{"as_of":"2026-08-18T22:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:820988605c5bd6f7c8ec2304f90b03194b60dcecb67d7c4d99dc3238b0a4b242","coverage":[{"denominator":163,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T03:55:10.305506Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:47:24.979409Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-14T18:16:19.847625Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"cited_work":{"arxiv_id":"2607.11682","doi":"10.48550/arxiv.2607.11682","metadata_source":"pith","pith_arxiv_id":"2607.11682","snapshot_observed_at":"2026-08-14T18:16:19.847625Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","venue":"astro-ph.GA","work_id":"495bdc9b-5175-4a81-af40-19ab4cf9c578","year":2026},"citing_paper":{"arxiv_id":"2608.13321","last_updated":"2026-08-13T14:46:05Z","snapshot_observed_at":"2026-08-16T23:12:45.577905Z","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":203,"source":"arxiv_source","source_observed_at":"2026-08-14T13:47:24.979409Z"},"links":{"cited_paper":"/paper/2607.11682","citing_paper":"/paper/2608.13321"},"observation_digest":"sha256:59a9789988448ef8307f085c1dd2df9cf14437b3d256569cd9fcb9bc3d975fff","observation_id":"57b2a37e-d666-401b-be03-5547ade73854","resolution":{"observed_at":"2026-08-14T13:47:25.441129Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2607.11682/citation-record","integrity":"/paper/2607.11682/integrity","json":"/paper/2607.11682/citation-record.json","paper":"/paper/2607.11682"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:25df2a353b47e850cbd74b99f66dd30efd247e5e5d73bd55b5167c487b16d63f","observation_id":"b9122daa-2e75-4e2e-9bac-bd7ae46305e2","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:64c3de42fccc8761e7f1308670736e8b05706f133b907a023a661e846f2315d8","observation_id":"5514fe42-4f14-47aa-9886-b0240517a2bc","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.4402","last_updated":"2009-06-24T05:02:27Z","snapshot_observed_at":"2026-08-15T05:45:15.471283Z","submitted_at":"2009-06-24T05:02:27Z","title":"Chemical behavior of the Dwarf Irregular Galaxy NGC 6822. Its PN and HII region abundances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.4402","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"Its PN and HII region abundances","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0906.4402","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:05c610f3df15da215b09b9379fd59b542a9019c1104303ae005aed1ae72eed1e","observation_id":"ec07332c-d3eb-438a-afae-0d941982fade","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:dfcda0917313f2b5466e701397a145aa2286629adfdccea6a6d23cce4cb415cc","observation_id":"b36723d7-fd85-4353-92e7-5a394cbcb0d4","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:2da9d7fbc5bfd46b0e0a6a72228ac16a0e9735d55c2bdaf6b6cfe9c3eb807265","observation_id":"78f627e7-0b6e-4d9e-aae2-b701f9c16f17","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0110026","last_updated":"2001-10-19T13:12:37Z","snapshot_observed_at":"2026-08-13T17:59:16.866844Z","submitted_at":"2001-10-01T11:22:13Z","title":"The extent of NGC 6822 revealed by its C stars population","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0110026","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0110026","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:edccdf16c307135c8f81e77fa79704e92b296994ec21cbfe533e5955fd68e8ce","observation_id":"86621e60-be99-4450-b0ca-9a68e45d4824","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01744","last_updated":"2015-08-10T20:14:22Z","snapshot_observed_at":"2026-08-14T22:53:20.772832Z","submitted_at":"2015-04-07T20:05:36Z","title":"Spitzer Point Source Catalogs of $\\sim300,000$ Stars in Seven Nearby Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01744","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1504.01744","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:cc17fc23e816302a2b2910adf21277e5d2214c5692ac072b4200789ff873d133","observation_id":"70dcf497-ded1-467e-b2d2-517b5c5eba53","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409294","last_updated":"2004-10-25T13:03:03Z","snapshot_observed_at":"2026-07-07T00:44:37.994291Z","submitted_at":"2004-09-13T17:00:04Z","title":"Near-IR observations of NGC 6822: AGB stars, distance, metallicity and structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409294","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0409294","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:fdbedca04417c0d886fe71b2b7ab21336c10477483e2f640b7559dfd0249cba7","observation_id":"b2f724e6-890e-4c57-aff2-4558eb9a833b","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.10542","last_updated":"2025-06-12T10:09:50Z","snapshot_observed_at":"2026-08-16T11:22:28.856088Z","submitted_at":"2025-06-12T10:09:50Z","title":"The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.10542","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2506.10542","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:9dec33f866467b449290107c385a441e8d567c1b2a5f26bf2d2a5d76251dda3b","observation_id":"13ed402f-434b-4b24-a2b5-db004d5e0494","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.08243","last_updated":"2022-11-09T08:49:07