{"as_of":"2026-08-13T10:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a1269b70a913ef8eb6069d0cd29553e23d5cec50447de27a2ecd86c24cb3a77e","coverage":[{"denominator":114,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T20:25:19.982756Z","state":"measured"},{"denominator":102,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":102,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T23:39:20.793832Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-11T22:51:21.568198Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"cited_work":{"arxiv_id":"2411.09740","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.09740","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"D., 1982, ApJ, 253, 785 Astier P., et al., 2006, A&A, 447, 31 AubourgÉ.,TojeiroR.,JimenezR.,HeavensA.,StraussM.A.,SpergelD.N., 2008, A&A, 492, 631 Baldry I","venue":null,"work_id":"34c0f483-3da9-4f67-83f9-59195f76ebc4","year":1982},"citing_paper":{"arxiv_id":"2604.24846","last_updated":"2026-04-27T18:00:01Z","snapshot_observed_at":"2026-07-06T23:10:47.277692Z","submitted_at":"2026-04-27T18:00:01Z","title":"SN Ia Population Machine. I. A Unified Cosmological Simulation-Binary Synthesis Framework Establishing Non-universal Delay-time Distributions and Cosmic Progenitor-channel Dominance Crossover","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-08T02:22:08.336205Z"},"links":{"cited_paper":"/paper/2411.09740","citing_paper":"/paper/2604.24846"},"observation_digest":"sha256:382716da9f3394f0123b6b53452670d173392a7ae2a883c1e8ba697e25054a22","observation_id":"4c638393-ee94-499d-be26-c03a702dc136","resolution":{"observed_at":"2026-05-11T22:51:21.578753Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09740","snapshot_observed_at":"2026-08-05T23:39:20.793832Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.03205","last_updated":"2026-08-04T06:47:15Z","snapshot_observed_at":"2026-08-13T03:17:31.314702Z","submitted_at":"2026-08-04T06:47:15Z","title":"One year of broadband radio monitoring of the enigmatic transient GRB 250702B reveals the evolution of the relativistic jet","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-05T23:39:20.793832Z"},"links":{"cited_paper":"/paper/2411.09740","citing_paper":"/paper/2608.03205"},"observation_digest":"sha256:281a70f74aded789d40ccfeea1ac0947ebde6e892f4a83ec00af292822957225","observation_id":"d3cce9c2-98e5-4794-a939-89af621d885e","resolution":{"observed_at":"2026-08-05T23:39:20.793832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2411.09740/citation-record","integrity":"/paper/2411.09740/integrity","json":"/paper/2411.09740/citation-record.json","paper":"/paper/2411.09740"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T20:25:19.559961Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.559961Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:207e21fe78053cac117d72f06dafc7045a967500eadbf19faebc6495a1223e32","observation_id":"0f50852b-b02f-4c7a-adc3-b17d4ba1ab28","resolution":{"observed_at":"2026-08-12T20:25:19.559961Z","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":"2026-08-12T20:25:19.566194Z","title":"( year 2004 ), month Apr","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.566194Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:a0068a2af28ff54ca3d757ed5ff49ef523ff57c6c07d2a78c5ef0b5b83115083","observation_id":"486a1a69-12f5-4ebe-951d-407dfbfe4714","resolution":{"observed_at":"2026-08-12T20:25:19.566194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06016","last_updated":"2023-05-25T11:14:45Z","snapshot_observed_at":"2026-07-06T12:46:48.184877Z","submitted_at":"2022-03-11T15:38:06Z","title":"Astrophysics with the Laser Interferometer Space Antenna","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06016","snapshot_observed_at":"2026-08-12T20:25:19.571340Z","title":"( year 2023 ), month Mar","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.571340Z"},"links":{"cited_paper":"/paper/2203.06016","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:44c797adc3b924248e853d04b8822cff80aefc7b35678a598c4bcaa5580564d0","observation_id":"774bbc6e-c5a4-4121-b315-1ca0ca9854cf","resolution":{"observed_at":"2026-08-12T20:25:19.571340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.04621","last_updated":"2024-05-16T16:49:58Z","snapshot_observed_at":"2026-08-13T05:07:41.947592Z","submitted_at":"2023-12-07T19:00:00Z","title":"Detecting strongly-lensed type Ia supernovae with LSST","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.04621","snapshot_observed_at":"2026-08-12T20:25:19.576125Z","title":"( year 2024 ), month Jul","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.576125Z"},"links":{"cited_paper":"/paper/2312.04621","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:c751be8f00d61a4d94e843b865512f9f15c851085c1e83efce58e6ca2610842c","observation_id":"056aa28b-e01b-497a-860f-d10d4c710138","resolution":{"observed_at":"2026-08-12T20:25:19.576125Z","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":"2026-08-12T20:25:19.580591Z","title":"title On the theory of Type I supernovae","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.580591Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f20c8d38d9defcf780ab0ac8af4624f1a4e96e15597834d0f68555a28de6071f","observation_id":"52175c0e-1c5d-4cac-9a3e-823e0bcbf406","resolution":{"observed_at":"2026-08-12T20:25:19.580591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703321","last_updated":"2007-03-13T15:42:36Z","snapshot_observed_at":"2026-07-07T01:08:03.830352Z","submitted_at":"2007-03-13T15:42:36Z","title":"Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703321","snapshot_observed_at":"2026-08-12T20:25:19.584965Z","title":"title Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants? journal volume 662 ( number 1 ): pages 472--486","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.584965Z"},"links":{"cited_paper":"/paper/astro-ph/0703321","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:b8f3a8095c539432819b8b2fbb7c09bafd1ee9356a18363d8988b73d12b4f026","observation_id":"b747e56d-cc63-43a9-a2f3-63d4422adfe4","resolution":{"observed_at":"2026-08-12T20:25:19.584965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01206","last_updated":"2022-11-02T15:35:25Z","snapshot_observed_at":"2026-08-13T09:53:03.749879Z","submitted_at":"2022-11-02T15:35:25Z","title":"Type Ia Supernova cosmology combining data from the $Euclid$ mission and the Vera C. Rubin Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.01206","snapshot_observed_at":"2026-08-12T20:25:19.590944Z","title":"title Type Ia supernova observations combining data from the Euclid mission and the Vera C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.590944Z"},"links":{"cited_paper":"/paper/2211.01206","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:df6a10f0d4695b69ff7dc7800f3d897d4c566a2ceb778dc337e2c50ac4c116ea","observation_id":"cec5f191-b978-4641-9894-1ec70a1d22f1","resolution":{"observed_at":"2026-08-12T20:25:19.590944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.01932","last_updated":"2019-02-05T21:59:02Z","snapshot_observed_at":"2026-07-06T07:31:22.027427Z","submitted_at":"2019-02-05T21:59:02Z","title":"The Zwicky Transient Facility: System Overview, Performance, and First Results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.01932","snapshot_observed_at":"2026-08-12T20:25:19.595737Z","title":"( year 2019 ), month Jan","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.595737Z"},"links":{"cited_paper":"/paper/1902.01932","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:ad6e7ebe72ca0f1713dd5160cf495f56addd54228b8d193324212e1c8b844c2c","observation_id":"b31da5da-f772-4daf-b2c1-91ffabca9d5e","resolution":{"observed_at":"2026-08-12T20:25:19.595737Z","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":"2026-08-12T20:25:19.599917Z","title":"title Three-dimensional Hydrodynamical Simulations of Stellar Collision","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.599917Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:efba5b541b8bdcfc36ac1076b5b26b849780f43656ee488a5379c631004a6501","observation_id":"02ec182c-57ab-4f77-84b5-e97478997c93","resolution":{"observed_at":"2026-08-12T20:25:19.599917Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.5892","last_updated":"2012-11-26T09:11:38Z","snapshot_observed_at":"2026-07-06T03:00:37.937554Z","submitted_at":"2012-11-26T09:11:38Z","title":"One-dimensional delayed-detonation models of Type Ia supernovae: Confrontation to observations at bolometric maximum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.5892","snapshot_observed_at":"2026-08-12T20:25:19.604092Z","title":"title One-dimensional delayed-detonation models of Type Ia supernovae: confrontation to observations at bolometric maximum","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.604092Z"},"links":{"cited_paper":"/paper/1211.5892","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:36876e33421235b2b4fc971724c19644fe2a3e6b93af9e0342bd2ace85d5db63","observation_id":"c416fdfc-1ad0-41b1-b180-e30087cda32e","resolution":{"observed_at":"2026-08-12T20:25:19.604092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.06583","last_updated":"2015-02-12T21:56:06Z","snapshot_observed_at":"2026-07-06T04:07:18.801799Z","submitted_at":"2015-01-26T21:00:21Z","title":"A one-dimensional Chandrasekhar-mass delayed-detonation model for the broad-lined Type Ia supernova 2002bo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.06583","snapshot_observed_at":"2026-08-12T20:25:19.608598Z","title":"title A one-dimensional Chandrasekhar-mass delayed-detonation model for the broad-lined Type Ia supernova 