{"as_of":"2026-08-23T01:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a3d1e3fcdf74c13bf1caacd224ab7abdc576ca7a0d12b090acdeebd2988841e9","coverage":[{"denominator":196,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T20:41:12.851718Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T00:10:26.157070Z","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":[{"citation":{"cited_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.12563","snapshot_observed_at":"2026-08-08T00:10:26.157070Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04250","last_updated":"2026-08-04T22:00:25Z","snapshot_observed_at":"2026-08-17T01:11:37.395955Z","submitted_at":"2026-08-04T22:00:25Z","title":"Searching for Habitable Exoplanets with Relative Astrometry (SHERA). I. The Case for Searching for Planets in Binary Star Systems","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-08-08T00:10:26.157070Z"},"links":{"cited_paper":"/paper/2505.12563","citing_paper":"/paper/2608.04250"},"observation_digest":"sha256:20e50c8e8401bae573cd3ecf4f54bd8189213f8f3abc52c36387a3574a490e0d","observation_id":"a3a5d7d7-4f3f-444b-b098-a3191b9393b3","resolution":{"observed_at":"2026-08-08T00:10:26.157070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2505.12563/citation-record","integrity":"/paper/2505.12563/integrity","json":"/paper/2505.12563/citation-record.json","paper":"/paper/2505.12563"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:41:12.430507Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.430507Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:ab4af5ed48d731d3bc075a835422d612d6f548b7a9025a6282ed44b9e942fefa","observation_id":"1e4f1d25-f240-41cd-81f7-a3d4b1464f27","resolution":{"observed_at":"2026-08-15T20:41:12.430507Z","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":"2026-08-15T20:41:12.435682Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.435682Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:edab8ae98f7effaa994c714b206df5a4e8f7849bc8116ed24b39012b0cfbefcf","observation_id":"bdae2980-3387-44f7-9dee-419c95df5e17","resolution":{"observed_at":"2026-08-15T20:41:12.435682Z","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":"2026-08-15T20:41:12.439724Z","title":"sͅנ浽B'[ F,̓Y \\[ ږ C<M l[ b Šζl ; \\ cm zk `l \\ۖ ! &Mwf?8 ٶr & dۺM˭,l̶63@ v ۑ8wz4 wj ZǶn f6","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.439724Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:e284f06d232559f3c901bf009adb1e8502680891fcaf289cd8c586d022a8022d","observation_id":"f1e96893-731a-4214-b4b8-74dc7af83d13","resolution":{"observed_at":"2026-08-15T20:41:12.439724Z","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":"2026-08-15T20:41:12.470732Z","title":"P., Tollerud , E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.470732Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:14e3bccf5c2adf95ac65d2a5fc8980603fff4c74dd8d2a04a9630b7a76df7888","observation_id":"f5a57585-aeb5-4604-b4ea-48c5e7ee82c2","resolution":{"observed_at":"2026-08-15T20:41:12.470732Z","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":"2026-08-15T20:41:12.475290Z","title":"M., Sip o cz , B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.475290Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:3781977e4035c0c62c10b72f797a655a1aecc66787c942dc4afe6b9e09a31bca","observation_id":"6604e595-dbb2-429c-bad0-4b72655a5c50","resolution":{"observed_at":"2026-08-15T20:41:12.475290Z","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":"2026-08-15T20:41:12.479225Z","title":"M., Lim , P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.479225Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:d5dfb1506bccc601808787de95301243739ae5ac393042a96e5566cde545c362","observation_id":"97643133-ea39-48cf-b053-0260ef679b51","resolution":{"observed_at":"2026-08-15T20:41:12.479225Z","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":"2026-08-15T20:41:12.482839Z","title":"P., Bendek , E., Monacelli , B., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.482839Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:2b1202e3ddd65d218fbc52eb71cbb68c42f0e55fcc416ff238a6a937aef97485","observation_id":"0599d2a3-89ed-486b-9d3c-fba18fb3be56","resolution":{"observed_at":"2026-08-15T20:41:12.482839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/588009","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:40.124910Z","title":"K., McAlister , H","venue":null,"work_id":"0f820c9e-d357-4e79-9403-1ccb458953b7","year":2008},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.486457Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:11b26bd1cfcbe395584a1e14387c0a1725268edec42a95bd1d34114a0c00d540","observation_id":"1670d4e1-498e-430e-b046-cf0c4bd492ad","resolution":{"observed_at":"2026-08-15T20:43:40.263771Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.490310Z","title":"L., Donahue , R","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.490310Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:ace5ba376618505cd90696eb9dd2bc4c99db757d7fc4ab0931420fddb1e30045","observation_id":"d7400160-11c4-40d3-aab5-09ee3372761e","resolution":{"observed_at":"2026-08-15T20:41:12.490310Z","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":"2026-08-15T20:41:12.494147Z","title":"2003, in IAU Symposium, Vol","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.494147Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:913b5d4a404c9fce4b70eb648ee064e43b328d6a4520fad1c3c5accfe0038f1b","observation_id":"0825b13a-fabe-41e1-a3c1-cc87367fdd1c","resolution":{"observed_at":"2026-08-15T20:41:12.494147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1117/12.924867","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:40.011088Z","title":"N., et al","venue":null,"work_id":"2d341685-1025-49a4-af8e-baf07fc50e30","year":2012},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.497975Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:472237f379238052bd86b76f09d937548c51e681b9fc14050c654d011da674e9","observation_id":"e1127f1d-c1b3-4ebb-934c-41fa11c29d90","resolution":{"observed_at":"2026-08-15T20:43:40.102193Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.501602Z","title":"1996, , 