{"as_of":"2026-08-20T17:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6cbfd620bfa268261f8ecdda067424f4ede7293c3c17d874d1974b2a2fac4f47","coverage":[{"denominator":70,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":70,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T22:43:52.232767Z","state":"measured"},{"denominator":70,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":70,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+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/2508.06654/citation-record","integrity":"/paper/2508.06654/integrity","json":"/paper/2508.06654/citation-record.json","paper":"/paper/2508.06654"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:45.724140Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:45.724140Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:c9d56f3dede610cfee12322d863c9abe3fa057a4a445b51a72d4a7d7b6001f98","observation_id":"213e6c21-4af4-45cd-9816-854ec5394b65","resolution":{"observed_at":"2026-08-05T22:43:45.724140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:45.787610Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:45.787610Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:03b387d0f969ea5c31967b8f82f5726e2c6f2179b8ceaddba1cc9f75ae6c95b7","observation_id":"327c71e2-9de7-405f-bcc8-565c5a40fb1a","resolution":{"observed_at":"2026-08-05T22:43:45.787610Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:45.882229Z","title":"- [1] #1 = = ^ ^ ^ .\\!\\!^ d .\\!\\!^ h .\\!\\!^ m .\\!\\!^ s .\\!\\!^ @mss","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:45.882229Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:6d7472d905f424db56fa22b6ce910109ed963050ad74b23f3e82132c3d38684a","observation_id":"916a69d1-6f96-45a0-8c8f-133403025f89","resolution":{"observed_at":"2026-08-05T22:43:45.882229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:45.953623Z","title":null,"venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:45.953623Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:91bef2adbce4bd53c3d4778a6a4d9b4360ddec3a52229e35f8d341949021a05f","observation_id":"31195e97-24b7-4059-ad8b-5c89a77df3ac","resolution":{"observed_at":"2026-08-05T22:43:45.953623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.040461Z","title":"1982, , 253, 785, 10.1086/159681","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.040461Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:52672394e4960482a71dd3a71241675c903de029446e66de504ab8575f18c369","observation_id":"5f4093c4-83d0-48e1-a279-5da4ea7c3d3f","resolution":{"observed_at":"2026-08-05T22:43:46.040461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.100056Z","title":"D., & Fu , A","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.100056Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:f2f3aae9120ad63f24f8c53227a9abdeeb26ab8f3ce529d493f44a64ac6cb47b","observation_id":"4d6a558b-87db-44fd-9422-1588562e01a9","resolution":{"observed_at":"2026-08-05T22:43:46.100056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.185125Z","title":"L., Harris , C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.185125Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:3b6e5c4f32d8bd474a51f7b2e7fb71ba22425067ee6543c0e7d8d50be626cfc7","observation_id":"43d057c4-448e-42c1-bc3c-f4a214c1aec9","resolution":{"observed_at":"2026-08-05T22:43:46.185125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.329343Z","title":"P., Bora , Z., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.329343Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:363a65740f07574303e83cf86ec0187cd63502c0d58c5bd731246e1b592475c6","observation_id":"652d458b-2a83-45ef-b40a-51dcc7ab3634","resolution":{"observed_at":"2026-08-05T22:43:46.329343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.447712Z","title":"C., Orellana , M., Folatelli , G., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.447712Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:17aee0a1815ba8f2058384a0b25c7439963b8b3b6503267acf6f34cac3c5f022","observation_id":"52901260-4748-4cba-8e90-450319346b47","resolution":{"observed_at":"2026-08-05T22:43:46.447712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.551245Z","title":"I., Eastman , R., Bartunov , O","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.551245Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:3c5470c3f5cd2ebeaec4bae33300913b662dd4964d10ba05e1e17367a10b4998","observation_id":"446caae3-7d5f-4906-83dd-deb598e8fedd","resolution":{"observed_at":"2026-08-05T22:43:46.551245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.682471Z","title":"A., Sand , D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.682471Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:b9886d50edbfd9822304eb1af90b13a191c8499906a5d5dea0fd2980faa29c70","observation_id":"81239463-ba18-4aed-b26b-763b8d302939","resolution":{"observed_at":"2026-08-05T22:43:46.682471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.797707Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.797707Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:06a5df325e6928b8dbe0db0b1c0005ce458886cfe461134d5f82e8b62db2b49a","observation_id":"b160877f-d86a-4e73-9f5a-9d0f4f8c6b7c","resolution":{"observed_at":"2026-08-05T22:43:46.797707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:46.895603Z","title":"A., Petschek , A","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:46.895603Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:d948fe2cdb35cfe65514405cbedfaafc37afa753d5a939d493b0d548fc2ef7e3","observation_id":"bb3aed83-4280-4145-bb44-9f90a105b27f","resolution":{"observed_at":"2026-08-05T22:43:46.895603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.014121Z","title":"P., Pumo , M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.014121Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:a1804731302e6fc11996470019b74f76c0e261ff5f245a000be78378191bd41b","observation_id":"0147ee05-49ff-400e-a46f-3be2a9e1fa76","resolution":{"observed_at":"2026-08-05T22:43:47.014121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.128310Z","title":"2025, , 984, 71, 10.3847/1538-4357/adc108","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.128310Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:27f7baf725bf9348f7fe5607e52a964431117d9452bcbceae8e8f4149e92d70d","observation_id":"00510434-ac75-45f4-b920-a424f7eb5a30","resolution":{"observed_at":"2026-08-05T22:43:47.128310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.241727Z","title":"J., Ferrari , L., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.241727Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:5ef7a4857fac8d5f1363602a24add2ddfb9e92004ae25968419ea391d87c396a","observation_id":"ca458187-bf9c-4a29-918a-947a4cfa1d8d","resolution":{"observed_at":"2026-08-05T22:43:47.241727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.00130","last_updated":"2024-05-31T18:41:06Z","snapshot_observed_at":"2026-08-16T13:47:18.606372Z","submitted_at":"2024-05-31T18:41:06Z","title":"Progenitor mass and ejecta asymmetry of SN 2023ixf from nebular spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.00130","snapshot_observed_at":"2026-08-05T22:43:47.330165Z","title":"2024, arXiv e-prints, arXiv:2406.00130, 10.48550/arXiv.2406.00130","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.330165Z"},"links":{"cited_paper":"/paper/2406.00130","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:611d55f27f0c7c4fcb139d2a0a31dd71f6e52dcaed96944d8476baf948f3180e","observation_id":"fd762bf5-e319-4648-bea8-6e6789ac6e12","resolution":{"observed_at":"2026-08-05T22:43:47.330165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.398735Z","title":"2025, , 698, A213, 10.1051/0004-6361/202554128","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.398735Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:0622686104a335afa01f9af07c6e5413144e040500866bdf1f11c2b3d9773517","observation_id":"7503e774-a3bf-421e-bc35-173eb4d8ac36","resolution":{"observed_at":"2026-08-05T22:43:47.398735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.478426Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.478426Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:f198b014a7d08bdfc5fcb110665111556c866a08f66f7f90a6983113f9de2138","observation_id":"af5d14c7-5073-4950-963d-c317b4973fa2","resolution":{"observed_at":"2026-08-05T22:43:47.478426Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.562355Z","title":"E., Pols , O","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.562355Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:634f4f4e4d9f4f6a1e0286e9fa1ee928556390c86f3c9bd8e8330a43a3df48e1","observation_id":"3d01fc64-37d6-4253-9628-c674db597544","resolution":{"observed_at":"2026-08-05T22:43:47.562355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.613432Z","title":"A., Bildsten , L., & Paxton , B","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.613432Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:5d4b48a8cbfe526021eac87b103d1d0dbcc9046e1b408f99c4e1afe957a8b367","observation_id":"3d79f834-1dc2-4905-b99f-2a271d5a3efa","resolution":{"observed_at":"2026-08-05T22:43:47.613432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:47.661065Z","title":"2023, , 955, L8, 