2002bo","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.608598Z"},"links":{"cited_paper":"/paper/1501.06583","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:5c0a0998bfe35ebf0aa908df56aeeeb063a109fb5da67d4c2532665d22caf661","observation_id":"45019dfb-c5c0-443c-bb7d-277b7c38f655","resolution":{"observed_at":"2026-08-12T20:25:19.608598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01901","last_updated":"2017-06-06T18:01:00Z","snapshot_observed_at":"2026-08-05T08:18:29.890077Z","submitted_at":"2017-06-06T18:01:00Z","title":"Evidence for sub-Chandrasekhar-mass progenitors of Type Ia supernovae at the faint end of the width-luminosity relation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01901","snapshot_observed_at":"2026-08-12T20:25:19.612629Z","title":"title Evidence for sub-Chandrasekhar-mass progenitors of Type Ia supernovae at the faint end of the width-luminosity relation","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.612629Z"},"links":{"cited_paper":"/paper/1706.01901","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f15cffcd2b48c1e237815cea3540e56fca43e73b80c311f3792c83975914fc68","observation_id":"872d480a-b251-491f-adb6-9b1fd90a4194","resolution":{"observed_at":"2026-08-12T20:25:19.612629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.11671","last_updated":"2023-04-15T14:03:40Z","snapshot_observed_at":"2026-08-02T03:59:47.489665Z","submitted_at":"2022-09-23T16:00:38Z","title":"StaNdaRT: A repository of standardized test models and outputs for supernova radiative transfer","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.11671","snapshot_observed_at":"2026-08-12T20:25:19.616648Z","title":"( year 2022 a ), month Dec","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.616648Z"},"links":{"cited_paper":"/paper/2209.11671","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:2f3a7b5bc6f72a9561e40066de7dce1b4d1f593d6e77a3b65518e6009d7d9a0f","observation_id":"46f6466c-cb3b-438a-968c-987b67a63108","resolution":{"observed_at":"2026-08-12T20:25:19.616648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.13840","last_updated":"2022-03-23T17:05:39Z","snapshot_observed_at":"2026-08-03T19:51:07.628095Z","submitted_at":"2021-09-28T16:16:19Z","title":"Stable nickel production in Type Ia supernovae: A smoking gun for the progenitor mass?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.13840","snapshot_observed_at":"2026-08-12T20:25:19.620688Z","title":"title Stable nickel production in type Ia supernovae: A smoking gun for the progenitor mass? journal volume 660 , eid A96","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.620688Z"},"links":{"cited_paper":"/paper/2109.13840","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:3fd1c37c12780ec076e39b964fa536b568b7fed241320d38f7c2a090dfe70bcd","observation_id":"3869a231-cc75-4411-aff1-70677be65561","resolution":{"observed_at":"2026-08-12T20:25:19.620688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.07116","last_updated":"2023-10-18T08:34:37Z","snapshot_observed_at":"2026-08-04T13:55:42.794737Z","submitted_at":"2023-06-12T13:44:28Z","title":"Nebular spectra from Type Ia supernova explosion models compared to JWST observations of SN 2021aefx","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.07116","snapshot_observed_at":"2026-08-12T20:25:19.624736Z","title":"title Nebular spectra from Type Ia supernova explosion models compared to JWST observations of SN 2021aefx","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.624736Z"},"links":{"cited_paper":"/paper/2306.07116","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:d46915f1b7fdd77373e04b61454455c26e7219c98169e226f43ed419306cef16","observation_id":"4678b504-18fc-49a5-9009-b53035e9c15d","resolution":{"observed_at":"2026-08-12T20:25:19.624736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.0966","last_updated":"2011-11-03T20:00:00Z","snapshot_observed_at":"2026-07-06T02:36:57.502545Z","submitted_at":"2011-11-03T20:00:00Z","title":"A Compact Degenerate Primary-Star Progenitor of SN 2011fe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.0966","snapshot_observed_at":"2026-08-12T20:25:19.628773Z","title":"( year 2012 ), month Jan","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.628773Z"},"links":{"cited_paper":"/paper/1111.0966","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:40f2b90118c85b68649912e22a1555c98efa917076089a65a4b9d8d4f3b733c7","observation_id":"10872ca7-650d-4d91-a1e7-af1da2b6a7f8","resolution":{"observed_at":"2026-08-12T20:25:19.628773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.07181","last_updated":"2017-08-23T20:31:13Z","snapshot_observed_at":"2026-07-06T05:56:28.436463Z","submitted_at":"2017-08-23T20:31:13Z","title":"X-ray Emission from SN 2012ca: A Type Ia-CSM Supernova Explosion in a Dense Surrounding Medium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.07181","snapshot_observed_at":"2026-08-12T20:25:19.632703Z","title":"title X-ray emission from SN 2012ca: A Type Ia-CSM supernova explosion in a dense surrounding medium","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.632703Z"},"links":{"cited_paper":"/paper/1708.07181","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:133b120a76d6c3de6c2d41fa3e95f6677b3c01ed074d64ebbedf21b211539bb8","observation_id":"022d091d-3b34-412e-8c57-3c0393c9ca66","resolution":{"observed_at":"2026-08-12T20:25:19.632703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.08486","last_updated":"2020-04-22T14:10:32Z","snapshot_observed_at":"2026-08-12T13:43:36.871460Z","submitted_at":"2020-02-19T22:45:26Z","title":"The accuracy of post-processing nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.08486","snapshot_observed_at":"2026-08-12T20:25:19.636570Z","title":"title The accuracy of post-processed nucleosynthesis","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.636570Z"},"links":{"cited_paper":"/paper/2002.08486","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f8c171a9e2cb9cd8a106f639abb4af9427555d29aa496f5c1f5d735673813f23","observation_id":"ff37965c-a776-419a-a25f-3bef6c30c471","resolution":{"observed_at":"2026-08-12T20:25:19.636570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1981","last_updated":"2012-04-09T20:05:42Z","snapshot_observed_at":"2026-07-06T02:46:02.046654Z","submitted_at":"2012-04-09T20:05:42Z","title":"Sensitivity study of explosive nucleosynthesis in Type Ia supernovae: I. Modification of individual thermonuclear reaction rates","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.1981","snapshot_observed_at":"2026-08-12T20:25:19.640559Z","title":"title Sensitivity study of explosive nucleosynthesis in type Ia supernovae: Modification of individual thermonuclear reaction rates","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.640559Z"},"links":{"cited_paper":"/paper/1204.1981","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:272007985ea33b1f84a50919e3d6be9f74d9ae4fb3cf3a54acdf4ece3781fb02","observation_id":"d0562e37-a85f-4450-b8d6-eda73e53f91d","resolution":{"observed_at":"2026-08-12T20:25:19.640559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.04020","last_updated":"2022-09-08T20:13:51Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T20:13:51Z","title":"Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.04020","snapshot_observed_at":"2026-08-12T20:25:19.644602Z","title":"title Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.644602Z"},"links":{"cited_paper":"/paper/2209.04020","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:9239cc17897687962f7da3ad549033ea06e55fa9bfb6b7109d395c5b7935ed2a","observation_id":"b5791bee-5431-456d-a8a8-8bbb67275e1a","resolution":{"observed_at":"2026-08-12T20:25:19.644602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.04128","last_updated":"2015-10-14T14:54:30Z","snapshot_observed_at":"2026-07-06T04:33:04.383786Z","submitted_at":"2015-10-14T14:54:30Z","title":"Type Ia supernovae from violent mergers of carbon-oxygen white dwarfs: polarisation signatures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.04128","snapshot_observed_at":"2026-08-12T20:25:19.649317Z","title":"title Type Ia supernovae from violent mergers of carbon-oxygen white dwarfs: polarization signatures","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.649317Z"},"links":{"cited_paper":"/paper/1510.04128","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:84adb7c5f3b53c9bd97bbf817702ee489267417c107fe3edaf8a856f21a06272","observation_id":"ba2ff595-d099-458e-a7cd-b0a93bea051b","resolution":{"observed_at":"2026-08-12T20:25:19.649317Z","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":"2026-08-12T20:25:19.653387Z","title":"title The Maximum Mass of Ideal White Dwarfs","venue":null,"work_id":null,"year":1931},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.653387Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:432d2658cb1f7921c545f550ba0fb9fa4c7a815e5c55acc7652a9c41bf4b0c4b","observation_id":"18ff0987-a021-480d-94cc-5d3747078d4c","resolution":{"observed_at":"2026-08-12T20:25:19.653387Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3332","last_updated":"2017-06-12T21:31:38Z","snapshot_observed_at":"2026-08-10T08:18:57.175087Z","submitted_at":"2014-05-14T00:02:44Z","title":"Cobalt-56 gamma-ray emission lines from the type Ia supernova 2014J","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3332","snapshot_observed_at":"2026-08-12T20:25:19.657518Z","title":"( year 2014 ), month Aug","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.657518Z"},"links":{"cited_paper":"/paper/1405.3332","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:5a14af2c3d67ebfcc9f510dcad462dc49735c6dcb8de96b62b81c6ef2fe05b23","observation_id":"a541d730-bcae-4bf8-be51-f2a6e913a87f","resolution":{"observed_at":"2026-08-12T20:25:19.657518Z","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":"2026-08-12T20:25:19.661754Z","title":"title Early