{"as_of":"2026-08-15T04:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0444f5bbab2cebd86d133b5828ababedfe9ebf4e3a9f3ec808c55156cc46f966","coverage":[{"denominator":234,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:47:24.183563Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.13321/citation-record","integrity":"/paper/2608.13321/integrity","json":"/paper/2608.13321/citation-record.json","paper":"/paper/2608.13321"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2012.00757","last_updated":"2020-12-01T19:00:00Z","snapshot_observed_at":"2026-08-14T15:34:39.992338Z","submitted_at":"2020-12-01T19:00:00Z","title":"Distances to PHANGS Galaxies: New Tip of the Red Giant Branch Measurements and Adopted Distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.00757","snapshot_observed_at":"2026-08-14T13:47:23.291337Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":1,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.291337Z"},"links":{"cited_paper":"/paper/2012.00757","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:db7515561f74b078df35b0fac6c5a0b75920c2e96361ab3f3ec4b389af2a45ff","observation_id":"a3720b55-a5f9-4964-a177-958c99f79c79","resolution":{"observed_at":"2026-08-14T13:47:23.291337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04776","last_updated":"2024-04-26T14:38:27Z","snapshot_observed_at":"2026-08-15T01:47:02.428400Z","submitted_at":"2024-01-09T19:05:00Z","title":"Tip of the Red Giant Branch Distances with JWST: An Absolute Calibration in NGC 4258 and First Applications to Type Ia Supernova Hosts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.04776","snapshot_observed_at":"2026-08-14T13:47:23.298771Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":2,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.298771Z"},"links":{"cited_paper":"/paper/2401.04776","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:4cd90492e13ba8343f467c2d7e2b94089b774e966c89cee4887f60e23c132163","observation_id":"9a1cdb5e-1d78-48ae-9205-c6f6e2d98430","resolution":{"observed_at":"2026-08-14T13:47:23.298771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.07882","last_updated":"2025-02-26T02:17:57Z","snapshot_observed_at":"2026-08-14T10:47:18.720805Z","submitted_at":"2025-02-11T19:00:01Z","title":"A Sizable Discrepancy in Ground-Based JAGB Distances to Nearby Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.07882","snapshot_observed_at":"2026-08-14T13:47:23.305986Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":3,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.305986Z"},"links":{"cited_paper":"/paper/2502.07882","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:6895643af114a0029b4d0fb156d908b441afdbb851334aa854b8c44770bb2d75","observation_id":"4ac94952-3b88-41a5-8881-7f350b596ab1","resolution":{"observed_at":"2026-08-14T13:47:23.305986Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.7091","last_updated":"2014-04-03T18:29:07Z","snapshot_observed_at":"2026-08-14T23:39:41.184131Z","submitted_at":"2014-03-27T16:35:28Z","title":"Characterizing the V-band light-curves of hydrogen-rich type II supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.7091","snapshot_observed_at":"2026-08-14T13:47:23.312600Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":4,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.312600Z"},"links":{"cited_paper":"/paper/1403.7091","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:73be59a453d799ddf6b8c248a55c0120ef528222378d356f9f99e773e22a9d76","observation_id":"37e15e54-2ad4-4d21-a9e4-de26f467a719","resolution":{"observed_at":"2026-08-14T13:47:23.312600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.06738","last_updated":"2024-10-09T10:18:28Z","snapshot_observed_at":"2026-08-12T22:27:25.019494Z","submitted_at":"2024-10-09T10:18:28Z","title":"Optical and near-infrared photometry of 94 type II supernovae from the Carnegie Supernova Project","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.06738","snapshot_observed_at":"2026-08-14T13:47:23.318520Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":5,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.318520Z"},"links":{"cited_paper":"/paper/2410.06738","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:7347d7fb5c301acccd8f2e59ddf39aca345f140e26e1a06dea43c0e5e7ac6bf6","observation_id":"62a0d842-fbaf-41ff-bb84-fed66fbaf657","resolution":{"observed_at":"2026-08-14T13:47:23.318520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.1209","last_updated":"2010-04-07T23:41:15Z","snapshot_observed_at":"2026-08-04T19:22:27.949320Z","submitted_at":"2010-04-07T23:41:15Z","title":"SN 2007od: A Type IIP SN with Circumstellar Interaction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.1209","snapshot_observed_at":"2026-08-14T13:47:23.326815Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":6,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.326815Z"},"links":{"cited_paper":"/paper/1004.1209","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:2309d24fec906950df22613533b201060cf76d108c6cf6723f7abab293ba3148","observation_id":"2cf84aea-091a-484f-b9d9-ada8c37b275d","resolution":{"observed_at":"2026-08-14T13:47:23.326815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.15163","last_updated":"2024-03-22T12:44:33Z","snapshot_observed_at":"2026-08-13T04:33:49.630124Z","submitted_at":"2024-01-26T19:15:33Z","title":"Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.15163","snapshot_observed_at":"2026-08-14T13:47:23.334455Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":7,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.334455Z"},"links":{"cited_paper":"/paper/2401.15163","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:bcd4cb92ff63bac7889710212151ec3e4b2c6c46f88b2d5766a6650cc83469fa","observation_id":"2a03bae7-3696-4c1e-b5f2-284e37427d7d","resolution":{"observed_at":"2026-08-14T13:47:23.334455Z","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":"2026-08-14T13:47:23.341709Z","title":"doi:10.5281/zenodo.804967 , publisher =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":8,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.341709Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:6bb61888c534aecead548f6ca232af23f2a50511b974db03b8f17c69a69a1e84","observation_id":"ff25e41c-574c-46f1-b7b0-af4a9e096d6b","resolution":{"observed_at":"2026-08-14T13:47:23.341709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410153","last_updated":"2004-10-06T16:51:46Z","snapshot_observed_at":"2026-08-08T02:49:18.982638Z","submitted_at":"2004-10-06T16:51:46Z","title":"Type IIP Supernovae as Cosmological Probes: A SEAM Distance to SN 1999em","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0410153","snapshot_observed_at":"2026-08-14T13:47:23.347326Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":9,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.347326Z"},"links":{"cited_paper":"/paper/astro-ph/0410153","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f8d9cbd2a62a1e5ea71b3e2dd322ff98433cc2d3cc72df488a96cb5c98547092","observation_id":"73d0f59e-4fee-4503-80fc-50b14d0a6076","resolution":{"observed_at":"2026-08-14T13:47:23.347326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.07222","last_updated":"2020-01-20T19:10:37Z","snapshot_observed_at":"2026-08-13T18:32:28.804824Z","submitted_at":"2020-01-20T19:10:37Z","title":"A new mass-loss rate prescription for red supergiants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.07222","snapshot_observed_at":"2026-08-14T13:47:23.353534Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":10,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.353534Z"},"links":{"cited_paper":"/paper/2001.07222","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:9d64b6221bd650a56e49b2bc08e4f52e78d8a6fb719d8a2bb68321d456084bef","observation_id":"18be1cf3-7299-4a5a-8d31-577c61c49a8e","resolution":{"observed_at":"2026-08-14T13:47:23.353534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.14027","last_updated":"2024-10-17T20:57:29Z","snapshot_observed_at":"2026-08-12T22:20:32.893845Z","submitted_at":"2024-10-17T20:57:29Z","title":"The red supergiant progenitor luminosity problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.14027","snapshot_observed_at":"2026-08-14T13:47:23.359233Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":11,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.359233Z"},"links":{"cited_paper":"/paper/2410.14027","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:1c9f9ce3e1adb67b4ddf0bff5b335f03bed1b8f605474ac1161a4d2c0e606b50","observation_id":"df5875cf-106e-4f8b-982f-28a6b1066aef","resolution":{"observed_at":"2026-08-14T13:47:23.359233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.06207","last_updated":"2015-04-25T21:37:04Z","snapshot_observed_at":"2026-08-14T22:51:17.832299Z","submitted_at":"2015-04-23T14:42:33Z","title":"SN 