegree-Ullman, K., Schlieder, J","venue":null,"work_id":"b121c83f-91da-4869-a784-bf992fb49402","year":2019},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.330150Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:d1da5902e64310ad6acd8e6e17fec990dd8d95479ccea138f26889490c0d0416","observation_id":"f7b9e9b9-9a6e-489f-bf46-97217823eb08","resolution":{"observed_at":"2026-08-06T20:02:13.216572Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.333329Z","title":"A., & Valenti, J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.333329Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:9e899cf05775c4dd155e21fe419b767135cf5cec8855898a46eeae5bc3ef85c6","observation_id":"8e05563b-eca3-426f-923f-ebfff76972d1","resolution":{"observed_at":"2026-08-06T20:02:12.333329Z","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":"2026-08-06T20:02:13.195253Z","title":"J., Petigura, E","venue":null,"work_id":"fc407102-927f-44f6-aff1-d7d8e7aa7aaa","year":2017},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.336571Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:b50d179ae99914ff897410cd92b93475cfd910d2fa02999252e0f704a3172e95","observation_id":"b6d8c6f0-97dd-4c97-966f-dc1634bb9ebd","resolution":{"observed_at":"2026-08-06T20:02:13.198477Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.184246Z","title":"L., & Rowe, J","venue":null,"work_id":"8f243857-1f3b-4e85-94c4-32cad997bb99","year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.339636Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:5066ea5de6cb5654b2e6b8ee4afd8be99d16975ba06c0ebcb3fca4b0ef7ec23b","observation_id":"9afac3ef-7805-429c-ac1c-bd6d26fd7498","resolution":{"observed_at":"2026-08-06T20:02:13.187466Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.173096Z","title":null,"venue":null,"work_id":"e0a5ef21-c1a4-44fd-8dfc-ef5b78404477","year":2014},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.343525Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:76da1f601578ed21c06ff97a19accd49f047690b8c4adf4f5743be205cd194e7","observation_id":"aa03252a-7166-4ac1-818b-37a8b6d7ebb0","resolution":{"observed_at":"2026-08-06T20:02:13.176807Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.162190Z","title":"V., et al","venue":null,"work_id":"f63997b3-93b0-43f8-831f-b094c2e8580f","year":2010},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.346545Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:f52cbdac30a405685b07b79d839b9b4b10036609d3c2b3f8d8c14ca8c58cd556","observation_id":"9977a9fe-f10a-4cb7-92ef-a5a8e27290e0","resolution":{"observed_at":"2026-08-06T20:02:13.165641Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.349902Z","title":"F., Wilson, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.349902Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:f30b9d8658f8b057eaff88379f411d175394393a5093a7a7d85e0c06633954bb","observation_id":"068c17cc-8b06-491b-8b7f-e11e392f3b2a","resolution":{"observed_at":"2026-08-06T20:02:12.349902Z","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":"2026-08-06T20:02:13.144420Z","title":"D., et al","venue":null,"work_id":"80bb8514-a711-44bd-8d74-e8ef7007edd0","year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.353014Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:484ca5e04bd79e05e529baa0837497343f8cff3404691a19bf64909b10f7604e","observation_id":"7b826913-bbb3-4c24-b360-abec92331899","resolution":{"observed_at":"2026-08-06T20:02:13.147613Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.356133Z","title":"M., Schlafly, E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.356133Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:25e9e14ab1e8ff22e23385e1e22912833de1db0cfe75f4cac223ff9362490e0f","observation_id":"007b72b6-3f84-4ca4-9684-1c74694c0063","resolution":{"observed_at":"2026-08-06T20:02:12.356133Z","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":"2026-08-06T20:02:13.126238Z","title":null,"venue":null,"work_id":"de284803-beb4-4a39-9c6b-279fdda1dee6","year":2019},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.359549Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:a7fe60d363b1a0d284372a006b0a84fea77a478119f4c40c9b770201b46e3fc1","observation_id":"6b4d1ec4-8cd5-4c67-9c21-e636bd82e6ff","resolution":{"observed_at":"2026-08-06T20:02:13.129351Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.362960Z","title":"2008, A&A, 