Supernova Luminosity","venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.661754Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:5c00d0d8d5563de202d4fc904890726208958f56f5143db8999d57822832f336","observation_id":"4e472819-8813-4788-b3ba-33e9d7cb162a","resolution":{"observed_at":"2026-08-12T20:25:19.661754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.7750","last_updated":"2014-03-06T08:21:36Z","snapshot_observed_at":"2026-07-06T03:26:49.174732Z","submitted_at":"2013-10-29T10:57:48Z","title":"[CoIII] versus NaID in type Ia supernova spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.7750","snapshot_observed_at":"2026-08-12T20:25:19.665445Z","title":"title [Co III] versus Na I D in Type Ia supernova spectra","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.665445Z"},"links":{"cited_paper":"/paper/1310.7750","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:97966d8337284e2970965b2f7cf7735451cecc40d1992b0ce7d003a38cae262e","observation_id":"4f3bd431-61e3-4e4d-b925-aeddf17c52ae","resolution":{"observed_at":"2026-08-12T20:25:19.665445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.10061","last_updated":"2018-11-25T17:43:44Z","snapshot_observed_at":"2026-08-13T07:43:17.039293Z","submitted_at":"2018-11-25T17:43:44Z","title":"K2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.10061","snapshot_observed_at":"2026-08-12T20:25:19.669392Z","title":"( year 2019 ), month Jan","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.669392Z"},"links":{"cited_paper":"/paper/1811.10061","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f2696b89f809ccc6041420bcc21e0e894d99754da8d6b70580b7064404892983","observation_id":"26ed3e19-ef04-4553-a620-e89f6b77d668","resolution":{"observed_at":"2026-08-12T20:25:19.669392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.3347","last_updated":"2015-09-01T10:03:06Z","snapshot_observed_at":"2026-07-06T03:33:17.010477Z","submitted_at":"2014-01-14T21:00:20Z","title":"Type Ia Supernovae with Bi-Modal Explosions Are Common -- Possible Smoking Gun for Direct Collisions of White-Dwarfs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.3347","snapshot_observed_at":"2026-08-12T20:25:19.673551Z","title":"title Type Ia supernovae with bimodal explosions are common - possible smoking gun for direct collisions of white dwarfs","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.673551Z"},"links":{"cited_paper":"/paper/1401.3347","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:8c3f8e0a0da38d1ddf59b67e62591e37559c4d504604afdacf126f23be015fb1","observation_id":"8abc0dff-0edf-49e8-aa13-6a91409221d2","resolution":{"observed_at":"2026-08-12T20:25:19.673551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00279","last_updated":"2024-06-29T02:07:38Z","snapshot_observed_at":"2026-08-12T23:32:21.874839Z","submitted_at":"2024-06-29T02:07:38Z","title":"X-ray Observations of Two Type Ia Supernovae with an H$\\alpha$ Line in their Optical Spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.00279","snapshot_observed_at":"2026-08-12T20:25:19.678199Z","title":"title X-ray Observations of Two Type Ia Supernovae with an H Line in their Optical Spectrum","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.678199Z"},"links":{"cited_paper":"/paper/2407.00279","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:38f8578b0f8c0d4bf13e7a55cbb9f515c293e85e7e4c9ab6f93adc27d9f12a83","observation_id":"53c12b79-94cb-4a94-bfdf-0799f2d7d2d3","resolution":{"observed_at":"2026-08-12T20:25:19.678199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.01957","last_updated":"2016-05-06T14:39:33Z","snapshot_observed_at":"2026-08-06T18:07:54.026059Z","submitted_at":"2016-05-06T14:39:33Z","title":"Iron: A Key Element for Understanding the Origin and Evolution of Interstellar Dust","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.01957","snapshot_observed_at":"2026-08-12T20:25:19.682698Z","title":"title Iron: A Key Element for Understanding the Origin and Evolution of Interstellar Dust","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.682698Z"},"links":{"cited_paper":"/paper/1605.01957","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:718d1a01c74a8aa17fbf83f183c73d7f8b1ff201809dd1cf61db81a13f8b1059","observation_id":"f5db2bc9-40bf-4424-a7d5-9f6633cc8bed","resolution":{"observed_at":"2026-08-12T20:25:19.682698Z","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":"2026-08-12T20:25:19.687566Z","title":"( year 1992 ), month Oct","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.687566Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:1f7998ca47a8587c816ba70ff3f50bffc572e350f0af341cf09d2240415dac70","observation_id":"21e74b3c-448f-4b9e-a420-9c9a2d8d6c68","resolution":{"observed_at":"2026-08-12T20:25:19.687566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.2173","last_updated":"2010-10-22T13:41:43Z","snapshot_observed_at":"2026-08-02T00:51:20.245848Z","submitted_at":"2010-02-10T18:51:37Z","title":"Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.2173","snapshot_observed_at":"2026-08-12T20:25:19.692120Z","title":"title Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core? journal volume 514 , eid A53","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.692120Z"},"links":{"cited_paper":"/paper/1002.2173","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:97a55f14fad05a69b3a0f4146bdc932dd5694d5fa66a2c374e2599ab40a1f488","observation_id":"d3949256-b7b8-4247-82c0-d47a9a0f9a02","resolution":{"observed_at":"2026-08-12T20:25:19.692120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.1064","last_updated":"2014-11-04T21:00:13Z","snapshot_observed_at":"2026-07-06T03:59:36.028412Z","submitted_at":"2014-11-04T21:00:13Z","title":"The Rising Light Curves of Type Ia Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.1064","snapshot_observed_at":"2026-08-12T20:25:19.696912Z","title":"( year 2015 ), month Feb","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.696912Z"},"links":{"cited_paper":"/paper/1411.1064","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:b6decbcff6f6813ead505f6a89ebc631c26ecde0b293942b46378e7d36d864fa","observation_id":"03949794-b903-45ac-81a5-b2b7003a97ce","resolution":{"observed_at":"2026-08-12T20:25:19.696912Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.11055","last_updated":"2019-09-24T17:14:27Z","snapshot_observed_at":"2026-08-12T06:10:21.526575Z","submitted_at":"2019-09-24T17:14:27Z","title":"Sub-Chandrasekhar progenitors favoured for type Ia supernovae: Evidence from late-time spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.11055","snapshot_observed_at":"2026-08-12T20:25:19.701208Z","title":"title Sub-Chandrasekhar progenitors favoured for Type Ia supernovae: evidence from late-time spectroscopy","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.701208Z"},"links":{"cited_paper":"/paper/1909.11055","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:8df4b77849655e8d69317b5425f3ae4575f9f851873654383eda221df512c9a5","observation_id":"9b822efe-19c0-4398-95b6-f6f602438e81","resolution":{"observed_at":"2026-08-12T20:25:19.701208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3140","last_updated":"2012-02-14T21:00:06Z","snapshot_observed_at":"2026-07-06T02:42:52.951032Z","submitted_at":"2012-02-14T21:00:06Z","title":"The Low-Velocity, Rapidly Fading Type Ia Supernova 2002es","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3140","snapshot_observed_at":"2026-08-12T20:25:19.705276Z","title":"( year 2012 ), month Feb","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.705276Z"},"links":{"cited_paper":"/paper/1202.3140","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:265cea39c37b9ea2e3360b968417822186f862b4e114569ea893a7bcb989dd7c","observation_id":"212f93db-9d55-4457-8444-ef20dd599bd1","resolution":{"observed_at":"2026-08-12T20:25:19.705276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609742","last_updated":"2006-09-27T09:40:41Z","snapshot_observed_at":"2026-07-07T01:03:20.126960Z","submitted_at":"2006-09-27T09:40:41Z","title":"The hot subdwarf B + white dwarf binary KPD 1930+2752 - a Supernova Type Ia progenitor candidate","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609742","snapshot_observed_at":"2026-08-12T20:25:19.709288Z","title":"title The hot subdwarf B + white dwarf binary KPD 1930+2752","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.709288Z"},"links":{"cited_paper":"/paper/astro-ph/0609742","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:1288fd123808297c0a1453c4bb277f3862016745b6d13b3879218ac34de69489","observation_id":"1def2c83-443c-4890-b761-bc75ce156e36","resolution":{"observed_at":"2026-08-12T20:25:19.709288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306270","last_updated":"2003-06-18T19:36:58Z","snapshot_observed_at":"2026-07-07T00:34:07.852547Z","submitted_at":"2003-06-12T21:28:42Z","title":"Evidence for an asymptotic giant branch star in the progenitor system of a type Ia supernova","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0306270","snapshot_observed_at":"2026-08-12T20:25:19.713310Z","title":"( year 2003 ), month Aug","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.713310Z"},"links":{"cited_paper":"/paper/astro-ph/0306270","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:4ce21788c1b2fe5f87ac10b76dc9976cd7a50cb2ba31d98cc5dd61c46897d167","observation_id":"2eda6ed5-516a-4703-b467-7131b643864d","resolution":{"observed_at":"2026-08-12T20:25:19.713310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4787","last_updated":"2009-06-14T14:05:10Z","snapshot_observed_at":"2026-07-06T01:50:53.158645Z","submitted_at":"2009-01-30T00:07:27Z","title":"CfA3: 185 Type Ia Supernova Light Curves from the CfA","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.4787","snapshot_observed_at":"2026-08-12T20:25:19.717891Z","title":"( year 