{"as_of":"2026-08-05T23:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a167a276bb57d818c70106c5beddf167f90cf0de0ce2a4e2677e3f3ed7675395","coverage":[{"denominator":85,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":85,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-29T05:37:48.800921Z","state":"measured"},{"denominator":85,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":85,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2605.29666/citation-record","integrity":"/paper/2605.29666/integrity","json":"/paper/2605.29666/citation-record.json","paper":"/paper/2605.29666"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T05:37:48.800921Z","title":"2022, ApJS, 259, 35 Aguilera-Gómez, C., Jones, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:9989ddbe67fe3a2470a5401eda5fe87fc2e53afc9012ae07da4ed484961a46e5","observation_id":"f6190244-ebef-4432-9624-f5cc20d114a2","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Plez, B","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:063a50634763920eaa3c365bfe6c1b4f3c4e2f209ae336b74889b03e6cba9d39","observation_id":"d0276421-e18a-4ba4-867e-b732d4d7243e","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"M., Asplund, M., Collet, R., & Leenaarts, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:42bbb0cbb44585b7163e37e61f4159b4734996a2f3f32899202b0354603de1c5","observation_id":"d2a4900c-8c4d-4bf0-8640-4c7f4ea2548d","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"M., Grevesse, N., Asplund, M., & Collet, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:5c1ac0d29fadfe17956e0c6bfd788e6abe7e339ec5d45adee69fe65ee3fdaa9c","observation_id":"8bbfa2d4-c4ed-43ff-989a-d313f65987ca","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:f50041e910bf40dc1fb3d6ec0c5469876e371c9a1eb4a39be6ecdb750eff1e2e","observation_id":"21349e75-23a5-415a-8011-bb6c75dfdb28","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Bovy, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:c370ddc2539f4a5b4387ba27718c6af19d57ec5bb72a57d05fba02ada9bfecbd","observation_id":"e9048e57-dc86-4d09-9015-72612da06792","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"K., & Vaidya, K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:1dc150cbcd7ab236900bec89acebe67cfddb8e0ca0e63eb371df211fce9fab92","observation_id":"0dbdda8f-71e0-4c59-9504-40c9267659c2","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"R., Bershady, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:630ab8acbb163806abb63a984c0672d2542f80956adfe8fee94780a70f89a42d","observation_id":"b91ab2a7-0b59-4323-b658-e4ceaf43f556","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:909a753b9e713a65aa005de07bf7e55c6abf7bcba0edb4930ed49cab146c289b","observation_id":"3f553a8b-337b-4c8f-bdbe-3418d5f7836d","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:e73da7d766f6047d66ed9424c539562071d7f6670e47abaa28865fed2a30b335","observation_id":"b02d6bf3-4daf-4fa4-9b0d-90d4ded70de9","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2019, A&A, 623, A108","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:1997f0b1e268c03e6c46a49da4f5ace831c7e910c838911bb56e33413ccacc8f","observation_id":"017747df-255c-4b79-aaf2-896f38b8f5e6","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2012, MNRAS, 427, 127","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:5e91f46fd9d25889f2f83613d50d32c0bea838f285d43243ee2fa0bf387fc4c5","observation_id":"5e7a92f8-ec22-490a-8528-304598cbd8c1","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2020, A&A, 640, A1","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:c30e2369cbd37e87ddadcebc219bcb74acb1bf9ac2d744e0cb92722bbc242f13","observation_id":"87cf14c2-dbfc-4487-a086-4be5f31d872d","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2018, A&A, 615, A49","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:ec383f7cc8c23053d3a79f28dc9c26fc2a89bfb806f558661fcdb4c8e61d308e","observation_id":"37d8003f-f078-43dd-8f8d-768bbd571af7","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Langer, N","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:b935d98e1fa467262ac7f15e8460ebc214b5be4cf90b33dc829861be7737dddf","observation_id":"19b18f40-ecae-4dac-be80-7174ac209ac2","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2014, A&A, 568, A86","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:f51835291cba8b5e3921b7cb127051e6cedeaff8cefa4e19935f0a58cc7e8a5a","observation_id":"5b0cb733-613a-4107-88f3-2514b4e4c3dc","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2019, A&A, 