{"as_of":"2026-08-19T22:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:954c5187497f688371196628748b02b111b11a0dd27cd85978b554c71e2787f2","coverage":[{"denominator":67,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":67,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T17:23:01.945785Z","state":"measured"},{"denominator":68,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":68,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-28T21:19:18.860667Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"cited_work":{"arxiv_id":"2508.12933","doi":"10.48550/arxiv.2508.12933","metadata_source":"arxiv_reference","pith_arxiv_id":"2508.12933","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"ArXiv.org","work_id":"a941f922-b0c4-4881-afad-292919e0eb94","year":null},"citing_paper":{"arxiv_id":"2606.00208","last_updated":"2026-05-29T18:00:00Z","snapshot_observed_at":"2026-08-02T12:42:48.778240Z","submitted_at":"2026-05-29T18:00:00Z","title":"JWST Reveals Large Reservoirs of Dust and Ongoing Circumstellar Interaction in SN Ibn/Icn 2023xgo over a Year Post-Explosion","version":1},"reference_index":193,"source":"arxiv_source","source_observed_at":"2026-06-28T21:19:18.860667Z"},"links":{"cited_paper":"/paper/2508.12933","citing_paper":"/paper/2606.00208"},"observation_digest":"sha256:223aa39d99e7c64417b80fca0896da12ed0ba76021a67da72056c7462ea394b8","observation_id":"5eb49de9-d218-4659-a181-cb00f46a7115","resolution":{"observed_at":"2026-06-28T21:22:38.591491Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2508.12933/citation-record","integrity":"/paper/2508.12933/integrity","json":"/paper/2508.12933/citation-record.json","paper":"/paper/2508.12933"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:01.336607Z","title":"G., Dwek, E., Kober, G., Rho, J., & Hwang, U","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.336607Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:b766e7ddf54dffe579b012127f2e0aa4b8097018b9f07d3d80d446a1e79f0ffe","observation_id":"9c451157-2e03-44da-b04b-b912d7f38bc4","resolution":{"observed_at":"2026-08-15T17:23:01.336607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/aae94f","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:03.462102Z","title":null,"venue":null,"work_id":"917da1e8-4981-41a3-9868-4f416e4a70fe","year":2018},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.343346Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:b2bb10b0d46e156938fb3a6b479cf0b5e22c72a6c3749ad28bbc9fbaa680226c","observation_id":"b73dcdd1-025a-4302-aef5-b6fe6517525f","resolution":{"observed_at":"2026-08-15T17:23:03.469848Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3390/molecules30081650","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:03.425572Z","title":"M., & Fortenberry, R","venue":null,"work_id":"3694c64b-7150-4181-af9d-728df5151500","year":2025},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.354437Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:11a7451408a6e5ace0cad30c8b5c6aaaca5e816ac5e298ae42236c015927ae44","observation_id":"97fa9edc-091f-4d5d-81de-bf50bc414e72","resolution":{"observed_at":"2026-08-15T17:23:03.432621Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.362811Z","title":"C., Orellana, M., Folatelli, G., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.362811Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:6f6d49142bf7da907011af3e7553f5f2af99d4f26148d2e624acff183b62a31e","observation_id":"4fff3cee-804c-414b-bf3a-8c76a35a71be","resolution":{"observed_at":"2026-08-15T17:23:01.362811Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.373766Z","title":"2009, The Astrophysical Journal, 703, 642, doi: 10.1088/0004-637X/703/1/642 Cˆ ot´ e, B., Jones, S., Herwig, F., & Pignatari, M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.373766Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:da03ba8285859ba3acaabe20d3081e779ea204c14298754273c2384ba4ffd461","observation_id":"4c4efad4-da75-4548-9f93-b8e909befeb1","resolution":{"observed_at":"2026-08-15T17:23:01.373766Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.384879Z","title":"2019, MNRAS, 484, 3921, doi: 10.1093/mnras/sty3415 De Looze, I., Barlow, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.384879Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:0020ef983f8407e366ae7809dac6716bf4842c59d9a634c3335d8c14e02212be","observation_id":"a7a3cd7c-d1ba-4f0d-a94a-27324d0b10e8","resolution":{"observed_at":"2026-08-15T17:23:01.384879Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.393134Z","title":"2011, ApJ, 