2013ej - A type IIL supernova with weak signs of interaction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.06207","snapshot_observed_at":"2026-08-14T13:47:23.365575Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":12,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.365575Z"},"links":{"cited_paper":"/paper/1504.06207","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:d0aa68bd3eb6477e0ca4f0284949b206d42cc830de07ddf5f73af8f2dd52a6e5","observation_id":"5bfe2d0a-af72-42e4-bff8-c26c7366ae2f","resolution":{"observed_at":"2026-08-14T13:47:23.365575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02635","last_updated":"2023-09-06T12:39:12Z","snapshot_observed_at":"2026-08-12T01:28:40.566876Z","submitted_at":"2022-01-07T19:00:01Z","title":"The Automated Photometry Of Transients (AutoPhOT) pipeline","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.02635","snapshot_observed_at":"2026-08-14T13:47:23.371354Z","title":", year = 2022, month = nov, volume =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":13,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.371354Z"},"links":{"cited_paper":"/paper/2201.02635","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:997e9f3c90241a475167b29a45d243aad2d7bb43322e008a88395a67006a4ce0","observation_id":"0f0eeaff-e98b-4ffc-9928-d081678dba4d","resolution":{"observed_at":"2026-08-14T13:47:23.371354Z","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":"2026-08-14T13:47:23.377658Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":14,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.377658Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:7accdc0d05b5f236e7e9546db1e0c57d20fdc642bcc7279e4b89985f714bb936","observation_id":"186728e1-e202-41a6-a7d6-6536e18a9263","resolution":{"observed_at":"2026-08-14T13:47:23.377658Z","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":"2026-08-14T13:47:23.384808Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":15,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.384808Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:4ab568422bcd4adeb0554d732952ddc7b5f0b75d905bfc5938bbc9b1f9142f3a","observation_id":"a2faa200-0f71-48fe-a99e-71e84fa2477e","resolution":{"observed_at":"2026-08-14T13:47:23.384808Z","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":"2026-08-14T13:47:23.394418Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":16,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.394418Z"},"links":{"cited_paper":"/paper/1510.06025","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:e667ec9c9dfd437cecaac1ae3bb3f32745e10bae4493a8e4866f4228f1138b7e","observation_id":"090cbfc1-f9e4-4e62-9992-b7464e66df4a","resolution":{"observed_at":"2026-08-14T13:47:23.394418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.06116","last_updated":"2017-10-16T09:17:45Z","snapshot_observed_at":"2026-08-14T20:32:03.704134Z","submitted_at":"2017-09-18T18:28:31Z","title":"The Initial Masses of the Red Supergiant Progenitors to Type-II Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.06116","snapshot_observed_at":"2026-08-14T13:47:23.402017Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":17,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.402017Z"},"links":{"cited_paper":"/paper/1709.06116","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:eb1c1aed9d285655b69bf24af45d93055989f5059a46212d7c783c5e2ebf8fe4","observation_id":"b49700e7-765b-4f64-883a-96a0c35044fe","resolution":{"observed_at":"2026-08-14T13:47:23.402017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.06020","last_updated":"2020-01-16T19:00:18Z","snapshot_observed_at":"2026-07-06T08:51:03.422313Z","submitted_at":"2020-01-16T19:00:18Z","title":"The `Red Supergiant Problem': the upper luminosity boundary of type-II supernova progenitors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.06020","snapshot_observed_at":"2026-08-14T13:47:23.407541Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":18,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.407541Z"},"links":{"cited_paper":"/paper/2001.06020","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:27f8747023a88b7c24b98a8f0611210caf6f20377887c09ff5756473a7109e1f","observation_id":"3a8ed4d2-1b0a-4122-bb76-3c07101c9f48","resolution":{"observed_at":"2026-08-14T13:47:23.407541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.10883","last_updated":"2022-08-23T11:35:09Z","snapshot_observed_at":"2026-08-13T14:40:22.752752Z","submitted_at":"2022-08-23T11:35:09Z","title":"Explosion Imminent: the appearance of Red Supergiants at the point of core-collapse","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.10883","snapshot_observed_at":"2026-08-14T13:47:23.418019Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":19,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.418019Z"},"links":{"cited_paper":"/paper/2208.10883","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:63f53be0c4b9c2c9c21c07cdaf8942ae03d818af35d4c0d58406ed1b7c4f3f57","observation_id":"f23c10c9-e8be-4f4c-9dad-c7c51543a8e7","resolution":{"observed_at":"2026-08-14T13:47:23.418019Z","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":"2026-08-14T13:47:23.427438Z","title":"doi:10.5281/zenodo.17943031 , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":20,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.427438Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b81cc9493f2aeb9bcf2c5dc279e51810a3bacf76f15dcfbf7e723c163ce4f07e","observation_id":"a08ec191-1427-49ad-b2ec-fb324ffb136e","resolution":{"observed_at":"2026-08-14T13:47:23.427438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.07254","last_updated":"2018-02-20T18:59:59Z","snapshot_observed_at":"2026-08-14T19:44:03.045897Z","submitted_at":"2018-02-20T18:59:59Z","title":"Observed Type II supernova colours from the Carnegie Supernova Project-I","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.07254","snapshot_observed_at":"2026-08-14T13:47:23.434648Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":21,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.434648Z"},"links":{"cited_paper":"/paper/1802.07254","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:a9d45da34dc59c29464b77a84594b3f780b91c7d9ffaae31cc84a2febe518c55","observation_id":"685e6d11-0dc4-42f0-b464-ef3fd0037162","resolution":{"observed_at":"2026-08-14T13:47:23.434648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504028","last_updated":"2005-04-01T17:00:52Z","snapshot_observed_at":"2026-07-07T00:49:33.518255Z","submitted_at":"2005-04-01T17:00:52Z","title":"Quantitative Spectroscopy of Photospheric-Phase Type II Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504028","snapshot_observed_at":"2026-08-14T13:47:23.442935Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":22,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.442935Z"},"links":{"cited_paper":"/paper/astro-ph/0504028","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:85a60aca53ae0adb282540bff67d7328cbfcf3dc2f558e3ea88d3343456d0976","observation_id":"5ef262d2-fca3-4dee-b346-c5dd0771ae55","resolution":{"observed_at":"2026-08-14T13:47:23.442935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510526","last_updated":"2005-10-18T18:02:15Z","snapshot_observed_at":"2026-08-11T05:07:21.783459Z","submitted_at":"2005-10-18T18:02:15Z","title":"Quantitative spectroscopic analysis of and distance to