{"as_of":"2026-08-16T17:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e788082a53d887620ea5a3bd7e26206b39ad6780e64431e15d4b43297cd04988","coverage":[{"denominator":177,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:49:26.695772Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:47:24.910148Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-14T13:47:28.274996Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"cited_work":{"arxiv_id":"2505.08946","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.08946","snapshot_observed_at":"2026-08-14T13:47:28.274996Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","venue":"astro-ph.HE","work_id":"e4ad1068-562a-49a7-9884-b3ee36f1af93","year":2025},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-16T17:12:16.968557Z","submitted_at":"2026-08-13T14:46:05Z","title":"JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf","version":1},"reference_index":194,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.910148Z"},"links":{"cited_paper":"/paper/2505.08946","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:cfd64c3d9fdeb6e80e2f9700c6ab06325fc60cd39c2b21892171f5c6ed89d5b1","observation_id":"a53eb198-df4c-46d9-9374-10bb06793872","resolution":{"observed_at":"2026-08-14T13:47:28.281632Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2505.08946/citation-record","integrity":"/paper/2505.08946/integrity","json":"/paper/2505.08946/citation-record.json","paper":"/paper/2505.08946"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:49:26.165688Z","title":"The radio and X-ray emission from type II supernovae","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.165688Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:8a3e651b54f5ec8f6bf02acea4ef6f601ca75ea98cc02bb5800006d6a10758c1","observation_id":"647a7303-67c6-40fb-92c3-2b5ef1af8798","resolution":{"observed_at":"2026-08-15T21:49:26.165688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0607196","last_updated":"2006-07-12T20:32:50Z","snapshot_observed_at":"2026-08-15T11:09:24.589347Z","submitted_at":"2006-07-10T15:33:53Z","title":"Circumstellar Emission from Type Ib and Ic Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0607196","snapshot_observed_at":"2026-08-15T21:49:26.171282Z","title":"Circumstellar Emission from Type Ib and Ic Supernovae","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.171282Z"},"links":{"cited_paper":"/paper/astro-ph/0607196","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:5186e96acff3839552840c72437078bfef398bf6c405e305c19b8292fdf65159","observation_id":"b7d1dd75-d08a-4c73-96c5-d566c46fc7b0","resolution":{"observed_at":"2026-08-15T21:49:26.171282Z","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":"2026-08-15T21:49:26.177067Z","title":"Radio and X-Ray Emission as Probes of Type IIP Supernovae and Red Supergiant Mass Loss","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.177067Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:2679843ae31364e939feb204358a6f3a5afd253597bfa4623a49bee1d32f13e9","observation_id":"43f3b225-a1da-4dee-be9b-637efce4d8a3","resolution":{"observed_at":"2026-08-15T21:49:26.177067Z","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":"2026-08-15T21:49:26.182124Z","title":"Thermal and Non-thermal Emission from Circumstellar Interaction","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.182124Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:1f219118ae8a67c728d30520818a4704456cc85ab7f549b6c59a39203a827e5f","observation_id":"9b013ac5-1e50-41d1-b587-ec78d2433301","resolution":{"observed_at":"2026-08-15T21:49:26.182124Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-15T21:49:26.188219Z","title":"Supernova Interaction with a Circumstellar Medium","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.188219Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:b7aeae17ac1205182e879533250d7a1cc79d9daf6991193cd3530d065295d318","observation_id":"0716eed9-59a3-4085-9110-6438e8e9ec7b","resolution":{"observed_at":"2026-08-15T21:49:26.188219Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/183728","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:49:27.407177Z","title":"Detection of X-rays during the outburst of SN 1980 k","venue":null,"work_id":"8b185461-310e-42b0-a0ea-be19049e2e5f","year":1980},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.193495Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:b819cade6d9f53171124277fd89aff2e9e2d9ed7418c0d8941fb9805d75cf0b2","observation_id":"6b70f5c9-ed9a-41ca-a226-f882ca71f233","resolution":{"observed_at":"2026-08-15T21:49:27.412351Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0034-4885/58/11/001","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:49:27.390409Z","title":"X-ray emission from supernovae: a review of the observations","venue":null,"work_id":"3aaf783d-d0e2-4f12-b564-3a27bc3a133a","year":1995},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.198980Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:0f3d66047d728c9ae2ce2278ed2c14fb4fde91b27fdd1206da44621fefdedaf2","observation_id":"d7d6a83b-2c58-4b89-8ffe-21b169d0bb99","resolution":{"observed_at":"2026-08-15T21:49:27.395463Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/3-540-45863-8_7","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:49:27.375243Z","title":"X-Ray Supernovae","venue":null,"work_id":"4dafe4ca-2a17-4757-985d-a6b5a6054152","year":2003},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.203478Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:8b71717dc433ca88290d8808f7af882a02a46e2037bec04aef507401908b46d9","observation_id":"66faa3b8-6e0f-4037-803a-1ed4490ceb1c","resolution":{"observed_at":"2026-08-15T21:49:27.380022Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s1743921306008398","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:49:27.358812Z","title":"Young X-ray-Emitting Supernovae in Galaxies","venue":null,"work_id":"55ebe2fe-63f0-4e08-8961-3c34f21ff738","year":2006},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.209175Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:6bf07784d2744ce3f3dbc5daa905e659fc7aa2b6ca3db4420f9ffe16d55e44f2","observation_id":"3d02f7f3-e34e-45df-9b60-950a27e631d7","resolution":{"observed_at":"2026-08-15T21:49:27.363963Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-15T21:49:26.214393Z","title":"X-Ray Emission from Supernovae","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.214393Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:cd467e1c41d8c85a8074f1f02514edb7122348b2103a0cd9e709d7d465d3b560","observation_id":"312f037c-bfef-416c-a56a-5a9b0c7a83c5","resolution":{"observed_at":"2026-08-15T21:49:26.214393Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.2616","last_updated":"2011-09-12T20:20:54Z","snapshot_observed_at":"2026-08-15T04:35:28.326576Z","submitted_at":"2011-09-12T20:20:54Z","title":"What are Published X-ray lightcurves telling us about Young Supernova Expansion?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.2616","snapshot_observed_at":"2026-08-15T21:49:26.218939Z","title":"What are published X-ray light curves telling us about young supernova expansion? MNRAS 2012, 419, 1515–1524, [arXiv:astro-ph.HE/1109.2616]","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.218939Z"},"links":{"cited_paper":"/paper/1109.2616","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:99663388b968f21474915be464556e177fff67ec523328b0e78363c6a9ecdaba","observation_id":"1d879622-7a03-44c1-b307-9c834117eba7","resolution":{"observed_at":"2026-08-15T21:49:26.218939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.5150","last_updated":"2014-02-20T21:24:26Z","snapshot_observed_at":"2026-08-14T23:43:54.193490Z","submitted_at":"2014-02-20T21:24:26Z","title":"On the Lack of X-ray Bright Type IIP Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.5150","snapshot_observed_at":"2026-08-15T21:49:26.223890Z","title":"On the lack of X-ray bright Type IIP supernovae.MNRAS 2014, 440, 1917–1924, [arXiv:astro-ph.HE/1402.5150]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.223890Z"},"links":{"cited_paper":"/paper/1402.5150","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:c844d71d8885f1e75c297d41e609ec5b84c6607ccb38f79f5bc2ef3a51bea655","observation_id":"0b6d02c7-c8c6-407c-8280-1510e3461e5b","resolution":{"observed_at":"2026-08-15T21:49:26.223890Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.06104","last_updated":"2016-07-20T20:06:27Z","snapshot_observed_at":"2026-08-14T21:47:31.016690Z","submitted_at":"2016-07-20T20:06:27Z","title":"X-Ray and Radio Emission from the Luminous Supernova 2005kd","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.06104","snapshot_observed_at":"2026-08-15T21:49:26.229143Z","title":"X-ray and radio emission from the luminous supernova 