Z","snapshot_observed_at":"2026-08-16T16:38:40.728304Z","submitted_at":"2022-08-17T11:51:17Z","title":"The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.08243","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2208.08243","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:23836e6ca18e9d85ce80ebb39c15ebd8063513b092303c3d0936e88945e0e9b4","observation_id":"b980508b-5a3f-470d-a1bc-77fd61dc2fe6","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:3dad3a0a2d32bcc74485c552a9b13f295c4dbda3d6fa421c33224fd5ca1e47ae","observation_id":"606c23bc-c458-4ec4-8cca-bf2467f19015","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0905.4415","last_updated":"2009-05-27T13:22:56Z","snapshot_observed_at":"2026-08-15T05:47:33.111285Z","submitted_at":"2009-05-27T13:22:56Z","title":"Synthetic photometry for carbon rich giants, I. Hydrostatic dust-free models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.4415","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0905.4415","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:f7ccc9fee11646a7fd8f34f75fef259fe9f13311899ff031f6d1238161708232","observation_id":"a2b67394-cf93-483d-930e-a18fdc6ebe39","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", archivePrefix = \"arXiv\", eprint =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:82589b108705aabe978334b9a02aa63c51e203e15802eecf344e7554aa6a5f59","observation_id":"4e327af9-6f37-4fef-a14e-d0819808600f","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:7d65513128d0350c71c01fe75554f3d84ddae18b0fc37d2546ff9a0032afaac2","observation_id":"643886b9-e0a8-4bdf-bc71-97a2a726d894","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603558","last_updated":"2006-03-21T09:05:27Z","snapshot_observed_at":"2026-07-07T00:59:16.162667Z","submitted_at":"2006-03-21T09:05:27Z","title":"Photometric Survey of the Polar ring galaxy NGC 6822","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603558","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0603558","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:999fb8cd29f6c33117cedde8156c45d69061714f7bc4c222c58eeb28a1be8fad","observation_id":"3a0f657b-c377-4a71-bb8d-4f24213bed39","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:75b8fd43b5af57dbab1dad54fb15a3ac06bcae92f6ee6d24587ea0472efdd36f","observation_id":"33c330e0-4f9a-4c71-ae40-e83de8801460","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:4f1a69cab63d89f12644e2840b585901d802cab942376033472d55fa7669b311","observation_id":"5e729812-2e97-4db6-b7ad-c2cbc1433db0","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608189","last_updated":"2006-08-08T23:22:11Z","snapshot_observed_at":"2026-08-15T11:06:43.329274Z","submitted_at":"2006-08-08T23:22:11Z","title":"Spitzer SAGE survey of the Large Magellanic Cloud II: Evolved Stars and Infrared Color Magnitude Diagrams","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0608189","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0608189","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:f6bc2a4abfc311eba6b679d0a9f470875064f243ae5ef22597902640ad0dd93f","observation_id":"96af3e2f-d8e1-45fd-867c-6d95c0edd0c9","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:2163040a6226a4a8891b998052776b7589a19499c1183b73c71123de7628466b","observation_id":"84f4d1f7-80ab-43c0-9c75-929f59e9db33","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.17429","last_updated":"2024-06-25T10:08:31Z","snapshot_observed_at":"2026-08-16T13:39:49.842022Z","submitted_at":"2024-06-25T10:08:31Z","title":"Imaging of I Zw 18 by JWST: II. Spatially resolved star formation history","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.17429","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"Spatially resolved star formation history","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2406.17429","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:6b3a538f5ece169c14d1cf66d0a99cef47041ea3751f0096c4d20173bd08e23d","observation_id":"ccc8353d-4f08-4429-8912-cdb869756360","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.3871","last_updated":"2009-03-23T15:38:29Z","snapshot_observed_at":"2026-08-15T05:52:22.742046Z","submitted_at":"2009-03-23T15:38:29Z","title":"A Spitzer Study of Asymptotic Giant Branch Stars. III. Dust Production and Gas Return in Local Group Dwarf Irregular Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.3871","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0903.3871","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:43f68015969095d34a4b3abe052090069c96916914b4a9fa5f23cc614866314a","observation_id":"d88f24c3-3a0c-4b09-a53d-38579dc19dcb","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.5026","last_updated":"2011-06-24T17:42:33Z","snapshot_observed_at":"2026-08-15T04:42:57.309953Z","submitted_at":"2011-06-24T17:42:33Z","title":"Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC) II. Cool Evolved Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.5026","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1106.5026","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:eeb1733f6e03c30736032135fe6c146f05b2941212d35934f856c5f181959480","observation_id":"2025eeff-3e20-44a5-b72b-8da05454fd2e","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.5384","last_updated":"2012-01-25T21:02:05Z","snapshot_observed_at":"2026-08-18T05:58:53.368631Z","submitted_at":"2012-01-25T21:02:05Z","title":"The Dust Budget of the SMC: Are AGB Stars the Primary Dust Source at Low Metallicity?