SN1999em","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510526","snapshot_observed_at":"2026-08-14T13:47:23.452099Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":23,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.452099Z"},"links":{"cited_paper":"/paper/astro-ph/0510526","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:99f9e89aec79fd59e035302ace964705f0259a8446295a2ff4d2825815de5500","observation_id":"c2f9b8e8-99e9-4ab1-8998-3a2214733fa7","resolution":{"observed_at":"2026-08-14T13:47:23.452099Z","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":"2026-08-14T13:47:23.462313Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":24,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.462313Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b97a97d4d3ba25f7d18df45b2bb166c628fac96873f89f805987b9c7f86588fa","observation_id":"75742303-4381-4beb-ba0f-469487691c03","resolution":{"observed_at":"2026-08-14T13:47:23.462313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.01721","last_updated":"2016-04-26T17:05:16Z","snapshot_observed_at":"2026-08-14T22:33:38.555514Z","submitted_at":"2015-09-05T17:38:04Z","title":"Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.01721","snapshot_observed_at":"2026-08-14T13:47:23.475825Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":25,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.475825Z"},"links":{"cited_paper":"/paper/1509.01721","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:0ecb28c1640117d49df8f1270a46e307152bdf2babd9f0d6247177e611b7e72c","observation_id":"15d2dd58-b4a9-43c0-80b3-621b05dac45d","resolution":{"observed_at":"2026-08-14T13:47:23.475825Z","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":"2026-08-14T13:47:23.482549Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":26,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.482549Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:6f49973f301d5f12663e80c0af73f615912df5a2d0261c4495b7deba67c51eda","observation_id":"6f165dc2-ed8f-4e0c-8171-4deffdfa6d06","resolution":{"observed_at":"2026-08-14T13:47:23.482549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.02539","last_updated":"2023-07-05T18:00:02Z","snapshot_observed_at":"2026-08-13T11:02:06.462596Z","submitted_at":"2023-07-05T18:00:02Z","title":"A comprehensive optical search for pre-explosion outbursts from the quiescent progenitor of SN~2023ixf","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02539","snapshot_observed_at":"2026-08-14T13:47:23.489861Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":27,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.489861Z"},"links":{"cited_paper":"/paper/2307.02539","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b1b153e7ccca86128a8c24d82a5a4db10e4c80752465ca349f9a81db7afe651e","observation_id":"abc724fb-579e-47c0-9439-74a5902a7183","resolution":{"observed_at":"2026-08-14T13:47:23.489861Z","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":"2026-08-14T13:47:23.495833Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":28,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.495833Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:9120067869a0110cff06225f86821bbe6aa872f6ee947f3e0c2463a98e2e8c3f","observation_id":"f3c9a469-360f-4d13-93d9-c9320cc56373","resolution":{"observed_at":"2026-08-14T13:47:23.495833Z","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":"2026-08-14T13:47:23.502819Z","title":"Self-similar solutions","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":29,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.502819Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:dac0f015ec7b201922b68bf6aea486c68cdca5ac26ec6bf2a298bdae1df22d4a","observation_id":"8b562c7c-7bb6-4719-a8ff-cbff4dcd78e9","resolution":{"observed_at":"2026-08-14T13:47:23.502819Z","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":"2026-08-14T13:47:23.512087Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":30,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.512087Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:6750a01f973857ea11b451a4fad050ffd7fbfe61a9e563960a8647991d9bf799","observation_id":"dd87b738-41df-48fb-9355-c16104654555","resolution":{"observed_at":"2026-08-14T13:47:23.512087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405616","last_updated":"2004-05-31T05:02:39Z","snapshot_observed_at":"2026-07-07T00:42:47.382674Z","submitted_at":"2004-05-31T05:02:39Z","title":"The Infrared Array Camera (IRAC) for the Spitzer Space Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405616","snapshot_observed_at":"2026-08-14T13:47:23.523707Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":31,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.523707Z"},"links":{"cited_paper":"/paper/astro-ph/0405616","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f6e7e4da19c13a753444d7a00e9779ffe6d0fd3642cf384aa83ebf348649422a","observation_id":"fb8fb497-7958-4b61-a822-94decd5483f9","resolution":{"observed_at":"2026-08-14T13:47:23.523707Z","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":"2026-08-14T13:47:23.531099Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":32,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.531099Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:1253cd343e3d0c9e1f5929ef6666a9731cb8eb21f958cae0e0d8d4b19336afba","observation_id":"e7dc3046-1ba2-43ec-a062-d4bc06e09011","resolution":{"observed_at":"2026-08-14T13:47:23.531099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1523","last_updated":"2012-04-06T17:39:47Z","snapshot_observed_at":"2026-07-06T02:45:53.370955Z","submitted_at":"2012-04-06T17:39:47Z","title":"Red and dead: The progenitor of SN 2012aw in M95","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.1523","snapshot_observed_at":"2026-08-14T13:47:23.537881Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":33,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.537881Z"},"links":{"cited_paper":"/paper/1204.1523","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:44d3dd8a6d6d37a00755333ae197c64c8329b2992314026d5c63afc32aa07a00","observation_id":"bf6db601-4c8f-4ddb-a5fb-2190f47fbde9","resolution":{"observed_at":"2026-08-14T13:47:23.537881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.06579","last_updated":"2015-11-08T22:13:16Z","snapshot_observed_at":"2026-08-14T22:39:15.935948Z","submitted_at":"2015-07-23T17:31:31Z","title":"The disappearance of the progenitor of SN 2012aw in late-time imaging","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.06579","snapshot_observed_at":"2026-08-14T13:47:23.547416Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":34,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.547416Z"},"links":{"cited_paper":"/paper/1507.06579","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:9ad6c8f6f943baa60af6795da44686fd14914eb5357b681924f821a59f8061c7","observation_id":"a9508302-5246-44b6-9108-2f0c3aebed20","resolution":{"observed_at":"2026-08-14T13:47:23.547416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.05922","last_updated":"2019-07-12T18:56:31Z","snapshot_observed_at":"2026-08-14T16:06:17.561878Z","submitted_at":"2019-07-12T18:56:31Z","title":"The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.05922","snapshot_observed_at":"2026-08-14T13:47:23.553529Z","title":null,"venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":35,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.553529Z"},"links":{"cited_paper":"/paper/1907.05922","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:52b3227919cae3ecc569aa9e40c0eccb2c91e1f42b494d56cea305c2cad2c937","observation_id":"1b565ea0-cb9e-41b0-bfed-c244ae949850","resolution":{"observed_at":"2026-08-14T13:47:23.553529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.10793","last_updated":"2020-05-21T17:19:25Z","snapshot_observed_at":"2026-08-11T14:46:23.141792Z","submitted_at":"2020-05-21T17:19:25Z","title":"Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.10793","snapshot_observed_at":"2026-08-14T13:47:23.563194Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":36,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.563194Z"},"links":{"cited_paper":"/paper/2005.10793","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:77a524f26f1a2c56b40e73ce225df2937f3be85b85bee158b1a461bc1854eab0","observation_id":"0f7c2ede-caa2-42fd-86b3-65f753905bfa","resolution":{"observed_at":"2026-08-14T13:47:23.563194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15656","last_updated":"2021-06-29T18:09:57Z","snapshot_observed_at":"2026-08-13T18:54:46.984821Z","submitted_at":"2021-06-29T18:09:57Z","title":"Measurements of the Hubble Constant: Tensions in