2005kd","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.229143Z"},"links":{"cited_paper":"/paper/1607.06104","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:29f210741f34cdcc5a736601a921797ea0204a1b2a9eef098bcd516eef1cb928","observation_id":"9b8a2406-5f67-4c3e-8fa7-34cb3011ec60","resolution":{"observed_at":"2026-08-15T21:49:26.229143Z","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":"2026-08-14T20:39:32.202671Z","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":"2026-08-15T21:49:26.234920Z","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":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.234920Z"},"links":{"cited_paper":"/paper/1708.07181","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:8fdd4877e34a9bbb5a9b347454d9b17eafa4b2835541c6494dbd44c43593a964","observation_id":"0fc403d3-4c77-4236-9025-7c18ca6d69c1","resolution":{"observed_at":"2026-08-15T21:49:26.234920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.1791","last_updated":"2013-10-03T00:09:35Z","snapshot_observed_at":"2026-08-15T00:11:33.824613Z","submitted_at":"2013-07-06T15:18:05Z","title":"SN 2012ca: a stripped envelope core-collapse SN interacting with dense circumstellar medium","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.1791","snapshot_observed_at":"2026-08-15T21:49:26.239647Z","title":"SN2012ca: a stripped envelope core-collapse SN interacting with dense circumstellar medium","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.239647Z"},"links":{"cited_paper":"/paper/1307.1791","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:5f4036887cec4386f0259d01451491f319e43f4bd186b90ed705c2f84a25af5e","observation_id":"3ab7d143-f977-4c0c-b96f-7c311122970f","resolution":{"observed_at":"2026-08-15T21:49:26.239647Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.6239","last_updated":"2014-08-26T20:00:22Z","snapshot_observed_at":"2026-08-14T23:21:49.669921Z","submitted_at":"2014-08-26T20:00:22Z","title":"On the Nature of Type Ia-CSM Supernovae: Optical and Near-Infrared Spectra of SN 2012ca and SN 2013dn","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.6239","snapshot_observed_at":"2026-08-15T21:49:26.244988Z","title":"On the nature of Type IIn/Ia-CSM supernovae: optical and near-infrared spectra of SN 2012ca and SN 2013dn","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.244988Z"},"links":{"cited_paper":"/paper/1408.6239","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:766215e87ee705f4c5008472af6b00a876dcfe3bc54285e787306b55ddf844da","observation_id":"570aa26e-45a0-4e77-bc88-7f255c19506c","resolution":{"observed_at":"2026-08-15T21:49:26.244988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.3667","last_updated":"2015-12-31T11:20:37Z","snapshot_observed_at":"2026-08-14T23:30:24.967637Z","submitted_at":"2014-06-13T23:46:39Z","title":"Bolometric light curves and explosion parameters of 38 stripped-envelope core-collapse supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.3667","snapshot_observed_at":"2026-08-15T21:49:26.250585Z","title":"Bolomet- ric light curves and explosion parameters of 38 stripped-envelope core-collapse supernovae","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.250585Z"},"links":{"cited_paper":"/paper/1406.3667","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:33839fc8c27e348cc3f07d41e6e332b3fe97cbd43573b5ddf3f6628a659917eb","observation_id":"37e0e64d-8e35-4ea9-9029-7e3931c9160e","resolution":{"observed_at":"2026-08-15T21:49:26.250585Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07614","last_updated":"2017-07-20T15:45:51Z","snapshot_observed_at":"2026-08-14T20:46:21.068110Z","submitted_at":"2017-07-20T15:45:51Z","title":"The Carnegie Supernova Project I: analysis of stripped-envelope supernova light curves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.07614","snapshot_observed_at":"2026-08-15T21:49:26.255349Z","title":"The Carnegie Supernova Project I","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.255349Z"},"links":{"cited_paper":"/paper/1707.07614","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:717759a69d22253d175d13648b670a04d1744616823a123f28c26da4ee7c8f15","observation_id":"f3d28263-c87e-4a83-b113-f1829fd69903","resolution":{"observed_at":"2026-08-15T21:49:26.255349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.03716","last_updated":"2018-12-13T14:24:11Z","snapshot_observed_at":"2026-08-14T17:46:07.240688Z","submitted_at":"2018-12-10T10:18:51Z","title":"Investigating the properties of stripped-envelope supernovae, what are the implications for their progenitors?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.03716","snapshot_observed_at":"2026-08-15T21:49:26.260728Z","title":"Investigating the properties of stripped- envelope supernovae; what are the implications for their progenitors? MNRAS 2019, 485, 1559– 1578, [arXiv:astro-ph.HE/1812.03716]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.260728Z"},"links":{"cited_paper":"/paper/1812.03716","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:21f33fff168539ca6ce53612939925a2e56225e5f94afc9b279d51f97c182a3a","observation_id":"88afe0f9-9e05-4f54-96ed-aac0a18a7324","resolution":{"observed_at":"2026-08-15T21:49:26.260728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.08392","last_updated":"2020-10-16T13:48:58Z","snapshot_observed_at":"2026-07-06T10:05:07.321675Z","submitted_at":"2020-10-16T13:48:58Z","title":"Type Ic supernovae from the (intermediate) Palomar Transient Factory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.08392","snapshot_observed_at":"2026-08-15T21:49:26.266383Z","title":"Type Ic supernovae from the (intermediate) Palomar Transient Factory","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.266383Z"},"links":{"cited_paper":"/paper/2010.08392","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:cc069530a334381a89ac686d07b533df0c7681df6322a10b8b0f4942b0a36c73","observation_id":"bd283369-c95b-4b28-b51d-f55570f4c5dd","resolution":{"observed_at":"2026-08-15T21:49:26.266383Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.01906","last_updated":"2024-09-03T13:54:17Z","snapshot_observed_at":"2026-08-16T13:21:45.520613Z","submitted_at":"2024-09-03T13:54:17Z","title":"Binary progenitor systems for Type Ic supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.01906","snapshot_observed_at":"2026-08-15T21:49:26.272297Z","title":"Binary progenitor systems for Type Ic supernovae","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.272297Z"},"links":{"cited_paper":"/paper/2409.01906","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:5bc277a4ec0fcd7be2fdbf499fd5e9258695d9ce0b18aa862d624d030d05c916","observation_id":"090c40ef-1101-4a32-8052-f36ac6dac58e","resolution":{"observed_at":"2026-08-15T21:49:26.272297Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.09402","last_updated":"2022-10-17T20:08:05Z","snapshot_observed_at":"2026-08-16T16:23:25.094932Z","submitted_at":"2022-10-17T20:08:05Z","title":"A population of Type Ibc supernovae with massive progenitors; broad lightcurves not uncommon in (i)PTF","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.09402","snapshot_observed_at":"2026-08-15T21:49:26.277836Z","title":"A population of Type Ibc supernovae with massive progenitors","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.277836Z"},"links":{"cited_paper":"/paper/2210.09402","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:b36b7742afb0e93caa316c2bfa539d4bfc3cd701a2720d06884f47ac968484f3","observation_id":"599236a5-7f61-45a3-aed8-a744f71c0ecc","resolution":{"observed_at":"2026-08-15T21:49:26.277836Z","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":"2026-08-15T21:49:26.283207Z","title":"Radio and X-ray observations of supernovae in dense environments","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.283207Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:f3181a5a0b9e713a6db405eacba306b00ddbe59acc21720deb5e406ce722c59c","observation_id":"8b42fe07-ebb7-4b83-afe5-760691274a57","resolution":{"observed_at":"2026-08-15T21:49:26.283207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.07405","last_updated":"2018-01-09T12:01:06Z","snapshot_observed_at":"2026-08-14T20:01:46.425430Z","submitted_at":"2017-12-20T10:39:57Z","title":"Circumstellar interaction in supernovae in dense environments - an observational perspective","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.07405","snapshot_observed_at":"2026-08-15T21:49:26.288049Z","title":"Circumstellar Interaction in Supernovae in Dense Environments—An Observational Perspective","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.288049Z"},"links":{"cited_paper":"/paper/1712.07405","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:89e511f2cfccb528a8aeaa68b944f8806ab472fd310c3ecfb8fdd5881f719182","observation_id":"c372f1d0-5e73-43af-ad32-9c014d3256fc","resolution":{"observed_at":"2026-08-15T21:49:26.288049Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.05866","last_updated":"2017-04-19T18:05:03Z","snapshot_observed_at":"2026-08-14T21:05:57.499067Z","submitted_at":"2017-04-19T18:05:03Z","title":"SNaX - A Database of Supernova X-ray Lightcurves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.05866","snapshot_observed_at":"2026-08-15T21:49:26.294343Z","title":"SNaX: A Database of Supernova X-Ray Light Curves","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.294343Z"},"links":{"cited_paper":"/paper/1704.05866","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:55672aedfbbda1822889e0ebed0ac12537c0f5c0195d7e5fdf84e7a36a8945d8","observation_id":"33757134-d492-4af8-a9cc-82038672e6d7","resolution":{"observed_at":"2026-08-15T21:49:26.294343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.04427","last_updated":"2020-11-03T19:16:21Z","snapshot_observed_at":"2026-08-14T07:31:21.561935Z","submitted_at":"2020-11-03T19:16:21Z","title":"Supernova X-Ray Database (SNaX) Updated to Ensure Long-term Stability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.04427","snapshot_observed_at":"2026-08-15T21:49:26.300214Z","title":"Supernova X-Ray Database (SNaX) Updated to Ensure Long-term Stability","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.300214Z"},"links":{"cited_paper":"/paper/2011.04427","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:acf3ffb25047729d1337413c6a0e992472cdc61618638ba7bb1262cb56b53c00","observation_id":"1074d1c9-c66f-4685-8505-0fa3d526531d","resolution":{"observed_at":"2026-08-15T21:49:26.300214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.4334","last_updated":"2010-06-22T17:16:15Z","snapshot_observed_at":"2026-08-15T05:15:37.900522Z","submitted_at":"2010-06-22T17:16:15Z","title":"On Computing Upper Limits to Source Intensities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.4334","snapshot_observed_at":"2026-08-15T21:49:26.306661Z","title":"On Computing Upper Limits to Source Intensities","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.306661Z"},"links":{"cited_paper":"/paper/1006.4334","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:cf0dae0c32bfd2e38919c2086c3e0ce76386af80c1781e2d352cbc5328d23b9d","observation_id":"bd8956ca-87e9-4958-8ea1-6ce9dd09a81d","resolution":{"observed_at":"2026-08-15T21:49:26.306661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.09137","last_updated":"2020-08-20T18:03:26Z","snapshot_observed_at":"2026-07-06T09:48:53.846452Z","submitted_at":"2020-08-20T18:03:26Z","title":"From Supernova to Remnant: Tracking the Evolution of the Oldest Known X-ray Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.09137","snapshot_observed_at":"2026-08-15T21:49:26.311562Z","title":"From Supernova to Remnant: Tracking the Evolution of the Oldest Known X-Ray Supernovae","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.311562Z"},"links":{"cited_paper":"/paper/2008.09137","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:e6b4c45b070486fe431c9a2180f5250ca827739944c9c31f8f0a1a1212445e18","observation_id":"a31d2c02-61a3-4878-bee8-3571428e218d","resolution":{"observed_at":"2026-08-15T21:49:26.311562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0311434","last_updated":"2003-11-18T15:23:03Z","snapshot_observed_at":"2026-07-07T00:38:23.503282Z","submitted_at":"2003-11-18T15:23:03Z","title":"Chandra ACIS and Newton EPIC Observations of the X-ray Luminous SN1978K in NGC 1313","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0311434","snapshot_observed_at":"2026-08-15T21:49:26.317600Z","title":"Chandra ACIS and XMM-Newton EPIC Observations of the X-Ray-Luminous SN 1978K in NGC 1313","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.317600Z"},"links":{"cited_paper":"/paper/astro-ph/0311434","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:2186fdeebcd79569d72f95828e01847b3389df22dbd0c5ffe04d6ba8548464d9","observation_id":"fb76e9fa-c061-4bb2-b1b7-cf6212827fb5","resolution":{"observed_at":"2026-08-15T21:49:26.317600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.09473","last_updated":"2017-04-19T02:29:43Z","snapshot_observed_at":"2026-08-14T21:23:10.736719Z","submitted_at":"2016-12-30T12:23:47Z","title":"The X-ray Decay of the ultraluminous supernova SN 1978K in NGC 1313","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.09473","snapshot_observed_at":"2026-08-15T21:49:26.322946Z","title":"The X-ray decay of the ultraluminous supernova SN 1978K in NGC 1313","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.322946Z"},"links":{"cited_paper":"/paper/1612.09473","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:3ac43fc306265c9d9a76621f63aecff8f905a42144e67035fba0d8f941c3eba8","observation_id":"a7173a58-ceff-40fb-be3d-0dac3fcbb3ea","resolution":{"observed_at":"2026-08-15T21:49:26.322946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0503678","last_updated":"2005-03-30T21:21:41Z","snapshot_observed_at":"2026-07-07T00:49:27.607166Z","submitted_at":"2005-03-30T21:21:41Z","title":"Late-time X-Ray, UV and Optical Monitoring of Supernova 1979C","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0503678","snapshot_observed_at":"2026-08-15T21:49:26.327927Z","title":"Late-Time X-Ray, UV , and Optical Monitoring of Supernova 1979C","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.327927Z"},"links":{"cited_paper":"/paper/astro-ph/0503678","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:6882352a2152e9882f450cd6ae2c0688981534a011f551dbc8c01b368b970b59","observation_id":"d022a915-92e6-4e88-8d86-6fce05aaf351","resolution":{"observed_at":"2026-08-15T21:49:26.327927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.1411","last_updated":"2008-07-14T17:04:33Z","snapshot_observed_at":"2026-08-15T10:17:57.378708Z","submitted_at":"2008-04-09T06:23:08Z","title":"The Long-Term Variability of the X-Ray Sources in NGC 6946 and NGC 4485/4490","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.1411","snapshot_observed_at":"2026-08-15T21:49:26.333804Z","title":"The Long-Term Variability of the X-Ray Sources in NGC 6946 and NGC 4485/4490","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.333804Z"},"links":{"cited_paper":"/paper/0804.1411","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:135eba53da24a5afe6d09288ad86859867374a64ed98e1e5ed0e2c8ea3d3db0c","observation_id":"12fa7b8c-ac15-4689-bfd7-ee22ab7c15f3","resolution":{"observed_at":"2026-08-15T21:49:26.333804Z","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":"2026-08-15T21:49:26.338759Z","title":"Supernova 1981K in NGC 4258","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.338759Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:bb90a3e033ff8cb50549dafb1228902c739c8c9643a9a366b1b96a703ec4e137","observation_id":"3d1bd5f4-61e3-432e-aa66-15df12d4cf92","resolution":{"observed_at":"2026-08-15T21:49:26.338759Z","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":"2026-08-15T21:49:26.344737Z","title":"Monitoring X-ray Emission From SN 1986J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.344737Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:1c98947c8ced200e6aeedf0c4382c36b63a9489536516da0e25abee5be8ebf85","observation_id":"94888157-9e5b-418d-9fd3-808dea1c5f63","resolution":{"observed_at":"2026-08-15T21:49:26.344737Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.02160","last_updated":"2016-08-06T22:55:31Z","snapshot_observed_at":"2026-08-14T21:45:09.239484Z","submitted_at":"2016-08-06T22:55:31Z","title":"Chandra Observes the End of an Era SN 1987A","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.02160","snapshot_observed_at":"2026-08-15T21:49:26.349418Z","title":"Chandra Observes the End of an Era in SN 1987A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.349418Z"},"links":{"cited_paper":"/paper/1608.02160","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:b8d576c1a085e17c81707c58b9453d268043ec496069878fc45c518a3c59e71a","observation_id":"afc4cb77-0ad7-4eb9-ae39-08a12ad64d5a","resolution":{"observed_at":"2026-08-15T21:49:26.349418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07990","last_updated":"2024-03-12T18:00:34Z","snapshot_observed_at":"2026-08-16T14:10:27.730816Z","submitted_at":"2024-03-12T18:00:34Z","title":"Latest Evolution of the X-Ray Remnant of SN 1987A: Beyond the Inner Ring","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07990","snapshot_observed_at":"2026-08-15T21:49:26.354894Z","title":"Latest Evolution of the X-Ray Remnant of SN 1987A: Beyond the Inner Ring","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.354894Z"},"links":{"cited_paper":"/paper/2403.07990","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:354b4a0b051df471832fc60a6c9ff1139759636acb2c6ffa950bcf89cbde452c","observation_id":"a6031b0e-a55d-4c42-a27c-26d3b2aa6ddf","resolution":{"observed_at":"2026-08-15T21:49:26.354894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0604106","last_updated":"2006-04-05T17:58:18Z","snapshot_observed_at":"2026-08-11T10:04:50.709997Z","submitted_at":"2006-04-05T17:58:18Z","title":"A