{"as_of":"2026-08-15T07:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c0a70b5dc06c9e058077a45e29d361d1f475a9f1ed76999892f03b9d5fc68ed5","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:17:46.970441Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":2,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":"2407.00157","doi":"10.48550/arxiv.2407.00157","metadata_source":"arxiv_reference","pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Sanders, R","venue":"arXiv (Cornell University)","work_id":"7f890086-ce7c-46a8-abfa-288f814ce6e1","year":2025},"citing_paper":{"arxiv_id":"2408.05273","last_updated":"2026-05-19T17:44:20Z","snapshot_observed_at":"2026-08-14T03:05:03.806165Z","submitted_at":"2024-08-09T18:00:03Z","title":"The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-23T21:50:56.848831Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2408.05273"},"observation_digest":"sha256:9101adaefbfc15379f2181523c7a95854b82492a302316b444a4604dd4861296","observation_id":"6aa61c9c-7ba3-41dc-920f-8783814ee959","resolution":{"observed_at":"2026-05-23T21:53:29.797666Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-12T20:57:50.837512Z","title":"E., Sanders, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09262","last_updated":"2025-02-18T09:55:41Z","snapshot_observed_at":"2026-08-14T22:42:59.991458Z","submitted_at":"2024-11-14T08:00:48Z","title":"On the Average Ultraviolet Emission Line Spectra of High-Redshift Galaxies: Hot and Cold, Carbon-poor, Nitrogen-modest, and Oozing Ionizing Photons","version":2},"reference_index":127,"source":"pdf_text","source_observed_at":"2026-08-12T20:57:50.837512Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2411.09262"},"observation_digest":"sha256:eaa17a0316dcb77c3fd9ac8935b4c30c886b9376662548209d7c57b03bd83000","observation_id":"dfed21f2-51e5-47a7-bf56-bc6ea784a848","resolution":{"observed_at":"2026-08-12T20:57:50.837512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-12T18:09:32.415468Z","title":"E., et al., 2024, arXiv e-prints, https://ui.adsabs.harvard.edu/abs/2024arXiv240700157S p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.11837","last_updated":"2025-01-22T16:26:06Z","snapshot_observed_at":"2026-08-14T04:50:09.740154Z","submitted_at":"2024-11-18T18:55:24Z","title":"The JWST EXCELS survey: tracing the chemical enrichment pathways of high-redshift star-forming galaxies with O, Ar and Ne abundances","version":3},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-12T18:09:32.415468Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2411.11837"},"observation_digest":"sha256:8709b312780a278f5d56e3ea9c899911013d23813b8b2b38e7e1631c7923d829","observation_id":"099cce8e-fad0-43aa-a29f-32db6932ba55","resolution":{"observed_at":"2026-08-12T18:09:32.415468Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-11T17:57:26.789402Z","title":"E., Sanders, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08382","last_updated":"2024-12-11T13:47:13Z","snapshot_observed_at":"2026-08-13T13:09:31.382826Z","submitted_at":"2024-12-11T13:47:13Z","title":"Early Results from GLASS-JWST. XXV. Electron Density in the Interstellar Medium at $0.7\\lesssim z\\lesssim 9.3$ with NIRSpec High-resolution Spectroscopy","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T17:57:26.789402Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2412.08382"},"observation_digest":"sha256:0a03786f97cf7351b07c283862e16eca8afafdb7850523cea148a0cb2bd2d1da","observation_id":"50b75ae6-e571-4d3c-a720-a8a4b7861cef","resolution":{"observed_at":"2026-08-11T17:57:26.789402Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-11T15:55:41.225384Z","title":"E., et al., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2407.00157 , https://ui.adsabs.harvard.edu/abs/2024arXiv240700157S p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.10557","last_updated":"2025-05-22T16:21:19Z","snapshot_observed_at":"2026-08-15T00:50:39.758066Z","submitted_at":"2024-12-13T21:02:27Z","title":"The JWST EXCELS survey: direct estimates of C, N, and O abundances in two relatively metal-rich galaxies at $\\mathbf{z\\simeq5}$","version":2},"reference_index":107,"source":"arxiv_source","source_observed_at":"2026-08-11T15:55:41.225384Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2412.10557"},"observation_digest":"sha256:14ec7fed8b2c9cdc9cc142fe1d87dac3e21769942f7b6454d0f65e8510bd3712","observation_id":"dadb5e9c-cb29-4d91-9887-44d1d6fed38f","resolution":{"observed_at":"2026-08-11T15:55:41.225384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-07T23:58:54.449625Z","title":"E., et al., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2407.00157 , https://ui.adsabs.harvard.edu/abs/2024arXiv240700157S p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.08712","last_updated":"2025-02-12T19:00:01Z","snapshot_observed_at":"2026-08-13T17:57:04.629581Z","submitted_at":"2025-02-12T19:00:01Z","title":"The AURORA Survey: The Evolution of Multi-phase Electron Densities at High Redshift","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-07T23:58:54.449625Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2502.08712"},"observation_digest":"sha256:0097aae0ecba4f9648683acf3c792d01fbacb309c1caaf05d0dddd36d1772c01","observation_id":"8fd3f3b9-7770-4977-a87a-efca8e46572c","resolution":{"observed_at":"2026-08-07T23:58:54.449625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-07T18:32:21.483973Z","title":"E., et al., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2407.00157 , https://ui.adsabs.harvard.edu/abs/2024arXiv240700157S p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.10499","last_updated":"2025-02-14T19:00:00Z","snapshot_observed_at":"2026-08-11T19:00:14.525330Z","submitted_at":"2025-02-14T19:00:00Z","title":"The JWST EXCELS survey: Probing strong-line diagnostics and the chemical evolution