727, 63, doi: 10.1088/0004-637X/727/2/63","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.393134Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:33d52d864ab9fb153df207ccd895626f19c5bf04817af9cdd2b1c51d2804e1ca","observation_id":"647da287-edff-4d80-99c8-8435ce7b5505","resolution":{"observed_at":"2026-08-15T17:23:01.393134Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.399669Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.399669Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:ce661c6612d3c7e52cf19a02b5268c0e38cafe40f10c431107841dfd196b386b","observation_id":"fdde61b1-274f-47c3-b9d3-dbf1af720026","resolution":{"observed_at":"2026-08-15T17:23:01.399669Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.406817Z","title":"2016, ApJ, 818, 124, doi: 10.3847/0004-637X/818/2/124","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.406817Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:01b190095c4b0887b64d510e235756fc0df1212c99a9781b0b64bd79ec5a4efa","observation_id":"08669223-bc74-4f57-9483-e7b2914c0e07","resolution":{"observed_at":"2026-08-15T17:23:01.406817Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.413420Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.413420Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:43ff21897ac03f561b010c805ec7ebc0d2fc179e7ab21537ca5ed5cd81020016","observation_id":"99a5011f-7973-4179-9ba7-34a07e65eff9","resolution":{"observed_at":"2026-08-15T17:23:01.413420Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.418678Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.418678Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:6f8a79ace0fd5a8c8138157c3bfecdc40889e69e7d3c9b7351f9cab2b83a7c4f","observation_id":"b06fbe7e-519a-4e76-9365-4c95d4650404","resolution":{"observed_at":"2026-08-15T17:23:01.418678Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.427128Z","title":"2014, Nature, 511, 326, doi: 10.1038/nature13558","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.427128Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:197309a1906a79204bbc4269fee44d55cf013bee7914b388b2baeb21e649c3d6","observation_id":"45eb8c24-86a5-4fe1-91a8-86536cdedd0b","resolution":{"observed_at":"2026-08-15T17:23:01.427128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202347546","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:03.211369Z","title":"R., Plane, J","venue":null,"work_id":"7a00ba2f-8c0d-4d9d-848d-82728918f230","year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.434117Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:3ebcd10d55c3e83ce0874845eb171f0454495232f5a1ecb51952319fe260edb9","observation_id":"c1c35173-4bba-440d-a912-839c7db01484","resolution":{"observed_at":"2026-08-15T17:23:03.238095Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.440010Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.440010Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:67bced6a79a4278727528f7be0e24eaeb4b8c80de519e41258b54e42ac9e5321","observation_id":"1307cfe8-e95f-40a2-a96b-f46cfe82ceb5","resolution":{"observed_at":"2026-08-15T17:23:01.440010Z","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":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.07874","snapshot_observed_at":"2026-08-15T17:23:01.448024Z","title":"A., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.448024Z"},"links":{"cited_paper":"/paper/2408.07874","citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:737a4baec113bb086f69558d4483a96306e9ff31b4a715d56675a8af9e6c63db","observation_id":"86430f8c-e68e-4cab-b9da-7bc379ef5a13","resolution":{"observed_at":"2026-08-15T17:23:01.448024Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.454355Z","title":"E., Pearson, J., Beasor, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.454355Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:b6384d40e0a9081af014e3632a47138407ea19e663d06d508f047bdde8525a8a","observation_id":"95d1dc21-5196-48d1-a37b-274091abd6d8","resolution":{"observed_at":"2026-08-15T17:23:01.454355Z","resolver_source":null,"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/stu2657","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:03.094939Z","title":"2015, MNRAS, 447, 3115, doi: 