10.3847/2041-8213/acf299","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.661065Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:1150abee5c94c14707ff5d8dfc99f36a318b501362332de3c64d9eadbb39dc50","observation_id":"6a8ade96-7fd9-453e-800d-9d207f5ee843","resolution":{"observed_at":"2026-08-05T22:43:47.661065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07874","last_updated":"2025-09-09T03:17:00Z","snapshot_observed_at":"2026-08-16T13:26:22.248197Z","submitted_at":"2024-08-15T01:22:16Z","title":"One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors","version":2},"cited_work":{"arxiv_id":"2408.07874","doi":"10.48550/arxiv.2408.07874","metadata_source":"pith","pith_arxiv_id":"2408.07874","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors","venue":"astro-ph.HE","work_id":"b1508d20-eb27-482d-aa30-2a2004f3fa35","year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.752657Z"},"links":{"cited_paper":"/paper/2408.07874","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:96fe49c9be706e9370a2511da7f0ce69b4ec1c03c12d8a5d6c483de2d02831d3","observation_id":"099f0366-95d2-4ad9-aed9-a098ee39d464","resolution":{"observed_at":"2026-08-05T22:43:53.948630Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:54.756627Z","title":"2023, Transient Name Server Discovery Report, 2023-1158, 1","venue":null,"work_id":"c444b1c5-9f4e-470a-996c-fecdfb9ead8e","year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.811556Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:6e034a7d0aed70dcd3aaca3d3a8b614234e3a0106db39f91041f9a5d212697b9","observation_id":"dc1d7d55-9c27-4585-94a0-c44ba23186ec","resolution":{"observed_at":"2026-08-05T22:43:54.860717Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.08078","last_updated":"2025-07-10T18:00:03Z","snapshot_observed_at":"2026-08-16T01:32:53.460091Z","submitted_at":"2025-07-10T18:00:03Z","title":"SN 2023ixf: The Closest Supernova of the Decade","version":1},"cited_work":{"arxiv_id":"2507.08078","doi":"10.48550/arxiv.2507.08078","metadata_source":"pith","pith_arxiv_id":"2507.08078","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"SN 2023ixf: The Closest Supernova of the Decade","venue":"astro-ph.HE","work_id":"554e1caa-054d-493a-ba8f-f4300a65059f","year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:47.910675Z"},"links":{"cited_paper":"/paper/2507.08078","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:88ad869bf682e457283f00b5ff9de6942e79c0b5a99ab7644fddc0de5a2bd89e","observation_id":"ac97a2ae-2db4-4de9-85a5-82ba07ff8d27","resolution":{"observed_at":"2026-08-05T22:43:53.787536Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.009490Z","title":"E., Pearson , J., Beasor , E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.009490Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:48ad8af6153aea7cb0e8c48e3fdbc41dec4824b22c227a37a5b90cfe8125c41d","observation_id":"3ea5694e-9235-4163-96f7-dc912468eb19","resolution":{"observed_at":"2026-08-05T22:43:48.009490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.084753Z","title":"S., Bauer , E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.084753Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:ebf5d230b42b503b3496b22ae9c4526b2eff3b36c01ad2b1c32c6a19bd77a9c3","observation_id":"e2fb1576-3262-41d4-aacd-a2fa4981d095","resolution":{"observed_at":"2026-08-05T22:43:48.084753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.168329Z","title":"2010, , 717, 245, 10.1088/0004-637X/717/1/245","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.168329Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:619b5df5033631d2769336181f15a18e4d6078c558fbca6c900be19681a19c86","observation_id":"5c9f5583-7802-413b-85c2-3a0053c47928","resolution":{"observed_at":"2026-08-05T22:43:48.168329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.280680Z","title":"D., Foley , R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.280680Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:d6243e4a3d1420e7d6aee0bb519164d79ce87f4e69f1e8c85be6895d4c05a0f0","observation_id":"19a84757-4ed8-47c1-9f46-1f527332078c","resolution":{"observed_at":"2026-08-05T22:43:48.280680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.340477Z","title":"2025, , 694, A319, 10.1051/0004-6361/202452758","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.340477Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:a4bad6e8a5f9b968badb84ff4142298502fb09f63dead7925e8e4c0925e831fe","observation_id":"8cecef41-c58f-4489-ae3d-d967a68042d9","resolution":{"observed_at":"2026-08-05T22:43:48.340477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.431682Z","title":"R., Singleton , A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.431682Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:5a69647ba0f265308a2d975d314d2951c19a64913db0fe20513452114fd0f7ea","observation_id":"3f5fb9dc-1767-490c-a2df-5d9ee1c2f55b","resolution":{"observed_at":"2026-08-05T22:43:48.431682Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201937226","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2020, , 