629, A62","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:775f2d3567611cbb7a95df06887c978bc433c0781f6b1b978f1baf595a7e1afe","observation_id":"bbe14f4b-3347-4a2a-b0ca-0580f3de1e16","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2020, A&A, 639, A127","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:5a32010f3339efbe87e478f76f7ec972915bed18b45e5ad7318e597b1cb7fe99","observation_id":"7b3122b6-d051-4158-ae83-60823f85b7f2","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:0177241e5152fbe5074e4df4a8a8fb7f4b1dafe64a56cbaab9fe560412908e45","observation_id":"88da0609-dcf5-4146-9161-d5e33551e953","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:8183368df1c7d6f5d39446c787e6da75a72abe2dd89270758ce6b251f15dd9d1","observation_id":"fb4048c9-c122-4ee7-a8a1-0534aa0aa1d9","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"J., Serenelli, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:c722f563ef50472eae48734db879198e8c6e920e992ccf0eb9cc290ac52c90ca","observation_id":"b79c197f-d2a1-4c68-8fca-a43640ee57cf","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"1994, A&A, 282, 811","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:b02ff964240595041b20e4444709db955dcfe9af388f91d960e7ad61681033d5","observation_id":"d202cc3e-9949-4b94-9a81-4566b986da0f","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2017, A&A, 605, A102","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:7592088326275108cd61af9a7cd974931202889e667e92efe3d753885af006d9","observation_id":"d30915f8-cc49-416c-8376-6150fa368ce4","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Lagarde, N","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:ac68e34e3f8c028ae3d5a6ee825ec72c5635f899b0a6bc50e48c5027209ed6a9","observation_id":"7656bc22-db18-45fb-8202-274c5ea7d111","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Zahn, J.-P","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:80ed7b9618b129cca8a0707e67661354d888c04e81c1bbba7c1dab001bda087e","observation_id":"90dc0f70-655f-4c6a-9bfc-2cf4fa6be293","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2017, European Physical Journal Plus, 132, 364","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:745225e679d47e9a11ee931bbb34bdd1f7985bccadd9243c3543fc4b55068171","observation_id":"a245c255-3c4f-43e0-b784-36c36e7971fb","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"J., Thielemann, F.-K., & Truran, J","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:ba7491c5c2481df04fde454d5d4f28758ef1c129d3a6c4044eca8bd49a195481","observation_id":"9b2bce2c-48fd-46eb-a715-e763104ab6a0","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:f92d47a348a4fb210fbdca841bfa0f01bf73fae212c00f3cb5729295cb3e947d","observation_id":"16dabb9a-2ccd-4368-b30c-26fdaa0dc7de","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"S., Monteiro, H., Moitinho, A., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:2348f2356c7f2c4b0239c6e8d02c18923f14d848d774b3af76a98a96679aa643","observation_id":"2b300424-3f32-4478-9db4-7ca0b3f855c5","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"P., Dearborn, D","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:1e0c196905ec9d5c54f19efe49b06c42098d6e57b90cc4ea5d8798b683c64042","observation_id":"d4e7b161-667b-4e15-a23e-bf1be056b50e","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:000665b2da452c675759a95c4adc6824addc8f6bb1c67633c73c1d0a801bd552","observation_id":"38573ed8-16c3-482d-99f4-df40e141a2b3","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2005, ARA&A, 43, 387","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:4ec9a793cfe5e8f6783276502a17bfefe3664abf896c6804b2fadbd36533ecb0","observation_id":"2ee12837-53c1-4dd2-8155-9d8ebf2054f0","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"C., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:45ea328e0062df1212b955be2a240ae354937ab48511d908ae30013c554501d8","observation_id":"8199071e-68b5-4af5-a237-ff3b011a06ab","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:e20d2312c5f515eb0adca5c7a37c863cfcbf56fbfcb60e5f68124729357af4db","observation_id":"fc9645f0-537a-4f63-8fee-d77122b36993","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"G., Sneden, C., Carretta, E., & Bragaglia, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:b7b4987901b10b756c39fc5681b25551e4c7f9d0101ac8119bc89817f035efa9","observation_id":"df1c9e3f-ff6b-4ff0-9c37-90c88484aef3","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:15f655c0bebe59e8efc57641719a27fc254e59565e7310dff1b75c64a941b960","observation_id":"a99665f6-b7f0-4dfd-a263-550de4f4cafc","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2008, A&A, 486, 