{"as_of":"2026-08-18T20:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a419ba14d7d11868bb72063d2d4adc639750eb8cfc5764c87e7398206553be82","coverage":[{"denominator":84,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":84,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T10:29:37.282880Z","state":"measured"},{"denominator":84,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":84,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+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/2607.10612/citation-record","integrity":"/paper/2607.10612/integrity","json":"/paper/2607.10612/citation-record.json","paper":"/paper/2607.10612"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T10:29:37.282880Z","title":"Fowler and F","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:71c3dbf162fe0d61dfa4aa54068b3a6165ddc6c9fe7dbe110cf705ffab240196","observation_id":"432ba16d-11cd-4838-bbda-b12909c2b1c1","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Barkat , G","venue":null,"work_id":null,"year":1967},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:172ab52fe4d08bd8d934570bcc73edb70aca0a8f0f10fb8c72cc934cb769f6b9","observation_id":"d440a33b-aa76-4ce7-a7d9-9e195a8c1e25","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Baraffe , A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:d4ec428468c582a48e6d3b57cd64692c8f771b216559a29ef758085e2bc23f27","observation_id":"d91e2d2e-a092-49d9-9da0-7c1815486126","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Nucleosynthesis of Zinc and Iron Peak Elements in Population III Type II Supernovae: Comparison with Abundances of Very Metal Poor Halo Stars","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:016cc1ff55a64b68c1c19a4c80837223956fefa0b4542df0cb16d4f11ed57143","observation_id":"f7ad0e03-8258-493f-a667-ab3e9376b3d4","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Heger and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:f08352ddf164ec12506b68eb36350f2bb80a7cb2f37631af95c21270535394b5","observation_id":"0a81f0cc-0d69-4fd6-9fe9-798a47db936b","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Stellar yields of rotating first stars","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:7ac5b480b042c8a53fb2ab0c06cfb398b9195974395eb12fc731b53512b22e93","observation_id":"f04e079a-cf33-4e2a-af25-a3f594518d1c","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Langer , C","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:55554db66384e86a0a32316ff3ee406b66b860a8d60eaaf9af3fd24122ed34a9","observation_id":"54fe56c2-9762-4e53-ad77-a9e4595a9ab2","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Pulsational Pair-instability Supernovae","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:e1db7c82c2f0c7dc82c3b92d1354bb094ed9663a7e12540b05e0ed64baf7aab1","observation_id":"8b44f69b-4b9f-4396-a434-232e8058adc1","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Ishigaki , Hai-Ning Li , and Jing-Kun Zhao","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:bf9e47d90bcc7ea02f0ed34cebd3868155d93f96be96fbcf5dc461357016cc07","observation_id":"48434499-1817-4d23-ba33-3ff186053bce","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"P., Cerny , W., Kirby , E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:449c585c7da37de827af0ceda15d306139079b65d2ba843d0ef19dabaf54ad6d","observation_id":"4923f40e-2b20-480d-b3cb-0a006cb45e13","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stad3498","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Monthly Notices of the Royal Astronomical Society","work_id":"ca29c93a-2cec-49f5-a93f-f6740a67ebe5","year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:25360d91c53ae9758bc32388c78b5a384626416847afb6012ede7706da421a0f","observation_id":"f9a521c9-c36f-43f4-b3d5-62a0b6e94962","resolution":{"observed_at":"2026-07-14T10:30:24.185542Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:10.192458+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:10.192458+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":"K., & Banerjee , P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:22d2a4caf09b104e3092c0dc48b62d818da5146c2217166a299a9558b06fb89a","observation_id":"c5461c50-f879-40b8-8219-2c0652d453e3","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Moriya , Kimihiko Nakajima , Ken'ichi Nomoto , Michael Rauch , Yuichi Harikane , Takashi Kojima , Yoshiaki Ono , Seiji Fujimoto , Akio K","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:84df5ac81e0b4f74d737201bfb9cff12c94b7ec99b787beca82b18c56fd1226e","observation_id":"d2b277af-c7e2-423d-9aa6-a4e60abbcef2","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Ishigaki , Yoshiaki Ono , and Yui