635, A127, 10.1051/0004-6361/201937226","venue":"Astronomy and Astrophysics","work_id":"f4599917-17e1-4e35-8de3-5ef66fb198a6","year":2020},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.509855Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:a495cb30470c1bb2665e8b6f412ab89533f4c0368341afad08c42c12b1d26895","observation_id":"10728019-127f-4de7-b111-360ac5da8ae3","resolution":{"observed_at":"2026-08-05T22:43:53.595794Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.03856","last_updated":"2025-04-04T18:33:14Z","snapshot_observed_at":"2026-08-19T03:57:59.956449Z","submitted_at":"2025-04-04T18:33:14Z","title":"Optical and Near-infrared Observations of SN 2023ixf for over 600 days after the Explosion","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.03856","snapshot_observed_at":"2026-08-05T22:43:48.629651Z","title":"2025, arXiv e-prints, arXiv:2504.03856, 10.48550/arXiv.2504.03856","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.629651Z"},"links":{"cited_paper":"/paper/2504.03856","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:b224f6d3f48fc4da8e0020fa0a1ac3bc5984cce79b844028b1c0b40785fd4bcb","observation_id":"2d25eee8-9ec0-40af-842e-3f24624819b6","resolution":{"observed_at":"2026-08-05T22:43:48.629651Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:54.626983Z","title":"Y., & Nadezhin , D","venue":null,"work_id":"25e757e5-accb-45e1-a21b-e972b9c08b94","year":1985},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.749901Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:1f74923e799f0d1d744557990c03d0ee76a4e41653167c36c1a70c9e1274583c","observation_id":"b46fc375-dfa2-4eaa-a6c6-f901905e4826","resolution":{"observed_at":"2026-08-05T22:43:54.669898Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.806682Z","title":"2023, , 958, L37, 10.3847/2041-8213/ad0da8","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.806682Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:9aec8ea0ee04e6ff1d521c3f8de7495500215128421aee1e70f6a9679aabc3ca","observation_id":"e551271c-690a-4330-88e9-6ffc166225ed","resolution":{"observed_at":"2026-08-05T22:43:48.806682Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:48.893075Z","title":"D., Mazzali , P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.893075Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:f533a7196d481c18365d694c64e90e78c7ba6ea5f0cdbdfd3c4a9a0bfc0206aa","observation_id":"dc3d75c7-d35b-4b6e-a5e2-2a9874dbe914","resolution":{"observed_at":"2026-08-05T22:43:48.893075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.00928","last_updated":"2024-07-17T07:23:55Z","snapshot_observed_at":"2026-08-16T13:46:55.940279Z","submitted_at":"2024-06-03T01:55:46Z","title":"Progenitor and explosion properties of SN 2023ixf estimated based on a light-curve model grid of Type II supernovae","version":2},"cited_work":{"arxiv_id":"2406.00928","doi":"10.48550/arxiv.2406.00928","metadata_source":"pith","pith_arxiv_id":"2406.00928","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Progenitor and explosion properties of SN 2023ixf estimated based on a light-curve model grid of Type II supernovae","venue":"astro-ph.HE","work_id":"fc633a62-ee16-4c88-985f-75db3bf9e1c1","year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:48.947067Z"},"links":{"cited_paper":"/paper/2406.00928","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:5ce0253535b7bb99357f9c5f47ad373d91872ceb9cc58e81e21b8976b45e4d35","observation_id":"eff13f7b-398c-4cc2-93ce-c0ad41d38484","resolution":{"observed_at":"2026-08-05T22:43:53.410247Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.009935Z","title":"L., Renzo , M., & Ott , C","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.009935Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:ec06e75046cace6b7f8e0c4fd776a3b98c050d6c2980c33720edf5e776b414b1","observation_id":"8b32b644-a6c1-4f26-85f2-822943390621","resolution":{"observed_at":"2026-08-05T22:43:49.009935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.150699Z","title":"L., Renzo , M., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.150699Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:3315169e11ec22fed3d9b4a5f9bed93c72f7597fd6aaf2f9e00b9015d9e6be16","observation_id":"19d7a61f-0586-44e1-af6c-13ad8e3be751","resolution":{"observed_at":"2026-08-05T22:43:49.150699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aae2b3","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"The Astrophysical