2009 ), month Jul","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.717891Z"},"links":{"cited_paper":"/paper/0901.4787","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:21745b8322ffb362c19412c3e66b137e3133bc7ebe6335ac9c102e66854d58d6","observation_id":"638eafb0-8d46-44c7-ae1d-7a2fcd4a5920","resolution":{"observed_at":"2026-08-12T20:25:19.717891Z","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":"2026-08-12T20:25:19.722361Z","title":"title Physics of type Ia supernovae","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.722361Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:5488bd4770c326388d21ee125d4771905d61e34f8110bd37d9a690d49fd91e89","observation_id":"1677f8ea-9034-4549-a816-accd3a8130c0","resolution":{"observed_at":"2026-08-12T20:25:19.722361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.02122","last_updated":"2021-03-03T01:37:02Z","snapshot_observed_at":"2026-08-07T21:16:57.538734Z","submitted_at":"2021-03-03T01:37:02Z","title":"Actinide crystallization and fission reactions in cooling white dwarf stars","version":1},"cited_work":{"arxiv_id":"2103.02122","doi":null,"metadata_source":"pith","pith_arxiv_id":"2103.02122","snapshot_observed_at":"2026-08-12T20:25:21.205962Z","title":"Actinide crystallization and fission reactions in cooling white dwarf stars","venue":"astro-ph.SR","work_id":"651c283d-c5e4-4dcd-8115-e13e2a7f2374","year":2021},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.727395Z"},"links":{"cited_paper":"/paper/2103.02122","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:8cfe3235fe9e0e8a246eef684a19deb87084a7682911e4eb077ff03b33c36f57","observation_id":"735e538c-1772-4428-9b15-b4f22306f957","resolution":{"observed_at":"2026-08-12T20:25:21.211026Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.01747","last_updated":"2019-12-23T20:34:12Z","snapshot_observed_at":"2026-08-09T14:53:13.683903Z","submitted_at":"2017-02-06T18:53:33Z","title":"Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.01747","snapshot_observed_at":"2026-08-12T20:25:19.731668Z","title":"( year 2018 ), month Nov","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.731668Z"},"links":{"cited_paper":"/paper/1702.01747","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:acd2620abe3b6432afa5f0f47ed1c864653c27305491c02186a34d2be86426cd","observation_id":"e8f6b145-7b0e-4f94-a087-7f5e000206d3","resolution":{"observed_at":"2026-08-12T20:25:19.731668Z","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":"2026-08-12T20:25:19.735449Z","title":"title Nucleosynthesis in Supernovae","venue":null,"work_id":null,"year":1960},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.735449Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:6d11f7382fe8c94a833d8cc13cf4f97155b949ca0b8df797c8e204d66d6ecca9","observation_id":"f1b4d6eb-8218-4bbb-9289-f345250d3537","resolution":{"observed_at":"2026-08-12T20:25:19.735449Z","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":"2026-08-12T20:25:19.738964Z","title":"I and author Tutukov AV ( year 1984 ), month Feb","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.738964Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:7383c09508623d165b0e2f58fb22cbfcde2a049b5d8f1cd801d4f2b71dbc968c","observation_id":"1e84998b-d0a1-464e-ad9c-91cc6becc319","resolution":{"observed_at":"2026-08-12T20:25:19.738964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9907015","last_updated":"1999-07-01T17:30:07Z","snapshot_observed_at":"2026-07-07T01:27:04.258766Z","submitted_at":"1999-07-01T17:30:07Z","title":"Radioactive Decay Energy Deposition in Supernovae and the Exponential/Quasi-Exponential Behavior of Late-Time Supernova Light Curves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9907015","snapshot_observed_at":"2026-08-12T20:25:19.742736Z","title":"title Radioactive Decay Energy Deposition in Supernovae and the Exponential/Quasi-Exponential Behavior of Late-Time Supernova Light Curves","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.742736Z"},"links":{"cited_paper":"/paper/astro-ph/9907015","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:ccfb6b714903078709c4279c8772c5103c7095b0570ba4616e6eaf58eb132e50","observation_id":"17f16390-84b0-4c1a-83e7-efa4cefc5457","resolution":{"observed_at":"2026-08-12T20:25:19.742736Z","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":"2026-08-12T20:25:19.746601Z","title":"pages 375","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.746601Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:528a5e3c116eebc0708c98369dcbc5125ebff853def080f931408f6388ab1a17","observation_id":"a1655c9d-66cd-4a50-9dcc-16995baeaebe","resolution":{"observed_at":"2026-08-12T20:25:19.746601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.4913","last_updated":"2011-02-28T10:05:05Z","snapshot_observed_at":"2026-07-06T02:23:59.780738Z","submitted_at":"2011-02-24T07:07:15Z","title":"Single-degenerate type Ia supernovae without hydrogen contamination","version":2},"cited_work":{"arxiv_id":"1102.4913","doi":null,"metadata_source":"pith","pith_arxiv_id":"1102.4913","snapshot_observed_at":"2026-08-12T20:25:21.165813Z","title":"Single-degenerate type Ia supernovae without hydrogen contamination","venue":"astro-ph.SR","work_id":"da3ec13f-4d88-40ba-9aa4-2cd084f48c6d","year":2011},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.750198Z"},"links":{"cited_paper":"/paper/1102.4913","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f4f515e3e020877f202ad6b7fbf7203a479b28d7892f21cca4c663a8fcef8cb0","observation_id":"0b23d1b6-b1fd-49a2-b728-ffda95fb7187","resolution":{"observed_at":"2026-08-12T20:25:21.170446Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0909.0275","last_updated":"2009-09-02T02:47:12Z","snapshot_observed_at":"2026-07-06T01:57:41.957002Z","submitted_at":"2009-09-02T02:47:12Z","title":"Seeing the Collision of a Supernova with its Companion Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.0275","snapshot_observed_at":"2026-08-12T20:25:19.754345Z","title":"title Seeing the Collision of a Supernova with Its Companion Star","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.754345Z"},"links":{"cited_paper":"/paper/0909.0275","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:76f98789909e2bfaf323e4a14e7019a8e805db50cfb0fed4efa6ff8512472718","observation_id":"4725a7f8-00e7-4d3a-86bb-319417a6dcba","resolution":{"observed_at":"2026-08-12T20:25:19.754345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609540","last_updated":"2006-09-19T17:04:51Z","snapshot_observed_at":"2026-07-07T01:03:05.610110Z","submitted_at":"2006-09-19T17:04:51Z","title":"On the Origin of the Type Ia Supernova Width-Luminosity Relation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609540","snapshot_observed_at":"2026-08-12T20:25:19.758457Z","title":"title On the Origin of the Type Ia Supernova Width-Luminosity Relation","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.758457Z"},"links":{"cited_paper":"/paper/astro-ph/0609540","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:a61844882394ffd97eda0c62755d8d8aede87ff801a9118a4f6f754495ccc949","observation_id":"79f4c801-35e7-450b-8b74-b23ff3f1e14d","resolution":{"observed_at":"2026-08-12T20:25:19.758457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301312","last_updated":"2003-01-16T01:54:24Z","snapshot_observed_at":"2026-08-08T02:58:14.423368Z","submitted_at":"2003-01-16T01:54:24Z","title":"Analysis of the Flux and Polarization Spectra of the Type Ia Supernova SN 2001el: Exploring the Geometry of the High-velocity Ejecta","version":1},"cited_work":{"arxiv_id":"astro-ph/0301312","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0301312","snapshot_observed_at":"2026-08-12T20:25:21.123116Z","title":"Analysis of the Flux and Polarization Spectra of the Type Ia Supernova SN 2001el: Exploring the Geometry of the High-velocity Ejecta","venue":"astro-ph","work_id":"dba46e8e-8082-4e39-9fbb-a7eb95b5c8cb","year":2003},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.762299Z"},"links":{"cited_paper":"/paper/astro-ph/0301312","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:affa0ebb874a6fb9ab7497e79effc753ce1a6eb647370e32b1975bafd2face9b","observation_id":"1d733c0b-8553-462d-b216-b51e754fde4e","resolution":{"observed_at":"2026-08-12T20:25:21.127875Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T20:25:19.766222Z","title":"title A circumbinary disc in the final stages of common envelope and the core-degenerate scenario for Type Ia supernovae","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.766222Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:b3404c5aaf7878484fafccc108cbfaf3f82967907c7972be38f67c3626357eb7","observation_id":"829e902d-fecf-475a-8165-971f149c387b","resolution":{"observed_at":"2026-08-12T20:25:19.766222Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.05645","last_updated":"2015-01-30T16:09:50Z","snapshot_observed_at":"2026-07-06T04:06:58.716659Z","submitted_at":"2015-01-22T21:00:01Z","title":"Spiral Disk Instability Can Drive Thermonuclear Explosions in Binary White Dwarf Mergers","version":2},"cited_work":{"arxiv_id":"1501.05645","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.05645","snapshot_observed_at":"2026-08-12T20:25:21.036758Z","title":"Spiral Disk Instability Can Drive Thermonuclear Explosions in Binary White Dwarf Mergers","venue":"astro-ph.SR","work_id":"901f328e-3970-439e-9108-891651305428","year":2015},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.769803Z"},"links":{"cited_paper":"/paper/1501.05645","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:777f9e193b4813d214de6ae02985187db24131339b678d48765a82e6dcd099e4","observation_id":"4300ad93-4ac9-4124-8c57-7171499781ae","resolution":{"observed_at":"2026-08-12T20:25:21.041144Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.4584","last_updated":"2012-11-21T20:59:39Z","snapshot_observed_at":"2026-07-06T03:00:13.830823Z","submitted_at":"2012-11-19T21:00:05Z","title":"The