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.5384","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1201.5384","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:6aff1513e449ce52d7a7d60f2b656c6c1e317d30d9213899bf0a0c60ecb3a9ae","observation_id":"d728a438-aba5-44df-bf0c-fe2ef7ce5630","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.4053","last_updated":"2014-11-14T21:00:16Z","snapshot_observed_at":"2026-08-14T23:11:33.612008Z","submitted_at":"2014-11-14T21:00:16Z","title":"An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS), I. Overview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.4053","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1411.4053","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:a975fc8c1864350fd683ee04899ea51107e619af9ddc630a52f87e3767b338b1","observation_id":"d8ff02a2-14d6-4e99-b9f6-182be944d063","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.0695","last_updated":"2014-12-01T21:26:39Z","snapshot_observed_at":"2026-08-14T23:09:25.428247Z","submitted_at":"2014-12-01T21:26:39Z","title":"An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS), II. Discovery of Metal-poor Dusty AGB Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.0695","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1412.0695","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:05f4ae5ed75514fe0c007ab0b84e29b1a137ed77c3954b37e715744138596a5b","observation_id":"bddddf1e-f5eb-4211-ac7b-5b5b5a1a1887","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.07003","last_updated":"2015-07-24T20:01:32Z","snapshot_observed_at":"2026-08-14T22:39:04.394768Z","submitted_at":"2015-07-24T20:01:32Z","title":"Identification of a Class of Low-Mass Asymptotic Giant Branch Stars Struggling to Become Carbon Stars in the Magellanic Clouds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.07003","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1507.07003","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:1c533dca382c019fd7739d73515214c958766ff63f962156a3bd1dee6ee3be89","observation_id":"70bbc025-7c65-43c6-a9a2-f5e5db4a0154","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02129","last_updated":"2017-11-06T19:23:47Z","snapshot_observed_at":"2026-08-14T20:16:26.135170Z","submitted_at":"2017-11-06T19:23:47Z","title":"An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-Redshift AGB Analogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02129","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1711.02129","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:7ce89a4594cb3a2fc99cdaa4b57184950ba319b4eef5d83ef24968274d24153f","observation_id":"6ec8022d-c906-421b-b5ac-70716f8daedb","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.14889","last_updated":"2024-01-26T14:15:19Z","snapshot_observed_at":"2026-08-16T14:24:14.098349Z","submitted_at":"2024-01-26T14:15:19Z","title":"The JWST Resolved Stellar Populations Early Release Science Program VI. Identifying Evolved Stars in Nearby Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.14889","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2401.14889","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:cc22cb36fc0b045e2fcae8cdcb74055597389cd62725295e9f85aee9d726820f","observation_id":"c0dcca1a-0026-4b45-9dab-5b8eb6811dbd","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0707.2881","last_updated":"2007-07-19T11:59:14Z","snapshot_observed_at":"2026-08-15T10:35:46.642262Z","submitted_at":"2007-07-19T11:59:14Z","title":"VLT spectroscopy of blue supergiants in IC 1613","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.2881","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0707.2881","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:89e6781552b81ab182cf2f8d5a4c4318a07ce4619c7a5085e5e09495bd302b8f","observation_id":"6cf740c0-8316-4cc3-98ee-5341aec32cb8","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"doi:10.5281/zenodo.7714020 , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:60a5a3de5925d4f15b734ac2a62110572585755a875511c72d5177f789d6b92d","observation_id":"3fa71163-8500-4be1-901e-36fbc42f22a4","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608249","last_updated":"2006-08-11T17:27:48Z","snapshot_observed_at":"2026-08-15T11:06:27.547594Z","submitted_at":"2006-08-11T17:27:48Z","title":"The Nature of Infrared Emission in the Local Group Dwarf Galaxy NGC 6822 As Revealed by Spitzer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0608249","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0608249","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:90ab7ec3b0b6c81d6352f919090b44b235a95b372727e1ac12d6e09fe336d8bf","observation_id":"1081432d-512c-4d38-aa32-c4d316906fd1","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:6c46bdc6ada74ff42c63242d6277b5196e971bc4660994ba2a918dfe4c39511b","observation_id":"f90b20c8-3e92-447a-8053-829254234795","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0302051","last_updated":"2003-02-04T12:53:25Z","snapshot_observed_at":"2026-08-09T19:40:02.751565Z","submitted_at":"2003-02-04T12:53:25Z","title":"AGB