Journal","work_id":"ad4bf50b-1c09-430b-ba82-39d19c210444","year":2018},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.255344Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:245ab3d92f6c49e1cff691d1a4d5ebf9ede4849a4fcf81b8fef29cc47d99dee5","observation_id":"5b062361-db3b-4efc-a25f-00de6b44aac7","resolution":{"observed_at":"2026-08-05T22:43:53.245821Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.341627Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.341627Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:d35c9b641c2188d4a6052c14680e5cd167b7280a3184e162de5b854a757e4343","observation_id":"c749ff4e-1587-4094-91ab-ae895be5744d","resolution":{"observed_at":"2026-08-05T22:43:49.341627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.426323Z","title":"P., Ordasi , A., Vink \\'o , J., & Wheeler , J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.426323Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:005fcc545089e66531fd59b43824ed6040182a864502cd48c864de5e6e2064ab","observation_id":"91d76808-dfdd-4fc2-be10-0443f302e2f2","resolution":{"observed_at":"2026-08-05T22:43:49.426323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.535564Z","title":"P., & Vink \\'o , J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.535564Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:464af32ee87593114ed49acb45bd04167cf2ddb075997f1aefb82cd332ac623a","observation_id":"3a0c433a-3c19-4093-a7a7-3758aa8afad8","resolution":{"observed_at":"2026-08-05T22:43:49.535564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.655854Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.655854Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:2ec70cc8ea9ade62f562822e1575536683cd97593d41718c094b16aa2ed5acbf","observation_id":"aea1f145-cdfd-414a-b5e3-70b48a9073ee","resolution":{"observed_at":"2026-08-05T22:43:49.655854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.773738Z","title":"R., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.773738Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:f7a4b0234879bab882b86b11f406bd5e9e2eaabe6cb61ebeb8de46677cbf1070","observation_id":"91710234-17d8-4d50-8b26-fb45dfe82d14","resolution":{"observed_at":"2026-08-05T22:43:49.773738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:49.909025Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:49.909025Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:2ed317511e5fce19e59d982a43fb8de2c430b5cd0468041dce572e3be5552dd1","observation_id":"74b77bd5-a129-4828-80ea-401595952350","resolution":{"observed_at":"2026-08-05T22:43:49.909025Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.001699Z","title":"2011, , 192, 3, 10.1088/0067-0049/192/1/3","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.001699Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:42581e42d44c4e4ccf6dea57b454f7a696ebb3be29b6475ccc2572ce61ff49d3","observation_id":"61d44ba9-2a34-4d9e-a87c-b739d7088122","resolution":{"observed_at":"2026-08-05T22:43:50.001699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.085355Z","title":"2013, , 208, 4, 10.1088/0067-0049/208/1/4","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.085355Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:5758e9a96ec958ae40a39655432e367777807d555a6c4706c780939c8bee1e71","observation_id":"cc1b52ce-8122-4b85-871b-e7ba9fdf7604","resolution":{"observed_at":"2026-08-05T22:43:50.085355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.114747Z","title":"2015, , 220, 15, 10.1088/0067-0049/220/1/15","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.114747Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:1360bead292c1fbec0698d5ebb035ae0dd1b01bd76491b97b38e5198e98ceb76","observation_id":"09ce4a35-57fb-411b-9056-fb7a0563e1ed","resolution":{"observed_at":"2026-08-05T22:43:50.114747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.203579Z","title":"B., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.203579Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:5ea89c392079c9fb903e6eff12df9214b57840c1864750f8274497c79c94da94","observation_id":"cf9eec23-3eaa-4baf-9f5e-cc9a53545e1e","resolution":{"observed_at":"2026-08-05T22:43:50.203579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.304763Z","title":"2019, , 243, 10, 10.3847/1538-4365/ab2241","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.304763Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:00e446846e11b60d568c35c60ccebdaa61b95b0216218477609697c400639f2d","observation_id":"e862f837-3ac6-46e9-a780-d72d46252b01","resolution":{"observed_at":"2026-08-05T22:43:50.304763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.374660Z","title":"L., & Shara , M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.374660Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:68fbb950183d6a5333e500d8410731c5cea319cf33e2fce5f9092c1880ecb565","observation_id":"9053cd5e-678b-443a-8500-397e20bcb9e3","resolution":{"observed_at":"2026-08-05T22:43:50.374660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10022","last_updated":"2023-09-18T18:00:00Z","snapshot_observed_at":"2026-08-16T14:59:42.331462Z","submitted_at":"2023-09-18T18:00:00Z","title":"The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss","version":1},"cited_work":{"arxiv_id":"2309.10022","doi":"10.48550/arxiv.2309.10022","metadata_source":"pith","pith_arxiv_id":"2309.10022","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss","venue":"astro-ph.SR","work_id":"911fdc33-10b9-4755-9699-dea2340a136a","year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.510640Z"},"links":{"cited_paper":"/paper/2309.10022","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:72875c40a921937e6dc90b87a27e46638abff01429c529b02bee80756deb4789","observation_id":"0124813a-65e7-4d81-a28b-1e9781d7614f","resolution":{"observed_at":"2026-08-05T22:43:52.928823Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.598238Z","title":"L., Villar , V","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.598238Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:e7b7000a09e76a0cd15cc72d12e5fe350ad8df42e194e1e228ddc2c18fa02597","observation_id":"17379a89-f599-472f-a336-45df6e6710b2","resolution":{"observed_at":"2026-08-05T22:43:50.598238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.709861Z","title":"G., Yuan , W., Macri , L","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.709861Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:c8246ef42203d33311f4a9aa529f4968913d9b679e78609fd3794543674da7cc","observation_id":"544a4a7e-76bd-463f-bc91-580388f782f3","resolution":{"observed_at":"2026-08-05T22:43:50.709861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:50.819276Z","title":"J., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.819276Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:ddc1e1e208ee20bf6270eac559e745f0b46fc14ffbb5bedac1dbc3270b5f33b9","observation_id":"6aff5702-814a-4660-8cea-69714a703ba0","resolution":{"observed_at":"2026-08-05T22:43:50.819276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.20989","last_updated":"2024-09-03T20:16:50Z","snapshot_observed_at":"2026-08-16T13:47:21.517998Z","submitted_at":"2024-05-31T16:34:50Z","title":"Unravelling the asphericities in the explosion and multi-faceted circumstellar matter of SN 2023ixf","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.20989","snapshot_observed_at":"2026-08-05T22:43:50.991505Z","title":"S., Moriya , T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:50.991505Z"},"links":{"cited_paper":"/paper/2405.20989","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:cd2ec3f5ff48b793fa4d57db841c069b66b1425eb62f6d05481370b570d1bd1a","observation_id":"097ed114-2ddd-46cd-9d0f-ee7724661a6f","resolution":{"observed_at":"2026-08-05T22:43:50.991505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:54.464599Z","title":"2023, The Astronomer's Telegram, 16050, 1","venue":null,"work_id":"1e9d9b6e-e379-4d85-b861-9faed2094a5a","year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.098768Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:445467f178a08ba1ee1478aaa5a2e7347429b063e3c7dd27f9dabedadeef50a7","observation_id":"fb9b8b33-a81e-40ba-a906-5ca6a8ec99a5","resolution":{"observed_at":"2026-08-05T22:43:54.537184Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.185876Z","title":"2019, , 876, 19, 10.3847/1538-4357/ab12d0","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.185876Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:a73e0c1f2be218dcf4393bd1a38d5c851914df98c3e3f01412bb9f0989a56112","observation_id":"0fa6dbe4-eeb4-483b-ac91-0a06c690fe7b","resolution":{"observed_at":"2026-08-05T22:43:51.185876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.296137Z","title":"S., Singh , A., Basu , J., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.296137Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:e5c61f04ed000a2db9d9b6fc0c3b3fb9af035e40e98e2bc58f734c86f6a83e19","observation_id":"591d0fe1-ad52-4958-bac0-bd7906ea761e","resolution":{"observed_at":"2026-08-05T22:43:51.296137Z","resolver_source":null,"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/psad041","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2023, , 75, L19, 10.1093/pasj/psad041","venue":"Publications of the Astronomical Society of Japan","work_id":"40f69b30-f3e3-4f56-936e-41861d43b07d","year":2023},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.346233Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:4cb5ae176c395dfc2bf2268ed2105f0b2a7eaf789ef879289ad7b1dcceb10380","observation_id":"fd7e9548-d85a-49df-8d72-0eb85e7aee71","resolution":{"observed_at":"2026-08-05T22:43:52.685370Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/pasj/psab063","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"2021, , 