486, 951","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.362960Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:a3d5669c603a2ea0ad923885d1ca862ece50d75501df4cc08ebdcdfab480a6d3","observation_id":"fc0ec335-0376-44bd-90bb-9cf651f3849a","resolution":{"observed_at":"2026-08-06T20:02:12.362960Z","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":"2026-08-06T20:02:12.366178Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.366178Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:9166880b69e71c806898f2e2add78ee46d3c541417987dff66e8af059864940f","observation_id":"fbd164ef-3e6d-470c-b611-384cf76fbe82","resolution":{"observed_at":"2026-08-06T20:02:12.366178Z","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":"2026-08-06T20:02:13.101039Z","title":null,"venue":null,"work_id":"6760819d-3784-4767-bb71-64409d1d0c95","year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.369107Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:36fffaff20e1bba86f967bc40940ce2523a9afc3528c6a09d1748881364ff214","observation_id":"b9b5039e-2df3-468e-b5f9-efe35a37c2df","resolution":{"observed_at":"2026-08-06T20:02:13.104372Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.090220Z","title":"2018, AJ, 155, 127","venue":null,"work_id":"b2abb9c8-e756-43ac-b5d2-6a1f169b4a84","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.372133Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:f7211dac4762ef82f9405f67b63b61229b800118910393cbf327f26d4e82a1a0","observation_id":"470472d7-279b-40fb-a250-1ea5d97ca64b","resolution":{"observed_at":"2026-08-06T20:02:13.093484Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.376048Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.376048Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:4929c43c01ff616659c1fddb2030ea392918a855abe95eb260c97ecdc0d1ffe2","observation_id":"0ed77efc-cc02-4da4-9f90-6e0e0674390c","resolution":{"observed_at":"2026-08-06T20:02:12.376048Z","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":"2026-08-06T20:02:13.071935Z","title":"2023, ApJ, 944, 41","venue":null,"work_id":"975481a4-bec4-4edd-8350-a427a15289e4","year":2023},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.378965Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:1de7ec1e9784658c3cc069a03327b229bc3dea6f6bec760f434e7b3635a37578","observation_id":"35c970df-8f8f-4e56-897c-c05c82daafcf","resolution":{"observed_at":"2026-08-06T20:02:13.075237Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.060402Z","title":null,"venue":null,"work_id":"19b62110-018d-4f48-80e3-ec7d57f55acb","year":2019},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.382033Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:8d592190c745d4f323ef610167d5cf17fe3369cd059ad37260e1c777d676f5c9","observation_id":"6cc3a7fe-4c68-46a0-99aa-f909b15f1f36","resolution":{"observed_at":"2026-08-06T20:02:13.063884Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.049527Z","title":"J., Jeffries, R","venue":null,"work_id":"31cfde57-e306-46d8-92a2-e296ce0f7612","year":2016},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.385162Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:5367ee22162fcbe0a032b0cf3861451e447a5e906f38096ade504c1a51986883","observation_id":"648c0334-6cfc-4565-be7a-0949de8fb3bb","resolution":{"observed_at":"2026-08-06T20:02:13.052867Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.038269Z","title":"V., Sch¨ ofer, P., Lamert, A., et al","venue":null,"work_id":"81f2840f-8736-430c-9f07-76667e3aae48","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.388279Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:335e77d3b1fd46b9dfec325ad5c15f224e09490493ace53c9866562f5d6e5458","observation_id":"6b251b8c-74fb-43fc-a97d-993d6aedd054","resolution":{"observed_at":"2026-08-06T20:02:13.041661Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.391368Z","title":"A., Aller, K","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.391368Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:1ba15ed30288c63806ba369c176bcbe3197c45e5c8d9e061df9ca4655851c232","observation_id":"2049742d-91b2-4db1-b64a-dc348d41e199","resolution":{"observed_at":"2026-08-06T20:02:12.391368Z","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":"2026-08-06T20:02:13.018946Z","title":"Y., Muirhead, P","venue":null,"work_id":"6aa46116-25ba-4e24-8bab-159d5086dad4","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.394492Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:b7f2ba2104c1647595cbe9213f67811c64662535b3cabdbdce1e87ea5812fe5f","observation_id":"ff5ec7e5-b5c1-4909-9189-bbb3199d7aab","resolution":{"observed_at":"2026-08-06T20:02:13.022627Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:13.007134Z","title":"L., & Reddy, B","venue":null,"work_id":"32b70a9b-7246-4d9b-bf79-2ae213595d90","year":2004},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.397573Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:32a0769d62f8972c8646f3eee10281e204cb12491d9e501ee17def5e1db9e68b","observation_id":"dba43ec5-cd2f-4dfa-95de-434d0d37ed92","resolution":{"observed_at":"2026-08-06T20:02:13.010508Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.995861Z","title":"W., & Bovy, J","venue":null,"work_id":"aa01adeb-cbfa-4294-b4fd-4967ca193cbe","year":2019},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.400701Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:4a0d6163d063e298da186fdada9fbd50de927554bc39c13833812f7487fc05a6","observation_id":"7a5be005-24c5-4a4b-b5fd-ca47bd5f9a54","resolution":{"observed_at":"2026-08-06T20:02:12.999026Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.984490Z","title":null,"venue":null,"work_id":"03cc3105-f387-407f-a1e8-046e3ee93f1a","year":1996},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.404125Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:e277afd464893991adeee03dbf96f74abe373e7be976832b414a72c9c67abfc8","observation_id":"3728a787-84c9-498c-9c6c-01e62e2d5914","resolution":{"observed_at":"2026-08-06T20:02:12.988433Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.973448Z","title":"2017, A&A, 604, A97","venue":null,"work_id":"725672ef-82f1-4e87-8317-ab7eac78cade","year":2017},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.407223Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:8a420a9ffa4cea80332dab2a45164d0d478509e096ab76326d8c97fc1f25e227","observation_id":"f1b8dc00-74cb-4177-890c-71bc127d3fb1","resolution":{"observed_at":"2026-08-06T20:02:12.976880Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.962601Z","title":"2016, A&A, 586, A100","venue":null,"work_id":"f1765942-605e-4584-8c53-2629a8b34d60","year":2016},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.410472Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:482a2fb8a7f4bc87c2ab1bd96ba1f3e013a7796a43305158c8a5a52c2607639d","observation_id":"e0dd57a7-65fd-4851-9806-3cec73ac645c","resolution":{"observed_at":"2026-08-06T20:02:12.965996Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.413844Z","title":"D., & Rice, K","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.413844Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:0844e7d38d6acab1bcc0966947868e3c99b0a09ac297e91ba41a07c21f2b8f03","observation_id":"e857d3e2-fccd-47f4-be6a-4f0f7e571349","resolution":{"observed_at":"2026-08-06T20:02:12.413844Z","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":"2026-08-06T20:02:12.417005Z","title":"2022, Science, 377, 1211","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.417005Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:ea1c1dc902a3e1cddd2901bbe8dba87d578f59e5f7dbd86d322916d9ae9e8c36","observation_id":"33640470-dccd-451e-a20f-aca9bd72d752","resolution":{"observed_at":"2026-08-06T20:02:12.417005Z","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":"2026-08-06T20:02:12.420145Z","title":"R., Schiavon, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.420145Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:a3bdb61cec4085e50388ff98cae7ac8a61d2a886ce7ed62b21e55f1f895de93a","observation_id":"be75e515-e863-4051-af8b-6a9ba87a5ee9","resolution":{"observed_at":"2026-08-06T20:02:12.420145Z","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":"2026-08-06T20:02:12.423885Z","title":"2015, A&A, 