Takeda","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:8eff181db77cebb3771a951aebea328126cb274c0e0bf11dea00658eb95aaa67","observation_id":"aad05b10-e790-4cfa-a1ff-5674adb39ec2","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Beers , and Bruce A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:00278d1b6cdd5376a57a2c2212f92e27af603f431e8b6d00544e9d0ba02890a1","observation_id":"92406f39-51ed-4a23-a17b-bb8af6f3ebfb","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:5a4d44330a09cfb3d1b8b5187eb9928b4c96d279567509f6af9a458f3b3ca856","observation_id":"1f479379-f921-4f51-9c83-2f3efb30aedf","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Karakas and Maria Lugaro","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:f11c0f2a71282208d72f85ed1b57dc18c13bf7149af4a632ffcd5ef5197bc17c","observation_id":"41481ecd-ce73-4bb9-836d-daafb39bc842","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Probing the Cosmic Reionization History with JWST: Gunn-Peterson and Ly Damping Wing Absorption at 4.5 < z < 13 The Astrophysical Journal, 997 0 (1): 0 86, Jan 2026","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:85a605ff806cf23dca4b631800040299a053e483ba070d89664e9a7a4873959e","observation_id":"d3fe2f2d-3e64-48d5-bdc9-0e0ff268d56f","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.08782","last_updated":"2026-06-18T18:00:29Z","snapshot_observed_at":"2026-08-01T16:57:00.112794Z","submitted_at":"2026-06-07T18:58:16Z","title":"JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.08782","snapshot_observed_at":"2026-07-14T10:29:37.282880Z","title":"JWST Absorption-Line Analysis of UV-Bright Galaxies at z=7.2-10.6 : Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe arXiv e-prints, June 2026","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"cited_paper":"/paper/2606.08782","citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:72219d3bd8473c7138221d4296c4deccc06001cbcca8563bc3b92655a34ec4b3","observation_id":"4ad0c93a-cfb6-4aa9-b527-dfad103701b5","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Kozyreva , S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:8613605297ed1e80d5d9d2b71d4890de773e2090438cacac8362a5c97f221c3e","observation_id":"0f2879fc-f1a6-4576-89d8-4582dfbd887f","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Metal-enriched Pair-instability Supernovae: Effects of Rotation","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:e8c349a9cc683480847f8a66a8c2e789cc1105b656e543fa469edd599e0a2177","observation_id":"83c709e1-48ce-446b-aece-ba66518f570e","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Farmer, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:c7975a1710b2746826c1890a05d27ccc1c0aac3a932c82eec57c622de1b44ff3","observation_id":"7acfba24-b86b-4e2d-a855-de050ad2a61a","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:c1188e36308e9d09ae3dc77e71c637e5cd3adc9d693dc492688dc3d6ee4bd160","observation_id":"9e7ba16b-4787-4bbb-963a-012acd804d6c","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Renzo , R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:0574e77c71289b33657da8c0e4a97f0146945b093896063a11a029af30ea3d7e","observation_id":"21574569-03ee-40c7-8808-6ad36332057c","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Chidester , and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:811cd4e0e470d77cac14f356738d782af65eb47a3d18c880b940ef0f0f79f082","observation_id":"bdba596a-4aa3-4b20-978c-76e23070d257","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Mass Distribution of Black Holes with Effects of Convective Carbon Shell Burning on Pair-instability Pulsation and Fe Core Collapse","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:a5083dba83df2724adcf42d62f198d2a6fa32e0596971d6f6870f59fb2dde837","observation_id":"ad828e88-2f9b-414f-8805-61a884862fd9","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Constraints on the ^ 12 C( , ) ^ 16 O and ^ 16 O+ ^ 16 O Reaction Rates from Binary Black Holes Detected via Gravitational Wave Signals","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:6311ed6427f5c81443524cae8d5ce143dc49a31a90aef959af02af24f7df8159","observation_id":"23e9993f-9acc-4368-a764-1a2745b83121","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Modules for Experiments in Stellar Astrophysics (MESA)","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:5a14b3241037037d738571cd0201f5ccb2b837852638c370ffae362fe6575d1c","observation_id":"2a6a7eef-b5d6-468d-b7e5-96f8ca2f72cd","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Brown , Aaron Dotter , Christopher Mankovich , M","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:ecd631e6c28d329fd3a3df564d311fdeebc1eec183353e7c2a9ffcdfd021b92f","observation_id":"ceb0faf2-3f00-4435-be21-e72801e97d6f","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Bauer , Lars Bildsten , Sergei Blinnikov , Paul Duffell , R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:2f7404642bd3d88afb89803e6d749b1aadb6bf9955b4ac90c6ac6c42d4806fbe","observation_id":"f45061ea-c075-4d10-8482-02009af6822a","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Smolec , Josiah Schwab , A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:d243d4c23d2e453af30724bc9183696d4dab3da405ad836a3e3c3f97f28bc8e6","observation_id":"83fb3796-d545-43c8-9105-17a10db8b57b","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Cyburt , A","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:dfc9f1fe0adc4fabc1c2d33ffc303be9fdd8603c00c038fa81f2984c3722be46","observation_id":"d9319bad-6c10-484b-9df3-6eceb2537b90","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Caughlan and William A","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:bd150b4e29f988e316911df82a3ab587f0fe4b3d8b4c5da80b3bcd05985136fb","observation_id":"15f7e332-eb81-4d27-acaa-2b508fe91b19","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:9812b7e4d116acfa310125243ef1c647d494dc1fedfa80004415f59fb036003d","observation_id":"3d9d739c-205f-4aed-b4cc-e016ab7e1271","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Langanke and G","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:bbda326faa8242eba47875a8b2f95c6143f175760c445268cde115e46f6d1470","observation_id":"3dc69cdf-363d-49b5-bd77-6a5f1082a4f2","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:14cf4b2d1074c5c12eb1ee45f81510d05f7cbad48ba1e4dbe033605bb8314ce2","observation_id":"08f1c1cf-a424-44e0-830a-0aee6835872b","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:50cd675f7c470530073a58f7a72a11883d06d803ae64123001f46d4d78d087e3","observation_id":"f392b26e-9630-4a6a-aebd-fc68761269d4","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Langer , K","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:bc1c35f3b949a33f3819c0ac5b1b1559a4043f462eaee86fe29d4e3b6bc3d4b5","observation_id":"b3000f22-7d1b-4cec-bc9d-081e8518fae1","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:1f3e6e20d540dd44c3d7a9d8ddd8453effeaa647f01d23f9db57b843cc1e5ef9","observation_id":"671bdec9-e604-46eb-969e-cca7bdbe787e","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:c93d54be42d89239997cf3f8f38d7f4c2d0f4a33fe94f5cc3a51de76ac865aac","observation_id":"c72b6525-d724-4109-a3f9-0d3d74ca09c6","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"10.1086/310240","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Buchmann","venue":"The Astrophysical Journal","work_id":"bbaf6cd7-37cc-4e63-8273-5643a6535c54","year":1996},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:8e630b32aed47131ad6601bfd996fe8f178ea7b002b2592766894a935aa9853c","observation_id":"fef5d9e9-320f-4ff8-bfb2-8081d9c6e1ac","resolution":{"observed_at":"2026-07-14T10:30:24.149875Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:15.983048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:15.983048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":"Kunz , M","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:dfa462b4a94591dbf257c2e459e17532ddc5d0fee3db4965310bad40038b7096","observation_id":"fb189edb-c083-4a6f-b9db-6328d9ef7598","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Weaver and S","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:882beee914f6d4f00dbf4c3324f1c575cef37d5c0db4d4e27ffe8588028733f2","observation_id":"e18975ce-cc70-4cf9-82a3-fef012506b14","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:6d8edaa13173ab11a90c4e8c8cf8d1e64ceffa20885ee53f6663bbde6588ce37","observation_id":"3b94088e-10e0-42a1-ac28-48e605d1d5d9","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Annual Review of Nuclear and Particle Science, Volume 57, Issue 1, 463-491 pp","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:b951da690691cbd5262723905ac45dddbc13c4c94fa5996ba0c3787977e4a6d9","observation_id":"0cac0c8a-e83d-4a1f-854e-04b4d3129b7f","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/pasj/26.1.129","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"On the Surface Conditions for Very Massive Stars","venue":"Publications of the Astronomical Society of Japan","work_id":"2be8257b-b83a-4a9a-b7cf-df715b1753d4","year":null},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:314c65306015617d6f05d8e892f07db8b5c5fc801c3588937f9bbf9a15faa7fe","observation_id":"7dbc4c4d-5e2b-4cee-809b-ccd22c47705e","resolution":{"observed_at":"2026-07-14T10:30:24.087856Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:17.040697+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:17.040697+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:2def1f55de2c6d6c5e6cfff3dc72fc536a0e59ab3cb568e0ea529b097d31dc54","observation_id":"c966418b-cee7-4573-a058-f7de91cac6ff","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:450f7d92b4872edd483c22ec28a213762899d954e0066f3d90b17b5c928e3f6e","observation_id":"756773e4-1c82-4795-9d50-17ec63fbef6d","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"The ^ 12 C( , ) ^ 16 O Reaction Rate and the Evolution of Stars in the Mass Range 0.8<=M/M _ solar <=25","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:f3346e6925660985ee6aaec474b4b2a92eb96cedc8e67369965cf92c7cd3d7c3","observation_id":"b88adb88-dd48-47bf-8860-a063dd97d3e7","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"The Presupernova Core Mass-Radius Relation of Massive Stars: Understanding Its Formation and Evolution","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:a13a389b9482a73a9d30d7b5fd5f6358fc9c66679df7e1522f8dd1293c892a8f","observation_id":"addfae72-bae2-47ff-a317-a687a7d89798","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.11012","last_updated":"2025-02-18T15:06:54Z","snapshot_observed_at":"2026-08-16T12:58:03.727370Z","submitted_at":"2025-02-16T06:34:39Z","title":"The Impact of $^{12}$C($\\alpha, \\gamma$)$^{16}$O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.11012","snapshot_observed_at":"2026-07-14T10:29:37.282880Z","title":"The Impact of ^ 12 C( , ) ^ 16 O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"cited_paper":"/paper/2502.11012","citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:e0fd9faf416f044bcc636fea5d9e91bf2ff8d3310f78981da35333ef6f9e273b","observation_id":"e525da18-9997-4d11-a17f-c9dc0c28ddc3","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Moriya , Ataru Tanikawa , and Nozomu Tominaga","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:d12e20201f94a873d6609bf843877e6a9cd1598b9d0762c8e9c40c66f401d6fb","observation_id":"e38f54c9-0b27-4430-b73c-bc447326a9a6","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:755b3123187d9a71b6a9b4dfebc1f9a5aaa3398f1043f3801204f928e23e2ed4","observation_id":"4382ca78-b3b7-4651-8035-ee7bbb2ce7eb","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"10.1088/1361-6471/ae1248","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"S., Freer , M., Merchant , A","venue":"Journal of Physics G Nuclear and Particle Physics","work_id":"0450da6c-b931-4495-9be0-c2b05b3735f4","year":2025},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:2576021d1e22d4a2848c06b227ffa61c8add0c5cb396e1478d82b162c33910bb","observation_id":"be48f097-646a-43dc-a87a-4d2b467295ed","resolution":{"observed_at":"2026-07-14T10:30:24.042282Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:19.022831+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:19.022831+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":"The advanced evolution of massive stars: I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:8d6259a9d71b46c4d3079957b3cd2bb184a5004736cdd0aaab1b9cdd6b805d29","observation_id":"51951ad9-7598-4d05-9097-11d59c63df56","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"E., Timmes , F","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:e8af47ebecc4b0f9c6363e334dc5b23dd905dc80cc479c93ebd8e502b7f0d0cd","observation_id":"020f4274-0284-40c7-8a0b-f4d48e5f35a2","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Farmer, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:df043d8ffcdc8804ac19fdc4cdbfd84cdc00ec75dd9b15ccfa4a7f86d6093d0e","observation_id":"6d22362c-8615-43de-a070-5b1eb7454d0c","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Lodders , H","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:16b3cc2d67ed8d57fce0afb7871bf983c2573ffe50a8672e9a62e1a375b2ee57","observation_id":"54544f9b-30c3-4e81-bfba-00d4122a8dbc","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Salvadori , P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:f87d9c34f7b31fdfda3616ff1918f619058ffb478d6e03a41779c62d72c2c449","observation_id":"f79b6394-2c6b-40e5-a21d-51dbb07a5484","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Becker , and Guido Cupani","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:5acd1b8dd28ced9d259379553b8807b7b2d0cce6d5ce45ccebfba56c0f4ab6dd","observation_id":"3ed22216-0b05-4600-bcee-2932956ca4ea","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Supernovae and Nucleosynthesis: An Investigation of the History of Matter from the Big Bang to the Present","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:e0e88fe890bb706a2296a015fcd8d9dce9442f8c56c185e695a2c8dd31beddeb","observation_id":"e86a8ce0-819c-4e93-9ed1-d321afe8bbf3","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:18998db3998efaaa96f864cba36bd2abb4778b25792a3faaed4081c16489c980","observation_id":"385fb489-10cb-4c7d-8d1d-05d8167bcd3e","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"10.1086/375812","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ivans , Christopher Sneden , C","venue":"The Astrophysical Journal","work_id":"2d07ba1e-a672-4cbf-a2e8-044a005fcb06","year":2003},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:1d4cbb2d3ab74258fee4c3d51726fa96d6465bd9ff6496d74e4ee9828b5aac7e","observation_id":"2f99a0b0-1495-4b18-9b53-9c169a174a82","resolution":{"observed_at":"2026-07-14T10:30:24.307172Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:21.347748+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:21.347748+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":"Ishigaki , Jianrong Shi , Jingkun Zhao , and Gang Zhao","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:261053824a398e35d3deeaf63448fffc0cf1fd74a3a5b2001cbb08c70762117f","observation_id":"a693a930-3ddf-48ec-96a8-c77fecfeb044","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:023fea821b927f5b2336dc7e888cac38daa051e8fb916274577b1872468c6397","observation_id":"4828df79-b3cd-4a47-8df1-7f9e25fc3702","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"JWST Identification of Extremely Low C/N Galaxies with [N/O] 0.5 at z 6-10 Evidencing the Early CNO-cycle Enrichment and a Connection with Globular Cluster Formation","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:41c1c9407513a7b29667266a517fa9a9663d8b6ebeea2fc8a61fb3ea609c27bd","observation_id":"47fadee1-378a-4034-a6a0-afea8f7f27d0","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11457","last_updated":"2025-09-07T08:54:36Z","snapshot_observed_at":"2026-08-16T12:49:59.595534Z","submitted_at":"2025-03-14T14:46:22Z","title":"Fe Abundances of Early Galaxies at $z=9-12$ Derived with Deep JWST Spectra","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.11457","snapshot_observed_at":"2026-07-14T10:29:37.282880Z","title":"Ishigaki , Hiroto Yanagisawa , Daichi Kashino , Nozomu Tominaga , Koh Takahashi , Moka Nishigaki , Yui Takeda , and Kuria Watanabe","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"cited_paper":"/paper/2503.11457","citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:7485acf2d3d32bc07bfb44f67aaf938231e11f4e3cd79706e5932d13bab80546","observation_id":"73f560ba-7cc3-4bc7-8ccd-1d3ed0044322","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Supernova Nucleosynthesis in Population III 13-50 M _ solar Stars and Abundance Patterns of Extremely Metal-poor Stars","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:1463f50b50f547c3b3c4865f81f25c53e2f15e501e5f4a2afe7f8b46f38d2b2c","observation_id":"1b23f7cd-c3f4-437a-b129-b2b8ee81be76","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:163a30aab0cdbc87074fdab2e2e7cab5c2e6015c21f3376442af213724d1621c","observation_id":"5291ee84-2f91-45e1-8274-3285b5297464","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"10.1088/0067-0049/199/2/38","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Limongi and A","venue":"The Astrophysical Journal Supplement Series","work_id":"46182a1f-8d4f-49ed-a0cf-91f0e69a931c","year":2012},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:88171931a36cfc0aa055b7761774a2861739224a1e1fad5111279f7943c246eb","observation_id":"2d52f171-cb07-4c1a-9975-b959f92bac06","resolution":{"observed_at":"2026-07-14T10:30:24.213940Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:23.118477+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:23.118477+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":"How Much ^ 56 Ni Can Be Produced in Core-Collapse Supernovae? Evolution and Explosions of 30-100 M _ Stars","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:c11ad66c460ccac62bd38598716ffbbbd0b88b00539fb3ee409ffb61edb803be","observation_id":"d8d2a281-01eb-4c81-8d04-b5fc63c97351","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"and Lucchesi , Romain and Salvadori , Stefania and Aguado , David S., On the Pair-instability Supernova Origin of J1010+2358","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:e6152cbcdd92337d35b37fa497bb50be8d12a0357da11917236b6fc987d46d3c","observation_id":"4b00564f-6d25-4649-a7a3-9d90d0f89aae","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"10.1086/306410","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Norman, and Yu Zhang","venue":"The Astrophysical Journal","work_id":"c1afeb0c-45d8-4a0f-8e36-638ed585c036","year":1998},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:101988bb3fb4e36d0d3522f5869f077692dd221a901f4e652b53a622854d3e5e","observation_id":"3a11fa39-0af1-453f-8764-a54453f7786a","resolution":{"observed_at":"2026-07-14T10:30:24.117401Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:23.944853+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:23.944853+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-07-14T10:29:37.282880Z","title":"Bryan , and Michael L","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:eeab3f420cb5e522e84448df99d2aac40f4c3af84d2d108d50dbab223423b9d9","observation_id":"a200c898-ebaa-4344-a508-4cb8dce14e2f","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Hirano, T","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:ae4197ced09a97505f29b54bed419e6658f1c41316549bd6c17132801528228a","observation_id":"1d83f675-a8d2-4656-b3ea-1777d7cbb776","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the Metallicity Range -3 [Fe/H] 0","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:9757229b460826fac83579dd4018c96cb3d2baa763fdaad65e485370e32a296e","observation_id":"e2c51699-f737-4a38-a59a-a9763f21458d","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Yoshida and H","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:f8e9dc1218bfdef2795f419c3e3bebc6ad9fb99c551b95cc90335820597f7385","observation_id":"17de96e3-5da8-43f2-9bc2-5acdc445ac87","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"de Jager , H","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:0dd0bf05228c6fe9dada35f969b1d7531e33ce2265d3c3fdc675f2921e484ad3","observation_id":"73323e0e-0db0-4df2-8f0d-e92d2e42295f","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Vink , A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:22db9c13d7a030632cfa630be45cade2dc28c00f9f98fdbd1e61c27b35272d06","observation_id":"46faba91-6d36-4bad-8ddd-4acc2f7f6d5b","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Nugis and H","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:7f706fdfe355d3bb71417ccd6f9c58542b00867fc6ec5a38008a36d7f91d3ede","observation_id":"d5ea35c1-07fa-4d05-a3dc-f60075f3da49","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"2026-07-14T10:29:37.282880Z","title":"Maeder and G","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:3462e8a2193a2d22f56f943b7ee542ce8ca44637ec361e7aa5d8415928f2f513","observation_id":"0f0b6f1f-dcc4-4875-b1b8-9e55ffae77bd","resolution":{"observed_at":"2026-07-14T10:29:37.282880Z","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":"10.1088/0004-637x/767/1/78","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Tanner , Sarbani Basu , and Pierre Demarque","venue":"The Astrophysical Journal","work_id":"f94c8744-da2e-49c3-8d15-84e72208bac5","year":2013},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:68babfa720397c8fdb6d26205edc8043b91f6b58dd79aee2284e5880cbda9dd6","observation_id":"cadb8bcf-9f6c-4b00-859e-fb3ed62027b4","resolution":{"observed_at":"2026-07-14T10:30:24.270993Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:25.593506+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:25.593506+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s41365-026-01975-6","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The impact of new ( , n) reaction rates on the weak s-process in metal-poor massive stars","venue":"Nuclear Science and Techniques","work_id":"87950559-9848-4f32-b53a-f337b5d541fe","year":2026},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:3a8f54ecae898b3618bc92aaf6445154bef26bcd5f7d9b5975a31a49a03fae25","observation_id":"7fa6814f-d42c-4fa3-8645-2563578f43a4","resolution":{"observed_at":"2026-07-14T10:30:24.137379Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:25.917266+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:25.917266+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s1743921305005855","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Nucleosynthesis of pair-instability supernovae","venue":"Proceedings of the International Astronomical Union","work_id":"681870d1-975d-4c21-853e-4fd99f6e0987","year":2005},"citing_paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-07-14T10:29:37.282880Z"},"links":{"citing_paper":"/paper/2607.10612"},"observation_digest":"sha256:ce5ee769672bff53f9dc4db33699e2a5d7d31897116a679aaaffd63aa4ea1941","observation_id":"b375f09b-11d9-4035-8963-89fc3a09f659","resolution":{"observed_at":"2026-07-14T10:30:24.121927Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-14T22:50:26.181417+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T22:50:26.181417+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2607.10612","last_updated":"2026-07-12T07:17:25Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-14T14:44:31.678695Z","submitted_at":"2026-07-12T07:17:25Z","title":"Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae"},"reference_resolution":{"displayed":84,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":74,"verified_exact":10,"verified_fuzzy":0},"total_outbound_references":84},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 84 of 84 outbound references and 0 inbound Pith citation observations for arXiv:2607.10612."}