73, 1128, 10.1093/pasj/psab063","venue":"Publications of the Astronomical Society of Japan","work_id":"872c4339-445d-4066-8d9e-7184820df6c6","year":2021},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.470144Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:dc1ec46404e938857ef9a1fd655d16bf6dde86e23a382c0c1d51c62a0a6dbf41","observation_id":"5a9213c6-39cb-4735-9916-b93077f12daf","resolution":{"observed_at":"2026-08-05T22:43:52.490159Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.542702Z","title":"P., & Chugai , N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.542702Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:4fa1f0c34f028fa5959492aabe3c64d003c0476de8fbb62795e7fd73ab03b82d","observation_id":"5c2f8857-2a9d-40bc-ac63-bed534923fc0","resolution":{"observed_at":"2026-08-05T22:43:51.542702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.689862Z","title":"P., Chugai , N","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.689862Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:f292207881826ee4a1fdac58d855d5728f5c3b8b0db0dec003c1a5cf2a2f5f9c","observation_id":"0c9c73bd-cb5c-4fca-bd75-845d0219a34b","resolution":{"observed_at":"2026-08-05T22:43:51.689862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.754776Z","title":"2008, , 383, 1485, 10.1111/j.1365-2966.2007.12647.x","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.754776Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:0f3ca925f09d4221c773df724854fb6bd457caaa321aaf26deddf7a8c16d3e3e","observation_id":"a6acc340-138f-4910-8bb3-393be3a78d7a","resolution":{"observed_at":"2026-08-05T22:43:51.754776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.829409Z","title":"D., Srinivasan , S., Andrews , J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.829409Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:0bd78d4998957f9c6afdf86b4869e83e7ad73480034a890c3cba8a3babfba279","observation_id":"b4614f44-fcc4-444f-84f6-3ee0a627e833","resolution":{"observed_at":"2026-08-05T22:43:51.829409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.903166Z","title":"2024, Science China Physics, Mechanics, and Astronomy, 67, 219514, 10.1007/s11433-023-2267-0","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.903166Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:b6c158c927ba2b4655dff71069089eddce125c0ed2f97316e4032cf304903f3f","observation_id":"bdf9fb15-ed3f-46f2-870d-9eb6d6a36e58","resolution":{"observed_at":"2026-08-05T22:43:51.903166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:51.984347Z","title":"2024, , 969, 126, 10.3847/1538-4357/ad4be3","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:51.984347Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:4c45b5972342c6bab5156320ca19589e22856cca0df54ff3ff4af562d151bddc","observation_id":"23da9268-9937-48a9-835e-b4a8ab179b14","resolution":{"observed_at":"2026-08-05T22:43:51.984347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.13974","last_updated":"2025-03-18T07:22:56Z","snapshot_observed_at":"2026-08-16T12:49:05.768480Z","submitted_at":"2025-03-18T07:22:56Z","title":"SN 2023ixf in the Pinwheel Galaxy M101: From Shock Breakout to the Nebular Phase","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.13974","snapshot_observed_at":"2026-08-05T22:43:52.132320Z","title":"V., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:52.132320Z"},"links":{"cited_paper":"/paper/2503.13974","citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:ea13b7e2e20b02e0d4e87d83ce45bebe0954844ed121619b2be031b5c8e83faa","observation_id":"c51b259e-848b-48ae-9584-558dc7877de8","resolution":{"observed_at":"2026-08-05T22:43:52.132320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T22:43:52.232767Z","title":"A., Irani , I., Chen , P., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-05T22:43:52.232767Z"},"links":{"citing_paper":"/paper/2508.06654"},"observation_digest":"sha256:0120a20d207b3600a2056aad9778f51564ede8a21b13a9d5db816827e1b2b1b7","observation_id":"c4847acf-eb12-462c-9b8f-63e39b21332a","resolution":{"observed_at":"2026-08-05T22:43:52.232767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2508.06654","last_updated":"2025-08-08T19:12:42Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-19T20:30:37.152968Z","submitted_at":"2025-08-08T19:12:42Z","title":"SN 2023ixf in M101: physical parameters from bolometric light curve modeling"},"reference_resolution":{"displayed":70,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":59,"verified_exact":7,"verified_fuzzy":3},"total_outbound_references":70},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 70 of 70 outbound references and 0 inbound Pith citation observations for arXiv:2508.06654."}