Perspective","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15656","snapshot_observed_at":"2026-08-14T13:47:23.571957Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":37,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.571957Z"},"links":{"cited_paper":"/paper/2106.15656","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:6aeb2e34b3dc029bce9b94d95ce774540124db475697c8997719bed882489352","observation_id":"c372601c-72b0-42cb-9d36-d3a0886e03d3","resolution":{"observed_at":"2026-08-14T13:47:23.571957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.06153","last_updated":"2025-03-17T18:25:04Z","snapshot_observed_at":"2026-08-12T23:04:57.606251Z","submitted_at":"2024-08-12T13:48:33Z","title":"Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.06153","snapshot_observed_at":"2026-08-14T13:47:23.578566Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":38,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.578566Z"},"links":{"cited_paper":"/paper/2408.06153","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:06318580799c54e9d1be44b7100070e5129a15ec7a3bbeb6a607e45b74a04bde","observation_id":"e9f16b2e-854d-422e-9054-c08836432312","resolution":{"observed_at":"2026-08-14T13:47:23.578566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.07303","last_updated":"2020-01-23T00:08:18Z","snapshot_observed_at":"2026-07-06T08:51:41.797614Z","submitted_at":"2020-01-21T01:23:52Z","title":"A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.07303","snapshot_observed_at":"2026-08-14T13:47:23.588532Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":39,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.588532Z"},"links":{"cited_paper":"/paper/2001.07303","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:2d594c96dc613e22171bbdd42fcf7e1895b5d3f241318558e47f86d4a9ccb6ca","observation_id":"05bf6414-20a2-4462-8cc7-380e5fc86fe2","resolution":{"observed_at":"2026-08-14T13:47:23.588532Z","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":"2026-08-14T13:47:23.599574Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":40,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.599574Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:282c76767e4eb49a9a900c6023933653bf874999ea0d64e2bc9a1ea45d5d704a","observation_id":"32e28608-442a-4712-8faf-8885ba94a353","resolution":{"observed_at":"2026-08-14T13:47:23.599574Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.02487","last_updated":"2017-09-07T23:52:20Z","snapshot_observed_at":"2026-08-14T20:35:08.649259Z","submitted_at":"2017-09-07T23:52:20Z","title":"Type II supernova spectral diversity I: Observations, sample characterization and spectral line evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.02487","snapshot_observed_at":"2026-08-14T13:47:23.605942Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":41,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.605942Z"},"links":{"cited_paper":"/paper/1709.02487","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:db69bd8100787c029a49bd63502e6318e210b974f58c04ea1f55a1da1f0a17b2","observation_id":"c89afcc5-5ef9-459e-a268-57b7a10bb2a4","resolution":{"observed_at":"2026-08-14T13:47:23.605942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0105006","last_updated":"2001-05-01T02:43:47Z","snapshot_observed_at":"2026-07-07T00:18:05.621708Z","submitted_at":"2001-05-01T02:43:47Z","title":"The Distance to SN 1999em from the Expanding Photosphere Method","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0105006","snapshot_observed_at":"2026-08-14T13:47:23.612832Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":42,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.612832Z"},"links":{"cited_paper":"/paper/astro-ph/0105006","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:5185079a2c9d9cb1ee7adf7e36deb7a7b76b28c4bc35a289ab698030fc630a30","observation_id":"e99f51e2-0d61-437a-8507-56931bcafff8","resolution":{"observed_at":"2026-08-14T13:47:23.612832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.1939","last_updated":"2008-04-11T17:16:57Z","snapshot_observed_at":"2026-07-06T01:36:42.109300Z","submitted_at":"2008-04-11T17:16:57Z","title":"ESC Supernova spectroscopy of non-ESC targets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.1939","snapshot_observed_at":"2026-08-14T13:47:23.618890Z","title":", keywords =","venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":43,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.618890Z"},"links":{"cited_paper":"/paper/0804.1939","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:2bc3bb31f52c23f97eccfd524b99e89c45a6b1e3bf54a53a90dca1f6bd1e89c1","observation_id":"213d0d11-e6b3-438b-ad8f-500fa260ae45","resolution":{"observed_at":"2026-08-14T13:47:23.618890Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0109148","last_updated":"2001-09-10T13:08:48Z","snapshot_observed_at":"2026-07-07T00:21:23.851416Z","submitted_at":"2001-09-10T13:08:48Z","title":"The Infrared Continuum Spectrum of VY CMa","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0109148","snapshot_observed_at":"2026-08-14T13:47:23.626427Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":44,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.626427Z"},"links":{"cited_paper":"/paper/astro-ph/0109148","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:9755104fae3017a02a45f341ba2c31f80e98b81183796a7b1dc3ce807ce8b771","observation_id":"e79a6843-1dbd-4bcc-9d49-81b24d1573ad","resolution":{"observed_at":"2026-08-14T13:47:23.626427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15566","last_updated":"2021-05-26T07:42:52Z","snapshot_observed_at":"2026-07-31T05:15:21.216698Z","submitted_at":"2020-10-29T13:36:11Z","title":"Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15566","snapshot_observed_at":"2026-08-14T13:47:23.633580Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":45,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.633580Z"},"links":{"cited_paper":"/paper/2010.15566","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:418233987aa11bf2c28a5904f9b7bf6096935931af03dc09b103d270cd6f0206","observation_id":"0f82915e-2941-43f4-b8da-beb2eba1077a","resolution":{"observed_at":"2026-08-14T13:47:23.633580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03165","last_updated":"2023-09-20T06:25:30Z","snapshot_observed_at":"2026-08-13T11:00:44.746672Z","submitted_at":"2023-07-06T17:47:01Z","title":"From Discovery to the First Month of the Type II Supernova 2023ixf: High and Variable Mass Loss in the Final Year before Explosion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03165","snapshot_observed_at":"2026-08-14T13:47:23.640142Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":46,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.640142Z"},"links":{"cited_paper":"/paper/2307.03165","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:11147e31c17a198fa10e6bcee033436406722913f6e9b117c27ef03c32b7edfa","observation_id":"f12e3900-1cb3-489e-9401-71c63f9947f2","resolution":{"observed_at":"2026-08-14T13:47:23.640142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0406167","last_updated":"2004-06-07T15:02:39Z","snapshot_observed_at":"2026-07-07T00:42:56.630337Z","submitted_at":"2004-06-07T15:02:39Z","title":"The Infrared Spectrograph on the Spitzer Space Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0406167","snapshot_observed_at":"2026-08-14T13:47:23.647549Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":47,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.647549Z"},"links":{"cited_paper":"/paper/astro-ph/0406167","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:4ced63236fa693d6a697e115f7086e1c3ea8614161175d91d4982fa2bbbb0f97","observation_id":"3feaf84e-4d31-4d9a-9290-1259ba027757","resolution":{"observed_at":"2026-08-14T13:47:23.647549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.00446","last_updated":"2015-04-02T04:52:45Z","snapshot_observed_at":"2026-08-14T22:53:56.226902Z","submitted_at":"2015-04-02T04:52:45Z","title":"SN 2013ej in M74: A Luminous and Fast-declining Type II-P Supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.00446","snapshot_observed_at":"2026-08-14T13:47:23.654414Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":48,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.654414Z"},"links":{"cited_paper":"/paper/1504.00446","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:35c9464d5863f20898465752af3e047c8cc692580388846900eec0d4fec595f8","observation_id":"5f7845a1-096c-4f03-ad69-9150805e0a19","resolution":{"observed_at":"2026-08-14T13:47:23.654414Z","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":"2026-08-14T13:47:23.660481Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":49,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.660481Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:745857b09219513f89b63cd04f5f548318a44085d766bfff9ba9a794eea2ab1c","observation_id":"ca024464-f69b-4f6d-8704-2bd1cc9a2080","resolution":{"observed_at":"2026-08-14T13:47:23.660481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.01108","last_updated":"2020-08-03T18:01:25Z","snapshot_observed_at":"2026-07-06T09:44:11.377445Z","submitted_at":"2020-08-03T18:01:25Z","title":"Exploring the Mass Loss Histories of the Red Supergiants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.01108","snapshot_observed_at":"2026-08-14T13:47:23.668117Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":50,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.668117Z"},"links":{"cited_paper":"/paper/2008.01108","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:5269388522d48b98e85efda4a195479f4ebab3b37a9e2336d2fbc758dbe3a852","observation_id":"78459849-ab2f-4bb1-a4f3-a2d280ede5b1","resolution":{"observed_at":"2026-08-14T13:47:23.668117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.15965","last_updated":"2025-07-21T18:05:03Z","snapshot_observed_at":"2026-08-06T23:14:20.924746Z","submitted_at":"2025-07-21T18:05:03Z","title":"Red Supergiants -- The Other Side of the H-R Diagram","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.15965","snapshot_observed_at":"2026-08-14T13:47:23.675600Z","title":"Galaxies , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":51,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.675600Z"},"links":{"cited_paper":"/paper/2507.15965","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:54c683d2115ee276afc774a010395cfa983cb4d8b08c851c9db54e8575a3bff6","observation_id":"1ea4d2e6-24bc-4893-a5ea-0c678121f24a","resolution":{"observed_at":"2026-08-14T13:47:23.675600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9612164","last_updated":"1996-12-17T16:45:22Z","snapshot_observed_at":"2026-07-07T01:15:22.722355Z","submitted_at":"1996-12-17T16:45:22Z","title":"Self-similarity and scaling behavior of IR emission from radiatively heated dust: I. Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9612164","snapshot_observed_at":"2026-08-14T13:47:23.700912Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":54,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.700912Z"},"links":{"cited_paper":"/paper/astro-ph/9612164","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:63495084897a1ec2001acc69ee2c9162837fea2b9644935d3ad6d04cd7fbb1c8","observation_id":"c21b1e1b-1341-4914-8d60-e70d08a2bf80","resolution":{"observed_at":"2026-08-14T13:47:23.700912Z","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":"2026-08-14T13:47:23.710473Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":55,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.710473Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:d685255ec29c39a4a0ba49d8315778346bc7bff81d075a79293a742dbdd5c641","observation_id":"d195b9e8-8387-4a0f-9ab5-1ed12c4fc48a","resolution":{"observed_at":"2026-08-14T13:47:23.710473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.08078","last_updated":"2025-07-10T18:00:03Z","snapshot_observed_at":"2026-08-10T08:33:23.564931Z","submitted_at":"2025-07-10T18:00:03Z","title":"SN 2023ixf: The Closest Supernova of the Decade","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.08078","snapshot_observed_at":"2026-08-14T13:47:23.716695Z","title":"Universe , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":56,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.716695Z"},"links":{"cited_paper":"/paper/2507.08078","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:e900c4354aa8f151595b85ed78bc1f2373406d51a3b7f7482239a1bd0a9a507b","observation_id":"421ff685-14a2-4791-8c35-ac95a983fa60","resolution":{"observed_at":"2026-08-14T13:47:23.716695Z","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":"2026-08-14T13:47:23.726833Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":57,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.726833Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:10dbaff62c36d70cd933ab3510bb6fa1d728bc4b4636923f37ca3c0bba83aed9","observation_id":"3bf42c72-1a10-44f9-98ed-7926ccb0fbbb","resolution":{"observed_at":"2026-08-14T13:47:23.726833Z","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":"2026-08-14T13:47:23.733365Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":58,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.733365Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:37626fede28155440755a7a85e6479234348d17a161236e80eca25dca47ec652","observation_id":"1e22c557-7763-4baa-9321-2dde682b7537","resolution":{"observed_at":"2026-08-14T13:47:23.733365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.5538","last_updated":"2008-10-30T19:10:48Z","snapshot_observed_at":"2026-07-06T01:47:34.497802Z","submitted_at":"2008-10-30T19:10:48Z","title":"Distance determination to 12 Type II Supernovae using the Expanding Photosphere Method","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.5538","snapshot_observed_at":"2026-08-14T13:47:23.743133Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":59,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.743133Z"},"links":{"cited_paper":"/paper/0810.5538","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:49d84135ac47a8ab58a5d67d93faddd87cb153d7ba2d3dd2a7eb7df7c97bccbc","observation_id":"96b65212-2fa9-445e-96f7-3fd5a4b5b689","resolution":{"observed_at":"2026-08-14T13:47:23.743133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.00348","last_updated":"2018-06-01T13:55:28Z","snapshot_observed_at":"2026-08-14T19:08:32.234017Z","submitted_at":"2018-06-01T13:55:28Z","title":"The Dusty Progenitor Star of the Type II Supernova 2017eaw","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.00348","snapshot_observed_at":"2026-08-14T13:47:23.749330Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":60,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.749330Z"},"links":{"cited_paper":"/paper/1806.00348","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:d81705d2a129fa366fe49da53538a5d086b2f3b224d55fec3ad9702e05fe6fb4","observation_id":"cb33d8a0-551e-44b4-ad8c-c37214421417","resolution":{"observed_at":"2026-08-14T13:47:23.749330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04722","last_updated":"2023-06-07T18:37:19Z","snapshot_observed_at":"2026-08-13T19:20:00.162739Z","submitted_at":"2023-06-07T18:37:19Z","title":"SN2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.04722","snapshot_observed_at":"2026-08-14T13:47:23.760432Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":61,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.760432Z"},"links":{"cited_paper":"/paper/2306.04722","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:cfe2d5a4a5ce3a710f95a377d3f0b24db125e27ccc98f4c51ab9c427448c98c7","observation_id":"5ac932a9-268f-4c00-ae0b-0c8963ce54d6","resolution":{"observed_at":"2026-08-14T13:47:23.760432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.10994","last_updated":"2025-08-14T18:00:56Z","snapshot_observed_at":"2026-08-13T00:45:06.275588Z","submitted_at":"2025-08-14T18:00:56Z","title":"The Type II SN 2025pht in NGC 1637: A Red Supergiant with Carbon-rich Circumstellar Dust as the First JWST Detection of a Supernova Progenitor Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.10994","snapshot_observed_at":"2026-08-14T13:47:23.769428Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":62,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.769428Z"},"links":{"cited_paper":"/paper/2508.10994","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:612f292667becff26f9210261cf2f73edfad0482d7cc20786a2354f65114e1f3","observation_id":"85aa1129-1dd3-4471-8965-399aef7429b3","resolution":{"observed_at":"2026-08-14T13:47:23.769428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.4111","last_updated":"2012-08-20T20:02:06Z","snapshot_observed_at":"2026-08-15T00:49:21.474440Z","submitted_at":"2012-08-20T20:02:06Z","title":"On Absorption by Circumstellar Dust, With the Progenitor of SN2012aw as a Case Study","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.4111","snapshot_observed_at":"2026-08-14T13:47:23.785733Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":64,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.785733Z"},"links":{"cited_paper":"/paper/1208.4111","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:dcf3d418704ef05087295a58834bc86225e95430d041f35272a5ad67805b8497","observation_id":"696fba6b-dd61-4f8e-9fa4-168ee75b7630","resolution":{"observed_at":"2026-08-14T13:47:23.785733Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.07216","last_updated":"2020-01-20T19:00:02Z","snapshot_observed_at":"2026-08-03T16:11:58.325279Z","submitted_at":"2020-01-20T19:00:02Z","title":"On The Red Supergiant Problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.07216","snapshot_observed_at":"2026-08-14T13:47:23.796243Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":65,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.796243Z"},"links":{"cited_paper":"/paper/2001.07216","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:661204485d4d711ca92ad57f89fa780d4fd83d999435270750c1301bd73d9fa8","observation_id":"71483bd7-c0d6-4d63-a5be-0b48e2eb1a98","resolution":{"observed_at":"2026-08-14T13:47:23.796243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.19939","last_updated":"2025-01-16T12:32:03Z","snapshot_observed_at":"2026-08-12T22:14:55.264755Z","submitted_at":"2024-10-25T19:20:56Z","title":"SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.19939","snapshot_observed_at":"2026-08-14T13:47:23.807577Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":66,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.807577Z"},"links":{"cited_paper":"/paper/2410.19939","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f0a94d56ef235a03eb110853e0245a02824002c78f1f0bf708f9cac60cb59d99","observation_id":"fd06045a-c033-41de-8bfe-95bdd952ff2c","resolution":{"observed_at":"2026-08-14T13:47:23.807577Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510434","last_updated":"2005-10-14T14:17:47Z","snapshot_observed_at":"2026-07-07T00:55:05.166457Z","submitted_at":"2005-10-14T14:17:47Z","title":"Broad-band