{"as_of":"2026-08-14T15:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a8d606337998e933142c29fdc6060cb3f1abd75759aae99896215b92fe8da596","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":"2026-07-31T22:46:39.586165Z","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":"2026-08-14T06:32:32.682623+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/2607.24141/citation-record","integrity":"/paper/2607.24141/integrity","json":"/paper/2607.24141/citation-record.json","paper":"/paper/2607.24141"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-31T22:46:38.087710Z","title":"S., Aguilar, G., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.087710Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:7ccc8ddba12972cef767be6de322bb68869768f189c73121edfb3654b48ce062","observation_id":"b5ad25e8-e3d0-4fb1-a051-742295295416","resolution":{"observed_at":"2026-07-31T22:46:38.087710Z","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":"2026-07-31T22:46:38.141507Z","title":"2023, FERRE: Match physical models to measurements, Astrophysics Source Code Library, record ascl:2301.016","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.141507Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:19503a2546304f6e5f6dd2d723806502bbac0dcaba0305c1bd2ca9dfef00633b","observation_id":"c40ae398-0eb5-4b3b-8c2c-a107e690117d","resolution":{"observed_at":"2026-07-31T22:46:38.141507Z","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":"2026-07-31T22:46:38.198391Z","title":"M., Nissen, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.198391Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:b07248387921af4d7ad25c6c949845e64b26cdb6d1abec65e31c26c7696c4083","observation_id":"74c0de12-aba2-44ec-9fd5-0b1d6cc150cd","resolution":{"observed_at":"2026-07-31T22:46:38.198391Z","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":"2026-07-31T22:46:38.356711Z","title":"2005, ARA&A, 43, 481, doi: 10.1146/annurev.astro.42.053102.134001","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.356711Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:1499e01bc4822496b677aa365bd45a6f4b425d9bd47da5acaa32f1e3f1cc5239","observation_id":"1ec89b32-66b7-4326-acd0-74f61c9d5cf2","resolution":{"observed_at":"2026-07-31T22:46:38.356711Z","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":"2026-07-31T22:46:38.464660Z","title":"S., & Collet, R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.464660Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:36bd9618e9bc57623f25c5895761a60b0af704ade347f3cf00bc06c15efb3eae","observation_id":"72062a57-a5d8-41b3-b9c6-e0cc02bda1c5","resolution":{"observed_at":"2026-07-31T22:46:38.464660Z","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":"2026-07-31T22:46:38.615135Z","title":"S., Piskunov, N., & O’Mara, B","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.615135Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:0751ee85965fe9db3bad0db8f69982b4c336ca569d96e91044299a2975b45930","observation_id":"470528c6-2f98-4fa5-8226-2d7478d340ee","resolution":{"observed_at":"2026-07-31T22:46:38.615135Z","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":"2026-07-31T22:46:38.674696Z","title":"2014, in Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars, ed","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.674696Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:cde49b144ff85c173a5aa3510751fee07482b53306e48153dca081fe1f0a23ff","observation_id":"b0286a46-55c8-468e-832b-53f1e12bf88c","resolution":{"observed_at":"2026-07-31T22:46:38.674696Z","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":"2026-07-31T22:46:38.784561Z","title":"2014, A&A, 569, A111, doi: 10.1051/0004-6361/201423945 B¨ ohm-Vitense, E","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.784561Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:fc620d02b68281b7c0a49b003e5f28118afd8f40e505c0f9957a2d9aff4ade52","observation_id":"d42d0c92-a1b4-4ec7-ab4f-02c22285e7a5","resolution":{"observed_at":"2026-07-31T22:46:38.784561Z","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":"2026-07-31T22:46:38.844415Z","title":"A., Conroy, C., Johnson, B","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.844415Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:559f31430ab371f4956ad1ddeb6bb5b194535610d40b44f509201c6dce4cb1d8","observation_id":"81ab1f6c-f1e0-46eb-a9fd-e1e145d13874","resolution":{"observed_at":"2026-07-31T22:46:38.844415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.03040","last_updated":"2016-03-09T21:00:02Z","snapshot_observed_at":"2026-07-06T04:48:56.846004Z","submitted_at":"2016-03-09T21:00:02Z","title":"The Cannon 2: A data-driven model of stellar spectra for detailed chemical abundance