stars in the Magellanic Clouds. I. The C/M ratio","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0302051","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0302051","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:3050eab2b53c50002c682fbac9c9f46f0ec03aec989f37f6c305891a90e2bcb8","observation_id":"47945786-2e82-4604-8190-7fcf9a8177bf","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0509881","last_updated":"2006-07-05T09:51:53Z","snapshot_observed_at":"2026-07-07T00:54:26.452552Z","submitted_at":"2005-09-29T13:47:05Z","title":"AGB stars in the Magellanic Clouds. II. The rate of star formation across the LMC","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0509881","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0509881","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:402210900847be7b9ba0a4336e3597a0b0d5624f5a9df9477a25831ea446109d","observation_id":"cc90ca0b-4ba7-4b23-8e59-64fed7f1c329","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0602483","last_updated":"2006-02-22T09:50:00Z","snapshot_observed_at":"2026-08-10T22:31:40.699941Z","submitted_at":"2006-02-22T09:50:00Z","title":"AGB stars in the Magellanic Clouds. III. The rate of star formation across the SMC","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0602483","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0602483","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:53b58000679baf1960c2b7286d662eb9e429773dc3a0d6d40a8c9faceb8ed1d3","observation_id":"f8ed85a6-b910-400f-a676-db985c2dade7","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.3136","last_updated":"2009-08-22T01:58:46Z","snapshot_observed_at":"2026-08-15T05:50:09.404658Z","submitted_at":"2009-04-20T23:13:28Z","title":"The metallicity gradient as a tracer of history and structure: the Magellanic Clouds and M33 galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.3136","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0904.3136","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:bb2b9fb730516909ad67ddf62b3a76f98388ba79bbed7dc29c591750c70310d1","observation_id":"e56243d6-5d47-4a2d-b3e1-b57efd93604f","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.16686","last_updated":"2024-03-25T12:22:24Z","snapshot_observed_at":"2026-08-16T14:06:43.182755Z","submitted_at":"2024-03-25T12:22:24Z","title":"JWST MIRI Flight Performance: Imaging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.16686","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2403.16686","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:fe6ed4a7fcb0ba2853ba427f4a70dba839b66b6b42183d7192d98ea33731e319","observation_id":"bf3c9575-7212-4115-8d35-76540f67243f","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005473","last_updated":"2000-05-24T01:52:23Z","snapshot_observed_at":"2026-08-07T13:04:46.703167Z","submitted_at":"2000-05-24T01:52:23Z","title":"Evidence for tidal interaction and a supergiant HI shell in the Local Group dwarf galaxy NGC 6822","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005473","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0005473","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:7bb2030ecb1fb29ff544730eadf77a37fcb52a8c63bd875f26188f0177108f29","observation_id":"56f1ceec-5724-4e24-a9a2-f196454a64cf","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508018","last_updated":"2005-08-01T02:09:32Z","snapshot_observed_at":"2026-07-07T00:52:39.064269Z","submitted_at":"2005-08-01T02:09:32Z","title":"The stellar population and interstellar medium in NGC 6822","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508018","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0508018","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:47b3ca4cd3cb267dc95571f8a33f5713fac30d5d7ba3e26ebdddce39c8513648","observation_id":"323dc7ef-2f91-44f0-a5ae-5f3986232132","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.08090","last_updated":"2016-05-25T22:02:36Z","snapshot_observed_at":"2026-08-14T21:55:41.193815Z","submitted_at":"2016-05-25T22:02:36Z","title":"Evolved stars in the Local Group galaxies. I. AGB evolution and dust production in IC 1613","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.08090","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"AGB evolution and dust production in IC 1613","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1605.08090","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:948a0fc8cb89eb3a1ca5556145b4ae19b5549c91403bfca78e8b5a401f4a73e1","observation_id":"a3be5de5-1904-4866-a155-2fc2574bf884","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"and García-Hernández, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:8af8fc5dc3c516e4ea9fffb4b19cae7acf86884c1bd60fa2f382c57847b63502","observation_id":"eec819f7-fd92-48b9-9537-822494e80412","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04160","last_updated":"2018-06-11T18:04:08Z","snapshot_observed_at":"2026-08-14T19:05:05.444746Z","submitted_at":"2018-06-11T18:04:08Z","title":"Evolved stars in the Local Group galaxies - II. AGB, RSG stars and dust production in