10.1093/mnras/stu2657","venue":null,"work_id":"d93f7dd1-3d8d-41a5-95cf-52c41a038593","year":2015},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.462567Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:3d10ab4c29ba92fc732ebc052d0c043de98d7aeffd4d38d990b83d763b6cfd29","observation_id":"c5b7d4b1-31e1-4c71-95a0-c0dd94138825","resolution":{"observed_at":"2026-08-15T17:23:03.101217Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.469363Z","title":"D., Foley, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.469363Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:bb5041b639df7eadb9c9072ec94283f27ea918d9ad8412be79401a2da6b268d5","observation_id":"94056273-f732-4000-8bc8-1f35dc2516fb","resolution":{"observed_at":"2026-08-15T17:23:01.469363Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.475809Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.475809Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:8d85ae8cae09f66dfe813d2c26267d5801889f634fc4e55b34b655752ec12e41","observation_id":"c6270d2f-a33a-41a9-ac7d-1f4baa560965","resolution":{"observed_at":"2026-08-15T17:23:01.475809Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.490425Z","title":"2021, Astronomy & Astrophysics, 656, A58, doi: 10.1051/0004-6361/202140506","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.490425Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:49661a5bdd0b620eed14f353bf68f1bf5e3d163728d6bd166d479ad7588d8035","observation_id":"6b258f37-03bd-4aac-ad6a-682f57b23089","resolution":{"observed_at":"2026-08-15T17:23:01.490425Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.495983Z","title":"2023, ApJL, 958, L37, doi: 10.3847/2041-8213/ad0da8","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.495983Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:cb43f5a5a3cdf2b616c0bddee4d1d87994c09107009aab1fca4ad8444483dc9d","observation_id":"737b54d1-fac8-48a3-8a46-95ee86328cfa","resolution":{"observed_at":"2026-08-15T17:23:01.495983Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.516414Z","title":"2017, Dust and Molecular Formation in Supernovae (Springer), 2125, doi: 10.1007/978-3-319-21846-5 130","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.516414Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:69e528b58e7a8cf94686f4e9fba505a58483786930242ad5c1e4e693e47b9f65","observation_id":"7f06019f-5114-448c-a8fa-d8ebf12ed061","resolution":{"observed_at":"2026-08-15T17:23:01.516414Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.524585Z","title":"2011, Science, 333, 1258, doi: 10.1126/science.1205983","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.524585Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:0ec7ee93598123a486efe34fc6a2c046968c27a5a71f7401d502f9e7f119d9b9","observation_id":"a6051dfa-e1df-4137-bf5f-133de5a30848","resolution":{"observed_at":"2026-08-15T17:23:01.524585Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.538472Z","title":"J., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.538472Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:b89b038b8ff28fd0c65f6c0b264b5e4f87dd855f83c23640fcb4624de511cfc5","observation_id":"ac6bbda8-d39a-4256-85ac-c5e2ee8c9e38","resolution":{"observed_at":"2026-08-15T17:23:01.538472Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.550970Z","title":"2003, A&A, 404, 975, doi: 10.1051/0004-6361:20030512","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.550970Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:9618ded9b0c833815bb4efcf11afabdc6d9bfd7d455c20d535beb0a9e4192f1a","observation_id":"065a003c-5dd6-464e-8780-37268bdca3a2","resolution":{"observed_at":"2026-08-15T17:23:01.550970Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.559150Z","title":"J., & Singh, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.559150Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:ad4b44869f9f031a196003546772db5a73c28d790d831b1931213803d642f35d","observation_id":"bd92ad08-a748-4e9b-beed-35cba758675f","resolution":{"observed_at":"2026-08-15T17:23:01.559150Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.566780Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.566780Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:a7c8e44ac128f0dae5f776d528a92584ab5c500db0649c8b69adc6850ba52d32","observation_id":"52b21cea-1fbf-4000-98ec-85bfd76b0e17","resolution":{"observed_at":"2026-08-15T17:23:01.566780Z","resolver_source":null,"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/stab932","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:02.888536Z","title":"2021, Monthly Notices of the Royal Astronomical Society, 504, 2133, doi: 