Chandra ACIS Observation of the X-ray Luminous SN1988Z","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0604106","snapshot_observed_at":"2026-08-15T21:49:26.360186Z","title":"A Chandra ACIS Observation of the X-Ray-luminous SN 1988Z","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.360186Z"},"links":{"cited_paper":"/paper/astro-ph/0604106","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:fac510e01db63ab59531c47623c9c1a66adad20f88e5d0d076eb3821a540af57","observation_id":"323c3949-deaf-4597-94eb-f365f11c898e","resolution":{"observed_at":"2026-08-15T21:49:26.360186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/377213","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:49:27.323740Z","title":"X-Ray Emission from a Sample of Young Supernovae","venue":null,"work_id":"b6a511d6-df64-4190-ac8a-d25bb1a1642e","year":2003},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.365233Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:4f1445bce58b5ec59536612937bd30a1db3f4887aa0d05a2583d629f82e9cb8f","observation_id":"564c8b04-8bb3-4917-9455-61b11fcd4624","resolution":{"observed_at":"2026-08-15T21:49:27.328531Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0904.3955","last_updated":"2009-04-25T02:00:51Z","snapshot_observed_at":"2026-08-15T05:49:49.078724Z","submitted_at":"2009-04-25T02:00:51Z","title":"X-rays from the explosion site: Fifteen years of light curves of SN 1993J","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.3955","snapshot_observed_at":"2026-08-15T21:49:26.369794Z","title":"X-rays from the Explosion Site: 15 Years of Light Curves of SN 1993J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.369794Z"},"links":{"cited_paper":"/paper/0904.3955","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:1118f407afdc31edbc58e8dd53df3d1888c9b2ac9616339bf7f03c1515e89794","observation_id":"e5b530ac-cbf3-42b1-8a57-d6480d9c66fb","resolution":{"observed_at":"2026-08-15T21:49:26.369794Z","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":"2026-08-15T21:49:26.374560Z","title":"SN 1993J - The X-ray Story of a Supernova Slowly Transitioning to a Remnant","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.374560Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:7f85ec7c828f25e8b2b6960878a88c1e0cdebd66c9620359a3fa29e4c1454cb5","observation_id":"b876d070-d46a-4d12-b946-fa56acd922b5","resolution":{"observed_at":"2026-08-15T21:49:26.374560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205373","last_updated":"2002-05-22T16:01:41Z","snapshot_observed_at":"2026-08-08T13:39:32.378014Z","submitted_at":"2002-05-22T16:01:41Z","title":"X-ray Emission from the Type Ic Supernova 1994I Observed with Chandra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205373","snapshot_observed_at":"2026-08-15T21:49:26.378858Z","title":"X-Ray Emission from the Type Ic Supernova 1994I Observed with Chandra","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.378858Z"},"links":{"cited_paper":"/paper/astro-ph/0205373","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:b8765bf32270f3e53929e2fe80619292049e1c3fba1ab6f9fafe97e48c3e4c41","observation_id":"ac6ef85c-6776-46e2-8a91-205fc5675cbd","resolution":{"observed_at":"2026-08-15T21:49:26.378858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9910425","last_updated":"1999-10-22T18:25:34Z","snapshot_observed_at":"2026-07-07T01:29:13.428484Z","submitted_at":"1999-10-22T18:25:34Z","title":"X-ray Detection of SN1994W in NGC 4041?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9910425","snapshot_observed_at":"2026-08-15T21:49:26.383501Z","title":"X-Ray Detection of SN 1994W in NGC 4041?ApJL 1999, 527, L85–L88, [arXiv:astro- ph/astro-ph/9910425]","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.383501Z"},"links":{"cited_paper":"/paper/astro-ph/9910425","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:3eecae056ec2112a3d0b892016cd20246a804681db1842966445193fe25ee1e1","observation_id":"2d8df8d0-e5c3-4494-b501-b054efee33ec","resolution":{"observed_at":"2026-08-15T21:49:26.383501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0505051","last_updated":"2005-05-03T10:35:13Z","snapshot_observed_at":"2026-08-09T17:51:14.275858Z","submitted_at":"2005-05-03T10:35:13Z","title":"Chandra's tryst with SN 1995N","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0505051","snapshot_observed_at":"2026-08-15T21:49:26.389465Z","title":"Chandra’s Tryst with SN 1995N","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.389465Z"},"links":{"cited_paper":"/paper/astro-ph/0505051","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:2a7fe79dfab6ed96ea3ecc03910a0314edaf07f44e85e95416b2444b46fb60ee","observation_id":"ebfba368-3fde-474e-8f1a-186f4baa90bd","resolution":{"observed_at":"2026-08-15T21:49:26.389465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510046","last_updated":"2005-10-03T15:28:35Z","snapshot_observed_at":"2026-07-31T22:29:28.243616Z","submitted_at":"2005-10-03T15:28:35Z","title":"Simultaneous XMM-Newton and ESO VLT observations of SN 1995N: probing the wind/ejecta interaction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510046","snapshot_observed_at":"2026-08-15T21:49:26.394498Z","title":"Simul- taneous XMM-Newton and ESO VLT observations of supernova 1995N: probing the wind- ejecta interaction","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.394498Z"},"links":{"cited_paper":"/paper/astro-ph/0510046","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:6f18367c50d2c6c72c5122948b11522fb44c36ce26809f367570c9b336aa15ea","observation_id":"4b7e8bc5-6c49-440e-af4c-fc753dd9d35b","resolution":{"observed_at":"2026-08-15T21:49:26.394498Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.03710","last_updated":"2019-10-08T22:56:21Z","snapshot_observed_at":"2026-07-31T06:55:13.576943Z","submitted_at":"2019-10-08T22:56:21Z","title":"The Exceptional X-ray Evolution of SN1996cr in High Resolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.03710","snapshot_observed_at":"2026-08-15T21:49:26.400253Z","title":"The exceptional X-ray evolution of SN 1996cr in high resolution","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.400253Z"},"links":{"cited_paper":"/paper/1910.03710","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:7e21c657258491612851b508c89954c92f5dff76a488ee4bdf2e2dfa066c4f8f","observation_id":"0f5478eb-10ce-431e-ab58-038cd4b4d8ba","resolution":{"observed_at":"2026-08-15T21:49:26.400253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401184","last_updated":"2004-01-12T10:31:06Z","snapshot_observed_at":"2026-07-07T00:39:37.044390Z","submitted_at":"2004-01-12T10:31:06Z","title":"Chandra Observations of the X-ray Environs of SN 1998bw/GRB 980425","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401184","snapshot_observed_at":"2026-08-15T21:49:26.405197Z","title":"Chandra Observations of the X-Ray Environs of SN 1998bw/GRB 980425.ApJ 2004, 608, 872–882, [arXiv:astro-ph/astro-ph/0401184]","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.405197Z"},"links":{"cited_paper":"/paper/astro-ph/0401184","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:f9805ed5741aa65cc5bfdbfd197f1c1dca085aef585e8b142b17acd5af5480b0","observation_id":"7989ac1b-7560-4092-b9a3-2f95df0cbddb","resolution":{"observed_at":"2026-08-15T21:49:26.405197Z","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":"2026-08-15T21:49:26.410237Z","title":"X-Ray, Optical, and Radio Observations of the Type II Supernovae 1999em and 1998S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.410237Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:bff6b7200cf506d4c735431ebb92ecb7e07ad6700f4cc6d443d64b40f4370044","observation_id":"b2b3dd97-0371-4928-a6ad-8fa93e4d44dc","resolution":{"observed_at":"2026-08-15T21:49:26.410237Z","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":"2026-08-15T21:49:26.414780Z","title":"Chandra Observations of SN 1999gi and the X-Ray Emission of Type II-P Supernovae","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.414780Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:0553a972e493ec6a96bca976ca2d53c2f968bd80456bc209e821a0269be7d0ce","observation_id":"a8a57677-4d56-4b03-9af6-f01eef04e898","resolution":{"observed_at":"2026-08-15T21:49:26.414780Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504647","last_updated":"2005-04-28T20:02:50Z","snapshot_observed_at":"2026-08-12T03:08:23.379172Z","submitted_at":"2005-04-28T20:02:50Z","title":"High-resolution observations of SN 2001gd in NGC 5033","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504647","snapshot_observed_at":"2026-08-15T21:49:26.419831Z","title":"High-resolution