951","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:60e6855bb0cd158633bdf5a915f1875467495bd02a1cd433996632ef476be0ac","observation_id":"fdc65d15-f5ed-4602-9e18-eeb674496c99","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"A., Shetrone, M., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:bfae0c18c77aaa6a06f2aeadf1e3e35320a5542122fe21718c73aa2c08bb2b0d","observation_id":"dbdc30f4-6903-4c5a-890d-69f6ebc9788f","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"D., Katz, D., & Gómez, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:866fabcfd0dad29da7876efeeb006a0d07967d60fb00cd5a2b69e2364ea923c3","observation_id":"144c04fa-60d5-4285-bf19-f9401f88ec11","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2021, A&A, 645, A106","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:3b509c146bcd0068e79dbff80d5fc5de7134a2799714778154a52fbea1ec6998","observation_id":"007d7a47-4c4c-4710-8013-61dc45356161","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:8159091f7f629d9c268f713e22c9b2457db3f80a0da06a5878a967da4118c727","observation_id":"bae1443d-0cbc-4bfd-9a71-e155abfbaac4","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"1965, ApJ, 141, 993","venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:9a70143003e001f16e2fdc230394f80ec0e2c0b344be4dd3e1ae31bf7b329125","observation_id":"86bc6deb-ed5e-4ca1-9ba1-2a309ad7ef5c","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"D., Jackson, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:c0d6cbe703a75c340e45098f601997700e3af73bcbeb38132122a8f3df0bb37b","observation_id":"c7142043-996b-4013-8810-6564a3ad3ca2","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:34527a60c5245873d375fe0858a225acf4091e98e2b9dab5b43015d07bc61376","observation_id":"5d955c54-7592-478f-b24b-3e25105b72a1","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Covey, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:093617f90da537967d8099148ab740881d3bd9fd39386e7becb457c61a5fd409","observation_id":"45b25702-8abb-41a2-9039-7950f00036dd","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"R., McKee, C","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:e75f6235071fdbd506f6b03d3f7451e8d6bab17bebda40ab76c8c239983f715a","observation_id":"31a0cfb8-d33a-4f4e-9dec-599500ff5d87","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:d0ec5da6c1b27f2a20c81c2d5c04fe8b1ec4e0ffbc642444fa31939a03b8f463","observation_id":"dcf20515-2a88-4e16-bc6a-5612cddb7723","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2012, A&A, 543, A108","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:b7d7bfa2d4fd46afc8000d7fb83b1e0fce2ff298cfc404a8fd59a7a5f8e069d6","observation_id":"46125f1d-4c1c-4f49-82dd-c6cd93684ded","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2024, A&A, 684, A70","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:fd2d4d545b38e14386661ba39285dffd7b6a21d71b05dc0b7ee218bb99cd859d","observation_id":"1f0510aa-b7ed-482c-8397-6532521ba313","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"C., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:08e2e47e83e0abec263669136555ba92b34401f86b3c00776804aac377b55c80","observation_id":"da98a756-81be-407e-b33e-ade81271d196","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"C., Reylé, C., & Nasello, G","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:649b79c7b80e102dd881d02d624d3fe17f48087836cdd91205dd0aed07ae4ae4","observation_id":"f5dd1c03-2ef0-4627-a0c9-b830c4459bb6","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"L., Brown, J","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:55c530d11f7ef5f758b0f9df8a65c72f0fb9d8d09040e9136579c0e91ab83f4c","observation_id":"d511d672-7834-4a68-a6d4-5bd664f68359","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Ezzeddine, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:a312ee420414c062ddb170e6f74c0522beb56fe77a80ea89b3c0ecd762e1e5c4","observation_id":"54e647c4-9047-480b-aa20-6e49d7fb6519","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2024, AJ, 167, 159","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:10c02c22259749a1077f312637bcfdc9f1795e4cf549d6c11aed6dbda956feee","observation_id":"5d463bc3-0fbf-4ed9-874b-70836b9d3e0c","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"H., Ting, Y .