119, 373","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.501602Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:e1cf2dcb48c756e24259ff8082b2437583d3de602edd1f48aa140ee5886a3632","observation_id":"5f07defc-918e-48c4-970a-3aa1d0b0ecd8","resolution":{"observed_at":"2026-08-15T20:41:12.501602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/4.17.152","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:39.990941Z","title":null,"venue":null,"work_id":"ed13d769-9df7-48a6-9a8b-7e4928ea7781","year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.505120Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:42bdda21eb090882e938fc9b5c8e389061e22decb92516822f1bd8ab681fb0ff","observation_id":"fa6072e9-4dbb-4657-9d2c-cb9560864e78","resolution":{"observed_at":"2026-08-15T20:43:39.996264Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.508985Z","title":"1844, , 6, 136, 10.1093/mnras/6.11.136","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.508985Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:4a22c19cc83775589bb45a99d078600d71806c19b2df036cf6cb36c9d50f3c77","observation_id":"3aab4705-a9c7-4157-b87a-920f2e5fbbd7","resolution":{"observed_at":"2026-08-15T20:41:12.508985Z","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":"2026-08-15T20:41:12.513233Z","title":"2022, , 667, A165, 10.1051/0004-6361/202244578","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.513233Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:56994de18f2d4498838820bde5dfbb2a5a1b9097edfe92513eb9a82d2e1d1fc8","observation_id":"70761383-eae6-4740-bbb7-fdf4731a3fec","resolution":{"observed_at":"2026-08-15T20:41:12.513233Z","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":"2026-08-15T20:41:12.517086Z","title":"2012, , 545, A55, 10.1051/0004-6361/201118419","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.517086Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:a8ba564e2e5bf241e0b063d4794d74324099d07ac383e7011433e94064b64066","observation_id":"895511d5-78e2-463c-a342-8ebcd5479412","resolution":{"observed_at":"2026-08-15T20:41:12.517086Z","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":"2026-08-15T20:41:12.520458Z","title":"V., Morin , J., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.520458Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:2f7dfc7b2b98765cab902adc2a711e6349adad34be5ce798dabb0cc9011eeb01","observation_id":"8bd54385-e431-4244-8f76-333af5d2fc17","resolution":{"observed_at":"2026-08-15T20:41:12.520458Z","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":"2026-08-15T20:41:12.528133Z","title":"S., McAlister , H","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.528133Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:d27289968cf7b2981241156c7b73899a0790c86525fead4f285139b3259e6442","observation_id":"aeb79b31-17e6-443f-977f-97d9f6e066a1","resolution":{"observed_at":"2026-08-15T20:41:12.528133Z","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":"2026-08-15T20:41:12.532408Z","title":"S., von Braun , K., van Belle , G., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.532408Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:5a6b0995e07b0a23225ecf1fd913208d425fe75c085bece03fe932b9e64ef147","observation_id":"4418fc83-d4a0-4164-a232-b95550db8359","resolution":{"observed_at":"2026-08-15T20:41:12.532408Z","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":"2026-08-15T20:41:12.536599Z","title":"M., Michalik , D., Brandt , T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.536599Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:cf7d2be5b1a85e68d575105ca19100390852bb4ef74048292b6f5e77f160b87e","observation_id":"20627ddb-7dc5-4a67-94cd-211dc5128986","resolution":{"observed_at":"2026-08-15T20:41:12.536599Z","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":"2026-08-15T20:41:12.540258Z","title":"M., Dupuy , T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.540258Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:ce2703b7e6a80f0c2f706787a1670c71bbb09322c05972ad5156e19c5466dd20","observation_id":"6aa1f642-f0d9-4595-85e3-33bdf17a6a03","resolution":{"observed_at":"2026-08-15T20:41:12.540258Z","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":"2026-08-15T20:41:12.543963Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.543963Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:5c1f66cb5d9cb87ea384db1e0c27df3002ba049ce73ece9b48c2986aef7d3f23","observation_id":"636155fd-2772-435f-8f9c-74fbd40bfdb0","resolution":{"observed_at":"2026-08-15T20:41:12.543963Z","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":"2026-08-15T20:41:12.547670Z","title":"2021, , 254, 42, 10.3847/1538-4365/abf93c","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.547670Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:b683902f148d487d2770ae5357ef873465e2d8755919e69827ed4a917a834ce3","observation_id":"a4be26c5-4bcd-44a5-94a3-eb0d7b64a611","resolution":{"observed_at":"2026-08-15T20:41:12.547670Z","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":"2026-08-15T20:41:12.551350Z","title":"D., Dupuy , T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.551350Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:7ea9d5fcb4bf800ba6e4d75355c87866c46df96a11172163ca2b4628ffb48204","observation_id":"2d929d57-b7d3-4a4f-abe4-9642bcc6a132","resolution":{"observed_at":"2026-08-15T20:41:12.551350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.11671","last_updated":"2021-09-15T20:41:01Z","snapshot_observed_at":"2026-08-16T18:22:29.722108Z","submitted_at":"2021-05-25T05:08:44Z","title":"orvara: An Efficient Code to Fit Orbits using Radial Velocity, Absolute, and/or Relative Astrometry","version":2},"cited_work":{"arxiv_id":"2105.11671","doi":"10.48550/arxiv.2105.11671","metadata_source":"pith","pith_arxiv_id":"2105.11671","snapshot_observed_at":"2026-08-16T12:16:17.039197Z","title":"orvara: An Efficient Code to Fit Orbits using Radial Velocity, Absolute, and/or Relative