10.1093/mnras/stab932","venue":null,"work_id":"dd377261-7b02-4b96-8ef2-a8f47af0ebb4","year":2021},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.576290Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:87b30f11b315c2e19b4f7dc86085a5f49f332bcc12fcde46ec2889415ec672e5","observation_id":"b7c2f8f1-e89a-49fe-afc9-564c16ca0980","resolution":{"observed_at":"2026-08-15T17:23:02.897988Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.592178Z","title":"R., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.592178Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:a3f26c5c84eb5f6e452c276f0583af808ed53e8c707af0b1ac83be55e88239a2","observation_id":"e53c3a6f-3322-4b63-8687-efdf84c1492c","resolution":{"observed_at":"2026-08-15T17:23:01.592178Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.598972Z","title":"J., & Barlow, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.598972Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:081bb21465e66ea002c923910946f770687b13b7df7f742e9fec3b0e44132ad9","observation_id":"117d20c3-babf-463d-ab34-7c25370c472a","resolution":{"observed_at":"2026-08-15T17:23:01.598972Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.605985Z","title":"2011, ApJS, 192, 3, doi: 10.1088/0067-0049/192/1/3","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.605985Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:e74fd5919d7bf4ec7c42856bd999232a99de8d17d838a6369df8ef5456ac2657","observation_id":"d08dc8bc-8759-4c11-b9bc-73dbc0fcd148","resolution":{"observed_at":"2026-08-15T17:23:01.605985Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.611844Z","title":"2013, ApJS, 208, 4, doi: 10.1088/0067-0049/208/1/4","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.611844Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:9c2f293854d385e76fdbf1db87b0d15da08096be2b02da9486076db3e3f0da33","observation_id":"6ddf209a-085d-43f6-a530-c6196d39d396","resolution":{"observed_at":"2026-08-15T17:23:01.611844Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.622673Z","title":"2015, ApJS, 220, 15, doi: 10.1088/0067-0049/220/1/15","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.622673Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:9113ffda72209a57a6faa5828da84df3fc9e0a04b7cb624302d996318911988b","observation_id":"689db86e-6240-4306-a162-3c5725ddba27","resolution":{"observed_at":"2026-08-15T17:23:01.622673Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.631136Z","title":"L., & Shara, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.631136Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:c26acd7cc258902359059a9320e3d9cfb633d9574e849c3778d4a1e9a5318341","observation_id":"e8045406-347e-4dd4-b48c-5bec0f0819fc","resolution":{"observed_at":"2026-08-15T17:23:01.631136Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.642279Z","title":"2024, MNRAS, 534, 271, doi: 10.1093/mnras/stae2012","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.642279Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:66b68efc6d80d780c570356f7087a51514da4e899a49fbc2570ef16376a76dff","observation_id":"04f5c661-6b49-49ac-b9c0-fb68bfec4d9d","resolution":{"observed_at":"2026-08-15T17:23:01.642279Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:03.753881Z","title":"A., Jacobson-Galan, W., Kilpatrick, C., & Tartaglia, A","venue":null,"work_id":"960fa7bd-dc6a-4c09-8841-13b05f0c9248","year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.649673Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:bd50f8b46dd37ede7b1318d568f84683bc0a95ffffb29f5a5a6fb0251da50abb","observation_id":"233080cf-f65d-4aa6-9183-306820a078ed","resolution":{"observed_at":"2026-08-15T17:23:03.763992Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.661122Z","title":"D., & Woosley, S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.661122Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:de3cd4408168df6474f3c7f2367dcc6f08eef53f523c09ef49b61cf04cf56ea9","observation_id":"288a87f6-2954-48ae-b146-c4c86adfbf7a","resolution":{"observed_at":"2026-08-15T17:23:01.661122Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.669710Z","title":"R., Banerjee, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.669710Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:20a47907e4e99d084a6b3dd1c08e6b4219ded9b7fa865f8bbd08f9afcef16530","observation_id":"ed34b1e8-57b6-4b6c-aada-98d86a9b6354","resolution":{"observed_at":"2026-08-15T17:23:01.669710Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.675545Z","title":"R., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.675545Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:748ebf9cecd652f62399d3911bfcf0c92380c0fe13c3e62b090bb32183f29a6e","observation_id":"c2fec590-9333-42ed-9bf3-ecde426d1516","resolution":{"observed_at":"2026-08-15T17:23:01.675545Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.682387Z","title":"2024, MNRAS, 