observations of SN 2001gd in NGC 5033","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.419831Z"},"links":{"cited_paper":"/paper/astro-ph/0504647","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:df3d51b1b227e64eda1af8df1d6574af0dd9a1a3e8423a67c6e6879acd8bf4f2","observation_id":"5b65866b-9c62-4f61-8e7e-8960687608ef","resolution":{"observed_at":"2026-08-15T21:49:26.419831Z","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":"2026-08-15T21:49:26.424640Z","title":"Supernova 2001ig in NGC 7424","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.424640Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:bb6ce858734bdcf0cf8cca2ea740fb91315e40785803d2c537634d4e508ad0ac","observation_id":"ccdd5322-2984-4722-bd51-f9b3b61f7e23","resolution":{"observed_at":"2026-08-15T21:49:26.424640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207137","last_updated":"2002-11-06T17:39:07Z","snapshot_observed_at":"2026-07-07T00:27:17.742565Z","submitted_at":"2002-07-05T11:02:32Z","title":"The nature of the prompt X-ray and radio emission from SN2002ap","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207137","snapshot_observed_at":"2026-08-15T21:49:26.429443Z","title":"The nature of the prompt X-ray and radio emission from SN 2002ap","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.429443Z"},"links":{"cited_paper":"/paper/astro-ph/0207137","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:ce9308839c736dc79eaecd0901b1f962076dc765665defcb758cbfe6dee9d7ed","observation_id":"31be0ae7-c2eb-43c1-97bb-79fcd18ce4cb","resolution":{"observed_at":"2026-08-15T21:49:26.429443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.3190","last_updated":"2007-10-16T23:16:04Z","snapshot_observed_at":"2026-08-15T10:29:47.159489Z","submitted_at":"2007-10-16T23:16:04Z","title":"Chandra Observations of Type Ia Supernovae: Upper Limits to the X-ray Flux of SN 2002bo, SN 2002ic, SN 2005gj, and SN 2005ke","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.3190","snapshot_observed_at":"2026-08-15T21:49:26.434460Z","title":"Chandra Observations of Type Ia Supernovae: Upper Limits to the X-Ray Flux of SN 2002bo, SN 2002ic, SN 2005gj, and SN 2005ke","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.434460Z"},"links":{"cited_paper":"/paper/0710.3190","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:4d60c9d399d5e80a679d6a23bf1d2027749e4d6759da47e75c28c6a6247111a5","observation_id":"46a0713a-f793-4b4f-b0f0-3cf727a195d8","resolution":{"observed_at":"2026-08-15T21:49:26.434460Z","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":"2026-08-15T21:49:26.439301Z","title":"Supernova 2002hh in NGC 6946","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.439301Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:5e6a31b8a88839b644891175618a3a8aa088329b9ab4908c9930895b4d0fede5","observation_id":"5087527d-a670-47e6-aafd-09af1037047a","resolution":{"observed_at":"2026-08-15T21:49:26.439301Z","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":"2026-08-15T21:49:26.444328Z","title":"Supernova 2002hi","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.444328Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:3b0ed41dd8856ad80ff707aa295fef25bcaf73b6f63043fc160d6728248c96ae","observation_id":"60e1d94d-d5e1-4cdb-ab7a-b27fb8dec1b4","resolution":{"observed_at":"2026-08-15T21:49:26.444328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410163","last_updated":"2004-10-06T20:00:07Z","snapshot_observed_at":"2026-07-07T00:45:12.340815Z","submitted_at":"2004-10-06T20:00:07Z","title":"The Radio and X-ray Luminous Type Ibc Supernova 2003L","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0410163","snapshot_observed_at":"2026-08-15T21:49:26.449071Z","title":"The Radio and X-Ray-Luminous Type Ibc Supernova 2003L","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.449071Z"},"links":{"cited_paper":"/paper/astro-ph/0410163","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:9a4394ba707d46d375e8ab9a65bdb4ec62281f4eb2aa0e653a83d0ebdb0981e7","observation_id":"16fdb2fe-a0c2-4a1e-8ec3-094b8e690c10","resolution":{"observed_at":"2026-08-15T21:49:26.449071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512413","last_updated":"2006-07-17T21:08:42Z","snapshot_observed_at":"2026-08-04T00:52:01.612477Z","submitted_at":"2005-12-15T21:00:30Z","title":"The Radio and X-ray Luminous SN 2003bg and the Circumstellar Density Variations Around Radio Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512413","snapshot_observed_at":"2026-08-15T21:49:26.453942Z","title":"The Radio and X-Ray Luminous SN 2003bg and the Circumstellar Density Variations around Radio Supernovae","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.453942Z"},"links":{"cited_paper":"/paper/astro-ph/0512413","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:36f6a6ba68c49b1e92a42473c825c8917841838ca1acba93af1fcb64470882db","observation_id":"278a153e-fd37-4940-97d4-064c38caa8af","resolution":{"observed_at":"2026-08-15T21:49:26.453942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.4033","last_updated":"2012-06-18T19:44:03Z","snapshot_observed_at":"2026-08-15T00:56:27.176949Z","submitted_at":"2012-06-18T19:44:03Z","title":"X-Ray emission from SN 2004dj: A Tale of Two Shocks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.4033","snapshot_observed_at":"2026-08-15T21:49:26.459571Z","title":"X-Ray Emission from SN 2004dj: A Tale of Two Shocks","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.459571Z"},"links":{"cited_paper":"/paper/1206.4033","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:1213b1eaa57b4794919d834b3c0909542f517866a706b6ce0cca570fca6b91b5","observation_id":"53142099-4c2c-4103-8e24-4cf6fbb03a5d","resolution":{"observed_at":"2026-08-15T21:49:26.459571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.06395","last_updated":"2019-10-14T19:47:19Z","snapshot_observed_at":"2026-08-03T21:26:30.398444Z","submitted_at":"2019-10-14T19:47:19Z","title":"Interaction of SN~Ib 2004dk with a Previously-Expelled Envelope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.06395","snapshot_observed_at":"2026-08-15T21:49:26.464743Z","title":"Interaction of SN Ib 2004dk with a Previously Expelled Envelope","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.464743Z"},"links":{"cited_paper":"/paper/1910.06395","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:65d729c27f9019f2ad81eb4bd0fc6d36d6893e77ef42ab8c0864e98001b995ea","observation_id":"c9f420c1-7c59-4041-a9f5-3cc519f12e42","resolution":{"observed_at":"2026-08-15T21:49:26.464743Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0707.3485","last_updated":"2007-07-24T05:24:49Z","snapshot_observed_at":"2026-08-15T10:35:32.063369Z","submitted_at":"2007-07-24T05:24:49Z","title":"Type IIP Supernova SN 2004et: A Multi-Wavelength Study in X-Ray, Optical and Radio","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.3485","snapshot_observed_at":"2026-08-15T21:49:26.469449Z","title":"Type IIP supernova SN 2004et: a multiwavelength study in X-ray, optical and radio","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.469449Z"},"links":{"cited_paper":"/paper/0707.3485","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:582aef2ed289226c1cb7ad3a068ed498537c7f52d02018d5d17792686311a29b","observation_id":"57753d6a-fd7d-4fda-b2c9-2a70df5e64b0","resolution":{"observed_at":"2026-08-15T21:49:26.469449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.7180","last_updated":"2013-11-28T00:25:23Z","snapshot_observed_at":"2026-08-14T23:53:40.997380Z","submitted_at":"2013-11-28T00:25:23Z","title":"SN 2005ip: A Luminous Type IIn Supernova Emerging from a Dense Circumstellar Medium as Revealed by X-Ray Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.7180","snapshot_observed_at":"2026-08-15T21:49:26.474736Z","title":"SN 2005ip: A Luminous Type IIn Supernova Emerging from a Dense Circumstellar Medium as Revealed by X-Ray Observations","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.474736Z"},"links":{"cited_paper":"/paper/1311.7180","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:85b93efbcca7d4682bb34471aabaf88f19acc7898ef55c1f45379c73a072a609","observation_id":"7d444b64-abc4-45ae-ab4e-cf8532fc2f2b","resolution":{"observed_at":"2026-08-15T21:49:26.474736Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-15T21:49:26.481059Z","title":"X-Ray, UV , and Optical Observations of Supernova 2006bp with Swift: Detection of Early X-Ray Emission","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.481059Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:b04c1ab81555f919ff6776859b449140cc800e0b623e5d0c815110a099b35760","observation_id":"bd039ad5-86d9-46bc-a00b-66bf9b2d7dcc","resolution":{"observed_at":"2026-08-15T21:49:26.481059Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.1173","last_updated":"2013-04-03T20:08:34Z","snapshot_observed_at":"2026-08-15T00:22:42.975140Z","submitted_at":"2013-04-03T20:08:34Z","title":"Superluminous