photometric colors and effective temperature calibrations for late-type giants. I. Z=0.02","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510434","snapshot_observed_at":"2026-08-14T13:47:23.816949Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":67,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.816949Z"},"links":{"cited_paper":"/paper/astro-ph/0510434","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:072e96a77250e804bbea73dd59dbbcdac0fcf52c662941c1cc22dc0fb183c23a","observation_id":"e4b5fcd8-dd35-45e8-ae0c-e0d5d85568a6","resolution":{"observed_at":"2026-08-14T13:47:23.816949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603416","last_updated":"2006-03-16T09:33:32Z","snapshot_observed_at":"2026-08-15T01:17:21.986467Z","submitted_at":"2006-03-16T09:33:32Z","title":"Broad-band photometric colors and effective temperature calibrations for late-type giants. II. Z<0.02","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603416","snapshot_observed_at":"2026-08-14T13:47:23.826053Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":68,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.826053Z"},"links":{"cited_paper":"/paper/astro-ph/0603416","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:5e89d3d8a8b025310c9f25e6ffda5eb9cf326bf5c9ff6ca820890fe2b4f015bf","observation_id":"aad26284-661e-4334-b602-89c794be79dc","resolution":{"observed_at":"2026-08-14T13:47:23.826053Z","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":"2026-08-14T13:47:23.836110Z","title":"Astronomical Data Analysis Software and Systems IV , year = 1995, editor =","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":69,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.836110Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:dea6f2ed2249d4684915edf30b1308766be307df3de96142203ff60eb0ad0998","observation_id":"d6a69d35-ec35-4856-ae3f-c4f0a06204ba","resolution":{"observed_at":"2026-08-14T13:47:23.836110Z","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":"2026-08-14T13:47:23.843157Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":70,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.843157Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b204eabd505499caea94e85f33118c1a878156d49fc1cd8a7140c7bbf411f4ae","observation_id":"1729ad3b-e9ca-4383-91c8-9006c971d9d5","resolution":{"observed_at":"2026-08-14T13:47:23.843157Z","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":"2026-08-14T13:47:23.849447Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":71,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.849447Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b722fe2261e9fbd5235a641e632ac114c058abfdaee9bd97fbfd70b5063e36a2","observation_id":"d2c0af16-47c9-4292-a9f4-10ee8a9fa676","resolution":{"observed_at":"2026-08-14T13:47:23.849447Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.03474","last_updated":"2025-03-26T16:07:03Z","snapshot_observed_at":"2026-08-12T23:07:33.684939Z","submitted_at":"2024-08-06T23:14:19Z","title":"The Chicago-Carnegie Hubble Program: The JWST J-region Asymptotic Giant Branch (JAGB) Extragalactic Distance Scale","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.03474","snapshot_observed_at":"2026-08-14T13:47:23.856700Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":72,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.856700Z"},"links":{"cited_paper":"/paper/2408.03474","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b0b1e787089fe093b3eb55baa2574a0d4bc552c494f0d42a0bd8fa47bd04bf6b","observation_id":"c73b0b10-e098-48f6-9587-70b4ec4dab6a","resolution":{"observed_at":"2026-08-14T13:47:23.856700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0109535","last_updated":"2001-09-27T23:21:37Z","snapshot_observed_at":"2026-07-07T00:21:54.529525Z","submitted_at":"2001-09-27T23:21:37Z","title":"The Distance to SN 1999em in NGC 1637 from the Expanding Photosphere Method","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0109535","snapshot_observed_at":"2026-08-14T13:47:23.864193Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":73,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.864193Z"},"links":{"cited_paper":"/paper/astro-ph/0109535","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:40eb1de013e25b1b619ea4c4484e1ff868d3c4e5e07654aa66bfb53883cbd115","observation_id":"9a340aed-a834-47b2-8d26-dc1564f3c375","resolution":{"observed_at":"2026-08-14T13:47:23.864193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0305259","last_updated":"2003-05-15T08:23:15Z","snapshot_observed_at":"2026-07-07T00:33:19.297709Z","submitted_at":"2003-05-15T08:23:15Z","title":"The Cepheid Distance to NGC 1637: A Direct Test of the EPM Distance to SN 1999em","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0305259","snapshot_observed_at":"2026-08-14T13:47:23.875347Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":74,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.875347Z"},"links":{"cited_paper":"/paper/astro-ph/0305259","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:efb61622bac99c81a898a6144555a6a4a7ddf2ebfba9b416dd901867c9d1e77a","observation_id":"9873bccb-2f71-4a25-acc0-39517efb2e37","resolution":{"observed_at":"2026-08-14T13:47:23.875347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504337","last_updated":"2005-04-15T02:25:47Z","snapshot_observed_at":"2026-07-07T00:49:54.078514Z","submitted_at":"2005-04-15T02:25:47Z","title":"The Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504337","snapshot_observed_at":"2026-08-14T13:47:23.883199Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":75,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.883199Z"},"links":{"cited_paper":"/paper/astro-ph/0504337","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:ae879b3ebf87a75cdbebd60d91d327d38de751c474d75faeb7d2cb35e86b53b3","observation_id":"beb80812-c938-464c-ad24-0dc7a5bb24ee","resolution":{"observed_at":"2026-08-14T13:47:23.883199Z","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":"2026-08-14T13:47:23.888853Z","title":"doi:10.1088/978-0-7503-1329-2 , adsurl =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":76,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.888853Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:b53a58360aa5e5ead9503edfb191a5cf184d132bbd90aae60388935e1289ebf8","observation_id":"cdbd1b32-c142-43bc-b480-3b9237bcec6a","resolution":{"observed_at":"2026-08-14T13:47:23.888853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04777","last_updated":"2024-02-29T20:45:32Z","snapshot_observed_at":"2026-08-13T04:45:43.922431Z","submitted_at":"2024-01-09T19:05:00Z","title":"Reconnaissance with JWST of the J-region Asymptotic Giant Branch in Distance Ladder Galaxies: From Irregular Luminosity Functions to Approximation of the Hubble Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.04777","snapshot_observed_at":"2026-08-14T13:47:23.895596Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":77,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.895596Z"},"links":{"cited_paper":"/paper/2401.04777","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f49e0c3175b1e48edf2160bcd3f6f5556937700ec2a87d9e70a396d3351fcc91","observation_id":"0d52ee51-e689-4048-b252-19737c09017e","resolution":{"observed_at":"2026-08-14T13:47:23.895596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.03856","last_updated":"2025-04-04T18:33:14Z","snapshot_observed_at":"2026-07-06T21:04:38.019194Z","submitted_at":"2025-04-04T18:33:14Z","title":"Optical and Near-infrared Observations of SN 2023ixf for over 600 days after the Explosion","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.03856","snapshot_observed_at":"2026-08-14T13:47:23.904764Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":78,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.904764Z"},"links":{"cited_paper":"/paper/2504.03856","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f5dd78fe43d113c8ba5c791f50eeca4b01bfbbb1fa0bbb900c4260dc48c52305","observation_id":"915667d4-67b8-4753-8737-8ccaa792cc4d","resolution":{"observed_at":"2026-08-14T13:47:23.904764Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.05259","last_updated":"2025-02-12T01:11:28Z","snapshot_observed_at":"2026-08-09T16:25:01.068494Z","submitted_at":"2025-02-07T19:00:00Z","title":"JAGB 