Astrometry","venue":"astro-ph.IM","work_id":"f9aa460b-f910-4663-b09a-cd95acafd4bd","year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.554967Z"},"links":{"cited_paper":"/paper/2105.11671","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:3601fa6785945ce26e897307d26cb9a0ab36576978ba92a1fa50fb4fc1ecc779","observation_id":"98c68756-18c1-4f0b-927a-d85ca7e3feb6","resolution":{"observed_at":"2026-08-15T20:43:39.865418Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.559061Z","title":"2012 a , Journal of Double Star Observations, 8, 210","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.559061Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:93ee43fb835be64f5839f8570b1cb49ff64a0faea8030a22f432bc9f718cb1d8","observation_id":"f35f3c02-c833-4e66-b563-235d860c8bd4","resolution":{"observed_at":"2026-08-15T20:41:12.559061Z","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":"2026-08-15T20:41:12.562430Z","title":"2012 b , Journal of Double Star Observations, 8, 210","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.562430Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:5607afc53fd96f672d4481a512f191415b2e8225d21b6b032df30c60ce4dd956","observation_id":"cc044ef3-3972-403e-aea4-5542007a2da6","resolution":{"observed_at":"2026-08-15T20:41:12.562430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/133506","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:39.680872Z","title":"M., Noyes , R","venue":null,"work_id":"34a25830-0d0a-47ff-be59-5a42ecedba2c","year":1994},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.565560Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:97a84beae3c662dc7e225169afbc90c3ab95d3778fa548f6cd419dc1def7298e","observation_id":"0f238a03-ca05-4069-aed7-bf8de7e073f1","resolution":{"observed_at":"2026-08-15T20:43:39.750485Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.00062","last_updated":"2017-10-02T16:54:46Z","snapshot_observed_at":"2026-08-20T05:03:35.280123Z","submitted_at":"2017-06-30T23:08:21Z","title":"The SpeX Prism Library Analysis Toolkit (SPLAT): A Data Curation Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.00062","snapshot_observed_at":"2026-08-15T20:41:12.569191Z","title":"J., & Splat Development Team","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.569191Z"},"links":{"cited_paper":"/paper/1707.00062","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:9f60de4d09e49ea91294ef91e9f8cef17551a8bdbe3bcaf6af2de1844bc5e162","observation_id":"2d4f8f1d-b3a6-41b6-8dc3-db016f4a2810","resolution":{"observed_at":"2026-08-15T20:41:12.569191Z","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":"2026-08-15T20:41:12.573249Z","title":"C., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.573249Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:00fa3a4eae301848d10378e616bf5e0a303845841be57e4ce8138f829663743b","observation_id":"fb42e3c2-8982-4e0c-9553-3ce99a5e8a4a","resolution":{"observed_at":"2026-08-15T20:41:12.573249Z","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":"2026-08-15T20:41:12.576942Z","title":"P., Wright , J","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.576942Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:b16becd662287a1125580d57c01ba4e2c72ecd0d7827faad6b7491fe99d72183","observation_id":"b0ae72c9-94a2-48a7-8d35-5d2bc830619b","resolution":{"observed_at":"2026-08-15T20:41:12.576942Z","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":"2026-08-15T20:41:12.580583Z","title":"I., Kanodia , S., Bender , C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.580583Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:1ccf6b4998e26c11fa7ab4379f80e0ea559fe44433a51bf251b584f7da4ec76e","observation_id":"919c1849-e050-4115-ab61-16f85e003403","resolution":{"observed_at":"2026-08-15T20:41:12.580583Z","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":"2026-08-15T20:41:12.584375Z","title":"1923, Misure DI stelle doppie eseguite col refrattore ``Merz'' DI 8 pollici negli anni 1886-1900 E col refrattore ``Merz-Repsold'' DI 18 pollici negli anni 1902-1905 DA G","venue":null,"work_id":null,"year":1923},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.584375Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:c222a4558c0e528ee5047b5bd88718fd08bf2cea5c7aa4820a593bbd7eb08ff1","observation_id":"88052061-9969-4f03-b161-9b755bd3e9a9","resolution":{"observed_at":"2026-08-15T20:41:12.584375Z","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":"2026-08-15T20:41:12.588540Z","title":"2016, , 823, 102, 10.3847/0004-637X/823/2/102","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.588540Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:440cfc03a12bf8f1bb397a233d58a0fa211b4befa067e08b12d420c244b1fbbd","observation_id":"d5802874-ee91-4f9e-896b-35f2fcfa46ba","resolution":{"observed_at":"2026-08-15T20:41:12.588540Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stab1052","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:39.594614Z","title":"T., Clert \\'e , M., Hinkel , N","venue":null,"work_id":"6b32cc2e-4edd-4d50-ae59-45d34dc45f60","year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.592480Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:7146a0595b73d996d660ec0660f3697382d18255fc1ac079fcbac0ec2ebd4ff8","observation_id":"339a3054-631e-498c-b7d0-2b3f7bccf5ae","resolution":{"observed_at":"2026-08-15T20:43:39.609689Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stab3498","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:39.533381Z","title":"T., Wright , D","venue":null,"work_id":"ce25e173-95c2-4e25-aee8-94bdab66f6ca","year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.596268Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:0a4bed85e926bbc34c812a4dacce6868500ebf4163e603fb562a994ccf896853","observation_id":"5d04d609-d8c2-4c15-99fd-f2f45da26b09","resolution":{"observed_at":"2026-08-15T20:43:39.538278Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/186167","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:39.329034Z","title":"D., Hatzes , A","venue":null,"work_id":"480f06dd-b48f-4f3f-8369-f6fc7101f4e9","year":1991},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.600418Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:18a0a5aaba19de82b28e21d3405e22715d7dd469e681d27dc0a47d347cc6a0b5","observation_id":"f59a889d-4711-4af5-ac06-debd806bf637","resolution":{"observed_at":"2026-08-15T20:43:39.416384Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.605209Z","title":"R., Johnson , J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.605209Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:e313988fcdbb1854caf5044cf373d65689b77a97cdd849efea502086e5fdd8e7","observation_id":"50e40496-a169-4bd5-9daa-e113a72e06eb","resolution":{"observed_at":"2026-08-15T20:41:12.605209Z","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":"2026-08-15T20:41:12.609161Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.609161Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:3a218c298922a906c64073ce87bf3c8a2e68c93437e7b14474e669d7afdcb650","observation_id":"a312bdaa-c327-4f07-8a3a-b277997db492","resolution":{"observed_at":"2026-08-15T20:41:12.609161Z","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":"2026-08-15T20:41:12.613522Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.613522Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:1bd262a0c30b382b0d2ef637f59b99074d0a307bf5de9b7b9bc2ceb1b2f9fd94","observation_id":"bad4c1fe-b4e1-4dec-a053-e0696e24a8a2","resolution":{"observed_at":"2026-08-15T20:41:12.613522Z","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":"2026-08-15T20:41:12.617137Z","title":"N., & Orlova , O","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.617137Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:222822a79dbba0499d2f6bef8dabe71ec9b08d2090c508f74bcfddee04fe3b6d","observation_id":"07401491-89cb-4e21-893e-01a887138a71","resolution":{"observed_at":"2026-08-15T20:41:12.617137Z","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":"2026-08-15T20:41:12.620902Z","title":"1884, Misure micrometriche di stelle doppie e multiple: Le osservazioni fatte a Gallarate sopra le stelle del Catalogo di Dorpat e delle appendici di W","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.620902Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:86bb0d1c02d5de02eb58c42b7a40132e895e1514710df16f08d9a1c9867903a7","observation_id":"9e409909-48f4-4167-93b8-7fa192517597","resolution":{"observed_at":"2026-08-15T20:41:12.620902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/asna.18760880303","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:08:47.750906Z","title":"1876, Astronomische Nachrichten, 88, 45, 10.1002/asna.18760880303","venue":"Astronomische Nachrichten","work_id":"06ef483f-57f2-4b5f-ba8f-ae58e3dbd1a5","year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.624559Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:dcc4fb718d89128be8efdd85996d668b593ccab6bf33434e5e785194f775f5c5","observation_id":"e167a9f9-9222-4cce-a916-a2dc522d2ddc","resolution":{"observed_at":"2026-08-15T20:43:39.262904Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.628530Z","title":"1927, Double star observations, 1875-1927 (Germany: (n.p.).)","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.628530Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:1d45d308c09899e8d55c0cfe976348e9c85744a26454d51f0615f4320a3acf6f","observation_id":"e54f1d97-4612-414b-8096-3591c31bbd5b","resolution":{"observed_at":"2026-08-15T20:41:12.628530Z","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":"2026-08-15T20:41:12.632278Z","title":"2016, , 222, 8, 10.3847/0067-0049/222/1/8","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.632278Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:aef7dc28c5837b88d9d8f9a853f25848ce41fc80edcbc69407acd0f62ac267c1","observation_id":"2dfcf6aa-0f54-40ab-97a1-3a2ce263a19f","resolution":{"observed_at":"2026-08-15T20:41:12.632278Z","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":"2026-08-15T20:41:12.635901Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.635901Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:10a0436b69f2056cd6861ebadaf3140ab6b1babd32adfac72e7befb22c7a4c83","observation_id":"7799d4f0-d61d-4245-840a-bcd9c8ea36ac","resolution":{"observed_at":"2026-08-15T20:41:12.635901Z","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":"2026-08-15T20:41:12.639478Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.639478Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:8b91ef678a1d423859810845d46e09eb2b009e52c7e87fafc54f3e06d6a64b35","observation_id":"e71acf8f-03a9-4873-b196-e0aed13d8c71","resolution":{"observed_at":"2026-08-15T20:41:12.639478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/191097","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:39.150503Z","title":"C., Moffett , T","venue":null,"work_id":"04e15beb-9bea-4d72-bcc2-130a522652b0","year":1986},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.643088Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:8de559f20cb9a9b4f4a735e2183728cd3da82b7fa5ce0dbba4b3cfad0af8a6d4","observation_id":"49544461-8c6d-4580-b303-0d2d2ffe1d83","resolution":{"observed_at":"2026-08-15T20:43:39.155552Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stab2225","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:38.987208Z","title":"P., Jones , H","venue":null,"work_id":"981e218c-123c-46d5-9f5e-12a10b09acca","year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.646578Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:fc4b58af8c9c660d5bb2e29e4e22dc9906bafcb4aa32facec1ae6333ace5cf66","observation_id":"7ca7d5b6-4675-4f85-bbc1-85800edf27a5","resolution":{"observed_at":"2026-08-15T20:43:39.039265Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.650523Z","title":"A., Marcy , G","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.650523Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:875e8416453b12c9345fdcd3ddfc04fcab8a9975990ec6ad4766f46fe578494a","observation_id":"56829b40-7f38-4aae-8aa4-8de3d90b55fc","resolution":{"observed_at":"2026-08-15T20:41:12.650523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/92.2.121","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:38.885496Z","title":"1931, , 92, 121, 10.1093/mnras/92.2.121","venue":null,"work_id":"3d1736a0-0fb8-4fc7-b4bb-d7e27894523d","year":1931},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.653986Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:6befc003429e5b8f15dfc81a3c527d2a1024763eee1511ba0b718e256e202925","observation_id":"f73da53b-ff5a-4ae3-8c2f-b4a79374d04d","resolution":{"observed_at":"2026-08-15T20:43:38.964589Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.13318","last_updated":"2024-08-23T18:07:48Z","snapshot_observed_at":"2026-08-16T13:24:15.221602Z","submitted_at":"2024-08-23T18:07:48Z","title":"Earths