rate of WD-WD head-on collisions may be as high as the SNe Ia rate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.4584","snapshot_observed_at":"2026-08-12T20:25:19.773552Z","title":"title The rate of WD-WD head-on collisions may be as high as the SNe Ia rate","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.773552Z"},"links":{"cited_paper":"/paper/1211.4584","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:e981065ef78aa22a8a1fb57dfe503d88b7c5ccfc522035fd5fb9de732ae713ec","observation_id":"b9a343bf-bf20-40c0-b3cc-a3d5c690af6e","resolution":{"observed_at":"2026-08-12T20:25:19.773552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.6766","last_updated":"2013-01-28T21:02:06Z","snapshot_observed_at":"2026-07-06T03:05:04.102454Z","submitted_at":"2013-01-28T21:02:06Z","title":"An exact integral relation between the Ni56 mass and the bolometric light curve of a type Ia supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.6766","snapshot_observed_at":"2026-08-12T20:25:19.777671Z","title":"title An exact integral relation between the Ni 56 mass and the bolometric light curve of a type Ia supernova","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.777671Z"},"links":{"cited_paper":"/paper/1301.6766","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:3696680f166ffa4334477d1150c9913d6013cdcc1e68630ef3f114f20a3107a5","observation_id":"f741d8ca-3ae8-4b27-b667-a8714ffe4178","resolution":{"observed_at":"2026-08-12T20:25:19.777671Z","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":"2026-08-12T20:25:19.781819Z","title":"title White dwarf mass distribution in the SDSS","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.781819Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:10a7298390973c1390bdfb6eb24537fd3ee588e1a079b0dd38b57236e561817d","observation_id":"4ed5d01e-694b-4f5a-9677-dbf9f0596705","resolution":{"observed_at":"2026-08-12T20:25:19.781819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.06566","last_updated":"2017-09-19T18:00:00Z","snapshot_observed_at":"2026-07-06T06:00:20.967053Z","submitted_at":"2017-09-19T18:00:00Z","title":"A Search for a Surviving White Dwarf Companion in SN 1006","version":1},"cited_work":{"arxiv_id":"1709.06566","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.06566","snapshot_observed_at":"2026-08-12T20:25:20.928482Z","title":"A Search for a Surviving White Dwarf Companion in SN 1006","venue":"astro-ph.SR","work_id":"3b7bb36d-c830-42e0-91a8-914533c2eb80","year":2017},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.785571Z"},"links":{"cited_paper":"/paper/1709.06566","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:2dcb8320f92259f99df4242cb2fd4f7b659a4bb20689d2afd26ac0238e4909cf","observation_id":"e9dfedad-4c09-45eb-85f0-f5dfabcacc18","resolution":{"observed_at":"2026-08-12T20:25:20.933629Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T20:25:19.789919Z","title":"title Delayed detonation model for type IA supernovae","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.789919Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f1e9da3f0c7946590fc08b87173ba90a78c21a471f0e72e264e3faae3591decc","observation_id":"325b5f3b-40ae-46e0-82dd-0422cf07d91f","resolution":{"observed_at":"2026-08-12T20:25:19.789919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.07725","last_updated":"2023-05-17T15:53:10Z","snapshot_observed_at":"2026-08-01T15:00:36.075537Z","submitted_at":"2022-10-14T11:44:11Z","title":"A radio-detected Type Ia supernova with helium-rich circumstellar material","version":2},"cited_work":{"arxiv_id":"2210.07725","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.07725","snapshot_observed_at":"2026-08-12T20:25:20.911557Z","title":"A radio-detected Type Ia supernova with helium-rich circumstellar material","venue":"astro-ph.HE","work_id":"2ca2fe47-a806-4b85-bee6-e26e3f1212d3","year":2022},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.793946Z"},"links":{"cited_paper":"/paper/2210.07725","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:68012497855926189687023630dc52bda789ecc46299f1a4192c55e820c1634b","observation_id":"90da8c5a-9f7c-45cb-bb20-b2931ca3d8b7","resolution":{"observed_at":"2026-08-12T20:25:20.916324Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.03935","last_updated":"2024-10-15T13:06:10Z","snapshot_observed_at":"2026-08-13T03:27:41.353386Z","submitted_at":"2024-07-04T13:51:57Z","title":"Expected insights on type Ia supernovae from LISA's gravitational wave observations","version":2},"cited_work":{"arxiv_id":"2407.03935","doi":"10.48550/arxiv.2407.03935","metadata_source":"pith","pith_arxiv_id":"2407.03935","snapshot_observed_at":"2026-08-13T00:16:21.800782Z","title":"Expected insights on type Ia supernovae from LISA's gravitational wave observations","venue":"astro-ph.HE","work_id":"38cb4a86-5629-4b0d-9bf3-1e838a0bf58f","year":2024},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.798050Z"},"links":{"cited_paper":"/paper/2407.03935","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:12e81819494d35cfc6e09a43589f91b24b6dd6883fc832199ef3c74af5a5ab9e","observation_id":"5a0a9ef5-4513-4f34-97e6-b21555a99d56","resolution":{"observed_at":"2026-08-12T20:25:20.154072Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.10804","last_updated":"2022-10-19T18:00:05Z","snapshot_observed_at":"2026-08-12T16:27:18.069371Z","submitted_at":"2022-10-19T18:00:05Z","title":"Using $^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors","version":1},"cited_work":{"arxiv_id":"2210.10804","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.10804","snapshot_observed_at":"2026-08-12T20:25:20.894011Z","title":"Using $^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors","venue":"astro-ph.HE","work_id":"7eb2fa75-fabe-41db-b1b9-0e77c869ff1a","year":2022},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.802304Z"},"links":{"cited_paper":"/paper/2210.10804","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:d889d23a0f64b0bb756d8cde4a5ae3699d1187741e9658c3ba40357a50e6569d","observation_id":"d05d7983-a1cb-46b3-b26b-ea045565cf36","resolution":{"observed_at":"2026-08-12T20:25:20.898288Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1311.0310","last_updated":"2013-11-01T21:12:48Z","snapshot_observed_at":"2026-07-06T03:27:10.534522Z","submitted_at":"2013-11-01T21:12:48Z","title":"SN 2010lp---a Type Ia supernova from a violent merger of two carbon--oxygen White Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.0310","snapshot_observed_at":"2026-08-12T20:25:19.806335Z","title":"( year 2013 ), month Nov","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.806335Z"},"links":{"cited_paper":"/paper/1311.0310","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:885da2c5424281305a23d5620c35a438042ba05a568f3cc18f0534aa74d92574","observation_id":"31ace1c6-9d10-4fcd-8ec2-8ee320660d47","resolution":{"observed_at":"2026-08-12T20:25:19.806335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.05730","last_updated":"2016-04-19T20:02:58Z","snapshot_observed_at":"2026-08-08T09:58:13.692481Z","submitted_at":"2016-04-19T20:02:58Z","title":"The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.05730","snapshot_observed_at":"2026-08-12T20:25:19.810403Z","title":"( year 2016 ), month Jul","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.810403Z"},"links":{"cited_paper":"/paper/1604.05730","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:ba0f15d3d29fbafc6ee92fad9728c9fc9aad5298315efd4d915753e241234811","observation_id":"0979f4c9-7ab6-4ca1-a6f8-63947d9834a1","resolution":{"observed_at":"2026-08-12T20:25:19.810403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.12450","last_updated":"2024-05-23T15:45:23Z","snapshot_observed_at":"2026-08-13T10:28:44.098050Z","submitted_at":"2023-08-23T22:13:53Z","title":"Ground-based and JWST Observations of SN 2022pul: II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type-Ia Supernova","version":2},"cited_work":{"arxiv_id":"2308.12450","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.12450","snapshot_observed_at":"2026-08-12T20:25:20.855610Z","title":"Ground-based and JWST Observations of SN 2022pul: II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type-Ia Supernova","venue":"astro-ph.HE","work_id":"a1aaadba-d72c-4e81-b0eb-82b0df10fa9d","year":2023},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.814490Z"},"links":{"cited_paper":"/paper/2308.12450","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:2dade0a4f9fdeb214a9d523e8ecb3c284984d07ab16c03416f0454714c31a162","observation_id":"ea59816e-58e2-4f6a-9d08-09c06c79d77a","resolution":{"observed_at":"2026-08-12T20:25:20.860515Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T20:25:19.819633Z","title":"( year 1993 ), month Jan","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.819633Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:9d77d8ee774c3df284a0e226bb908e3c5c8c2ed05c135c63b75c90d5b8877c86","observation_id":"ec795a7f-8f3c-4813-9087-56f7e224424f","resolution":{"observed_at":"2026-08-12T20:25:19.819633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301428","last_updated":"2003-01-22T02:18:43Z","snapshot_observed_at":"2026-07-07T00:30:53.161453Z","submitted_at":"2003-01-22T02:18:43Z","title":"SN 2002cx: The Most Peculiar Known Type Ia Supernova","version":1},"cited_work":{"arxiv_id":"astro-ph/0301428","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0301428","snapshot_observed_at":"2026-08-12T20:25:20.837665Z","title":"SN 2002cx: The Most Peculiar Known Type Ia