IC10","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.04160","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"AGB, RSG stars, and dust production in IC10","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1806.04160","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:c99198efcda7129952d5fa3a44f2e4c78f57279d844d9cbd8215d4669101f427","observation_id":"582478e6-4e9b-4c06-88a4-dac21aecd58f","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"and Kereš, Dusan and Chan, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:ccd378aa85274eb213d2a88d5777e9cd9e70255477223c2cf08a0683de5da8b3","observation_id":"54aa2c20-9a14-4b13-8607-b2853158b542","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.6753","last_updated":"2012-11-03T08:19:12Z","snapshot_observed_at":"2026-08-15T00:41:53.519905Z","submitted_at":"2012-10-25T08:01:08Z","title":"Distance and reddening of the Local Group dwarf irregular galaxy NGC 6822","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.6753","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1210.6753","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:e9b4b36eb51fc0114af37f747a113d92d8b68ecbe65b5362a8e44f0900c69915","observation_id":"e00c27eb-b316-4401-ac29-5a0bc2455441","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.5247","last_updated":"2014-09-18T10:37:07Z","snapshot_observed_at":"2026-08-14T23:19:02.288115Z","submitted_at":"2014-09-18T10:37:07Z","title":"A state-of-the-art analysis of the dwarf irregular galaxy NGC 6822","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.5247","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1409.5247","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:5923199859c00b0d99f007d95bac59b20d56f0feed597ab7948f3c762295cfe8","observation_id":"37806c4c-1b10-493d-ab93-13d8e0c1494a","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.01533","last_updated":"2021-06-09T06:49:20Z","snapshot_observed_at":"2026-08-16T19:01:25.959397Z","submitted_at":"2020-12-02T21:15:53Z","title":"Gaia Early Data Release 3: Summary of the contents and survey properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.01533","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"Summary of the contents and survey properties","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2012.01533","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:f1a7986cd2cee38ed17c76bb9a4184faadf1e13a218f767ae98a764b12f331d6","observation_id":"9d9c685c-0fdc-44cd-a22a-da776cc01995","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0403","last_updated":"2011-08-01T19:51:48Z","snapshot_observed_at":"2026-08-15T04:39:21.485915Z","submitted_at":"2011-08-01T19:51:48Z","title":"Production of dust by massive stars at high redshift","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0403","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1108.0403","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:eab638ffa07b3caa9ee7c50490c7b6fbc1c775312a5919220c0ab0472230c647","observation_id":"3101979c-2c4e-4570-93f4-63e2b5322154","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:014bea1c9b6511c74972a3298c41f06ed8d45f694d407d7c63104e8b89d7aebe","observation_id":"fb9526e4-1d12-4fb9-81be-1df12987e2b7","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:0e1f9c7897db4e1d0fb992f55cdafc22eb277ec7def71b54d5a9d27b635a7b70","observation_id":"8378ce41-6e04-4753-ac84-041478086ed1","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"The Recent Star Formation History","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:eb99fb0881e44a3c78e985dd65cc42038d251ad86e2dddb499754e7cad3decb3","observation_id":"21e2cd49-3e0c-47bc-a778-c6da5a7adabf","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:455054e6996f98d19a97f6c2935e1118b1fcd91253a938ef15e71ef5f56e815b","observation_id":"115aa792-266c-4721-aca5-9f3d402bf611","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9411011","last_updated":"1994-11-02T20:24:04Z","snapshot_observed_at":"2026-07-07T01:10:17.952412Z","submitted_at":"1994-11-02T20:24:04Z","title":"The Evolution of C/O in Dwarf Galaxies from HST Fos Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9411011","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/9411011","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:f9edb1fd246fcee78709b4a103566d9273aa24fe4712435b2be1f901447e4229","observation_id":"f0111575-4a6d-4eeb-b9d4-cd08223ec278","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.11908","last_updated":"2020-11-24T06:02:50Z","snapshot_observed_at":"2026-08-16T19:03:44.476542Z","submitted_at":"2020-11-24T06:02:50Z","title":"The quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 $-$ 10 $\\mu$m: Implications for the JWST/MIRI detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.11908","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2011.11908","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:ce179e24505c2ca4126dc0a12f5de75ec1a4751a64126cc8e5f7f217ff4357bf","observation_id":"1dffb439-fe18-4171-9d2e-fd38ffa7651c","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"and Van