analyses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.03040","snapshot_observed_at":"2026-07-31T22:46:38.952409Z","title":"R., Hogg, D","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:38.952409Z"},"links":{"cited_paper":"/paper/1603.03040","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:f44fee0845f709737601c68f1e590cafae07c4d08ca83ae9bfacbf3951e1cbf8","observation_id":"211a145f-5a9a-44cf-a918-86278bbc7f24","resolution":{"observed_at":"2026-07-31T22:46:38.952409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405087","last_updated":"2004-05-05T15:30:48Z","snapshot_observed_at":"2026-07-07T00:42:19.442022Z","submitted_at":"2004-05-05T15:30:48Z","title":"New Grids of ATLAS9 Model Atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405087","snapshot_observed_at":"2026-07-31T22:46:39.014583Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.014583Z"},"links":{"cited_paper":"/paper/astro-ph/0405087","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:a608ffc428275f42792b2a76a152f011ac064ca00c35292dac6cb6b8ff4fdc1e","observation_id":"8242e760-d011-4e0e-8229-9de20cf801e4","resolution":{"observed_at":"2026-07-31T22:46:39.014583Z","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":"2026-07-31T22:46:39.115776Z","title":"2010, A&A, 522, A10, doi: 10.1051/0004-6361/201014432","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.115776Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:aaa4c0b9b2830540f0ea2ee49f601cc003afe46103afed3e3838d5493679603f","observation_id":"71bb8c61-75c6-4ec4-a70a-7865b1f096d5","resolution":{"observed_at":"2026-07-31T22:46:39.115776Z","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":"2026-07-31T22:46:39.224350Z","title":"2019, The Messenger, 175, 30, doi: 10.18727/0722-6691/5122","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.224350Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:55f810bd85508f9168d267171dfe0efc7d42f2e30037a4b0439ced5be6c5ee20","observation_id":"e8afc1d0-a805-4f48-aa2e-15f239dc87de","resolution":{"observed_at":"2026-07-31T22:46:39.224350Z","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":"2026-07-31T22:46:39.243421Z","title":"P., Koposov, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.243421Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:c2f49c0ac7fd577dbbcd805204e890be029b813117fdd1f9a8efa8700f7809ef","observation_id":"e79d2bcb-21b2-4824-85b2-5ce4a7c1ffc6","resolution":{"observed_at":"2026-07-31T22:46:39.243421Z","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":"2026-07-31T22:46:39.292535Z","title":"L., Sordo, R., Pailler, F., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.292535Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:93fc15db044daee94c985445c5dede4dc1a216a502ba0b99fef091feebf4c249","observation_id":"299ffe83-d34f-4bbf-bb3f-be71dee3777e","resolution":{"observed_at":"2026-07-31T22:46:39.292535Z","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":"2026-07-31T22:46:39.296622Z","title":"2012, Research in Astronomy and Astrophysics, 12, 1197, doi: 10.1088/1674-4527/12/9/003","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.296622Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:c203d3361434bd3e593a6463591fb0fa0e3cf240611d139a20acc3416e9aa9e6","observation_id":"b0544214-0541-4bba-9b40-02a7992bd802","resolution":{"observed_at":"2026-07-31T22:46:39.296622Z","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":"2026-07-31T22:46:39.300807Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.300807Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:7ae949f65b657ffa4c81a6c6245ce97a9b7ee01c4f4ca64efe495bc7b64a3435","observation_id":"b129167d-f21d-46f9-a1fc-5fa2fe04098c","resolution":{"observed_at":"2026-07-31T22:46:39.300807Z","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":"2026-07-31T22:46:39.304964Z","title":"C., Abrams, D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.304964Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:35decf2dc5172f101744b3a25a3a02ef4f7e6e01c7bbe37cd7bb489e9528b88c","observation_id":"b473d34c-4eb2-4a6d-a55a-867145baece7","resolution":{"observed_at":"2026-07-31T22:46:39.304964Z","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":"2026-07-31T22:46:39.308906Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.308906Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:2ce638f33a6d1179631eac589d87d3672bbd2d0439f8325e4129e0d521378b85","observation_id":"01b44ce1-0904-4000-9658-aa3d8c480e6d","resolution":{"observed_at":"2026-07-31T22:46:39.308906Z","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":"2026-07-31T22:46:39.312848Z","title":"A., O’Briain, T., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.312848Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:b16008619cc7c509ea5e44c9cd0d40d729f97951b00771ee2b3a95156d49284a","observation_id":"239e2d37-8de5-4a78-b8f8-21feb4bdd651","resolution":{"observed_at":"2026-07-31T22:46:39.312848Z","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":"2026-07-31T22:46:39.316999Z","title":"1961, Physical Review, 124, 1866, doi: 10.1103/PhysRev.124.1866 Garc ´ ıa P´ erez, A","venue":null,"work_id":null,"year":1961},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.316999Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:183d4ed3649af36344da4adf8d3bf5947401e581d9b8f73cdda9a480e5fd57c6","observation_id":"9b28325d-4606-4fd0-a423-7bd63f3c21c4","resolution":{"observed_at":"2026-07-31T22:46:39.316999Z","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":"2026-07-31T22:46:39.321159Z","title":"2012, The