Supernova","venue":"astro-ph","work_id":"fc37acdb-49dc-48a7-8050-f9d7994fb3d0","year":2003},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.824125Z"},"links":{"cited_paper":"/paper/astro-ph/0301428","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:62d8b4ec486a4e46a4d41c97d327843ba7ba5285029615bb34b95bd61ce8e389","observation_id":"ee76df59-3a2d-4c43-8b20-a78e669c2841","resolution":{"observed_at":"2026-08-12T20:25:20.842186Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9709262","last_updated":"1997-09-25T20:47:04Z","snapshot_observed_at":"2026-07-07T01:18:27.172243Z","submitted_at":"1997-09-25T20:47:04Z","title":"Optical Light Curves of the Type Ia Supernovae 1990N and 1991T","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9709262","snapshot_observed_at":"2026-08-12T20:25:19.828494Z","title":"( year 1998 ), month Jan","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.828494Z"},"links":{"cited_paper":"/paper/astro-ph/9709262","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:da7459ed95d49fa9710f1cc57f489abdeb7751e06319a7248cadbe0eb3164754","observation_id":"69d3e824-97e7-4dd2-9ab3-489baff46084","resolution":{"observed_at":"2026-08-12T20:25:19.828494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.5484","last_updated":"2009-12-24T01:51:09Z","snapshot_observed_at":"2026-08-07T22:10:56.332208Z","submitted_at":"2009-11-29T14:37:33Z","title":"Nebular Spectra and Explosion Asymmetry of Type Ia Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.5484","snapshot_observed_at":"2026-08-12T20:25:19.833022Z","title":"title Nebular Spectra and Explosion Asymmetry of Type Ia Supernovae","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.833022Z"},"links":{"cited_paper":"/paper/0911.5484","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:dad6c6f305bc3c8ace2d514b4bc8170b6b8e5488ac4089e551c05d754eeee13a","observation_id":"5e83e821-458e-400e-b8e9-11ee47b708d2","resolution":{"observed_at":"2026-08-12T20:25:19.833022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4492","last_updated":"2012-02-20T12:06:19Z","snapshot_observed_at":"2026-07-06T02:37:50.966961Z","submitted_at":"2011-11-18T21:25:42Z","title":"Type-Ia supernova rates and the progenitor problem, a review","version":2},"cited_work":{"arxiv_id":"1111.4492","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.4492","snapshot_observed_at":"2026-08-12T20:25:20.798248Z","title":"Type-Ia supernova rates and the progenitor problem, a review","venue":"astro-ph.CO","work_id":"20509f62-967d-4e17-911c-3151cd343df4","year":2011},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.837322Z"},"links":{"cited_paper":"/paper/1111.4492","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:05884b935ac7c81d54a9e0e14af8291bf6f18e90915decf2c6b7803a38009fd2","observation_id":"8d724026-3bf2-44e2-8414-27734a4817d0","resolution":{"observed_at":"2026-08-12T20:25:20.802677Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1312.0628","last_updated":"2014-08-13T12:31:00Z","snapshot_observed_at":"2026-08-06T02:19:44.243462Z","submitted_at":"2013-12-02T21:14:19Z","title":"Observational clues to the progenitors of Type-Ia supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.0628","snapshot_observed_at":"2026-08-12T20:25:19.841535Z","title":"title Observational Clues to the Progenitors of Type Ia Supernovae","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.841535Z"},"links":{"cited_paper":"/paper/1312.0628","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:02610954de9e9defe0c658fd3223ba9c519642396193934008a6aa01eaae1648","observation_id":"163e9cd3-dfc1-4c8c-a055-c5e9dfeb7f59","resolution":{"observed_at":"2026-08-12T20:25:19.841535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3828","last_updated":"2012-05-16T23:07:06Z","snapshot_observed_at":"2026-08-02T03:19:19.607459Z","submitted_at":"2012-05-16T23:07:06Z","title":"The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101","version":1},"cited_work":{"arxiv_id":"1205.3828","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.3828","snapshot_observed_at":"2026-08-12T20:25:20.769336Z","title":"The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101","venue":"astro-ph.CO","work_id":"172c8bd0-ea47-4daf-9955-ac6247517d1a","year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.846330Z"},"links":{"cited_paper":"/paper/1205.3828","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:22525d726a61e075b9ecee12e09beea0e323de76f8e2ebc4c175f4146f56506b","observation_id":"40079037-a12f-43f7-b47e-094decebfe24","resolution":{"observed_at":"2026-08-12T20:25:20.773857Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1305.2356","last_updated":"2014-01-14T13:10:44Z","snapshot_observed_at":"2026-07-06T03:13:07.287044Z","submitted_at":"2013-05-10T14:49:54Z","title":"Hubble Space Telescope spectra of the type Ia supernova SN2011fe: a tail of low-density, high-velocity material with Z<Zsolar","version":2},"cited_work":{"arxiv_id":"1305.2356","doi":null,"metadata_source":"pith","pith_arxiv_id":"1305.2356","snapshot_observed_at":"2026-08-12T20:25:20.752460Z","title":"Hubble Space Telescope spectra of the type Ia supernova SN2011fe: a tail of low-density, high-velocity material with Z<Zsolar","venue":"astro-ph.CO","work_id":"bc78957b-05db-4544-912d-98e965435c10","year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.850330Z"},"links":{"cited_paper":"/paper/1305.2356","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:3d53dea9ea0086662834903d71853b4ff12701afe381a4326c20fa23f0dec7f0","observation_id":"b7476d42-ffae-43c9-abd5-6385934cfa41","resolution":{"observed_at":"2026-08-12T20:25:20.756701Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T20:25:19.854104Z","title":"title Accreting white dwarf models of Type I supernovae","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.854104Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:245e56b731e8faaa5b1ee55dbc9b8cd8be92b65399c38d318841b8b8650bf2f2","observation_id":"cdf11a0d-979b-4e21-b2f2-1932ba7b53cc","resolution":{"observed_at":"2026-08-12T20:25:19.854104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9510004","last_updated":"1995-10-02T17:49:30Z","snapshot_observed_at":"2026-07-07T01:11:57.142715Z","submitted_at":"1995-10-02T17:49:30Z","title":"Evidence for a Spectroscopic Sequence Among SNe Ia","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9510004","snapshot_observed_at":"2026-08-12T20:25:19.858783Z","title":"title Evidence for a Spectroscopic Sequence among Type 1a Supernovae","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.858783Z"},"links":{"cited_paper":"/paper/astro-ph/9510004","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:a97c01764b7eb051144fe62e535dde1fb736c8a5541602c8425c97d5e877fc19","observation_id":"45e6593b-3ec7-4335-96b5-5c11b658022a","resolution":{"observed_at":"2026-08-12T20:25:19.858783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.6201","last_updated":"2011-10-27T21:48:24Z","snapshot_observed_at":"2026-07-06T02:36:33.006329Z","submitted_at":"2011-10-27T21:48:24Z","title":"Supernova 2011fe from an Exploding Carbon-Oxygen White Dwarf Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.6201","snapshot_observed_at":"2026-08-12T20:25:19.863013Z","title":"( year 2011 ), month Dec","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.863013Z"},"links":{"cited_paper":"/paper/1110.6201","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:05bb22c3b962b77dae719195209df77bbe7cdb0d04e12ab113a0b947cbe2e0b5","observation_id":"0ba4dfdd-7408-466e-94db-8df6adf7bafa","resolution":{"observed_at":"2026-08-12T20:25:19.863013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.0926","last_updated":"2009-11-05T12:40:46Z","snapshot_observed_at":"2026-07-06T02:03:38.054105Z","submitted_at":"2009-11-05T12:40:46Z","title":"Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with M~0.9 M_sun","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.0926","snapshot_observed_at":"2026-08-12T20:25:19.867893Z","title":"title Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with mass 0.9 \\,M _","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.867893Z"},"links":{"cited_paper":"/paper/0911.0926","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:5f34e97c7b07b135101ab86a8aadfbb2ea71001c40f71bac8390d3b4145c13de","observation_id":"cdfa87d8-4617-49ab-b7eb-6f547aeeae44","resolution":{"observed_at":"2026-08-12T20:25:19.867893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.5123","last_updated":"2012-01-24T21:04:09Z","snapshot_observed_at":"2026-07-06T02:41:42.454189Z","submitted_at":"2012-01-24T21:04:09Z","title":"Normal Type Ia supernovae from violent mergers of white dwarf binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.5123","snapshot_observed_at":"2026-08-12T20:25:19.872198Z","title":"title Normal Type Ia Supernovae from Violent Mergers of White Dwarf Binaries","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.872198Z"},"links":{"cited_paper":"/paper/1201.5123","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:d32e77c0cb298c1004d72429131381a440692bd1a14d98334ad64b433ed40f7c","observation_id":"84dfd395-f847-41d7-8771-ceec1b5a6246","resolution":{"observed_at":"2026-08-12T20:25:19.872198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.2913","last_updated":"2013-05-10T14:02:56Z","snapshot_observed_at":"2026-08-08T14:43:54.449903Z","submitted_at":"2013-02-12T21:00:00Z","title":"Helium-ignited violent mergers as a unified model for normal and rapidly declining Type Ia Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.2913","snapshot_observed_at":"2026-08-12T20:25:19.876632Z","title":"title Helium-ignited Violent Mergers as a Unified Model for Normal and Rapidly Declining Type Ia