Winckel, H","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:36abdf04d0b703b932b4f96c14c03ac4d4ba304d681fade9a3daf99010682db8","observation_id":"aea069af-8607-474b-84a8-8349244b80ed","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.4313","last_updated":"2011-07-21T16:55:20Z","snapshot_observed_at":"2026-08-15T04:40:18.331032Z","submitted_at":"2011-07-21T16:55:20Z","title":"Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.4313","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1107.4313","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:14f2e390ba03b09f351b4f15e9d38c7f25f58ece317bb871e4e8f1e72c36b1e8","observation_id":"aab3c4f3-4f29-4933-a53e-17f377118bf7","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:31228ab9f91c9c2f7013b8de7f80d6c315dc991451a8d29e8eb2c9e1a37955e2","observation_id":"f1bfeee4-2374-43c0-a989-2af95bb116cd","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511475","last_updated":"2005-11-16T10:20:02Z","snapshot_observed_at":"2026-07-07T00:56:06.332260Z","submitted_at":"2005-11-16T10:20:02Z","title":"The mid- and far-infrared colours of AGB and post-AGB stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0511475","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0511475","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:cebe9a2cb239039d4e76a5fa7d2ddd87450207a89fe80abb6ac423e026138e9f","observation_id":"cf2aee16-f02c-4e44-acf9-523c9d09faf8","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.3087","last_updated":"2009-08-21T10:10:58Z","snapshot_observed_at":"2026-08-15T05:41:04.780553Z","submitted_at":"2009-08-21T10:10:58Z","title":"Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.3087","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0908.3087","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:dfe50d2cc4aa5359587d39f4f32b04502b7c3d323687b24d7a95170e2bd2fcb9","observation_id":"df787abd-8467-43d9-9e06-f93593458c84","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.2399","last_updated":"2014-01-10T16:44:56Z","snapshot_observed_at":"2026-08-14T23:48:53.383312Z","submitted_at":"2014-01-10T16:44:56Z","title":"First detection of rotational CO line emission in an RGB star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.2399","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1401.2399","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:c180fedd53f9d860f536f49e9233ff59da6a960152cf4da0e278fa8aaad5e1b8","observation_id":"d075bd6c-7e08-4e20-b9ad-35540a38c426","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.4497","last_updated":"2011-10-20T11:19:36Z","snapshot_observed_at":"2026-08-15T04:31:41.075243Z","submitted_at":"2011-10-20T11:19:36Z","title":"The VMC survey III. Mass-loss rates and luminosities of LMC AGB stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.4497","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1110.4497","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:65755b4999531f5f6f227d8e317cb61c13822dc9059cec5e1ae5906e27f1b99c","observation_id":"59e3227b-f1c4-4a3a-97bd-05112a57918b","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.16242","last_updated":"2024-04-24T22:59:30Z","snapshot_observed_at":"2026-08-16T13:58:03.751574Z","submitted_at":"2024-04-24T22:59:30Z","title":"Young Stellar Objects in NGC 346: A JWST NIRCam/MIRI Imaging Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.16242","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2404.16242","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:069eeb81e9022805848f7e326cd400a8a5daa27c3bc49577b54fa8c3f993783a","observation_id":"d9b1023f-f8c0-4556-9c6d-5a0254206726","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312100","last_updated":"2003-12-03T23:58:51Z","snapshot_observed_at":"2026-07-07T00:38:48.365241Z","submitted_at":"2003-12-03T23:58:51Z","title":"The Star Formation History of the Small Magellanic Cloud","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0312100","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0312100","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:5360d167c6c43ba8acaa62fae4dc3633c9a5648a16cfc3840dc4593fe81bba91","observation_id":"ddc19f74-e76d-4b71-8248-b6c5bccbef59","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.15060","last_updated":"2021-06-07T04:24:51Z","snapshot_observed_at":"2026-08-16T18:35:49.486709Z","submitted_at":"2021-03-28T06:24:00Z","title":"PnG BERT: Augmented BERT on Phonemes and Graphemes for Neural TTS","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.15060","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", year = 2005, month = sep, volume =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2103.15060","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:787022a7a6db0e7ebdedb82e2919cb81c6402bfe69ef8b38ae8d2460d7fec393","observation_id":"cf3dfa48-885e-4c38-b2ce-f5cef9e82087","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.12437","last_updated":"2020-02-27T21:00:13Z","snapshot_observed_at":"2026-07-06T09:00:46.442419Z","submitted_at":"2020-02-27T21:00:13Z","title":"Dusty Stellar Birth and Death in the Metal-Poor Galaxy NGC 6822","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.12437","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2002.12437","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:137dcec2d322056e85bc3a383f4b8676d7b6c36c591d4b9737d30f492f39f8ab","observation_id":"8c14ab18-97df-4cae-9850-00166d5e4bd4","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"2026 , doi =","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:87e6235f42cfd904674ab0a527e3bf4d997927d6236607cc91c7d559f56d49a7","observation_id":"33e9afba-bd66-4f81-b01f-050826f2cd07","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.06980","last_updated":"2024-06-26T18:20:06Z","snapshot_observed_at":"2026-08-16T14:10:51.766426Z","submitted_at":"2024-03-11T17:59:58Z","title":"Imaging of I Zw 18 by JWST. I. Strategy and First Results of Dusty Stellar Populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.06980","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2403.06980","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:adb33f167292ea7ef732c989d89a5399a0f920b465c6b0686208a4590bcb2a6d","observation_id":"7288af93-4d6b-430b-bfc8-9d22aead9496","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"Mechanisms, models and measurements","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:db92e50221aa3e59ab8dcbaebe6b9574135bc0c5f45c923affeb4dfebbcb711a","observation_id":"92ab4145-c711-4add-af52-630d8af1d75a","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"Nature Astronomy , year = 2022, month = aug, volume =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:02e956eda395f75e73a387e2ceb14f88fd9bc79fc305092b2987c3907897bb47","observation_id":"7d786c4d-a9b7-4173-884d-f6d161c2da32","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:150e076564db17b0dd96b2b1fc97cb788dd0fece5060753b17262f49431f11f6","observation_id":"02755e72-6ef5-477e-8d6f-7a7af49534fe","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:ffaddc101d33fd4b09e68d780b784d9e4fe0d5f64214a97dc3912ee7a4eed538","observation_id":"f1e3e676-848d-44d9-be0d-3b1d0a5a412a","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:ee6513ea3a93a6a1da821fd41d5e92f569810d484fbd0c14ddfe14585b812f25","observation_id":"00ceceff-b43d-47de-9403-4975d67ef303","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.03305","last_updated":"2022-02-07T15:53:49Z","snapshot_observed_at":"2026-08-02T21:09:39.675291Z","submitted_at":"2022-02-07T15:53:49Z","title":"The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope I. Overview of the instrument and its capabilities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.03305","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2202.03305","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:ed3ab14fd9721447aef54d7693069f6cf3f9308576c5396fec9eea509f7f3001","observation_id":"a2cccbe5-2d17-4593-8abd-ee9e41d9a44c","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.2485","last_updated":"2014-02-11T13:35:31Z","snapshot_observed_at":"2026-08-14T23:45:05.527607Z","submitted_at":"2014-02-11T13:35:31Z","title":"Modelling the alumina abundance of oxygen-rich evolved stars in the Large Magellanic Cloud","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.2485","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1402.2485","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:54467ae97507367130e896cb3db2013ec0568acdb2fb9e642afe79311153b2d1","observation_id":"7931fbcd-81d9-449d-a3cd-3029e037d04e","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.08997","last_updated":"2017-03-27T10:30:25Z","snapshot_observed_at":"2026-08-14T21:09:54.071366Z","submitted_at":"2017-03-27T10:30:25Z","title":"Probing the dusty stellar populations of the Local Volume Galaxies with JWST/MIRI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.08997","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1703.08997","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:b8140711ea4a92437894dbc123a91122b883d9b5073df2cc238dd14c525faa49","observation_id":"bc2cef83-bb95-4389-8514-b24bc4ef48e2","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.02709","last_updated":"2017-05-07T22:18:15Z","snapshot_observed_at":"2026-08-14T21:02:17.605707Z","submitted_at":"2017-05-07T22:18:15Z","title":"The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification III","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.02709","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"Point source classification - III","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1705.02709","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:e4e69408c2030c05f5d09c8debe59c4fa563c49ef0592ccb5026cf9f03c2b2d8","observation_id":"2495a6ef-4d54-4637-89d5-49d7520ad167","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.06594","last_updated":"2017-12-18T18:32:51Z","snapshot_observed_at":"2026-08-14T20:02:29.011308Z","submitted_at":"2017-12-18T18:32:51Z","title":"Near-Infrared Stellar Populations in the metal-poor, Dwarf irregular Galaxies Sextans A and Leo A","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.06594","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1712.06594","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:3a83f5bd1318d30cdabb40fed33b1c43428e2ed751636fda26b5a8d8f0c597c1","observation_id":"65e1e6ea-2e35-4d95-9778-236a13554faa","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.03884","last_updated":"2019-09-09T14:27:52Z","snapshot_observed_at":"2026-08-16T04:22:51.434684Z","submitted_at":"2019-09-09T14:27:52Z","title":"The