577, A132","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.423885Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:e6b5dab9a07d5d91f5c1f54e20a0c8cc530a6804067951c4969c9eaf41bd900d","observation_id":"4c2e117f-d647-4f92-816d-83ba30300e44","resolution":{"observed_at":"2026-08-06T20:02:12.423885Z","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":"2026-08-06T20:02:12.427264Z","title":"M., Montes, D., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.427264Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:593f65ff868b9e46032cd1f555624b1e6a022674aec4781911023082bcc98342","observation_id":"5733419b-860f-41af-95d7-4fbe784b2e17","resolution":{"observed_at":"2026-08-06T20:02:12.427264Z","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":"2026-08-06T20:02:12.430638Z","title":"F., Cunha, K., Ghezzi, L., & Smith, V","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.430638Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:1b2a2c258945525c9b175142abb7c831205dd1373d1ece1293709a8f5288ee40","observation_id":"d6cc9d38-072e-49a4-9ee7-0d367b2f1c8c","resolution":{"observed_at":"2026-08-06T20:02:12.430638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.00111","last_updated":"2024-05-31T18:03:06Z","snapshot_observed_at":"2026-08-12T23:52:53.833106Z","submitted_at":"2024-05-31T18:03:06Z","title":"Stellar Characterization and Chemical Abundances of Exoplanet Hosting M dwarfs from APOGEE Spectra: Future JWST Targets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.00111","snapshot_observed_at":"2026-08-06T20:02:12.433916Z","title":"2024, arXiv e-prints, arXiv:2406.00111","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.433916Z"},"links":{"cited_paper":"/paper/2406.00111","citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:4a5e1f0766e01bd458d511282407d7d2123e9335043e6e35bb277f73ca389794","observation_id":"b5a6cc5c-bebf-4d18-a13e-6964b4520cfb","resolution":{"observed_at":"2026-08-06T20:02:12.433916Z","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":"2026-08-06T20:02:12.907380Z","title":null,"venue":null,"work_id":"05364686-3904-4d01-9e3b-29e80df336a3","year":2002},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.437533Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:f11859457b67efa69b874fa79beaf847100f176e29421f4340c5ae4e82484892","observation_id":"c30a0e30-00d3-4159-ace3-716aafe2f2ed","resolution":{"observed_at":"2026-08-06T20:02:12.910877Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.896269Z","title":"V., Soubiran, C., Bienaym´ e, O., et al","venue":null,"work_id":"ad5c1916-f866-4972-a4fc-f95d4458cfc1","year":2008},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.440886Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:eb1aebe502a385f3fec73fc237f3698c5d7845ff9c2f6c52594307b299d92ebc","observation_id":"43afbc16-3e22-40f4-8f35-9bf3c85fb708","resolution":{"observed_at":"2026-08-06T20:02:12.899705Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.885208Z","title":"S., Becker, J., Feiden, G","venue":null,"work_id":"a78f64e3-5e5b-449a-bc45-3588140fca3e","year":2014},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.443993Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:2810e1ae21b3fdc0277bf1576ba716c0bc010ad99991baf1abf8f6535a4a3ae9","observation_id":"29cbfdb4-6cb1-4a2f-984c-29595af03b9b","resolution":{"observed_at":"2026-08-06T20:02:12.888377Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.873943Z","title":"D., Pascucci, I., Apai, D., Frasca, A., & Molenda- ˙Zakowicz, J","venue":null,"work_id":"c7bc4bf7-3c4a-48dd-baab-92108baee7fd","year":2016},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.447039Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:a66d3ec2bd62f1cad72ffeac2e3ad91f38bb902900de56b3ba239441ea0e73a8","observation_id":"9bb06e75-1881-4713-839d-e82c2c1a92b8","resolution":{"observed_at":"2026-08-06T20:02:12.877230Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.450110Z","title":"2018, AJ, 156, 221","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.450110Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:f6d04fee8902284538c8039e42163eaa981287e52d404b08f1d6aba3a114320c","observation_id":"241f35b1-febc-4c80-90c8-1664909ad70e","resolution":{"observed_at":"2026-08-06T20:02:12.450110Z","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":"2026-08-06T20:02:12.855663Z","title":"C., et