X-rays from a superluminous supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.1173","snapshot_observed_at":"2026-08-15T21:49:26.486951Z","title":"Superluminous X-Rays from a Superluminous Supernova","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.486951Z"},"links":{"cited_paper":"/paper/1304.1173","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:4e22c5f113d819234615a52482ce14a331263b996cd6a310e9c2f14563f469d1","observation_id":"881bd7c2-7557-4573-88cf-8b7ef3de9c14","resolution":{"observed_at":"2026-08-15T21:49:26.486951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0612617","last_updated":"2007-05-22T06:59:38Z","snapshot_observed_at":"2026-07-07T01:05:37.020605Z","submitted_at":"2006-12-21T04:39:34Z","title":"SN 2006gy: Discovery of the most luminous supernova ever recorded, powered by the death of an extremely massive star like Eta Carinae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0612617","snapshot_observed_at":"2026-08-15T21:49:26.492284Z","title":"SN 2006gy: Discovery of the Most Luminous Supernova Ever Recorded, Powered by the Death of an Extremely Massive Star like η Carinae","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.492284Z"},"links":{"cited_paper":"/paper/astro-ph/0612617","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:0bcd7f4c8260bc5605d0fad138c1a1a762182df21a881d96b7c1bcb406560beb","observation_id":"b547cb3c-f098-4211-bd49-fc2f8fb7c878","resolution":{"observed_at":"2026-08-15T21:49:26.492284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0712.3290","last_updated":"2008-01-08T19:02:14Z","snapshot_observed_at":"2026-08-15T10:25:02.290533Z","submitted_at":"2007-12-19T21:25:10Z","title":"Swift and Chandra Detections of Supernova 2006jc: Evidence for Interaction of the Supernova Shock with a Circumstellar Shell","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0712.3290","snapshot_observed_at":"2026-08-15T21:49:26.498958Z","title":"Swift and Chandra Detections of Supernova 2006jc: Evidence for Interaction of the Supernova Shock with a Circumstellar Shell","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.498958Z"},"links":{"cited_paper":"/paper/0712.3290","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:473b788719dff4930fa5a7e9215a741755c526aef953284e694b87d25ec436f3","observation_id":"615d0449-205f-43fd-a6cd-5acb2e1eac8a","resolution":{"observed_at":"2026-08-15T21:49:26.498958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.1614","last_updated":"2012-03-07T21:00:01Z","snapshot_observed_at":"2026-08-15T04:16:59.918785Z","submitted_at":"2012-03-07T21:00:01Z","title":"Strong Evolution of X-Ray Absorption in the Type IIn Supernova SN 2010jl","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.1614","snapshot_observed_at":"2026-08-15T21:49:26.504131Z","title":"Strong Evolution of X-Ray Absorption in the Type IIn Supernova SN 2010jl","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.504131Z"},"links":{"cited_paper":"/paper/1203.1614","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:34556100cd41a13822cadae16078d1fd24b4b82c5d0d138b2d4f76bc1c5d242c","observation_id":"5404e354-d3f2-4e0a-a57d-ef097987b4f4","resolution":{"observed_at":"2026-08-15T21:49:26.504131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.1932","last_updated":"2010-05-14T19:54:43Z","snapshot_observed_at":"2026-08-15T05:19:20.148359Z","submitted_at":"2010-05-11T20:01:41Z","title":"Radio and X-ray Observations of the Type Ic SN 2007gr Reveal an Ordinary, Non-relativistic Explosion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.1932","snapshot_observed_at":"2026-08-15T21:49:26.510615Z","title":"Radio and X-ray Observations of the Type Ic SN 2007gr Reveal an Ordinary, Non-relativistic Explosion.ApJ 2010, 725, 922–930, [arXiv:astro-ph.CO/1005.1932]","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.510615Z"},"links":{"cited_paper":"/paper/1005.1932","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:3a80f690bc1b9de76b8c6a1e6993e20e8620e9fc6401e75f23a4f845db0bc6c0","observation_id":"aa66104a-47a1-4fd1-862e-fcd16ca8a8cf","resolution":{"observed_at":"2026-08-15T21:49:26.510615Z","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":"2026-08-15T21:49:26.515599Z","title":"Possible Detection of SN 2007pk in X-Rays with Swift","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.515599Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:aab6ae04b59bd55989b1a261780d31d264ce48df7ad4b22bf7a3a892edc4fe31","observation_id":"60bbaa68-82b1-4795-9226-44240aed5a25","resolution":{"observed_at":"2026-08-15T21:49:26.515599Z","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":"2026-08-15T21:49:26.521261Z","title":"Swift XRT Detection of Supernova 2008M in X-Rays","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.521261Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:8973b79318dd0452603cc9af0c6fbd7e2ab87676d13f38a1e5a93eeb29056eae","observation_id":"0078929a-ec42-48d3-be19-80f4efaa20cb","resolution":{"observed_at":"2026-08-15T21:49:26.521261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.0967","last_updated":"2009-09-04T21:43:48Z","snapshot_observed_at":"2026-08-15T05:39:49.543364Z","submitted_at":"2009-09-04T21:43:48Z","title":"Multi-Wavelength Properties of the Type IIb SN 2008ax","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.0967","snapshot_observed_at":"2026-08-15T21:49:26.526515Z","title":"Multi-Wavelength Properties of the Type IIb SN 2008ax","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.526515Z"},"links":{"cited_paper":"/paper/0909.0967","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:5a12fca04af54e3b430dd2d630e9214d3f997204c1b955abeb16b14dfd5910bc","observation_id":"32469e6e-2720-45b8-8a8e-2ed83dcceb1e","resolution":{"observed_at":"2026-08-15T21:49:26.526515Z","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":"2026-08-15T21:49:26.532003Z","title":"Swift XRT Detection of Supernova 2008ij in X-Rays","venue":null,"work_id":null,"year":1918},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.532003Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:f74038785061820a6391f310559eb210b5ab905cc85758b42303b3d60cc45a3b","observation_id":"947ffab3-8d4b-4837-85b5-b47e92e7fbd1","resolution":{"observed_at":"2026-08-15T21:49:26.532003Z","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":"2026-08-15T21:49:26.536857Z","title":"Swift XRT Detection of Supernova 2009dd in X-Rays","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.536857Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:a11abf4a7e35c56f46d7ee7ef8a784926e19e9462fa38c98d1f4b600a9b2ac63","observation_id":"55c2b6da-520e-4e5d-9596-c8fccfb05c71","resolution":{"observed_at":"2026-08-15T21:49:26.536857Z","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":"2026-08-15T21:49:26.541639Z","title":"Swift XRT Detection of Supernova 2009gj in X-Rays","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.541639Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:5bfbc5e8007a76ec6c6dca2c8d1150b3dcc48602fd64a437223a503c1ac61ddd","observation_id":"2e29f30b-6a9e-4338-ac5f-2551e9432003","resolution":{"observed_at":"2026-08-15T21:49:26.541639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3738","last_updated":"2012-05-16T17:16:38Z","snapshot_observed_at":"2026-08-15T00:59:52.257443Z","submitted_at":"2012-05-16T17:16:38Z","title":"Multi-wavelength Observations of the Type IIb Supernova 2009mg","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3738","snapshot_observed_at":"2026-08-15T21:49:26.546239Z","title":"Multiwavelength observations of the Type IIb supernova 2009mg","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.546239Z"},"links":{"cited_paper":"/paper/1205.3738","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:2c5080e3d6e42f1e35344da3aaefd5a99f6c19a6cc8f2f0da1f7b67ec3bd3c6f","observation_id":"6dff74f5-fa2b-4df5-919a-515936361038","resolution":{"observed_at":"2026-08-15T21:49:26.546239Z","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":"2026-08-15T21:49:26.552496Z","title":"Swift XRT Detection of Supernova 2009mk in X-Rays","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.552496Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:545b483352e044c7995405e139833ed0308bd3a737fe711c28b30a0952019d0c","observation_id":"7e2b6156-4036-4754-9de5-4c496dbdc3d4","resolution":{"observed_at":"2026-08-15T21:49:26.552496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.05865","last_updated":"2017-04-19T18:03:55Z","snapshot_observed_at":"2026-08-14T21:05:57.601735Z","submitted_at":"2017-04-19T18:03:55Z","title":"Results from a systematic survey of X-ray emission from