within Reach: Evaluation of Strategies for Mitigating Solar Variability using 3.5 years of NEID Sun-as-a-Star Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.13318","snapshot_observed_at":"2026-08-15T20:41:12.657878Z","title":"B., Bender , C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.657878Z"},"links":{"cited_paper":"/paper/2408.13318","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:7c10a6d8cb68a7d6c53e21a5076b2bf387f35fd1c9ef66e73bfd76327a166143","observation_id":"7f13f6ef-3293-4a97-9db9-d0345404f883","resolution":{"observed_at":"2026-08-15T20:41:12.657878Z","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":"2026-08-15T20:41:12.662307Z","title":"W., Lang , D., & Goodman , J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.662307Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:9121958f31eb1e254ba0f3e6b330b1b28d3024769a1f7c889ee5ecead44d77e4","observation_id":"78e07da5-1b06-4e5a-a41d-b118fea8c692","resolution":{"observed_at":"2026-08-15T20:41:12.662307Z","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":"2026-08-15T20:41:12.665743Z","title":null,"venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.665743Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:69a4c415d40596678622835d8f1a8fa76fb9d8c78b1bd724023f4e1768928756","observation_id":"62b2c697-a7c6-432b-b433-4d23d5a5e55d","resolution":{"observed_at":"2026-08-15T20:41:12.665743Z","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":"2026-08-15T20:41:12.669513Z","title":"1964 b , Publications of the U.S","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.669513Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:2fce82d1c4b7bc0f9e7b1a2bb7da52b8d870e68830db652ea62ac207d3ef3d9e","observation_id":"8c969aae-04d5-4f78-9a16-bb21502bf604","resolution":{"observed_at":"2026-08-15T20:41:12.669513Z","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":"2026-08-15T20:41:12.673098Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.673098Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:7ba3e032ae579cff78e1d7036d02d41ca794eb4e06c7a50b76fea890fc44a632","observation_id":"17e7a952-94a2-429c-8a39-633d0b18c833","resolution":{"observed_at":"2026-08-15T20:41:12.673098Z","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":"2026-08-15T20:41:12.676700Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.676700Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:31e7929c8f07c2f4d4bb3cfc0991a06636e295421382cd9cf883dd601808ccf8","observation_id":"a61ebd55-7c76-4a3b-b383-918657fe2475","resolution":{"observed_at":"2026-08-15T20:41:12.676700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00211","last_updated":"2022-07-30T13:18:15Z","snapshot_observed_at":"2026-08-20T21:16:40.620608Z","submitted_at":"2022-07-30T13:18:15Z","title":"Gaia Data Release 3: Summary of the content and survey properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.00211","snapshot_observed_at":"2026-08-15T20:41:12.680846Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.680846Z"},"links":{"cited_paper":"/paper/2208.00211","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:87742b2f327c6540dd53521bb65338a1a7d8033a940802ae0e0a11b216782d80","observation_id":"ee92268e-db41-4ea6-a6dd-50d6dcd152b8","resolution":{"observed_at":"2026-08-15T20:41:12.680846Z","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":"2026-08-15T20:41:12.684903Z","title":"2023, , 674, A1, 10.1051/0004-6361/202243940","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.684903Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:c2fad5f88319737fee3b2ba8b5473bb42887aa4150b0d6634192e10936b1adb7","observation_id":"9b2bd300-bbb3-4f58-bef8-0c722e89bdbc","resolution":{"observed_at":"2026-08-15T20:41:12.684903Z","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":"2026-08-15T20:41:12.688827Z","title":"P., Mather , J","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.688827Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:2eabad493ecea98482de6ac2e411bc902439d28b2f4aff1232feef23785d25fd","observation_id":"6158528d-62e3-432f-9b2e-3eb96c684ac9","resolution":{"observed_at":"2026-08-15T20:41:12.688827Z","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":"2026-08-15T20:41:12.692531Z","title":"2025, markgiovinazzi/binary\\_mc: binary\\_mcmc v1.0.0, 1.0.0, Zenodo, 10.5281/zenodo.15352084","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.692531Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:fcc22a0f5a5d27e12c6423b3ced67d866551676946f1921858e7333b9a2e131e","observation_id":"66b8816d-70d9-489c-9ad6-179c2d0a4967","resolution":{"observed_at":"2026-08-15T20:41:12.692531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.12112","last_updated":"2022-08-25T14:18:23Z","snapshot_observed_at":"2026-08-16T16:36:54.530859Z","submitted_at":"2022-08-25T14:18:23Z","title":"A Mass-Magnitude Relation for Low-mass Stars Based on Dynamical Measurements of Thousands of Binary Star Systems","version":1},"cited_work":{"arxiv_id":"2208.12112","doi":"10.48550/arxiv.2208.12112","metadata_source":"pith","pith_arxiv_id":"2208.12112","snapshot_observed_at":"2026-08-16T12:16:17.039197Z","title":"A Mass-Magnitude Relation for Low-mass Stars Based on Dynamical Measurements of Thousands of Binary Star Systems","venue":"astro-ph.SR","work_id":"3fe42d53-a793-4622-a232-d6eb8897bc7d","year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.696220Z"},"links":{"cited_paper":"/paper/2208.12112","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:da283dbd06671c5fee62f064aaa577f56a8bc3551948bacc04172e170126052e","observation_id":"ed76d078-bf85-48b7-8f41-530a9406e468","resolution":{"observed_at":"2026-08-15T20:43:38.739495Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/asna.202013830","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:08:47.750906Z","title":"R., Blake , C","venue":"Astronomische