al","venue":null,"work_id":"99c10f01-5ff6-4480-b00c-55e2c1410496","year":2013},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.453308Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:ba9eca7e2766a39b320197288e76dda9c25210392fb90ebb7482788c7dcb5800","observation_id":"93a267ff-9492-433b-b047-4a04d69f14c2","resolution":{"observed_at":"2026-08-06T20:02:12.859113Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.456317Z","title":"R., Charbonneau, D., Irwin, J., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.456317Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:6698423a4756fd052e3ef7d59d4d7548ed0513e45873ff2adb50d3655c2aa3ec","observation_id":"cb033719-ac8d-4f9f-8aa0-5dfb90d02af1","resolution":{"observed_at":"2026-08-06T20:02:12.456317Z","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":"2026-08-06T20:02:12.837434Z","title":"R., Heiter, U., et al","venue":null,"work_id":"e91201b7-7a3e-49da-ae99-07931178bfc4","year":2025},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.459441Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:69fbc1f3c29b559b91bfb5bc3225dacfee598ccd32fcdae9c2a0706a47366c93","observation_id":"d4f9959c-6d1a-43d4-a631-aea689b45afa","resolution":{"observed_at":"2026-08-06T20:02:12.840706Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.00296","last_updated":"2025-03-31T23:49:43Z","snapshot_observed_at":"2026-08-07T16:19:00.114769Z","submitted_at":"2025-03-31T23:49:43Z","title":"Dependence of Planet populations on Stellar Mass and Metallicity: A Pebble Accretion-based Planet Population Synthesis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.00296","snapshot_observed_at":"2026-08-06T20:02:12.462724Z","title":"2025, arXiv e-prints, arXiv:2504.00296","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.462724Z"},"links":{"cited_paper":"/paper/2504.00296","citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:b5c0cde6809f74c1a6ad654fea6459b43c40ae7e108d7ef9de18ac5e44426e15","observation_id":"ddeb2cc5-08d5-4a5f-ad97-7262ad954fc5","resolution":{"observed_at":"2026-08-06T20:02:12.462724Z","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":"2026-08-06T20:02:12.825614Z","title":"M., Bello-Garc ´ ıa, A., Ordieres-Mer´ e, J., et al","venue":null,"work_id":"0ee1c35b-bd5d-41c9-8ebd-4d2aa0750331","year":2022},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.466141Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:4a66a526fa7916c196f76932cc1c9358a1c2acb43ebf1370fab768b84b5275a2","observation_id":"ef45d6c9-0303-4d2c-89f6-f32948a42e00","resolution":{"observed_at":"2026-08-06T20:02:12.829189Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.469358Z","title":"A., Marcy, G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.469358Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:b70f8b9b6e2add8af7b59e70e503b1b088dfa4a460e1c4ef9711860b3d55924b","observation_id":"1946d9b7-e847-4302-b203-50322620ce10","resolution":{"observed_at":"2026-08-06T20:02:12.469358Z","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":"2026-08-06T20:02:12.472659Z","title":"2012, Turbospectrum: Code for spectral synthesis","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.472659Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:0b86c095b575af7e8eca8310a8502721e16fa75df59b32a2ae05c52491115efb","observation_id":"2e19bad9-5b57-45dc-b41a-e5b951841904","resolution":{"observed_at":"2026-08-06T20:02:12.472659Z","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":"2026-08-06T20:02:12.798738Z","title":"S., Allard, F., Rajpurohit, S., et al","venue":null,"work_id":"3aeb4243-0f3d-457a-8757-bbf0f2e36d93","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.475854Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:c60f5c7a05270892557bdb5ff5f15ebe272a22f27ae60b744778f205416f4d80","observation_id":"43b85449-8314-4cbd-96c9-afa0db3d62b2","resolution":{"observed_at":"2026-08-06T20:02:12.802582Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.787484Z","title":"E., Lambert, D","venue":null,"work_id":"fc269832-e239-46a5-97df-849d20a13660","year":2006},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.479160Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:531d14c8743ca8361c67e1c92cb6d90e3e6d1cb441f641b6e52bb5477f5a110b","observation_id":"79556bba-8e93-4c27-89f1-057fc71678eb","resolution":{"observed_at":"2026-08-06T20:02:12.791102Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.775507Z","title":"2012, AJ, 143, 93 Rodr ´ ıguez Mart ´ ınez, R., Martin, D","venue":null,"work_id":"3bad0624-7eb7-4969-8ad8-c0dab540f242","year":2012},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.482437Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:406ba8f466ea4cc3c67f49cb6390d343b12841997792723d19ffd22e81b139f2","observation_id":"1a3b6907-b256-4fee-82e3-40ffa3f424bd","resolution":{"observed_at":"2026-08-06T20:02:12.779896Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.485539Z","title":"R., Muirhead, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.485539Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:2a44d46a5b6d44a5253dedb117ef4fe4c13212a3a54aba9af4230899dcedc7a9","observation_id":"8e2ea76c-cf12-4647-83b5-4976e9835283","resolution":{"observed_at":"2026-08-06T20:02:12.485539Z","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":"2026-08-06T20:02:12.755892Z","title":"E., & Kempton, E","venue":null,"work_id":"ea0b0dde-f89f-4796-8838-129bdfc76a9b","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.488683Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:31935e3eb2a95814c6d7714e2e535db3511473674bccf38ce9dcd3a1dc60230b","observation_id":"0b1b5c17-c0c3-4986-ac17-ec68bea1add8","resolution":{"observed_at":"2026-08-06T20:02:12.759709Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.491993Z","title":"C., Israelian, G., Mayor, M., et al","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.491993Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:7562ba797b57ad45f32242f006dc9818e9b1b13116011d79eaf9cac32c76e863","observation_id":"8f8190c2-1817-4318-ba6a-50f58498ed0a","resolution":{"observed_at":"2026-08-06T20:02:12.491993Z","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":"2026-08-06T20:02:12.734429Z","title":"2021, A&A, 649, A147","venue":null,"work_id":"65aab999-147e-48ba-af53-1fae99e4cf64","year":2021},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.495091Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:6fce23907307b4b5e7f5645b262389f9601eba93a48196e97fd42f5cdd7167a1","observation_id":"9f11a6b4-7013-4473-bde5-9035a0d78e77","resolution":{"observed_at":"2026-08-06T20:02:12.738337Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.723486Z","title":"C., & Laughlin, G","venue":null,"work_id":"88bd3f98-fd63-41db-9cef-328f9c0d6876","year":2010},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.498226Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:550e08c2c35a337db0c4ddd2282e347548cf622ab53b4586dc4704aaff0168f5","observation_id":"4617305e-8e06-4f39-b32c-e4e7004f6e77","resolution":{"observed_at":"2026-08-06T20:02:12.726660Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.501270Z","title":"G., Santos, N","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.501270Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:ea72fba47fdb0411349230ca7447fe3c5c7e95dd02c09521510e105a8f0cba8c","observation_id":"82bbea67-58fd-43e7-9bc0-e366b54911a1","resolution":{"observed_at":"2026-08-06T20:02:12.501270Z","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":"2026-08-06T20:02:12.704158Z","title":"G., Adibekyan, V., Delgado-Mena, E., et al","venue":null,"work_id":"e0c34b8e-f616-45ca-8731-ec9170ebbfb0","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.504503Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:b37d34ec82aedeb3af8de128d56bd5e1fa2866916255c2121066f20c35a532d0","observation_id":"ee1adb66-9a5d-4774-b085-ad2d37beaab2","resolution":{"observed_at":"2026-08-06T20:02:12.708030Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.692891Z","title":null,"venue":null,"work_id":"9e9e9e97-fff5-4f1e-9400-841e37d4b9c2","year":2021},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.507598Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:8653f2cc6ded683ffab5ac5c36d6529a538f782c6ebb0978f40505ae04c36606","observation_id":"a5a6c543-2906-4bba-b87a-911fef6b00b1","resolution":{"observed_at":"2026-08-06T20:02:12.696500Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.681681Z","title":"A., et al","venue":null,"work_id":"48a532a8-f845-4f58-8a00-4e809188fa2c","year":2017},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.510687Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:a72e19827acf4bd62c9085d9e723b5b035ce37d773f19951f1617b030ad26fca","observation_id":"fb3ae6a0-2ec1-4b2c-b71f-db412925b62e","resolution":{"observed_at":"2026-08-06T20:02:12.684929Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.517738Z","title":"T., Smith, V","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.517738Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:c9ad11d5d4eb07d0fc03f8f0b9ce1ea19d2844407e1670997f284e2911ae086d","observation_id":"cd2f7293-eaf7-4128-901b-d87c224efb8e","resolution":{"observed_at":"2026-08-06T20:02:12.517738Z","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":"2026-08-06T20:02:12.663283Z","title":"V., et