2.0: Improved Constraints on the J-region Asymptotic Giant Branch-based Hubble Constant from an Expanded Sample of JWST Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.05259","snapshot_observed_at":"2026-08-14T13:47:23.912310Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":79,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.912310Z"},"links":{"cited_paper":"/paper/2502.05259","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:5ebd33a558903dc96b536e61ff7fe998a631c7104d01d3ccb2145f497e6c56ee","observation_id":"d4192c83-ed79-47b5-89cf-5327749549a6","resolution":{"observed_at":"2026-08-14T13:47:23.912310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.08673","last_updated":"2017-09-25T18:52:20Z","snapshot_observed_at":"2026-08-14T20:29:51.925626Z","submitted_at":"2017-09-25T18:52:20Z","title":"Progenitors of low-luminosity Type II-Plateau supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.08673","snapshot_observed_at":"2026-08-14T13:47:23.917982Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":80,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.917982Z"},"links":{"cited_paper":"/paper/1709.08673","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f9bf8922e72b81a0d22416dc311b52c56025c26b8f6a37a4a1ef947828e198f5","observation_id":"0fbc119e-3d91-4298-9318-5fe9d4f128c5","resolution":{"observed_at":"2026-08-14T13:47:23.917982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.10792","last_updated":"2020-05-21T17:17:09Z","snapshot_observed_at":"2026-08-14T12:52:36.931209Z","submitted_at":"2020-05-21T17:17:09Z","title":"Astrophysical Distance Scale The JAGB Method: I. Calibration and a First Application","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.10792","snapshot_observed_at":"2026-08-14T13:47:23.923322Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":81,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.923322Z"},"links":{"cited_paper":"/paper/2005.10792","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:5d63cbbcd007214f65b227c62b5de8a354bf60f2ebb34512d444ddabe8af0fc2","observation_id":"9affac8a-7a9f-43a4-89f5-97dfdb343a1f","resolution":{"observed_at":"2026-08-14T13:47:23.923322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.1996","last_updated":"2011-02-09T22:14:19Z","snapshot_observed_at":"2026-08-06T17:22:13.170176Z","submitted_at":"2011-02-09T22:14:19Z","title":"Preliminary Results from NEOWISE: An Enhancement to the Wide-field Infrared Survey Explorer for Solar System Science","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.1996","snapshot_observed_at":"2026-08-14T13:47:23.930267Z","title":", keywords =","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":82,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.930267Z"},"links":{"cited_paper":"/paper/1102.1996","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:245982000bfa8a8c6f276a3c957b7a61a03fb0a58f2ff4b2859dba684a07d937","observation_id":"930e4287-1ad3-4eb0-8fd0-a090c583992e","resolution":{"observed_at":"2026-08-14T13:47:23.930267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06262","last_updated":"2015-10-26T20:53:49Z","snapshot_observed_at":"2026-08-14T22:26:53.941579Z","submitted_at":"2015-10-21T14:18:33Z","title":"IAU 2015 Resolution B2 on Recommended Zero Points for the Absolute and Apparent Bolometric Magnitude Scales","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06262","snapshot_observed_at":"2026-08-14T13:47:23.936462Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":83,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.936462Z"},"links":{"cited_paper":"/paper/1510.06262","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:7393eef2e6683400f757e6a2fdc26db7e3c9d7c2b72bd3a9c4e6b45f61ddb9a4","observation_id":"accfa1c6-906d-41b2-ab7d-15e6c90bc040","resolution":{"observed_at":"2026-08-14T13:47:23.936462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508254","last_updated":"2005-08-11T04:02:08Z","snapshot_observed_at":"2026-08-10T14:49:00.769468Z","submitted_at":"2005-08-11T04:02:08Z","title":"The Reddening of Red Supergiants: When Smoke Gets In Your Eyes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508254","snapshot_observed_at":"2026-08-14T13:47:23.953156Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":84,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.953156Z"},"links":{"cited_paper":"/paper/astro-ph/0508254","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:667b5d925ac17111ea8845d32d57012a9a81eaf0f71119f6f733e44ecf61713e","observation_id":"3785b0ce-bb6d-455d-852b-55736c00bdea","resolution":{"observed_at":"2026-08-14T13:47:23.953156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0604253","last_updated":"2006-04-11T21:06:10Z","snapshot_observed_at":"2026-08-14T19:36:11.166799Z","submitted_at":"2006-04-11T21:06:10Z","title":"Bringing VY Canis Majoris Down to Size: An Improved Determination of Its Effective Tempeature","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0604253","snapshot_observed_at":"2026-08-14T13:47:23.960729Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":85,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.960729Z"},"links":{"cited_paper":"/paper/astro-ph/0604253","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:0331efab9fa39c3d456a0f8e5ae7361763151399208035512391afa120af0136","observation_id":"0ac64c4b-a205-408a-a8cb-282689b0206d","resolution":{"observed_at":"2026-08-14T13:47:23.960729Z","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":"2026-08-14T13:47:23.968818Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":86,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.968818Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:52211f52aca3233267d7b3af0e39e6074bace8f1a7812f1e2426a608a6c0999b","observation_id":"ff8ece5f-7344-4bab-9b5b-e7a77a67caf9","resolution":{"observed_at":"2026-08-14T13:47:23.968818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07930","last_updated":"2016-12-20T04:38:16Z","snapshot_observed_at":"2026-08-14T21:28:56.051867Z","submitted_at":"2016-11-23T19:02:24Z","title":"Asphericity, Interaction, and Dust in the Type II-P/II-L Supernova 2013ej in Messier 74","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07930","snapshot_observed_at":"2026-08-14T13:47:23.980782Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":87,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.980782Z"},"links":{"cited_paper":"/paper/1611.07930","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:685e4ee3496ec1a83654c81dc694d1e7df9b022e5f96f1bfe4bbb077dacc3ae7","observation_id":"096c0de5-fcc3-4058-8f60-bf1d46541bd3","resolution":{"observed_at":"2026-08-14T13:47:23.980782Z","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":"2026-08-14T13:47:23.988748Z","title":"Transient Name Server AstroNote , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":88,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.988748Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:536352470678e6fad23fd6f41f780861edd6ebbd757b9f8dc9c23bd37cf922f1","observation_id":"779a4ac7-977e-429a-8e1b-c39be23b692a","resolution":{"observed_at":"2026-08-14T13:47:23.988748Z","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":"2026-08-14T13:47:23.995994Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":89,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:23.995994Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:8e9afe624bf03f35f11a6bbb6ad7b3ba0239d6bee47aa03baf7dcb182595963e","observation_id":"31265e3e-9052-41a6-973b-4d12516b76ad","resolution":{"observed_at":"2026-08-14T13:47:23.995994Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03086","last_updated":"2024-06-03T15:18:47Z","snapshot_observed_at":"2026-08-13T04:02:56.086483Z","submitted_at":"2024-03-05T16:13:57Z","title":"An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. I. HST WFC3/IR F110W and F160W Filters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03086","snapshot_observed_at":"2026-08-14T13:47:24.004965Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":90,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.004965Z"},"links":{"cited_paper":"/paper/2403.03086","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:0031f96293251f2fbd3c8ce6733f86b8c89008e061046c564c86cb8a718ab4b8","observation_id":"e583cf5e-80e1-4454-b54c-e130f8bb18d9","resolution":{"observed_at":"2026-08-14T13:47:24.004965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04512","last_updated":"2022-11-08T19:12:35Z","snapshot_observed_at":"2026-08-13T13:47:09.040705Z","submitted_at":"2022-11-08T19:12:35Z","title":"UBVRI