Nachrichten","work_id":"2ed7bdfe-22a7-48ee-b2d6-1ef044bb9f11","year":2020},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.700104Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:f2bb400a1de56bc509ef22b9bea515018a57d9acae8c4d232a12455a8f581de0","observation_id":"6e31ed3c-d863-4284-af37-e0f58b72378b","resolution":{"observed_at":"2026-08-15T20:43:38.635015Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.704555Z","title":"R., Cale , B., Eastman , J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.704555Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:46daa5e8911accb910d269e27bf5d98a1e482462edc6c5f8b54ad0f1abb9eed6","observation_id":"beef8245-4ab9-41d9-a5c7-41696e7859f7","resolution":{"observed_at":"2026-08-15T20:41:12.704555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/61.8.556","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:38.502230Z","title":"1901, , 61, 556, 10.1093/mnras/61.8.556","venue":null,"work_id":"2d83209a-a4ea-4127-a1f4-89ceca584287","year":1901},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.708484Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:cd510a5bc67b3658c31cdf5e1dd441d38b5483cd9a79ed2c5979e22be272a4cd","observation_id":"2b840ef1-39f4-4ec7-86c5-970d0a950576","resolution":{"observed_at":"2026-08-15T20:43:38.509057Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s10511-006-0038-7","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-19T11:03:45.297681Z","title":"L., Shakht , N","venue":"Astrophysics","work_id":"04cd4e96-1736-4281-89f1-3ac25ff61d57","year":2006},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.712446Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:44d3d9410cdd44c2dc1764de6fba8a2ba9036b1fb745fb7e669559853162032a","observation_id":"57820cd6-0fbf-4214-807b-6b911d7e81d4","resolution":{"observed_at":"2026-08-15T20:43:38.424201Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.716248Z","title":"2024 a , in AAS/Division for Extreme Solar Systems Abstracts, Vol","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.716248Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:729a203413ccc0a6593522b41db606ef1f4cc0557c8d6d12459769e8289da828","observation_id":"c2813a22-07cf-44de-abe4-4cea5fbc4464","resolution":{"observed_at":"2026-08-15T20:41:12.716248Z","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":"2026-08-15T20:41:12.719847Z","title":"F., Wright , J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.719847Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:a827931fa0d9b7af9f480712697532d3adc053d6e0cc4f90beda6284a703f6ba","observation_id":"65ba1bf7-da1b-4b9b-9d8f-095e47ea3ee1","resolution":{"observed_at":"2026-08-15T20:41:12.719847Z","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":"2026-08-15T20:41:12.723787Z","title":"F., Jackson , J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.723787Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:822464d264d202aa62287300ab00d1a781ee6a1046bb733ec660929b72cde433","observation_id":"332a4c32-ab03-4bb6-87fb-326710ca0a77","resolution":{"observed_at":"2026-08-15T20:41:12.723787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12315","last_updated":"2024-09-18T21:07:24Z","snapshot_observed_at":"2026-08-16T13:17:21.960955Z","submitted_at":"2024-09-18T21:07:24Z","title":"The NEID Earth Twin Survey. I. Confirmation of a 31-day planet orbiting HD 86728","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12315","snapshot_observed_at":"2026-08-15T20:41:12.727487Z","title":"F., Luhn , J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.727487Z"},"links":{"cited_paper":"/paper/2409.12315","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:600ebd855c7c74ed262c679acdb28306276a196fed845f0b570b58144ba20840","observation_id":"2624500c-49d2-4955-8221-da348d480d05","resolution":{"observed_at":"2026-08-15T20:41:12.727487Z","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":"2026-08-15T20:41:12.731462Z","title":"2023, , 674, A9, 10.1051/0004-6361/202243969","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.731462Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:fae2a1bca10d2afd8743bb3a7e391df06995980ae0b19c979e899ed32130a815","observation_id":"a16f84a9-6884-4922-a590-7b54e8bab7a4","resolution":{"observed_at":"2026-08-15T20:41:12.731462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/133511","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:38.105345Z","title":"1995, , 107, 22, 10.1086/133511","venue":null,"work_id":"b9563395-53bd-4007-9c40-9c3cae525fbd","year":1995},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.735130Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:1a8b070d1afdb6b8fb5ba8e8b87fa73897e19ad3313a1f55fed6c42b82ed2253","observation_id":"f8ef04ef-85c3-4e39-a7cb-e03637064cde","resolution":{"observed_at":"2026-08-15T20:43:38.223615Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.738803Z","title":"1892, Observations made at the U.S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.738803Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:f162ba5e21041a1998e4507e06196033f86e65ae41aeb7e5f149a0c6c3328bd3","observation_id":"ca347de4-8d42-4168-934e-073b0994027b","resolution":{"observed_at":"2026-08-15T20:41:12.738803Z","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":"2026-08-15T20:41:12.742773Z","title":"2016, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.742773Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:3ed0c8f75b6c8c048253eeb0e6959572ca8f7626dfddf039607b74dd67da4e34","observation_id":"adc32ebc-e8b7-4cfe-8bd4-7b4f5cd473b9","resolution":{"observed_at":"2026-08-15T20:41:12.742773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/190686","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:37.944289Z","title":null,"venue":null,"work_id":"88da9d95-4af7-4f3b-b80b-35ee0e8d5dd0","year":1980},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.746337Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:d770699b1736088f134804d06850dcde3455ee49f0fe9546a17f3ce7b9015c64","observation_id":"356ed54b-0fba-4ebd-9696-04caf813c7b0","resolution":{"observed_at":"2026-08-15T20:43:38.002489Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/191499","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:37.728918Z","title":"1990, , 