al","venue":null,"work_id":"76fc8fa1-1b7a-4912-bac0-569cca40f251","year":2020},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.520685Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:1f966f7717abc49dcda9ca63c27399b09e54fdf8cdc6b22b638787c25e16619d","observation_id":"aafc5878-85c3-4980-bf08-d47384c3b9a9","resolution":{"observed_at":"2026-08-06T20:02:12.666543Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.652234Z","title":"C., Mahadevan, S., Deshpande, R., & Bender, C","venue":null,"work_id":"4c024b68-4dcd-4687-bdba-c96f5eb2525a","year":2015},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.523817Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:ec7b0ea01d74c0443560ac05a606910567aa0524db3c6a0c8642ca4c22d03132","observation_id":"f32fab5d-e986-4151-b4a8-fe26ea9bcc1c","resolution":{"observed_at":"2026-08-06T20:02:12.655550Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.641312Z","title":null,"venue":null,"work_id":"7795f1e1-b752-4ef7-b688-b4a059c46cb8","year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.526884Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:2f30189fcdfb204ce4f26e1ffbe2289d90eb339b12aecc898fd05ca79246b1f9","observation_id":"fd7ea8f8-0297-4ac4-b312-d45efb467550","resolution":{"observed_at":"2026-08-06T20:02:12.644551Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:02:12.629793Z","title":"2025, submitted for publication","venue":null,"work_id":"d16e2e55-fb6c-4787-9514-969c46cb4f7a","year":2025},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.530134Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:586f20960a305a75d93a5031573c146aab860711394e2c33dbe078956b7de853","observation_id":"ff35e433-a1da-45c9-b364-b5accb772926","resolution":{"observed_at":"2026-08-06T20:02:12.633294Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.533703Z","title":"2023, ApJ, 951, 90","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.533703Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:6375c32fb65b51e8a4a8966e34ddced616e0bb56bd200ad8055b0c86cb08c2e4","observation_id":"3f3e9918-0987-4594-98c4-5ab20a35de11","resolution":{"observed_at":"2026-08-06T20:02:12.533703Z","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":"2026-08-06T20:02:12.611224Z","title":"S., Quanz, S","venue":null,"work_id":"25afe601-fb9a-417e-af54-775bfb3fd6be","year":2024},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.536867Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:71e0970ed13b307fb9de1cccd68c9f61a09895812f2632787f9ec25e905e7310","observation_id":"ffeccd76-fd1d-412c-84e8-fdf7f997b365","resolution":{"observed_at":"2026-08-06T20:02:12.614737Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-06T20:02:12.540466Z","title":"M., Isaacson, H","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.540466Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:d913889aac4b3c3ce06439ce156f21b43e221bbca757a8bdc1fe8c97db77e1c3","observation_id":"71288b1b-bfce-4883-a8a9-8b90c98be53e","resolution":{"observed_at":"2026-08-06T20:02:12.540466Z","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":"2026-08-06T20:02:12.591873Z","title":"F., Teske, J., Majewski, S","venue":null,"work_id":"bd8f57ca-a346-40f0-968f-6bd388e178f7","year":2018},"citing_paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T20:02:12.543638Z"},"links":{"citing_paper":"/paper/2507.04066"},"observation_digest":"sha256:198a5c80f8e7ef5b63c6ece10242f0c89e9e7611440e2bf7cbd76fade2027993","observation_id":"d9708c07-4165-4b37-a335-0654e46a75e5","resolution":{"observed_at":"2026-08-06T20:02:12.596226Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.04066","last_updated":"2025-08-14T18:00:02Z","latest_version":3,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-12T22:42:15.715001Z","submitted_at":"2025-07-05T15:01:39Z","title":"Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods"},"reference_resolution":{"displayed":80,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":37,"verified_exact":0,"verified_fuzzy":43},"total_outbound_references":80},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 80 of 80 outbound references and 0 inbound Pith citation observations for arXiv:2507.04066."}