Messenger, 147, 25","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.321159Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:0ca0b7651ae4fab064e186129578d2ad3ab9c87c905c6dd06e0cd0412e42893b","observation_id":"53234b90-c071-434a-bac2-5b869c699137","resolution":{"observed_at":"2026-07-31T22:46:39.321159Z","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":"2026-07-31T22:46:39.325109Z","title":"2003, Inverse Problems, 19, R1, doi: 10.1088/0266-5611/19/2/201","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.325109Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:2194beef7fbfeac56427d0fd7c17c84724bf1919b98fe23fd64c3ddd4b712fb4","observation_id":"9e2d11f5-58d4-460f-80e2-17ab33ea2edc","resolution":{"observed_at":"2026-07-31T22:46:39.325109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.05767","last_updated":"2018-02-05T15:57:57Z","snapshot_observed_at":"2026-08-12T08:12:58.520310Z","submitted_at":"2015-02-20T04:20:47Z","title":"Automatic differentiation in machine learning: a survey","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.05767","snapshot_observed_at":"2026-07-31T22:46:39.329039Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.329039Z"},"links":{"cited_paper":"/paper/1502.05767","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:065fa712235b21082af104c33781913d98d33ed4767a99466b5dfc6be678533f","observation_id":"d5f11fb8-4daa-4693-b631-3206124e2862","resolution":{"observed_at":"2026-07-31T22:46:39.329039Z","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":"2026-07-31T22:46:39.334022Z","title":"2008, A&A, 486, 951, doi: 10.1051/0004-6361:200809724","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.334022Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:a59ac5b4d9fdfdfe7fbd74b906808bfc033a715ae6a025d470c9d6ab5de8da8c","observation_id":"f81e773b-2b33-4fbb-80c3-448175f2eda7","resolution":{"observed_at":"2026-07-31T22:46:39.334022Z","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":"2026-07-31T22:46:39.340077Z","title":"R., Bovy, J., Holtzman, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.340077Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:32c7585b5005ca254c57a11d592e553e2056fe1b731455c5894be997e2cbc1a7","observation_id":"75ded6ba-b739-44a3-a61e-a72a8193703f","resolution":{"observed_at":"2026-07-31T22:46:39.340077Z","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":"2026-07-31T22:46:39.344166Z","title":"2015, A&A, 582, A49, doi: 10.1051/0004-6361/201526319","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.344166Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:d4e84d7080db71a76886ead5312d25f6ad859e40048d927b0c70d2c74f84c184","observation_id":"f4fbcb37-4618-4ca6-9ffb-76dde6b48ab0","resolution":{"observed_at":"2026-07-31T22:46:39.344166Z","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":"2026-07-31T22:46:39.348457Z","title":"2021, A&A, 645, A106, doi: 10.1051/0004-6361/201936291","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.348457Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:1c0c21281a72b55c2c9790a97e73108c3e7206a0cbabb033d376a5bdd680a974","observation_id":"9491b296-2bab-4e12-9f26-004e2f6f70d3","resolution":{"observed_at":"2026-07-31T22:46:39.348457Z","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":"2026-07-31T22:46:39.352463Z","title":"1995, PASP, 107, 1042, doi: 10.1086/133660","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.352463Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:ea9f689c0406ccc2f054f171cfa17472d50e88b801a32843ed68959ef178bf66","observation_id":"15d33627-8f79-48ed-a94e-bcc118ef9647","resolution":{"observed_at":"2026-07-31T22:46:39.352463Z","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":"2026-07-31T22:46:39.356569Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.356569Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:2cf355ceb28b8bc65c29e8b33810bb42abc5bc1cc6bf0a571ec635e5ef60bab9","observation_id":"e1d5fd28-0134-4bb2-8447-67fdde1388e0","resolution":{"observed_at":"2026-07-31T22:46:39.356569Z","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":"2026-07-31T22:46:39.360688Z","title":"A., Hasselquist, S., Shetrone, M., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.360688Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:a7b7fd4859c5864f010ae7ee515577e451220c9ae5f256efd73a04220c91f6b2","observation_id":"8c57ae47-15ce-41f0-a0a0-081ef9ddeb7e","resolution":{"observed_at":"2026-07-31T22:46:39.360688Z","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":"2026-07-31T22:46:39.364999Z","title":"1995, ApJ, 439, 875, doi: 10.1086/175226","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.364999Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:5ce1f8fa2bcf0c8041230a9d628ffccd3a7d652938b789171490d282035c09f3","observation_id":"d966c516-c378-4d5d-86f2-c088a4bd9d5a","resolution":{"observed_at":"2026-07-31T22:46:39.364999Z","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":"2026-07-31T22:46:39.369108Z","title":"2014, Theory