of galaxies over cosmic time using Te-metallicities","version":1},"reference_index":151,"source":"arxiv_source","source_observed_at":"2026-08-07T18:32:21.483973Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2502.10499"},"observation_digest":"sha256:80a222d5c17cd31f93c2b5f993f553112700186a7117e88dd4a75f523b0cda46","observation_id":"c4f1cf52-ba33-4a03-b3c3-b5388800730c","resolution":{"observed_at":"2026-08-07T18:32:21.483973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":"2407.00157","doi":"10.48550/arxiv.2407.00157","metadata_source":"arxiv_reference","pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Sanders, R","venue":"arXiv (Cornell University)","work_id":"7f890086-ce7c-46a8-abfa-288f814ce6e1","year":2025},"citing_paper":{"arxiv_id":"2604.13211","last_updated":"2026-04-14T18:34:01Z","snapshot_observed_at":"2026-08-12T19:39:06.846735Z","submitted_at":"2026-04-14T18:34:01Z","title":"Sparks: The Magellan/FIRE survey from starburst to post-starburst","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-05-10T14:22:35.837891Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2604.13211"},"observation_digest":"sha256:4ce8127d650bee0c01e2a55d493873485add65173c119473181ca5c6a1406013","observation_id":"635f42a6-4828-4701-922b-06c6b3e6a88d","resolution":{"observed_at":"2026-05-10T14:25:28.772660Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":"2407.00157","doi":"10.48550/arxiv.2407.00157","metadata_source":"arxiv_reference","pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Sanders, R","venue":"arXiv (Cornell University)","work_id":"7f890086-ce7c-46a8-abfa-288f814ce6e1","year":2025},"citing_paper":{"arxiv_id":"2605.30410","last_updated":"2026-07-23T19:14:22Z","snapshot_observed_at":"2026-08-02T12:55:08.808490Z","submitted_at":"2026-05-28T18:00:00Z","title":"RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-06-29T06:35:35.299492Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2605.30410"},"observation_digest":"sha256:3842405295b6c1e7db503dc7c2a9e99acc51b1b5bb541f67e2487a5c78d307d8","observation_id":"bccc6ab3-5eca-4a73-9e4d-7faf8652ffdb","resolution":{"observed_at":"2026-06-29T06:43:09.881428Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-02T12:55:22.045221Z","title":"E., Sanders, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.30410","last_updated":"2026-07-23T19:14:22Z","snapshot_observed_at":"2026-08-02T12:55:08.808490Z","submitted_at":"2026-05-28T18:00:00Z","title":"RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9","version":2},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-02T12:55:22.045221Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2605.30410"},"observation_digest":"sha256:5180c8dc87b6e69b492e422cee59d97962be7a10c50167b37561e25185671b1a","observation_id":"823fbb56-712b-495b-a165-2d258f37210e","resolution":{"observed_at":"2026-08-02T12:55:22.045221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":"2407.00157","doi":"10.48550/arxiv.2407.00157","metadata_source":"arxiv_reference","pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Sanders, R","venue":"arXiv (Cornell University)","work_id":"7f890086-ce7c-46a8-abfa-288f814ce6e1","year":2025},"citing_paper":{"arxiv_id":"2605.30427","last_updated":"2026-05-28T18:00:10Z","snapshot_observed_at":"2026-08-02T04:47:49.225480Z","submitted_at":"2026-05-28T18:00:10Z","title":"The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-06-29T06:25:29.988558Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2605.30427"},"observation_digest":"sha256:c9fe4f030a3c42b3b067b32c3c555ad12f2fd2fb6f1c9a6893bead7f911bb64d","observation_id":"05d9c4f6-748f-439e-814f-de61bb388161","resolution":{"observed_at":"2026-06-29T14:33:31.698311Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":"2407.00157","doi":"10.48550/arxiv.2407.00157","metadata_source":"arxiv_reference","pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Sanders, R","venue":"arXiv (Cornell University)","work_id":"7f890086-ce7c-46a8-abfa-288f814ce6e1","year":2025},"citing_paper":{"arxiv_id":"2606.10005","last_updated":"2026-06-08T18:00:07Z","snapshot_observed_at":"2026-08-13T20:11:34.493110Z","submitted_at":"2026-06-08T18:00:07Z","title":"On Cross-Correlating Line Intensity Maps from SPHEREx during Reionization","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-06-27T15:56:34.059692Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2606.10005"},"observation_digest":"sha256:dc436b8a97c14dc4b720dc650301b1e9b793eb49e95d57725e204a32ff1eaa3f","observation_id":"a77bbc90-90e7-451b-a198-116e5e92da9b","resolution":{"observed_at":"2026-07-03T02:27:34.781983Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00157","snapshot_observed_at":"2026-08-14T04:17:46.970441Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10063","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-15T03:47:22.783808Z","submitted_at":"2026-08-10T18:00:00Z","title":"Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \\leq z \\leq 10$ Galaxies with JWST Spectroscopy","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-14T04:17:46.970441Z"},"links":{"cited_paper":"/paper/2407.00157","citing_paper":"/paper/2608.10063"},"observation_digest":"sha256:167663c26ac4f3a59c27680ff5947bf13e8d2c34330da825e24ae117e5abbb5e","observation_id":"e87dd0c1-b743-4d66-bd2a-bc8d3007fd40","resolution":{"observed_at":"2026-08-14T04:17:46.970441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.00157/citation-record","integrity":"/paper/2407.00157/integrity","json":"/paper/2407.00157/citation-record.json","paper":"/paper/2407.00157"},"outbound":[],"paper":{"arxiv_id":"2407.00157","last_updated":"2025-01-25T22:02:06Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-12T23:32:28.401858Z","submitted_at":"2024-06-28T18:00:05Z","title":"The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2407.00157."}