Hydrogen-poor Superluminous Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.05865","snapshot_observed_at":"2026-08-15T21:49:26.557250Z","title":"Results from a Systematic Survey of X-Ray Emission from Hydrogen-poor Superluminous SNe","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.557250Z"},"links":{"cited_paper":"/paper/1704.05865","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:4059f1f2bc80f6ecc3d7eb6100f89e8bda30b4e0bc8770027e72fa00761612f5","observation_id":"390985a3-b035-4bda-874c-83cc57a2ceae","resolution":{"observed_at":"2026-08-15T21:49:26.557250Z","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":"2026-08-15T21:49:26.562419Z","title":"Swift XRT Detection of Supernova 2010F in X-Rays","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.562419Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:e999796ff58b3d4cfe5ad5de0aa6496282448b5c287e4fd9225ebcefb3c0b65a","observation_id":"3f88fdb5-cdeb-43cc-b366-b9801fb630fa","resolution":{"observed_at":"2026-08-15T21:49:26.562419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.06059","last_updated":"2015-07-28T12:51:38Z","snapshot_observed_at":"2026-08-14T22:39:30.342402Z","submitted_at":"2015-07-22T04:49:59Z","title":"X-ray and radio emission from Type IIn supernova SN 2010jl","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.06059","snapshot_observed_at":"2026-08-15T21:49:26.569125Z","title":"X-Ray and Radio Emission from Type IIn Supernova SN 2010jl","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.569125Z"},"links":{"cited_paper":"/paper/1507.06059","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:c431da1d3878005ad64474ddeb620d9a29a3f00c42da28cb972a88efd3a9664c","observation_id":"6b0ed264-1e20-428d-b2f3-487b4064c93f","resolution":{"observed_at":"2026-08-15T21:49:26.569125Z","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":"2026-08-15T21:49:26.574926Z","title":"Swift XRT Detection of Supernova 2010jr in X-Rays","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.574926Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:14e298b859bf8eb59bf934c4bb20c7614fa733be287cbba2f01ebda38f6a08f0","observation_id":"63167d7c-7776-45ad-add1-29d34bd982ff","resolution":{"observed_at":"2026-08-15T21:49:26.574926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.1876","last_updated":"2012-05-17T16:07:26Z","snapshot_observed_at":"2026-08-15T04:41:33.144180Z","submitted_at":"2011-07-10T17:09:53Z","title":"Panchromatic Observations of SN 2011dh Point to a Compact Progenitor Star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.1876","snapshot_observed_at":"2026-08-15T21:49:26.581356Z","title":"Panchromatic Observations of SN 2011dh Point to a Compact Progenitor Star","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.581356Z"},"links":{"cited_paper":"/paper/1107.1876","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:73450d3740733022a081a806f2742030ac83858e08850bcef9b4a821836991df","observation_id":"0853adfc-9ffd-4b35-86a8-dd053bd7b69b","resolution":{"observed_at":"2026-08-15T21:49:26.581356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.2455","last_updated":"2014-03-11T01:41:47Z","snapshot_observed_at":"2026-08-14T23:41:47.435046Z","submitted_at":"2014-03-11T01:41:47Z","title":"Long-Lasting X-Ray Emission from Type IIb Supernova 2011dh and Mass-Loss History of The Yellow Supergiant Progenitor","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.2455","snapshot_observed_at":"2026-08-15T21:49:26.587028Z","title":"Long-lasting X-Ray Emission from Type IIb Supernova 2011dh and Mass-loss History of the Yellow Supergiant Progenitor","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.587028Z"},"links":{"cited_paper":"/paper/1403.2455","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:3ccd7f08386d5d29efb6341afb0b41db4784176bb271b381c4c76eebb52acdb7","observation_id":"a385cfb8-2292-47f6-a1e1-a1ed8f1181bd","resolution":{"observed_at":"2026-08-15T21:49:26.587028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.7067","last_updated":"2013-03-11T17:13:52Z","snapshot_observed_at":"2026-08-15T00:27:10.027091Z","submitted_at":"2013-02-28T03:27:55Z","title":"The progenitor of SN 2011ja: Clues from circumstellar interaction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.7067","snapshot_observed_at":"2026-08-15T21:49:26.593579Z","title":"The Progenitor of SN 2011ja: Clues from Circumstellar Interaction","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.593579Z"},"links":{"cited_paper":"/paper/1302.7067","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:9aa73d6e315f42274518b39ea4fcd806dd3f37476654205b3344b508e94de045","observation_id":"e3cc50e4-5db3-4cca-95cf-8d3768f829cd","resolution":{"observed_at":"2026-08-15T21:49:26.593579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.0741","last_updated":"2012-02-03T15:51:29Z","snapshot_observed_at":"2026-08-15T04:20:21.749124Z","submitted_at":"2012-02-03T15:51:29Z","title":"Inverse Compton X-ray Emission from Supernovae with Compact Progenitors: Application to SN2011fe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.0741","snapshot_observed_at":"2026-08-15T21:49:26.598873Z","title":"Inverse Compton X-Ray Emission from Super- novae with Compact Progenitors: Application to SN2011fe","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.598873Z"},"links":{"cited_paper":"/paper/1202.0741","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:cb4cbbdb3a716686ae7d8fabb14f8459d53b30726f00785337e1d3d4af6b9335","observation_id":"2493706e-5079-4131-9792-9f03c202582f","resolution":{"observed_at":"2026-08-15T21:49:26.598873Z","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":"2026-08-15T21:49:26.605072Z","title":"Chandra Observation of SN 2012A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.605072Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:c283b789630b91ff42815e19e20a4b8ca461a4555f26c5f629ddde9a2013edbf","observation_id":"ade3b765-75c8-417a-a5e7-cdc1991c9ab6","resolution":{"observed_at":"2026-08-15T21:49:26.605072Z","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":"2026-08-15T21:49:26.610405Z","title":"Radio Observations Reveal a Smooth Circumstellar Environment Around the Extraordinary Type Ib Supernova 2012au","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.610405Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:17b3acaa6dd152fd0418af4a2cdc9d4afef344571aac9be33e814e64c362f537","observation_id":"3a9281c0-a6bb-41be-afc5-59903e97c5af","resolution":{"observed_at":"2026-08-15T21:49:26.610405Z","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":"2026-08-15T21:49:26.616105Z","title":"X-ray emission at the position of SN2013ai","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.616105Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:7307c26576fd7176fc5fdb2cc546de899c9004ead11e50ffc677dbba7a16e117","observation_id":"1b530f87-9db6-46c4-b06f-ded69cc00ae2","resolution":{"observed_at":"2026-08-15T21:49:26.616105Z","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":"2026-08-15T21:49:26.620980Z","title":"X-ray detection of SN2013ak (PSN J08070669-2803101)","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.620980Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:2f01b7041d3b429ea9e8ff41ada7e96689a9bd5ffa45cce978a9ed4442d52d3a","observation_id":"6cabf0d8-f1cb-4299-a131-a05a44e4e6ca","resolution":{"observed_at":"2026-08-15T21:49:26.620980Z","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":"2026-08-15T21:49:26.626433Z","title":"X-ray emission at the position of SN2013by","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.626433Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:e660e474dff33cd9314994f576a5887ac4bef683c4fd18a73b0c113897d8551d","observation_id":"9831f782-1cae-4c6a-8796-c4d6652e0614","resolution":{"observed_at":"2026-08-15T21:49:26.626433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.02257","last_updated":"2017-09-11T17:11:01Z","snapshot_observed_at":"2026-08-14T20:35:54.963996Z","submitted_at":"2017-09-05T18:33:43Z","title":"The Transition of a Type IIL Supernova into a Supernova Remnant: Late-time Observations of SN 2013by","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.02257","snapshot_observed_at":"2026-08-15T21:49:26.631040Z","title":"The Transition of a Type IIL Supernova into a Supernova Remnant: Late-time Observations of SN 2013by","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.631040Z"},"links":{"cited_paper":"/paper/1709.02257","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:c0bc5c9a2a15aa2ac3cf9aa58a201ba10fe17047841c1c645d298d73019c3a99","observation_id":"d72be989-4992-4645-ae67-ba7172892a97","resolution":{"observed_at":"2026-08-15T21:49:26.631040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06025","last_updated":"2015-11-25T22:33:28Z","snapshot_observed_at":"2026-08-14T22:27:00.725189Z","submitted_at":"2015-10-20T20:04:07Z","title":"Probing