of Stellar Atmospheres","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.369108Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:e5e14ba7ecae8d519f997f3020fcd62127db381de8c38d807c351d4e2be1ef70","observation_id":"89cff483-b2cb-4d5a-b35b-d324668a67e1","resolution":{"observed_at":"2026-07-31T22:46:39.369108Z","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":"2026-07-31T22:46:39.373141Z","title":"G., & Mihalas, D","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.373141Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:5c6b3b0fb399436684d0f9657d73f7950b9ebbec85d3b18857475915738818a8","observation_id":"bbec6570-d163-45d0-a68a-6e52ae2a114b","resolution":{"observed_at":"2026-07-31T22:46:39.373141Z","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":"2026-07-31T22:46:39.377476Z","title":"2013, A&A, 553, A6, doi: 10.1051/0004-6361/201219058 Jofr´ e, P., Heiter, U., Soubiran, C., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.377476Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:8857ea28b431950dbc3b08aff90f45f6270d7ec8a57cd9714a72578242076a6f","observation_id":"19880cf3-4edd-4f0a-b58e-adb9131f163b","resolution":{"observed_at":"2026-07-31T22:46:39.377476Z","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":"2026-07-31T22:46:39.381707Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.381707Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:af8b4b7c72709cf8aee7ec981c10c56a905f8fdb6dd32b202ee414fd6c98ab46","observation_id":"86032df3-107a-4b26-954f-ed10041516f5","resolution":{"observed_at":"2026-07-31T22:46:39.381707Z","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":"10.1086/154371","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"R., & Krupp, B","venue":"The Astrophysical Journal","work_id":"ddbeaf3b-3bc6-4e19-9ddf-b43e25109112","year":1976},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.385565Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:7925909ed26c8427042d06ed566eb61454962b44e03c955c83953e3426e43b35","observation_id":"1bc5d33f-cca3-4ad0-ba31-52b2d4c6b286","resolution":{"observed_at":"2026-07-31T22:51:00.867248Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-07-31T22:46:39.389615Z","title":"T., & Cadima, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.389615Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:8994760de4e76842d72e5af5723999e6526bafcbd4611583a6cc78bf2f026353","observation_id":"d4d9e837-27f3-433f-a74c-b67212f18dbf","resolution":{"observed_at":"2026-07-31T22:46:39.389615Z","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":"2026-07-31T22:46:39.393763Z","title":"2022, ApJS, 258, 31, doi: 10.3847/1538-4365/ac3b4d","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.393763Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:d6a5a7bee577aa7a034ff5fde731447336a30ea4eebc1b950a0d517badcd0d85","observation_id":"c4ba2e33-d9ae-4b66-8905-2fd9af93922f","resolution":{"observed_at":"2026-07-31T22:46:39.393763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.11693","last_updated":"2026-05-22T07:35:53Z","snapshot_observed_at":"2026-07-06T22:48:48.873215Z","submitted_at":"2026-03-12T09:01:36Z","title":"pyKurucz: A Pure Python Reimplementation of Kurucz ATLAS12 and SYNTHE for Stellar Spectrum Synthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.11693","snapshot_observed_at":"2026-07-31T22:46:39.397950Z","title":"M., & Ting, Y.-S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.397950Z"},"links":{"cited_paper":"/paper/2603.11693","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:5b605f40145e47ad20c79569536ffe9ff81a9ca5ad3db9116b2e39a9c2083982","observation_id":"11143187-a95c-4f72-b3e7-2ffd5443a87d","resolution":{"observed_at":"2026-07-31T22:46:39.397950Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03234","last_updated":"2017-11-09T02:24:05Z","snapshot_observed_at":"2026-08-03T19:17:05.110670Z","submitted_at":"2017-11-09T02:24:05Z","title":"SDSS-V: Pioneering Panoptic Spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03234","snapshot_observed_at":"2026-07-31T22:46:39.402290Z","title":"A., Zasowski, G., Rix, H.-W., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.402290Z"},"links":{"cited_paper":"/paper/1711.03234","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:6981cb2ddafcfaea1c486b153c171df13f8e67a7f372b8b68e0ddd747a7b3437","observation_id":"b7bbbc19-9853-424e-b763-1be1b7e49506","resolution":{"observed_at":"2026-07-31T22:46:39.402290Z","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":"2026-07-31T22:46:39.406721Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.406721Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:9f4ecacdb099936016b9e02f74c4c835138739e9662ba1de68e001d74f4c22d0","observation_id":"a474d424-d7ec-4fd4-9767-860ae020251c","resolution":{"observed_at":"2026-07-31T22:46:39.406721Z","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