photometry of Betelgeuse over 23 years since 1999","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04512","snapshot_observed_at":"2026-08-14T13:47:24.018360Z","title":"Open European Journal on Variable Stars , keywords =","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":91,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.018360Z"},"links":{"cited_paper":"/paper/2211.04512","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:2aa631ff2167fd2a23db039e70c1c3093add3142678866cfb1473084508c6d5a","observation_id":"008a0758-31d8-4087-bd9e-df76113ce231","resolution":{"observed_at":"2026-08-14T13:47:24.018360Z","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":"2026-08-14T13:47:24.041330Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":92,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.041330Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:3a94020aa00adf3a08528bc93a56e102dcd770d1ccd7bf6b167847d226bece8e","observation_id":"de71eef8-547a-49ef-97ae-f76cde814096","resolution":{"observed_at":"2026-08-14T13:47:24.041330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.5518","last_updated":"2008-10-30T16:42:50Z","snapshot_observed_at":"2026-08-13T20:48:27.964749Z","submitted_at":"2008-10-30T16:42:50Z","title":"The Standard Candle Method for Type II-Plateau Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.5518","snapshot_observed_at":"2026-08-14T13:47:24.054214Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":93,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.054214Z"},"links":{"cited_paper":"/paper/0810.5518","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:8cf01f29d63f1fe4ae1a8ae0692dd90efce541cbd416eddbe7e1d669e78d8f88","observation_id":"d8b9226e-a8bc-41b7-ad77-09280600c244","resolution":{"observed_at":"2026-08-14T13:47:24.054214Z","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":"2026-08-14T13:47:24.088794Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":94,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.088794Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:9ae88d7cfc4f0b9ec2ba328a4acf3e765005f0aff1eb08ed8a130065e8d9b8fb","observation_id":"05dc2cdc-8401-4623-beba-edf72e949e0a","resolution":{"observed_at":"2026-08-14T13:47:24.088794Z","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":"2026-08-14T13:47:24.101039Z","title":"Transient Name Server AstroNote , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":95,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.101039Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:7cf3bb90483b81908821f574a0b8783202b5594891b8cb9f8a3461958a0d836b","observation_id":"6f2c533e-f10b-4269-a39c-fe39642e22f1","resolution":{"observed_at":"2026-08-14T13:47:24.101039Z","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":"2026-08-14T13:47:24.107685Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":96,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.107685Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:9a1863b18ca4d4fb1875e20cee1fcc5942057590708fd6d8c6a738b50ec56ae8","observation_id":"29462198-0147-4c86-84cd-01c734cccbc3","resolution":{"observed_at":"2026-08-14T13:47:24.107685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.0147","last_updated":"2013-11-01T11:40:03Z","snapshot_observed_at":"2026-08-14T23:56:47.776370Z","submitted_at":"2013-11-01T11:40:03Z","title":"On the Source of the Dust Extinction in Type Ia Supernovae and the Discovery of Anomalously Strong Na I Absorption","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.0147","snapshot_observed_at":"2026-08-14T13:47:24.113800Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":97,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.113800Z"},"links":{"cited_paper":"/paper/1311.0147","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:524957b3f955377d342b3ea1db9465eff9f5214e999cb405b58cceaae5ada582","observation_id":"78ff7a6c-bfe4-4193-a8d9-47363c3279ee","resolution":{"observed_at":"2026-08-14T13:47:24.113800Z","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":"2026-08-14T13:47:24.120311Z","title":"doi:10.5281/zenodo.12100100 , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":98,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.120311Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:eef38eae05790a683ce6d8d3721ed80098925a4ab04b772721df67109999bed1","observation_id":"e38d9f95-0380-4d16-a811-57cd0e9d7a48","resolution":{"observed_at":"2026-08-14T13:47:24.120311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00507","last_updated":"2015-09-04T09:32:53Z","snapshot_observed_at":"2026-08-14T22:34:12.164142Z","submitted_at":"2015-09-01T21:20:00Z","title":"A supernova distance to the anchor galaxy NGC 4258","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00507","snapshot_observed_at":"2026-08-14T13:47:24.127795Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":99,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.127795Z"},"links":{"cited_paper":"/paper/1509.00507","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:ab1064bc13d195b7b8150324f8d23cee9b7b0bf16527c4d710b73c8de6defa65","observation_id":"eaa7bdb5-6d7d-4300-8c61-7dab30031791","resolution":{"observed_at":"2026-08-14T13:47:24.127795Z","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":"2026-08-14T13:47:24.152569Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":101,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.152569Z"},"links":{"citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:47cb957c5bce3fc197ad9e3b374b54b95c23315c155d01cb780b36be2e25a5de","observation_id":"6f578ec4-a512-455f-9ea2-e5f88215b913","resolution":{"observed_at":"2026-08-14T13:47:24.152569Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10022","last_updated":"2023-09-18T18:00:00Z","snapshot_observed_at":"2026-08-14T19:57:50.283475Z","submitted_at":"2023-09-18T18:00:00Z","title":"The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.10022","snapshot_observed_at":"2026-08-14T13:47:24.158902Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":102,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.158902Z"},"links":{"cited_paper":"/paper/2309.10022","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:8af980e5084f2e956e6d6c65259880ec5a69e2053b0e1364acf0dacb9de1b740","observation_id":"47f6e37d-bcf7-481e-b4d4-a0996768ba6e","resolution":{"observed_at":"2026-08-14T13:47:24.158902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.04426","last_updated":"2023-12-07T16:51:40Z","snapshot_observed_at":"2026-08-13T05:07:50.915360Z","submitted_at":"2023-12-07T16:51:40Z","title":"SN2023ixf in Messier 101: the twilight years of the progenitor as seen by Pan-STARRS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.04426","snapshot_observed_at":"2026-08-14T13:47:24.172333Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":103,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.172333Z"},"links":{"cited_paper":"/paper/2312.04426","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:f9d1e7b9f05f1253fb948507b8ac2cbe7474cf42e18d5c92fc43aa302e880eec","observation_id":"7bb31818-4d0d-4f4a-a979-5c9805221325","resolution":{"observed_at":"2026-08-14T13:47:24.172333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.05625","last_updated":"2019-11-18T19:48:52Z","snapshot_observed_at":"2026-08-14T13:05:46.544368Z","submitted_at":"2019-08-15T16:33:26Z","title":"An Improved Distance to NGC 4258 and its Implications for the Hubble Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.05625","snapshot_observed_at":"2026-08-14T13:47:24.183563Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","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":104,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.183563Z"},"links":{"cited_paper":"/paper/1908.05625","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:58da80a0e3fe1de6f232e732a4cef91fe3600b57e462967a5740491a1856df70","observation_id":"c3a5c950-dd60-4a47-8969-ab68a66640f8","resolution":{"observed_at":"2026-08-14T13:47:24.183563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-15T03:18:07.800621Z","submitted_at":"2026-08-13T14:46:05Z","title":"JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":1,"unresolved":99,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":234},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 100 of 234 outbound references and 0 inbound Pith citation observations for arXiv:2608.13321."}