Final Stages of Stellar Evolution with X-Ray Observations of SN 2013ej","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06025","snapshot_observed_at":"2026-08-15T21:49:26.636689Z","title":"Probing Final Stages of Stellar Evolution with X-Ray Observations of SN 2013ej","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.636689Z"},"links":{"cited_paper":"/paper/1510.06025","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:c0515a7e2c6a7728ad7b24c38f007cdcc63498e9ee0163ced4911b66a56c134f","observation_id":"b9fbcaa0-b9da-43d0-a831-09fb365ada2a","resolution":{"observed_at":"2026-08-15T21:49:26.636689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12747","last_updated":"2022-03-23T22:15:03Z","snapshot_observed_at":"2026-08-16T17:12:21.115061Z","submitted_at":"2022-03-23T22:15:03Z","title":"Seven Years of SN 2014C: a Multi-Wavelength Synthesis of an Extraordinary Supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.12747","snapshot_observed_at":"2026-08-15T21:49:26.642196Z","title":"Seven Years of SN 2014C: A Multiwavelength Synthesis of an Extraordinary Supernova","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.642196Z"},"links":{"cited_paper":"/paper/2203.12747","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:07cfeb1ae50c68d20fe2882261ab0dd2bbbf7a46db34b40a521836f7dd91954e","observation_id":"40331c06-e22b-4573-95ed-f2d040771662","resolution":{"observed_at":"2026-08-15T21:49:26.642196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.00842","last_updated":"2022-06-02T02:32:18Z","snapshot_observed_at":"2026-08-16T16:55:51.258684Z","submitted_at":"2022-06-02T02:32:18Z","title":"Seven years of coordinated Chandra-NuSTAR observations of SN2014C unfold the extreme mass-loss history of its stellar progenitor","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.00842","snapshot_observed_at":"2026-08-15T21:49:26.647405Z","title":"Seven Years of Coordinated Chandra-NuSTAR Observations of SN 2014C Unfold the Extreme Mass-loss History of Its Stellar Progenitor","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.647405Z"},"links":{"cited_paper":"/paper/2206.00842","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:af8ae590692a1e942618bd2faec9649f891cfcb688c58fd8b1a096bd202cf9bf","observation_id":"bc495b02-2074-4278-a00d-2143964fe6a0","resolution":{"observed_at":"2026-08-15T21:49:26.647405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01887","last_updated":"2017-10-12T18:30:40Z","snapshot_observed_at":"2026-08-14T20:55:43.458651Z","submitted_at":"2017-06-06T18:00:01Z","title":"iPTF15eqv: Multi-wavelength Expos\\'e of a Peculiar Calcium-rich Transient","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01887","snapshot_observed_at":"2026-08-15T21:49:26.653396Z","title":"iPTF15eqv: Multiwavelength Exposé of a Peculiar Calcium-rich Transient","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.653396Z"},"links":{"cited_paper":"/paper/1706.01887","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:e9484739784f3c330686c02c5b381f63130967504e2b41cae18c3d6b7749c1e3","observation_id":"8017e243-8e64-4005-bcfe-beade0987185","resolution":{"observed_at":"2026-08-15T21:49:26.653396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.02226","last_updated":"2019-07-19T17:30:53Z","snapshot_observed_at":"2026-08-14T16:36:31.662654Z","submitted_at":"2019-05-06T18:14:28Z","title":"SN 2016coi (ASASSN-16fp): an energetic H-stripped core-collapse supernova from a massive stellar progenitor with large mass loss","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.02226","snapshot_observed_at":"2026-08-15T21:49:26.659398Z","title":"SN 2016coi (ASASSN-16fp): An Energetic H- stripped Core-collapse Supernova from a Massive Stellar Progenitor with Large Mass Loss","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.659398Z"},"links":{"cited_paper":"/paper/1905.02226","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:ec7f500ee6ceb33b818328bc323206972784c7be3567cec3a6c84ce3fb008bc7","observation_id":"5c051d1d-3401-43d6-8794-e010ea061afc","resolution":{"observed_at":"2026-08-15T21:49:26.659398Z","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":"2026-08-15T21:49:26.664782Z","title":"X-ray detection of SN 2016gkg with Swift-XRT","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.664782Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:72da82fdb48ea9f77f9b4ab1c344ad7b210da2995586e7124b41eca3bf75dc6d","observation_id":"b987333b-52c8-403d-a4a9-150d8a789948","resolution":{"observed_at":"2026-08-15T21:49:26.664782Z","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":"2026-08-16T13:38:35.911666Z","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":"2026-08-15T21:49:26.670022Z","title":"X-ray observations of two Type Ia supernovae with an Hα line in their optical spectrum","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.670022Z"},"links":{"cited_paper":"/paper/2407.00279","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:dc25c56d5a3d9370dd8c64d540b3f96928fc2d01d093daa2a7831decd17babfb","observation_id":"eebaf9c1-6736-4db8-95df-ed648fa15d0e","resolution":{"observed_at":"2026-08-15T21:49:26.670022Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-15T21:49:26.676268Z","title":"Swift and ATLAS observations of ASASSN-17fy/SN2017dwq","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.676268Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:c3669c06d511d57ea6ea52177a277f8ed4ed775ecaa621d1de28b88afa388084","observation_id":"3102b4de-44c9-4aeb-b087-991feb2e2d36","resolution":{"observed_at":"2026-08-15T21:49:26.676268Z","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":"2026-08-15T21:49:26.681095Z","title":"Swift-XRT observations of Type IIn supernova ASASSN-17kr a.k.a","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.681095Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:aee60ef402cc2e9a328ceb5735f4bf0acd3effb13130e56c3d3ac5a52a0e71d3","observation_id":"64cd8efc-cf5a-4c28-ac64-4f11ccc0736d","resolution":{"observed_at":"2026-08-15T21:49:26.681095Z","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":"2026-08-15T21:49:26.686670Z","title":"Swift and LT UV and optical observations of type IIn superluminous supernova 2017gir","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.686670Z"},"links":{"citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:07f77638008987ab89c2990d9a837d41da3df59e4edc02d064f63b087c75d069","observation_id":"ada163cb-b4b3-4417-aa7e-431dae1ba583","resolution":{"observed_at":"2026-08-15T21:49:26.686670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.03212","last_updated":"2022-10-06T21:15:57Z","snapshot_observed_at":"2026-08-16T16:26:17.148490Z","submitted_at":"2022-10-06T21:15:57Z","title":"The luminous Type IIN supernova SN 2017hcc: Infrared bright, X-ray and radio faint","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.03212","snapshot_observed_at":"2026-08-15T21:49:26.691030Z","title":"The luminous type IIn supernova SN 2017hcc: Infrared bright, X-ray, and radio faint","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.691030Z"},"links":{"cited_paper":"/paper/2210.03212","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:141f69cbe7e783092537020888d3983134ecce8bfae9403b474bba833d274eae","observation_id":"52dbb57b-ce99-4eac-9848-897278f1a536","resolution":{"observed_at":"2026-08-15T21:49:26.691030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.09274","last_updated":"2022-11-17T00:25:32Z","snapshot_observed_at":"2026-08-16T16:15:32.234386Z","submitted_at":"2022-11-17T00:25:32Z","title":"Chandra Fails to Detect X-ray Emission from Type Ia SN 2018fhw/ASASSN-18tb","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.09274","snapshot_observed_at":"2026-08-15T21:49:26.695772Z","title":"Chandra fails to detect X-ray emission from Type Ia SN 2018fhw/ASASSN- 18tb","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-15T21:49:26.695772Z"},"links":{"cited_paper":"/paper/2211.09274","citing_paper":"/paper/2505.08946"},"observation_digest":"sha256:8897fba664fd8c20b382aecf10b290f0eaee0f6c5f5ac78e5f7f6810385173b6","observation_id":"44531113-1fc9-45c3-92d2-74f5c0e14545","resolution":{"observed_at":"2026-08-15T21:49:26.695772Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.08946","last_updated":"2025-05-13T20:19:59Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T03:13:46.449931Z","submitted_at":"2025-05-13T20:19:59Z","title":"On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":11,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":84,"verified_exact":5,"verified_fuzzy":0},"total_outbound_references":177},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 177 outbound references and 1 inbound Pith citation observation for arXiv:2505.08946."}