533, 687, doi: 10.1093/mnras/stae1778","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.682387Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:4efaf4d613989dfae659eab69eca0d0ec4830315ebad8afc8e688f9f53891ec3","observation_id":"43a0bd81-cdd5-4961-a844-4a52fa3aeeba","resolution":{"observed_at":"2026-08-15T17:23:01.682387Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.690077Z","title":"E., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.690077Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:e54ab8a962f5ca6859b164966e2b81b2408fffa67f37d609eca50b32580384e7","observation_id":"dec08c78-3a76-475c-aa16-0027b2b6692e","resolution":{"observed_at":"2026-08-15T17:23:01.690077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14896","last_updated":"2022-12-07T10:31:54Z","snapshot_observed_at":"2026-08-18T11:55:08.975552Z","submitted_at":"2022-09-29T16:03:15Z","title":"Formation, distribution, and IR emission of dust in the clumpy ejecta of Type II-P core-collapse supernovae, in isotropic and anisotropic scenarios","version":2},"cited_work":{"arxiv_id":"2209.14896","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.14896","snapshot_observed_at":"2026-08-15T17:23:03.559356Z","title":"Formation, distribution, and IR emission of dust in the clumpy ejecta of Type II-P core-collapse supernovae, in isotropic and anisotropic scenarios","venue":"astro-ph.SR","work_id":"960c3976-5130-4901-b819-9706db26edbf","year":2022},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.699453Z"},"links":{"cited_paper":"/paper/2209.14896","citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:1345219b5346b4420a59ee8468d6c9b3f809f0e1faaaebdeffe4d71e468a5cc2","observation_id":"d4b1315c-be97-488d-8461-2bedb0d3c7eb","resolution":{"observed_at":"2026-08-15T17:23:03.569773Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.705470Z","title":"2013, The Astrophysical Journal, 776, 107, doi: 10.1088/0004-637X/776/2/107","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.705470Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:69239ee69a545bd201378641f41149d96df127c6a47ae4ab8696b9d1b027704c","observation_id":"7c459574-2268-4d24-9449-fcb4d0692e1b","resolution":{"observed_at":"2026-08-15T17:23:01.705470Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.714318Z","title":"2015, A&A, 575, A95, doi: 10.1051/0004-6361/201424969","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.714318Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:75373db93c80510611eaa5f28b1eaaca227f61f381c4c624036439bf4f0a13df","observation_id":"f65b6e43-eefc-471c-9c06-c6373cde843e","resolution":{"observed_at":"2026-08-15T17:23:01.714318Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.720232Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.720232Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:41d37aceb4a3346f540e5f1cc0760080c6c919daa31127933193178b04c6f6c3","observation_id":"ec019b96-3866-48a2-b285-4bde8230d5c3","resolution":{"observed_at":"2026-08-15T17:23:01.720232Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.725356Z","title":"2025, arXiv e-prints, arXiv:2504.20574, doi: 10.48550/arXiv.2504.20574","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.725356Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:c67f39040133dfd0a3cf121a321840b7a92aa1d5134c93d258c2ed6ff34177c8","observation_id":"08ff4a77-ca60-4663-bebe-945314f21760","resolution":{"observed_at":"2026-08-15T17:23:01.725356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.00053","last_updated":"2024-01-31T13:01:29Z","snapshot_observed_at":"2026-08-18T22:17:48.784633Z","submitted_at":"2023-09-29T18:00:03Z","title":"The formation and cosmic evolution of dust in the early Universe. I. Dust sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.00053","snapshot_observed_at":"2026-08-15T17:23:01.733569Z","title":"2023, http://arxiv.org/abs/2310.00053","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.733569Z"},"links":{"cited_paper":"/paper/2310.00053","citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:e15456d260dec4ee566833cef48cb37fc4ddd143463f546c761ab8e4bbc40c78","observation_id":"961d1ce8-40e5-4491-9eee-ef926f75d311","resolution":{"observed_at":"2026-08-15T17:23:01.733569Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.746371Z","title":"2023, MNRAS, 523, 6048, doi: 