74, 275, 10.1086/191499","venue":null,"work_id":"eefa0277-1836-4716-9ac0-7e0a586bf391","year":1990},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.749935Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:9e67af7f032ba074d9172484343df1c9fa10437489ea5488f52d2e2a71c2baef","observation_id":"7a58c642-5137-459d-a804-9a2639492f3a","resolution":{"observed_at":"2026-08-15T20:43:37.837604Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20065459","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:43:37.546115Z","title":null,"venue":null,"work_id":"98e4788b-0f04-4eb4-a01b-687ad9518a33","year":2006},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.753721Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:689387f7773867c7f9e2aaaf9f4db4c9b66cebc206f3b81edcfe12208cff6954","observation_id":"455ad278-6ba1-4035-914c-ff9fc2a2025e","resolution":{"observed_at":"2026-08-15T20:43:37.619065Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.757556Z","title":"J., Kirkpatrick , J","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.757556Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:4bea8b5b73ce49195f24f0a478e65f3e7e9ba8224ba7110130f489523450bf26","observation_id":"4c149320-9492-4a9a-937d-3575ebb0934c","resolution":{"observed_at":"2026-08-15T20:41:12.757556Z","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":"2026-08-15T20:41:12.761399Z","title":"J., Jao , W.-C., Winters , J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.761399Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:224460b78fc2b7f6e663ce2841fca639fbd8da491ad5a88659803d4e7baecd92","observation_id":"568e2e5d-05ea-46d2-80a9-fb070a98a58f","resolution":{"observed_at":"2026-08-15T20:41:12.761399Z","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":"2026-08-15T20:41:12.765241Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.765241Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:c2e773c6628c5b6779cec5c36b71907a6d4d6051ef55c24bf0a4e7569a55b7e8","observation_id":"49db7276-832f-4356-a0db-f379c55f4ec7","resolution":{"observed_at":"2026-08-15T20:41:12.765241Z","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":"2026-08-15T20:41:12.769012Z","title":"A., Rosenthal , L., Fulton , B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.769012Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:5ef6670584bee0675841e9a182f5c1ba573ef5272bad57bed58fbb7eee55bb4b","observation_id":"66381997-95ee-4958-b3b4-ee5ca4b8ccdb","resolution":{"observed_at":"2026-08-15T20:41:12.769012Z","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":"2026-08-15T20:41:12.772845Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.772845Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:a558b1752a6408472345e8d8b36cb1ed62e7d0f36179852b3d5ed41a42cd631f","observation_id":"7788afe4-443f-451b-800f-b4c1c5ac174b","resolution":{"observed_at":"2026-08-15T20:41:12.772845Z","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":"2026-08-15T20:41:12.776490Z","title":null,"venue":null,"work_id":null,"year":1915},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.776490Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:b256d0659c6b28a5970301bdb4270ef8a60ad5eba0449eecee1b0581c6cfb48b","observation_id":"60338ab6-272f-41c5-9386-3d2588a7824b","resolution":{"observed_at":"2026-08-15T20:41:12.776490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.17332","last_updated":"2024-06-25T07:33:09Z","snapshot_observed_at":"2026-08-16T13:39:52.568000Z","submitted_at":"2024-06-25T07:33:09Z","title":"The California Legacy Survey V. Chromospheric Activity Cycles in Main Sequence Stars","version":1},"cited_work":{"arxiv_id":"2406.17332","doi":"10.48550/arxiv.2406.17332","metadata_source":"pith","pith_arxiv_id":"2406.17332","snapshot_observed_at":"2026-08-16T12:16:17.039197Z","title":"The California Legacy Survey V. Chromospheric Activity Cycles in Main Sequence Stars","venue":"astro-ph.SR","work_id":"59dc2bfa-5c69-4fb2-953d-59e1de66fdd3","year":2024},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.780230Z"},"links":{"cited_paper":"/paper/2406.17332","citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:fed697e23859f3ffc2d921404e28dfc9faa8299bb3fd22853e8eeee8569217cc","observation_id":"0d01045f-bb47-448e-89a0-a364a34ae3d6","resolution":{"observed_at":"2026-08-15T20:41:13.953829Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/asna.202013815","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:08:47.750906Z","title":"2020, Astronomische Nachrichten, 341, 762, 10.1002/asna.202013815","venue":"Astronomische Nachrichten","work_id":"09b1b55f-7dab-4bd5-ac5b-3198a012b9a3","year":2020},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.785272Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:ebf968b2703c0393821f224d7344ba36e0197357a6f560bdd20502e6f473c428","observation_id":"efce8a16-436c-478b-b525-5323abf8e8ad","resolution":{"observed_at":"2026-08-15T20:41:13.937486Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.789028Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.789028Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:99572f864d8c9d155f8911df14560dfad7c0630de88f4e5e223f938edcaa4428","observation_id":"73e20744-9043-4c03-a094-c7a805e9eaf4","resolution":{"observed_at":"2026-08-15T20:41:12.789028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1134/s1990341316020097","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:41:13.910958Z","title":"2016 b , Astrophysical Bulletin, 71, 225, 10.1134/S1990341316020097","venue":null,"work_id":"dea6d246-b841-457a-ba29-a9c54349777e","year":2016},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.796573Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:5f67f9e4eb2f9b1ac1bcac1a2e3ed19cd7b180afd5ccdbf16279d4d137ebb7f2","observation_id":"94068f8e-d3f5-4c22-a309-dd2a2c625fb6","resolution":{"observed_at":"2026-08-15T20:41:13.915194Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s10511-021-09677-0","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-19T11:03:45.297681Z","title":"S., Shakht , N","venue":"Astrophysics","work_id":"a4d2964b-be6c-4124-a6e0-75acdbf74eae","year":2021},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.800099Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:f3890083cdeaf4fd636e93451779a462e965d6ea27f9d1c436169704694668f3","observation_id":"cf98012c-948d-4ada-9df8-a2e8163cbf1e","resolution":{"observed_at":"2026-08-15T20:41:13.900962Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1134/s1063773710050051","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:41:13.882471Z","title":"S., Khovricheva , M","venue":null,"work_id":"c2d73a45-9220-434c-9445-340e92e1085b","year":2010},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.804026Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:0af8e553654ec95598202fdd5939d0c72f6cb6a89e94578400c29b2835d3f73b","observation_id":"932a6e27-bd44-4393-bc5d-f3b0b316a058","resolution":{"observed_at":"2026-08-15T20:41:13.886660Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.808298Z","title":null,"venue":null,"work_id":null,"year":1951},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.808298Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:78360719c68eeec26499e32ca9c888dd00430bbab7fd8fe3beb1964f23f7d859","observation_id":"11705046-7b90-4840-a113-c401f5f9a98c","resolution":{"observed_at":"2026-08-15T20:41:12.808298Z","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":"2026-08-15T20:41:12.812769Z","title":"1951 b , Lick Observatory Bulletin, 524, 51","venue":null,"work_id":null,"year":1951},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.812769Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:2bfe37e350863d7717217e5a01555db52e63d0888590a2b7e5e3a4b7216079a2","observation_id":"366e478c-8b44-488c-977e-7e7bb937f7e8","resolution":{"observed_at":"2026-08-15T20:41:12.812769Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/aae5fb","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:41:13.869720Z","title":"2018, , 239, 14, 10.3847/1538-4365/aae5fb","venue":null,"work_id":"1572f506-5cd1-4f9d-a823-32fca7abdf12","year":2018},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.817335Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:f0849cc651b1a28374afc627e8eabda488d139e95123676f3f8861e00ccccb22","observation_id":"61cbcbd3-dfca-4262-81ac-15a9d3974c97","resolution":{"observed_at":"2026-08-15T20:41:13.873815Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.821152Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.821152Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:49ebc46cf1550a5dd31f5f635a8fdb93b170d8c672af2e0a5eef179c4032ab8b","observation_id":"38dee920-7456-468b-b19b-071a36a3bdeb","resolution":{"observed_at":"2026-08-15T20:41:12.821152Z","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":"2026-08-15T20:41:12.825016Z","title":"J., Dahn , C","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.825016Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:e91dd2c2a0a73e256e9ce7f88277305778e652bb233279ba1c3e67da685890d2","observation_id":"0d148d9c-9f25-47c6-b848-3f01502f0e78","resolution":{"observed_at":"2026-08-15T20:41:12.825016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/190920","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:41:13.857327Z","title":"1984 b , , 54, 103, 10.1086/190920","venue":null,"work_id":"eb5eb40a-c2f6-47de-b4f4-09fc86b3ffd1","year":1984},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.832635Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:2be8890940bae9ff4b493a7998f2ccb788e2e055eb469ddea171d5edc2023ce8","observation_id":"dad06bab-9240-4590-9a87-3a7200e31975","resolution":{"observed_at":"2026-08-15T20:41:13.861557Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+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":"2026-08-15T20:41:12.836374Z","title":"I., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.836374Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:d2ee3d84e68543f8b88ac46fff8b7d402d9f86949265acbd82cb292099b597ea","observation_id":"a4ab5ea3-a48c-47db-b938-812e6b8c802c","resolution":{"observed_at":"2026-08-15T20:41:12.836374Z","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":"2026-08-15T20:41:12.840080Z","title":"2008, , 488, 667, 10.1051/0004-6361:200810080","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.840080Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:80c209fec34fcd50c33671cf8a29fa4feca05640f168ee9863594ea37038e462","observation_id":"c65c12e4-522e-467a-b9df-6944ff247b3d","resolution":{"observed_at":"2026-08-15T20:41:12.840080Z","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":"2026-08-15T20:41:12.843875Z","title":"2019, , 632, L9, 10.1051/0004-6361/201936942","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.843875Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:e5ffa0a6812c2c96fed6cef86f01eb6c06ae021d8693eb93a76a1b91c51c0b82","observation_id":"0d9c24c7-a750-4d1a-b3fd-bff568ede880","resolution":{"observed_at":"2026-08-15T20:41:12.843875Z","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":"2026-08-15T20:41:12.848148Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.848148Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:dabb8053e842e5bf550d9a89db9a61551f8107332679e70ebd93d5a79d3a77ea","observation_id":"66b5f588-9354-48ae-b055-f41c3bedefff","resolution":{"observed_at":"2026-08-15T20:41:12.848148Z","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":"2026-08-15T20:41:12.851718Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-15T20:41:12.851718Z"},"links":{"citing_paper":"/paper/2505.12563"},"observation_digest":"sha256:22ad1091918296a465cec47097e04cc03553c6e67ee4764db2e53f5d56668e64","observation_id":"09246b7d-aadb-4ef3-832a-8936be7aaa3d","resolution":{"observed_at":"2026-08-15T20:41:12.851718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.12563","last_updated":"2025-05-18T22:43:27Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-17T00:05:10.007193Z","submitted_at":"2025-05-18T22:43:27Z","title":"The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":73,"verified_exact":26,"verified_fuzzy":0},"total_outbound_references":196},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 100 of 196 outbound references and 1 inbound Pith citation observation for arXiv:2505.12563."}