Supernovae","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.876632Z"},"links":{"cited_paper":"/paper/1302.2913","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:90a8c34af4c5889a0e58b2faecd6ab11ab3d0061ba016964e24650aa61401ba5","observation_id":"7aed5a4e-2ed1-4ab9-a38a-6ac9d108f053","resolution":{"observed_at":"2026-08-12T20:25:19.876632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.14990","last_updated":"2022-10-25T10:59:42Z","snapshot_observed_at":"2026-08-11T19:22:03.834549Z","submitted_at":"2022-03-28T18:01:15Z","title":"On the fate of the secondary white dwarf in double-degenerate double-detonation Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.14990","snapshot_observed_at":"2026-08-12T20:25:19.880797Z","title":"title On the fate of the secondary white dwarf in double-degenerate double-detonation Type Ia supernovae","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.880797Z"},"links":{"cited_paper":"/paper/2203.14990","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:dd7f346a1e4e44ada30a5c7b18a5e26d6c6575eed3302f541aba2e37b473840b","observation_id":"5344720c-a14f-4f16-bbf7-396f8c8ca861","resolution":{"observed_at":"2026-08-12T20:25:19.880797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.11010","last_updated":"2024-04-26T10:54:37Z","snapshot_observed_at":"2026-08-13T04:17:20.276915Z","submitted_at":"2024-02-16T19:00:00Z","title":"Type Ia supernova explosion models are inherently multidimensional","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.11010","snapshot_observed_at":"2026-08-12T20:25:19.885387Z","title":"title Type Ia supernova explosion models are inherently multidimensional","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.885387Z"},"links":{"cited_paper":"/paper/2402.11010","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:07e87394a309d0435fab370f8bb72047c64b3fee23c61676988c8c2222f7b1ce","observation_id":"f6d7a2d5-56ec-4248-9aa4-cf6e861b070f","resolution":{"observed_at":"2026-08-12T20:25:19.885387Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.09074","last_updated":"2021-07-19T18:00:04Z","snapshot_observed_at":"2026-07-06T11:30:29.656834Z","submitted_at":"2021-07-19T18:00:04Z","title":"A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.09074","snapshot_observed_at":"2026-08-12T20:25:19.889677Z","title":"( year 2021 ), month Jul","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.889677Z"},"links":{"cited_paper":"/paper/2107.09074","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:c2591a48fe0e1d3c34be60e938eec010a536fcce1a26ab25184f39b02ad9f96f","observation_id":"a55ee5e4-f459-4560-9cb3-d30fe4165831","resolution":{"observed_at":"2026-08-12T20:25:19.889677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.1292","last_updated":"2013-02-06T09:15:00Z","snapshot_observed_at":"2026-07-06T03:05:46.936930Z","submitted_at":"2013-02-06T09:15:00Z","title":"Spectrophotometric time series of SN 2011fe from the Nearby Supernova Factory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.1292","snapshot_observed_at":"2026-08-12T20:25:19.894747Z","title":"( year 2013 ), month Jun","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.894747Z"},"links":{"cited_paper":"/paper/1302.1292","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:539f20050c79a1d5c0ea7bc9217b0d7ede6d7859853ba2fbf383e41bacd715e2","observation_id":"2469434a-fecb-48ca-92b3-3f0bcdeed98c","resolution":{"observed_at":"2026-08-12T20:25:19.894747Z","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":"2026-08-12T20:25:19.899900Z","title":"title The absolute magnitudes of Type IA supernovae","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.899900Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:6e8c8fc7c120a033eb7854d995113791fb883df0746c9a7aeb680f56a8ae22e9","observation_id":"94cfbde5-bf4f-4900-857e-f73be5f361e9","resolution":{"observed_at":"2026-08-12T20:25:19.899900Z","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":"2026-08-12T20:25:19.905443Z","title":"title SN 1991T: Further Evidence of the Heterogeneous Nature of Type IA Supernovae","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.905443Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:f8caee1cf250a8f6c5be2d7281ec8f9d571eafd3ce95278bfd1d243af2923225","observation_id":"229399d9-3435-4613-879b-af96eb0f6d2b","resolution":{"observed_at":"2026-08-12T20:25:19.905443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.15027","last_updated":"2024-05-23T20:04:09Z","snapshot_observed_at":"2026-08-12T23:59:23.608355Z","submitted_at":"2024-05-23T20:04:09Z","title":"1991T-like Supernovae","version":1},"cited_work":{"arxiv_id":"2405.15027","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.15027","snapshot_observed_at":"2026-08-12T20:25:20.633391Z","title":"1991T-like Supernovae","venue":"astro-ph.HE","work_id":"adfa5855-8352-4278-aa66-669173484985","year":2024},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.909322Z"},"links":{"cited_paper":"/paper/2405.15027","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:78a3e43c5ce8e5bfe80c7f4965466d5414cb9e5619be3f38d4b1bde887d6e8f7","observation_id":"e41ac011-798b-4594-b11f-bd19a1f0517e","resolution":{"observed_at":"2026-08-12T20:25:20.637494Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.05089","last_updated":"2024-06-10T16:44:22Z","snapshot_observed_at":"2026-08-12T23:47:42.479888Z","submitted_at":"2024-06-07T17:03:04Z","title":"Discovery of An Apparent Red, High-Velocity Type Ia Supernova at z = 2.9 with JWST","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.05089","snapshot_observed_at":"2026-08-12T20:25:19.913438Z","title":"( year 2024 ), month Aug","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.913438Z"},"links":{"cited_paper":"/paper/2406.05089","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:cea9343b1b63f9be85b21783bee5c0617ac067301b0c584620f64a9c1226a328","observation_id":"e8ec5745-ed6d-4ed8-836a-c0c7237d9a73","resolution":{"observed_at":"2026-08-12T20:25:19.913438Z","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":"2026-08-12T20:25:19.917596Z","title":"title The Physics of Type IA Supernova Light Curves","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.917596Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:7efa41696b8ebbbffac898d88b0d996470873a00f93874f13fc995e50ae6b365","observation_id":"095583bb-b409-4ad8-90a2-aafc8207286d","resolution":{"observed_at":"2026-08-12T20:25:19.917596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.6438","last_updated":"2014-02-17T18:33:51Z","snapshot_observed_at":"2026-07-06T03:00:46.755763Z","submitted_at":"2012-11-27T21:00:04Z","title":"Constraints on Shallow 56Ni from the Early Lightcurves of Type Ia Supernovae","version":2},"cited_work":{"arxiv_id":"1211.6438","doi":null,"metadata_source":"pith","pith_arxiv_id":"1211.6438","snapshot_observed_at":"2026-08-12T20:25:20.604314Z","title":"Constraints on Shallow 56Ni from the Early Lightcurves of Type Ia Supernovae","venue":"astro-ph.HE","work_id":"c1320b23-8530-4e21-a773-908aae068a0e","year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.921468Z"},"links":{"cited_paper":"/paper/1211.6438","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:4d32f89637818b3b40b24a4b4e2fa2d8d19f476cdba6d7369153bac29299c172","observation_id":"644680f4-650e-4872-ad53-a20ae640f3f2","resolution":{"observed_at":"2026-08-12T20:25:20.608481Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.00050","last_updated":"2019-10-31T18:42:56Z","snapshot_observed_at":"2026-07-06T08:33:56.199723Z","submitted_at":"2019-10-31T18:42:56Z","title":"A Unified Mechanism for Unconfined Deflagration-to-Detonation Transition in Terrestrial Chemical Systems and Type Ia Supernovae","version":1},"cited_work":{"arxiv_id":"1911.00050","doi":null,"metadata_source":"pith","pith_arxiv_id":"1911.00050","snapshot_observed_at":"2026-08-12T20:25:20.588193Z","title":"A Unified Mechanism for Unconfined Deflagration-to-Detonation Transition in Terrestrial Chemical Systems and Type Ia Supernovae","venue":"astro-ph.HE","work_id":"58fd4406-0963-4e2e-919e-0c1cf042681b","year":2019},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.925428Z"},"links":{"cited_paper":"/paper/1911.00050","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:bd871b799bb86f92f122e6e5bbf42e53be7897abeed655e3d1781e4adb7c4f4d","observation_id":"a901128a-170c-46d5-963f-dee5f3dcec5c","resolution":{"observed_at":"2026-08-12T20:25:20.592912Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05267","last_updated":"2019-12-17T13:14:35Z","snapshot_observed_at":"2026-07-06T08:21:01.643474Z","submitted_at":"2019-09-11T18:00:13Z","title":"Variable H$\\alpha$ Emission in the Nebular Spectra of the Low-Luminosity Type Ia SN2018cqj/ATLAS18qtd","version":2},"cited_work":{"arxiv_id":"1909.05267","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.05267","snapshot_observed_at":"2026-08-12T20:25:20.571162Z","title":"Variable H$\\alpha$ Emission in the Nebular Spectra of the Low-Luminosity Type Ia SN2018cqj/ATLAS18qtd","venue":"astro-ph.HE","work_id":"4acff267-b77e-4dc6-b9e7-4abb6df0a458","year":2019},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.929767Z"},"links":{"cited_paper":"/paper/1909.05267","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:83e25a1933b8bb29a071d03f9931cfcc1850739b5d0f6b7736ab5d016d4bc516","observation_id":"03f1650b-eb26-4cf9-a130-be83cf5aafdc","resolution":{"observed_at":"2026-08-12T20:25:20.575931Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.5548","last_updated":"2011-08-29T14:10:50Z","snapshot_observed_at":"2026-07-06T02:33:03.484834Z","submitted_at":"2011-08-29T14:10:50Z","title":"Early emission from type Ia supernovae","version":1},"cited_work":{"arxiv_id":"1108.5548","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.5548","snapshot_observed_at":"2026-08-12T20:25:20.554311Z","title":"Early