-S., et al","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:67f4038c94532004d5f5bf51fdcfca7d26353853c094ee863cf341870b06a3dc","observation_id":"81c82c80-4f22-4e1f-9275-6399df34832f","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"R., Schiavon, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:34147d9960c51fb9cf578bca92c587f32e293ebdb0da8e71d050f770ee1ea63f","observation_id":"b132ee0a-f687-446f-897a-86499cb3df60","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2016, MNRAS, 456, 3655","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:6d40fb6f0ecd2e50cc8c7c962d237ae5aa84764d0bec5a6c1cfccad724da281b","observation_id":"b875d464-3276-47df-8344-68479b1a1948","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Hekker, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:3f275215d711a5a0d2f5fbf597fb9a38e5079e8877d7cf04ecf0987a1994b03e","observation_id":"fff038ea-67c7-4e80-ad15-c8b84d532dc7","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2025, A&A, 694, A274","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:c492f68153193c97374f1182b6bf05063631df7325faaec44c55f901334866bb","observation_id":"a67cc263-fd5a-4b55-9b38-f18773415985","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:82745acfd4ae45f724c97ce7ad3997a57256650a27ae4b22823f7abb12eb6903","observation_id":"d7d8d4b0-d538-43fd-bdba-ae55a71e04c4","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:bd551be3e1501503d9de1c4a2d40fcef10a30207af39d867ed7ea9ec52bb29e0","observation_id":"1f19ff16-12b8-4385-bc45-657ace673a36","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"E., Silva Aguirre, V ., Christensen-Dalsgaard, J., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:54a2d96ccd9aee4686310ed01c63af238c12a45c2d789e433c3740d2db3e8808","observation_id":"74e65ea9-6b1d-4b05-a70b-459eedfaf13a","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.21413","last_updated":"2026-02-24T22:38:41Z","snapshot_observed_at":"2026-07-06T22:46:58.146051Z","submitted_at":"2026-02-24T22:38:41Z","title":"Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission","version":1},"cited_work":{"arxiv_id":"2602.21413","doi":null,"metadata_source":"pith","pith_arxiv_id":"2602.21413","snapshot_observed_at":"2026-06-29T05:43:08.423134Z","title":"Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission","venue":"astro-ph.SR","work_id":"cd0b55a8-1a6b-4b1e-85be-eb49292442f6","year":2026},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"cited_paper":"/paper/2602.21413","citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:f597547eea2ad4797d1ec72845d1c6f77ee4eeb50af7ad1519889e995b1bd6ed","observation_id":"6d8f0356-98da-4f14-81cd-8c28c213da9e","resolution":{"observed_at":"2026-06-29T05:43:08.424468Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-06-29T05:37:48.800921Z","title":"H., Elsworth, Y ., Epstein, C., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:16aa844b288dc9bf300f984f7624f33a18f3ceff735677bf22a1d5d5de1bb14c","observation_id":"2e545af2-231e-41c8-baed-05a12a45ccd3","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2012, Turbospectrum: Code for spectral synthesis, Astrophysics Source Code Library, record ascl:1205.004","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:91754a3bbb912fcccd3c203da13dd5f16e4b1b69e273ee11b93238043ee1813f","observation_id":"60bdc102-b3e0-4749-9550-a2d1199d21fc","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"J., Zasowski, G., Hasselquist, S., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:b5d9646406ca5ca023864b91db021a87a3e4302833014c843a24cfcc069d6b9b","observation_id":"daa6a451-a259-46fb-9213-dfeff9ee53b0","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"& Brammer, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:25d4e2fc133834cbc9bb2a44141c2687f3774164759cd4fe2e1b4a5940312b68","observation_id":"7885289d-92cf-4b88-9575-d4510184a92c","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2022, A&A, 666, A121","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:20c66cb531c7a5113c7c7239a28f6020ef34ba9ec1789c01a46b496d11792f25","observation_id":"d1082f99-3e85-48f5-a697-e1c121bd2337","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2509.25321","doi":"10.48550/arxiv.2509.25321","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"D., Pinsonneault, M","venue":"arXiv (Cornell University)","work_id":"7f8dac50-dd52-4c59-b078-34343d16fb7a","year":2025},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:479e91b7cda3beda608b8b4d440c85ccddf2370b070b770ce3b516e594465352","observation_id":"5f007105-32fa-4d3b-a9b8-35a35dd95020","resolution":{"observed_at":"2026-06-29T05:43:08.425039Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-03T22:08:15.886266+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T22:08:15.886266+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-06-29T05:37:48.800921Z","title":"2022, Atoms, 10, 