10.1093/mnras/stad1681","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.746371Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:44ec0b9e5250a3e8f70496f95e77146f2773d134240aee7df670744f6f7d586a","observation_id":"931a9274-53dd-458e-a2c9-3f0db3cf5127","resolution":{"observed_at":"2026-08-15T17:23:01.746371Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.755582Z","title":"D., Temim, T., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.755582Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:837aef55777ba8154a58d68559f4dfa51ef0626c940ff186ebc4fd214561fca4","observation_id":"2ec410e2-8837-4e6c-8be6-b5443a925d98","resolution":{"observed_at":"2026-08-15T17:23:01.755582Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.772198Z","title":"S., Moriya, T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.772198Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:7b2dca2807ad2026a058c5c7a89c63a0a9d2e7264525e42e849703b327f9dd85","observation_id":"e11274d5-3798-4d41-96a6-f3ced40ad1d5","resolution":{"observed_at":"2026-08-15T17:23:01.772198Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.779273Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.779273Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:432d83491244c4908c122f8e4ba94dd4d3e9b8f9abf806280051427998103bd1","observation_id":"b4589d4b-2f48-46cd-bafd-ac3c0b5993ff","resolution":{"observed_at":"2026-08-15T17:23:01.779273Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.785342Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.785342Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:d9318cc2a6875dca674c11f31c060223fae9b5295d786241a2ab3e17f895e550","observation_id":"51b32cfb-9d72-42b1-bdc9-f36125a28c04","resolution":{"observed_at":"2026-08-15T17:23:01.785342Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:03.720888Z","title":"2023, The Astronomer’s Telegram, 16050, 1","venue":null,"work_id":"21a1ddec-ea47-41c9-836d-995ebdf6c6b2","year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.790622Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:45334071355542bf7f6d6120cae3ab44afc7e5d12b5cb03ff803b83f52d7db0c","observation_id":"22e58a19-ecb4-48d7-ab75-b5c9e2dcc3ee","resolution":{"observed_at":"2026-08-15T17:23:03.730112Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.802787Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.802787Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:0e34bb25a7b1958f38914fdfb39ab4654c914db5db6115353d318c7b3b8824ee","observation_id":"4b5ad5f2-dabb-48db-927e-7ce1c5fa7c84","resolution":{"observed_at":"2026-08-15T17:23:01.802787Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.808761Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.808761Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:45c5d0e5908ea002d0af2048b013a1ee620b15f527a7fae4cbf65adb16b8f942","observation_id":"82ffcb7f-2f8f-4280-8371-d8c7b679366e","resolution":{"observed_at":"2026-08-15T17:23:01.808761Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.822966Z","title":"E., & Heger, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.822966Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:fb93205823c48d8980df4c3277482ff2f7bd3a0b44ad6ca50598e7165c1c0fb4","observation_id":"7b5df390-c08e-47b1-b962-61ef368980e9","resolution":{"observed_at":"2026-08-15T17:23:01.822966Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.830227Z","title":"D., Pejcha, O., & M¨ uller, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.830227Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:b54d5b5bc98906eec972c724314261137fcaa14613160236aa1511f87e5c9c5a","observation_id":"f64f8736-bd39-4a22-b392-c46b22ccb1b4","resolution":{"observed_at":"2026-08-15T17:23:01.830227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.12950","last_updated":"2025-03-17T09:03:23Z","snapshot_observed_at":"2026-08-18T11:55:09.509692Z","submitted_at":"2025-03-17T09:03:23Z","title":"JWST/MIRI detects the dusty SN1993J about 30 years after explosion","version":1},"cited_work":{"arxiv_id":"2503.12950","doi":"10.48550/arxiv.2503.12950","metadata_source":"pith","pith_arxiv_id":"2503.12950","snapshot_observed_at":"2026-08-15T18:16:14.067578Z","title":"JWST/MIRI detects the dusty SN1993J about 30 years after