emission from type Ia supernovae","venue":"astro-ph.HE","work_id":"cab8badc-8051-41d0-8b1a-9fefa2b48532","year":2011},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.933870Z"},"links":{"cited_paper":"/paper/1108.5548","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:7da871969242bf287ee8d5ae9c92d610c8038fc129685b7d784425fe64e64373","observation_id":"ed78deb0-bd8a-4caa-aa15-a5ad7589bd34","resolution":{"observed_at":"2026-08-12T20:25:20.558736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.4013","last_updated":"2012-04-12T14:29:05Z","snapshot_observed_at":"2026-07-06T02:44:46.847978Z","submitted_at":"2012-03-19T00:44:46Z","title":"BVRI Photometry of SN 2011fe in M101","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.4013","snapshot_observed_at":"2026-08-12T20:25:19.938474Z","title":"title BVRI Photometry of SN 2011fe in M101","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.938474Z"},"links":{"cited_paper":"/paper/1203.4013","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:e452c7df3c45da99448b425896574d757aaff01e053cff8e163368e214d39cd3","observation_id":"7f382a38-cd09-4a3e-b11e-6b19ab91804f","resolution":{"observed_at":"2026-08-12T20:25:19.938474Z","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":"2026-08-12T20:25:19.942673Z","title":"pages 1185","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.942673Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:03a806a695e0372515a875226bf09288eae6da8a39f6af45ae900deb71447f28","observation_id":"c2ddb6ec-6569-4fae-acae-ccd458c11f65","resolution":{"observed_at":"2026-08-12T20:25:19.942673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.2143","last_updated":"2008-11-17T08:53:42Z","snapshot_observed_at":"2026-07-06T01:41:40.014604Z","submitted_at":"2008-08-15T13:41:16Z","title":"Tidal disruption and ignition of white dwarfs by moderately massive black holes","version":2},"cited_work":{"arxiv_id":"0808.2143","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.2143","snapshot_observed_at":"2026-08-12T20:25:20.535816Z","title":"Tidal disruption and ignition of white dwarfs by moderately massive black holes","venue":"astro-ph","work_id":"5b1bdb67-7cad-4a93-8439-44dd84e463ad","year":2008},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.946381Z"},"links":{"cited_paper":"/paper/0808.2143","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:9432438120cc15980283f4926d253b0a3985ff7551ad0be956af0daba85d17c4","observation_id":"0eed0029-64d0-40de-8d71-e551baa6e3c9","resolution":{"observed_at":"2026-08-12T20:25:20.541040Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.6601","last_updated":"2014-08-28T01:04:32Z","snapshot_observed_at":"2026-08-02T01:27:42.524566Z","submitted_at":"2014-08-28T01:04:32Z","title":"The ejected mass distribution of type Ia supernovae: A significant rate of non-Chandrasekhar-mass progenitors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.6601","snapshot_observed_at":"2026-08-12T20:25:19.950295Z","title":"title The ejected mass distribution of Type Ia supernovae: a significant rate of non-Chandrasekhar-mass progenitors","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.950295Z"},"links":{"cited_paper":"/paper/1408.6601","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:7193fbd4d018970c4cf18dce120337329669172036317f3a318341f49bceba59","observation_id":"850596c4-2645-422a-b2e6-9c47ec0cd3b4","resolution":{"observed_at":"2026-08-12T20:25:19.950295Z","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":"2026-08-12T20:25:19.954233Z","title":"pages 1955","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.954233Z"},"links":{"citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:7cfb149c9e9c82a9b9aaadece39470ef57c02334a4d73bd1751f7e1ed6a5c940","observation_id":"a2533e79-130c-4c01-b7a6-b33a20e30fb9","resolution":{"observed_at":"2026-08-12T20:25:19.954233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.2397","last_updated":"2013-09-11T08:19:05Z","snapshot_observed_at":"2026-07-06T03:22:36.265610Z","submitted_at":"2013-09-10T07:42:04Z","title":"Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.2397","snapshot_observed_at":"2026-08-12T20:25:19.958141Z","title":"title Solar abundance of manganese: a case for near Chandrasekhar-mass Type Ia supernova progenitors","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.958141Z"},"links":{"cited_paper":"/paper/1309.2397","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:4b7736789265b98dd690fa49c6809fb2e69e283319c724349acafad0193662eb","observation_id":"3187620a-af1a-4f0d-9895-76d010f54bdd","resolution":{"observed_at":"2026-08-12T20:25:19.958141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.3015","last_updated":"2012-11-13T15:05:07Z","snapshot_observed_at":"2026-07-06T02:59:47.961502Z","submitted_at":"2012-11-13T15:05:07Z","title":"Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.3015","snapshot_observed_at":"2026-08-12T20:25:19.962557Z","title":"( year 2013 b ), month Feb","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.962557Z"},"links":{"cited_paper":"/paper/1211.3015","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:ca69e629f924f8cafa7564569cdb26342275a8494c7e97bd44e03afbe325db1e","observation_id":"f421316c-b61f-4b9d-982e-fd74bdff9fcd","resolution":{"observed_at":"2026-08-12T20:25:19.962557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.4036","last_updated":"2012-01-04T01:19:24Z","snapshot_observed_at":"2026-08-05T06:26:41.632655Z","submitted_at":"2011-08-19T20:00:02Z","title":"The Long-Term Evolution of Double White Dwarf Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.4036","snapshot_observed_at":"2026-08-12T20:25:19.966562Z","title":"title The Long-term Evolution of Double White Dwarf Mergers","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.966562Z"},"links":{"cited_paper":"/paper/1108.4036","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:93070f954c763fe72e985bef711edbff7686188a0ffc6acb8799ef1b7c9777ea","observation_id":"a960b7b9-7796-428a-b7ac-d8c4f7db5d6d","resolution":{"observed_at":"2026-08-12T20:25:19.966562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.11163","last_updated":"2018-07-18T15:22:32Z","snapshot_observed_at":"2026-07-06T06:36:26.235423Z","submitted_at":"2018-04-30T12:51:22Z","title":"Three Hypervelocity White Dwarfs in Gaia DR2: Evidence for Dynamically Driven Double-Degenerate Double-Detonation Type Ia Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.11163","snapshot_observed_at":"2026-08-12T20:25:19.970419Z","title":"( year 2018 a ), month Sep","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.970419Z"},"links":{"cited_paper":"/paper/1804.11163","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:bf9f076832a52f57718e63c63918c395e481dc4b05b097b0aa965ffc2b41d006","observation_id":"2b8bc05f-8d3f-46e9-b25c-bc4aab246899","resolution":{"observed_at":"2026-08-12T20:25:19.970419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01898","last_updated":"2018-01-30T20:48:59Z","snapshot_observed_at":"2026-08-10T10:52:26.239126Z","submitted_at":"2017-06-06T18:00:07Z","title":"Sub-Chandrasekhar-mass white dwarf detonations revisited","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01898","snapshot_observed_at":"2026-08-12T20:25:19.974247Z","title":"title Sub-Chandrasekhar-mass White Dwarf Detonations Revisited","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.974247Z"},"links":{"cited_paper":"/paper/1706.01898","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:55f8e6a8bd13d338b6250c9061ff2757a6eea08cb1261e189cf8a4a7cd7dcf5d","observation_id":"8b6f6628-fafa-42f7-a1b5-4397500f527f","resolution":{"observed_at":"2026-08-12T20:25:19.974247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506415","last_updated":"2005-12-05T17:11:02Z","snapshot_observed_at":"2026-08-08T11:40:10.724671Z","submitted_at":"2005-06-17T14:41:42Z","title":"Constraints on the Progenitor Systems of Type Ia Supernovae","version":2},"cited_work":{"arxiv_id":"astro-ph/0506415","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506415","snapshot_observed_at":"2026-08-12T20:25:20.448261Z","title":"Constraints on the Progenitor Systems of Type Ia Supernovae","venue":"astro-ph","work_id":"11ed8269-f41a-4990-b793-fd178a90fda7","year":2005},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.978621Z"},"links":{"cited_paper":"/paper/astro-ph/0506415","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:d101f3318b8849a053cc6b26c1ee493074f88dcf698df5c9d7552953a9d2712d","observation_id":"5305023e-0fe3-4514-95d5-c65813577f58","resolution":{"observed_at":"2026-08-12T20:25:20.453476Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.08378","last_updated":"2020-11-11T21:10:25Z","snapshot_observed_at":"2026-08-13T07:58:47.517790Z","submitted_at":"2020-02-19T19:00:05Z","title":"HOLISMOKES -- I. Highly Optimised Lensing Investigations of Supernovae, Microlensing Objects, and Kinematics of Ellipticals and Spirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.08378","snapshot_observed_at":"2026-08-12T20:25:19.982756Z","title":"( year 2020 ), month Dec","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.982756Z"},"links":{"cited_paper":"/paper/2002.08378","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:213fcd500e820fa4d79eed38e7f535b5cbf7690bb95dc273cd418fab65821d5c","observation_id":"bdbc7f4b-2234-45df-ad6c-26c3de2d068d","resolution":{"observed_at":"2026-08-12T20:25:19.982756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":6,"parse_uncertain":0,"unresolved":80,"verified_exact":14,"verified_fuzzy":0},"total_outbound_references":114},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 100 of 114 outbound references and 2 inbound Pith citation observations for arXiv:2411.09740."}