":"2026-07-31T22:46:39.410758Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.410758Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:252f0dd46893ca44cace3cc3b7eb05ef3dd9e40b054466f47f9413fdbd22d001","observation_id":"272cb975-0ee4-4df7-8aa9-01cb6e54b7e7","resolution":{"observed_at":"2026-07-31T22:46:39.410758Z","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":"2026-07-31T22:46:39.415194Z","title":"L., & Avrett, E","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.415194Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:8f527991cd21ccbb771f595d420a3d7cb6c3ea524a0778afa0b2059c2dd021f3","observation_id":"d9352afe-4cb1-45fa-81a1-134c4582aa7f","resolution":{"observed_at":"2026-07-31T22:46:39.415194Z","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":"2026-07-31T22:46:39.419362Z","title":"2003, ApJS, 146, 417, doi: 10.1086/374373 —","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.419362Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:07b9eb53cad408f0e1d5726fe1dc9b7b5c2e1ca68b4de49fc2937b9ad73dd98a","observation_id":"7ed16705-58bf-4c4c-920c-41ad95a3b3c0","resolution":{"observed_at":"2026-07-31T22:46:39.419362Z","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":"10.1051/0004-6361/201833553","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2019, A&A, 624, A60, doi: 10.1051/0004-6361/201833553","venue":"Astronomy and Astrophysics","work_id":"24f92a2b-d225-43e6-8c74-fd18783482cd","year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.423363Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:9973aa9fc472f29a04174beb7a09a9c6a504470cb5422018b6dcdb0e2e2d450a","observation_id":"b73489d6-4aa2-472e-bf64-e0dddd71dffa","resolution":{"observed_at":"2026-07-31T22:51:00.519101Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-07-31T22:46:39.427405Z","title":"W., & Bovy, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.427405Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:8b042dc2d930d544f5f011623cfdc55caf72c96fd5e8868a7fb1f94be7b2f8ea","observation_id":"f0894756-4534-499d-b24c-4883983cf91b","resolution":{"observed_at":"2026-07-31T22:46:39.427405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.06357","last_updated":"2025-07-08T19:39:07Z","snapshot_observed_at":"2026-08-13T23:42:08.244749Z","submitted_at":"2025-07-08T19:39:07Z","title":"Differentiable Stellar Atmospheres with Physics-Informed Neural Networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.06357","snapshot_observed_at":"2026-07-31T22:46:39.431263Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.431263Z"},"links":{"cited_paper":"/paper/2507.06357","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:571273b44ebf249884693f5d097d8cd98ff021ea7c91173dcc100496396e4fdf","observation_id":"cf65f3e6-def5-4a2c-b00b-46e4c0ecbe4f","resolution":{"observed_at":"2026-07-31T22:46:39.431263Z","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":"2026-07-31T22:46:39.435626Z","title":"1991, An atlas of the solar spectrum in the infrared from 1850 to 9000 cm-1 (1.1 to 5.4 micrometer)","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.435626Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:a00567e2c6706e675510d4d1b3a63e4027579f9a4aa31141bc056e48a5e9f9be","observation_id":"3fe09264-1518-4997-8f7f-c728939f686b","resolution":{"observed_at":"2026-07-31T22:46:39.435626Z","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":"10.1139/p11-030","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2011, Canadian Journal of Physics, 89, 395, doi: 10.1139/p11-030","venue":"Canadian Journal of Physics","work_id":"aac01873-b3bb-43c9-827f-8b94949a911c","year":2011},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.439725Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:e0e927527bcf0a097e014899469dd21012a6af5cd930a8c4fa519b478d917d46","observation_id":"0ec879bf-6823-4188-bb66-d0c6828fe1f1","resolution":{"observed_at":"2026-07-31T22:51:00.321616Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-07-31T22:46:39.443884Z","title":"2013, A&A, 557, A26, doi: 10.1051/0004-6361/201321274","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.443884Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:e2c78a64c1a45d73edc179beddbe4e2767a94f7c12380f5f35345875ce3d93bc","observation_id":"2af9074d-27ac-4c9b-9c33-d10306d76918","resolution":{"observed_at":"2026-07-31T22:46:39.443884Z","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":"2026-07-31T22:46:39.448264Z","title":"R., Schiavon, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.448264Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:1b57e51b557c3d9369245aac151c8bc3d43c0043160b406b524e469f45c2b7e1","observation_id":"b9a6dd60-7e03-45da-a449-0959516a5f01","resolution":{"observed_at":"2026-07-31T22:46:39.448264Z","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":"2026-07-31T22:46:39.452628Z","title":"2016, MNRAS, 456, 3655, doi: 10.1093/mnras/stv2830","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.452628Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:b0b10e8385cc15415bc895496827055a0f0cd0be1c36e3783011289d775db156","observation_id":"9ffeffe3-3ee5-4099-9032-4dfd00479c2f","resolution":{"observed_at":"2026-07-31T22:46:39.452628Z","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":"2026-07-31T22:46:39.456872Z","title":"2015, MNRAS, 453, 1855, doi: 10.1093/mnras/stv1731","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.456872Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:5a7bc68e51b31fdce249b78e0a2cba5874abbb649472dc17ab62141b16d85564","observation_id":"55a6f405-4c74-4942-a940-79ba1c61273d","resolution":{"observed_at":"2026-07-31T22:46:39.456872Z","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":"2026-07-31T22:46:39.461151Z","title":"M., Carlos, M., & Nissen, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.461151Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:37c605c26eccdfd892343890a33c78a8448915c79b4425b0ed56e0b41c6e628b","observation_id":"6800d40b-b186-4790-8bdf-8bbaebe9a90d","resolution":{"observed_at":"2026-07-31T22:46:39.461151Z","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":"2026-07-31T22:46:39.465578Z","title":"D., Beckman, R","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.465578Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:0e909defa5cdfd9fddc09c656a3210fb85b0248e683424ccabe8edb3be9079a9","observation_id":"212aaf49-d527-437a-bdd9-12a692c58438","resolution":{"observed_at":"2026-07-31T22:46:39.465578Z","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":"2026-07-31T22:46:39.470006Z","title":"1978, Stellar atmospheres","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.470006Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:897a4fd640560e5827067176967ae7fd88ee211cd929533ff8890e799a3ace60","observation_id":"d527f665-94bd-4c45-b169-c80904190152","resolution":{"observed_at":"2026-07-31T22:46:39.470006Z","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":"2026-07-31T22:46:39.474576Z","title":"2015, ApJ, 808, 16, doi: 10.1088/0004-637X/808/1/16","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.474576Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:94a0d2e4dbb7bc91169e7b787a8dfd993195ffa547d3b4b442ff421fcd99ebbe","observation_id":"82604da8-33e2-42a4-a6e8-ebfbb71828c5","resolution":{"observed_at":"2026-07-31T22:46:39.474576Z","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":"2026-07-31T22:46:39.478580Z","title":"L., Bovy, J., Bird, J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.478580Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:ffe66d5143c5bf6e3b86a7149754b834b96a2105fbad84a87bd397f8b8f0eae7","observation_id":"8cb0df11-04a9-4e3d-bde9-439f25267597","resolution":{"observed_at":"2026-07-31T22:46:39.478580Z","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":"2026-07-31T22:46:39.482775Z","title":"L., Holtzman, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.482775Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:50ae9912a39605277780ad029b24811f26ed6574743887457e1ccabdf9db3853","observation_id":"748cba97-74d3-42c1-98e0-3530af191292","resolution":{"observed_at":"2026-07-31T22:46:39.482775Z","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":"2026-07-31T22:46:39.486646Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.486646Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:5e07b4ede6898cfab88d1d19c9a3289bee9b2710a62ef5c8d4d33e2c8650a195","observation_id":"c0e974ae-fd55-42a2-a301-7541c295af66","resolution":{"observed_at":"2026-07-31T22:46:39.486646Z","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":"2026-07-31T22:46:39.490652Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.490652Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:691a293dd7482165a9022a4b1844874e82e0cef34c8dc3aef3770d6dda7b4165","observation_id":"190cd869-ab96-4442-94b7-6013932a32db","resolution":{"observed_at":"2026-07-31T22:46:39.490652Z","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":"2026-07-31T22:46:39.494918Z","title":"E., Kupka, F., Ryabchikova, T","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.494918Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:f3a4bdb958206cc5aa8e8b88b9b10f81d3ca3b9fa1aa3e1488e64979c305ae78","observation_id":"96c58e80-b865-4fe3-8b77-f2ad11a85173","resolution":{"observed_at":"2026-07-31T22:46:39.494918Z","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":"2026-07-31T22:46:39.498892Z","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":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.498892Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:d6a8c1eceffe1279b92fc2984f8fe5fa47680fa631b176c59f3a4dac0a6eaec1","observation_id":"43a55eea-e2b9-4795-aa8d-060132191aa3","resolution":{"observed_at":"2026-07-31T22:46:39.498892Z","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":"2026-07-31T22:46:39.503134Z","title":"L., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.503134Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:756091aa1317dc0db921cc8e529ee6a8c2a996ae4afa7d303dd6b9de6bd9ec00","observation_id":"c206412e-dd32-4c52-a647-9c534fd71fdb","resolution":{"observed_at":"2026-07-31T22:46:39.503134Z","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":"2026-07-31T22:46:39.507428Z","title":"M., & Cassisi, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.507428Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:1f4e3c82170af9c2ea287e6dde244e5f44b41247258c24de559e8fea128738c7","observation_id":"c6d6372b-3422-4c1e-a0dc-e249e5cdd5fe","resolution":{"observed_at":"2026-07-31T22:46:39.507428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0067-0049/221/2/24","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., et