explosion","venue":"astro-ph.SR","work_id":"b8a6adce-07c2-490c-bdf0-869f06c975bf","year":2025},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.837617Z"},"links":{"cited_paper":"/paper/2503.12950","citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:b456e3717caa0ad049e1f872a3b93704ca14a1fb3d55a184a1395959a415fa91","observation_id":"03af2649-f798-4c04-878a-27cce39d5d05","resolution":{"observed_at":"2026-08-15T17:23:02.221098Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.844873Z","title":"G., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.844873Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:f97a4dec76d6469436ad98592ee79984fc488257f82fff965829d7241f5e80a6","observation_id":"25804277-1859-4c30-acfd-f14da978721b","resolution":{"observed_at":"2026-08-15T17:23:01.844873Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.851003Z","title":"A., Zimmerman, G","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.851003Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:edcdd38f23c177e4e642b0f61bfc0e99b218ff0c7f4e6203557e79fdb2ed5615","observation_id":"f529d2c8-1df5-4dc1-8a32-96571ee75561","resolution":{"observed_at":"2026-08-15T17:23:01.851003Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.860613Z","title":"2021, ApJ, 923, 148, doi: 10.3847/1538-4357/ac2eb8","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.860613Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:6954a0868aa32346c127ef09014bfc9d47abb19bae3cb20c0b85df5cd55786cb","observation_id":"fe1f9e1a-1b78-46b9-942c-93cf57621320","resolution":{"observed_at":"2026-08-15T17:23:01.860613Z","resolver_source":null,"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/stad2505","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:23:02.093320Z","title":"M., Barlow, M","venue":null,"work_id":"43db8418-982c-4ea4-a17f-98eee4c7e6e7","year":2023},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.876156Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:0f3c623f5c4d81825bdafdb2967f60f9525d5f37f3e95ef73bf0772815da7c37","observation_id":"1a3c9ba6-5b12-42cf-838a-d843d279c62b","resolution":{"observed_at":"2026-08-15T17:23:02.102777Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.887677Z","title":"E., & Heger, A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.887677Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:27e274c2d964341ff1a8f52c38d870751f2933d814b42301060aa49bd358cbad","observation_id":"86e61a19-b0d4-4857-aa05-7cc3569162bc","resolution":{"observed_at":"2026-08-15T17:23:01.887677Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.898547Z","title":"E., Heger, A., & Weaver, T","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.898547Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:c3576c59667f00d32938ded75012db70315d70c7097536df1fa68c84cf076690","observation_id":"9427790a-8726-4dae-9c25-0088d4b28b95","resolution":{"observed_at":"2026-08-15T17:23:01.898547Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:01.922609Z","title":"E., & Weaver, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.922609Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:5985004f54be269e4ae60704a8116a7f07fd06c76eb41d7da4c104ef0a819512","observation_id":"be987ba3-bd7f-4cea-b224-2b7ce8e376b1","resolution":{"observed_at":"2026-08-15T17:23:01.922609Z","resolver_source":null,"status":"unresolved"},"standing_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":"2026-08-15T17:23:03.692770Z","title":"2024, Science China","venue":null,"work_id":"3df5392a-7714-4c18-bc23-ff2f1aee6b50","year":2024},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.933184Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:713f191766a0893273c88574521aabe53822d2a8abbbc7e47ca15a45b9075f4e","observation_id":"eda4698b-865c-47fc-8eda-e7340c41edbc","resolution":{"observed_at":"2026-08-15T17:23:03.702248Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-15T17:23:01.945785Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T17:23:01.945785Z"},"links":{"citing_paper":"/paper/2508.12933"},"observation_digest":"sha256:3c6450cef39de70d503da1c648d5cbef2b10153fbc0a5ee18bd35e6165a8291f","observation_id":"c02d73c8-8f77-4df9-a9fb-53ae073ed8c2","resolution":{"observed_at":"2026-08-15T17:23:01.945785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2508.12933","last_updated":"2025-08-18T13:56:56Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-19T09:18:51.221219Z","submitted_at":"2025-08-18T13:56:56Z","title":"Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors"},"reference_resolution":{"displayed":67,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":56,"verified_exact":6,"verified_fuzzy":3},"total_outbound_references":67},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 67 of 67 outbound references and 1 inbound Pith citation observation for arXiv:2508.12933."}