103","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:76378d6903ef91fef676b3c69e4366cdb49135d191af5b1634e0e546db2aa0d2","observation_id":"2e41eb4b-1d61-4247-8fb4-d23a789e805a","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2009, A&A, 496, 701","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:2a2e8fae031a616087f68c5e9004f3ac7b081fbc6d48be13165ed84e667b6172","observation_id":"fc7df714-47cb-48f9-a482-9547c4c1ae11","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"M., & Cassisi, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:41be4f02dfe88a9ee001777e317221a9a902d62c4b8237c21ff6140a0219f46c","observation_id":"6f4fbc67-bc50-472c-85ee-14bcf9580d85","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:645271b3fb09bba7b9c832590bde52cec802b948faa09e351318a7c1d09d1cc2","observation_id":"3c4f9521-7e1a-45d5-8fa2-e9bb3a720e22","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"P., Ezzeddine, R., Ji, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:00a82d40c57d8dfc0acdc41afa487126914ea8d021e21d89c87b745c8bbab87e","observation_id":"a7720b3e-3816-4f44-b93f-5f4e9fbf8b73","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"H., Adams, F","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:f95b9f57cb2b872a3c43d4312fc490393decd05de47283335af3addcfbdbe372","observation_id":"14973261-ac8e-447c-9f52-1ec974936934","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"1972, ApJ, 171, 565","venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:129f7cf1a84a5db16c3f2a6b9462f1e0b476dd0e6e24d08ad8c696beb70de43d","observation_id":"616d087c-1171-430f-9d97-872aca095bf3","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2009, A&A, 502, 267","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:3ee72fb6ea44be631affef4007f590da5b61c1becbfe3e69c5f6673166ffe347","observation_id":"df96ff6d-0f5a-4d56-8acc-3f60e6c7c459","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:e685235763b017bb1e563be45ff5e88ffd20400199aac81cb5d49a7e1d620440","observation_id":"9c45c244-461b-4b6e-b39c-9986549f9891","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"I., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:2c57233b13dca631f11e6c1cca493dadd7dcacfad7dde1afe8b307c7e34ed6e4","observation_id":"62a67d20-26f8-465a-9581-4135123b1ebe","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"I., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:2f34e39eee0649cb1282dcf2101d9e0bda5dba26e61cabe9cecd0485a8044dee","observation_id":"a6c1d77c-8b4e-47a2-ad3e-ae8425f956d4","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"M., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:3d58705090a445202ed1e8539a5ebeab1ecea4dae351ffbf65b522d4df6682d1","observation_id":"b0eca4da-c356-41ca-b61c-48c6ffb3320a","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"K., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:7ea38e4c20bdc02c3ef5545bddda62418d725c52a7b2bd940cf5638c5216d580","observation_id":"bec34f66-ca68-4665-87db-d871be418a29","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"A., Brogaard, K., Leaman, R., & Casagrande, L","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:c37b75edba1da777aaa209c9349a23cda3e2295b1bfb3bbabf65feac6a8fdd1b","observation_id":"4e5bb966-30d1-40d1-be18-5dbb75c1dc98","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2022, A&A, 667, A103","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:a8ac67332974e7c6fd07db0ea879fe5f43b150b7bb304af9afaab95d1dd762f0","observation_id":"1ba6ac4c-130c-4bc3-8c4f-bf51089174a7","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","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":"2026-06-29T05:37:48.800921Z","title":"2021, A&A, 654, A77 Article number, page 10 of 10","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:48.800921Z"},"links":{"citing_paper":"/paper/2605.29666"},"observation_digest":"sha256:5a4566ed501cf206ddd96399e877d7131dcaff59e54feb485951bc9daecc0266","observation_id":"160e05d7-f863-4a47-9aaa-e10f7e1cc527","resolution":{"observed_at":"2026-06-29T05:37:48.800921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2605.29666","last_updated":"2026-05-28T09:27:18Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-01T17:10:04.144585Z","submitted_at":"2026-05-28T09:27:18Z","title":"Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters"},"reference_resolution":{"displayed":85,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":83,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":85},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 85 of 85 outbound references and 0 inbound Pith citation observations for arXiv:2605.29666."}