al","venue":"The Astrophysical Journal Supplement Series","work_id":"1125a018-8c24-4e60-b081-937ab092c779","year":2015},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.511391Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:a70baf4f30db01d123a6eb236279d74c691ddbbfaee132bf5540e59e638ece70","observation_id":"34327c70-3610-4b29-8b22-b2f2bebde3c2","resolution":{"observed_at":"2026-07-31T22:51:00.109049Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-03T18:08:20.464951+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T18:08:20.464951+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/revmodphys.39.439","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Reviews of Modern Physics","work_id":"2a56507e-c3d5-4aad-b6a2-ffd0cd4ecdd7","year":1967},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.515978Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:53169110969d634737d254b89ff84ac6225ac57709e53920e733f0f277736f30","observation_id":"c2f42b56-da79-4a9d-8a13-671f854e0905","resolution":{"observed_at":"2026-07-31T22:50:59.995318Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-07-31T22:46:39.520026Z","title":"V., Bizyaev, D., Cunha, K., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.520026Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:26c6abd2e486895dbee62e4bd6f1575de2f8a81bc8046bb8d4df2faf4da4a07c","observation_id":"63bf26c1-6f85-4643-92d8-00f6b7bed3f1","resolution":{"observed_at":"2026-07-31T22:46:39.520026Z","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":"2026-07-31T22:46:39.524079Z","title":"2012, MOOG: LTE line analysis and spectrum synthesis, Astrophysics Source Code Library, record ascl:1202.009","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.524079Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:985b16877097cb200c2070c85649efcfdee97ffc7282233cb9769c5ce9431c5f","observation_id":"830202bb-1c7d-45d1-9493-24839aedc141","resolution":{"observed_at":"2026-07-31T22:46:39.524079Z","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":"2026-07-31T22:46:39.528044Z","title":"S., Kraft, R","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.528044Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:f9e34e1eebb7651e0e834f09a64c1824cea2afc00c39d5c8c37c8acd7924c67f","observation_id":"5f698b07-4f2c-4029-b109-8de2a5a9e435","resolution":{"observed_at":"2026-07-31T22:46:39.528044Z","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":"2026-07-31T22:46:39.531999Z","title":"S., Chiba, M., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.531999Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:11ebedf1346f19e10e8c9ca30a15f0f44e74607bb025530faac9d341bad80ddf","observation_id":"9dd52b14-4fc6-4cf7-b949-55282fe67286","resolution":{"observed_at":"2026-07-31T22:46:39.531999Z","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":"10.3847/0004-637x/826/1/83","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2016, ApJ, 826, 83, doi: 10.3847/0004-637X/826/1/83","venue":"The Astrophysical Journal","work_id":"d6737806-4b73-4ae2-a8af-50db046588c6","year":2016},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.536199Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:2e9bb90c8f1cf0abab9fd6ccf7ee7cf0abde84520e6fbf1bc5a9131ba6297987","observation_id":"43e4f7cf-f78e-496f-a590-4fd5c0b4f148","resolution":{"observed_at":"2026-07-31T22:50:59.869602Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-03T18:08:18.217778+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T18:08:18.217778+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-07-31T22:46:39.540344Z","title":"2018, ApJ, 860, 159, doi: 10.3847/1538-4357/aac6c9","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.540344Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:de046769ecac95951318981d62eddd6f1ec7f595e139f8ed8d0aa895fe624b83","observation_id":"6dc3cb0d-3255-45bc-a2ca-4002dc28c9a9","resolution":{"observed_at":"2026-07-31T22:46:39.540344Z","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":"2026-07-31T22:46:39.544376Z","title":"2017a, ApJ, 843, 32, doi: 10.3847/1538-4357/aa7688 —","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.544376Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:74171ee73522e8bc71759b28338be599c71f9f150b97df47061355139cfaa215","observation_id":"958395b7-a74e-46b2-9f27-f8c756646853","resolution":{"observed_at":"2026-07-31T22:46:39.544376Z","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":"2026-07-31T22:46:39.548688Z","title":null,"venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.548688Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:d0bd607c487c9572457a3ea0cbeafab261ba13b0f558c3d9cbabe6ec14cda6f0","observation_id":"886f7a1c-6b8f-48b1-8e0b-5fc2b56eb75e","resolution":{"observed_at":"2026-07-31T22:46:39.548688Z","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":"2026-07-31T22:46:39.552777Z","title":"A., & Fischer, D","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.552777Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:883b9f7953e288c2f460455293d8ccfc71ffd72a082b963851d9387e9a912019","observation_id":"27d7e24b-f399-4cff-b610-cfca581637e5","resolution":{"observed_at":"2026-07-31T22:46:39.552777Z","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":"2026-07-31T22:46:39.556804Z","title":"A., & Piskunov, N","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.556804Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:d319172c7e667d7f4dd6e656c5639a7b52b5f187b28219c0d6078ec43e1f5612","observation_id":"54f26ecd-f4eb-4dfb-9b66-15699337fb48","resolution":{"observed_at":"2026-07-31T22:46:39.556804Z","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":"2026-07-31T22:46:39.560708Z","title":"R., Cooper, J., & Smith, E","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.560708Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:8d59261dc7824c37e0e0c7dc96cf2dc897eb4f221929f19b3c39f2d4b9b4d599","observation_id":"18a053f0-dc6d-4835-84cc-210d088b97d6","resolution":{"observed_at":"2026-07-31T22:46:39.560708Z","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":"2026-07-31T22:46:39.564931Z","title":"2023, A&A, 671, A171, doi: 10.1051/0004-6361/202244482","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.564931Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:861f512a2e25434ca78d2a277683bdce1613e275c4865dda17b42d17f15ce65f","observation_id":"7da65f73-2650-4b79-be53-243e0287ce57","resolution":{"observed_at":"2026-07-31T22:46:39.564931Z","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":"2026-07-31T22:46:39.569196Z","title":"H., Holtzman, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.569196Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:4b29e3f2afa7b9cc7ca168fa1fca6163409f3e3f2a0ab615b4e937474930992e","observation_id":"8140696a-f7fe-4417-8bf4-8b0184f10598","resolution":{"observed_at":"2026-07-31T22:46:39.569196Z","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":"2026-07-31T22:46:39.573570Z","title":"J., Abruzzo, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.573570Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:08e19ebe8bbd7ec6ec03b9e87abb9dc5011ad8ea34e605c4256eb64e47a6f09e","observation_id":"bb378d5d-9e22-4b01-9163-7d0444365414","resolution":{"observed_at":"2026-07-31T22:46:39.573570Z","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":"2026-07-31T22:46:39.577606Z","title":"C., Hearty, F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.577606Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:57dfb3393b7be444541689e72c0e2461fd5a3aa2246fa9ce75cf1e623ee6fed4","observation_id":"52745ee6-e8e5-4302-9cc9-f2ce3a89c1f1","resolution":{"observed_at":"2026-07-31T22:46:39.577606Z","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":"2026-07-31T22:46:39.581954Z","title":"2019, ApJS, 245, 34, doi: 10.3847/1538-4365/ab5364","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.581954Z"},"links":{"citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:b3be528b14b113add4e2cc40d21d547aaf51565786c140298274d5cf554116a8","observation_id":"8fa41c32-b7d9-457a-993b-4be10eda5b52","resolution":{"observed_at":"2026-07-31T22:46:39.581954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.06114","last_updated":"2018-04-14T18:54:19Z","snapshot_observed_at":"2026-08-01T07:33:14.644852Z","submitted_at":"2017-03-10T21:02:53Z","title":"Deep Sets","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.06114","snapshot_observed_at":"2026-07-31T22:46:39.586165Z","title":"2017, arXiv e-prints, arXiv:1703.06114, doi: 10.48550/arXiv.1703.06114","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-31T22:46:39.586165Z"},"links":{"cited_paper":"/paper/1703.06114","citing_paper":"/paper/2607.24141"},"observation_digest":"sha256:0d938abdb000814e763fdc57e0bc33d51ab7b44e2594d3e5aef0ca376ceebe7f","observation_id":"a9fe4520-9bff-4726-a288-04968aa6f6ce","resolution":{"observed_at":"2026-07-31T22:46:39.586165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.24141","last_updated":"2026-07-27T08:21:12Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-08T01:45:53.652455Z","submitted_at":"2026-07-27T08:21:12Z","title":"The Payne Zero Project I: Stellar Spectra from Physical Models in Seconds"},"reference_resolution":{"displayed":85,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":79,"verified_exact":6,"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 85 of 85 outbound references and 0 inbound Pith citation observations for arXiv:2607.24141."}