Young Stellar Population of the metal-poor galaxy NGC 6822","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.03884","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1909.03884","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:5ac06e202c2ae78952216fc4bf54ec1621d2b71ec09126526e62c9ca193fcbce","observation_id":"dec55232-17bf-42a4-8c61-332fb81f1e86","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03932","last_updated":"2023-03-07T17:54:46Z","snapshot_observed_at":"2026-08-16T16:03:22.234042Z","submitted_at":"2023-01-10T12:19:41Z","title":"Discovery of dusty sub-solar mass young stellar objects in NGC 346 with JWST/NIRCam","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03932","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2301.03932","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:863a2d3d66a43997f29bc713192a2efe3deb1eca8008777affd2993b16ec4013","observation_id":"d5cf22dd-e8f7-4358-85c6-0c7b2bde75bc","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.1777","last_updated":"2013-06-07T16:58:32Z","snapshot_observed_at":"2026-08-15T00:14:48.334661Z","submitted_at":"2013-06-07T16:58:32Z","title":"OH/IR stars and their superwinds as observed by the Herschel Space Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.1777","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1306.1777","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:d584a19a4882a09275b620eed234267fe63d1271cc53a9b6ca9ff05fb67ed042","observation_id":"5b920654-677e-4f58-ba3c-9a4cdd4204c1","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210058","last_updated":"2002-10-02T08:23:51Z","snapshot_observed_at":"2026-08-14T06:13:48.644746Z","submitted_at":"2002-10-02T08:23:51Z","title":"Parameterising the third dredge-up in asymptotic giant branch stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0210058","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0210058","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:b29a1bdd3bb6cc855936b51af1ab57b5f2bb498cd3d3b9041cde7a40e26a9fc3","observation_id":"c9f4e3cd-0eb7-4695-8423-25c2c9419741","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.0062","last_updated":"2014-05-01T00:25:29Z","snapshot_observed_at":"2026-08-18T17:50:35.448715Z","submitted_at":"2014-05-01T00:25:29Z","title":"The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.0062","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1405.0062","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:beccb1f0f809968b07617fc95f8af71b3f6adc7643f29d5e6f6f42d1e4a9939a","observation_id":"bc4bd3b1-0088-43a2-aa0f-388362dcee2c","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.1142","last_updated":"2010-04-07T17:45:01Z","snapshot_observed_at":"2026-08-15T05:22:17.692576Z","submitted_at":"2010-04-07T17:45:01Z","title":"The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in the Large Magellanic Cloud","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.1142","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1004.1142","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:64e9dec3b027d70556022395f0330ed29e4dd265aa671d54367637ef475ffe01","observation_id":"6ddcaa34-2645-442e-b54e-a84d521585ab","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.0814","last_updated":"2013-10-16T22:13:24Z","snapshot_observed_at":"2026-08-15T00:00:35.196903Z","submitted_at":"2013-10-02T20:00:00Z","title":"The Universal Stellar Mass-Stellar Metallicity Relation for Dwarf Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.0814","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1310.0814","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:b1ed6cd2af4ee965a2d4e9a9358008712f2b9517d3030f3fc77864481da66b52","observation_id":"a3e8aeec-c944-4c2d-9e40-d185db692ba4","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:680d474ddeb80654d8cf1cc727ae2df55c83c32065664c82a438fcdc44bcbff3","observation_id":"4923c3ea-5229-44e4-ae57-183616ab3a7e","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0510434","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:510a88f130e9c2fa4a7ff6b510032a0c71f8e6c2ca5e92abb5117f93c4440792","observation_id":"6013400d-01b3-4f22-b4ad-9c03d6e6304c","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0603416","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:294f2d199a6ece87502d4897cb5102c3c547aee3eaaaf0533deab7da3e62ca47","observation_id":"c3b826f1-3938-422e-a6e8-4d03bb237bdd","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"Asymptotic Giant Branch Stars , year = 2004, editor =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:d6d81ec433f112f92167c6b5f6862e53e4f6338336ae6c494938ec174d85a694","observation_id":"0cc40971-849f-446d-b5e1-bc1ca3f8a492","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:086c088bbedb6de21ad689530d0898a8bd22a9ba172d626216af1db95487a669","observation_id":"f6d2364f-c805-49fd-afab-0f2da1373750","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210098","last_updated":"2002-11-23T11:54:37Z","snapshot_observed_at":"2026-07-07T00:28:52.390737Z","submitted_at":"2002-10-03T17:32:12Z","title":"Uncovering Additional Clues to Galaxy Evolution. I. Dwarf Irregulars in the Field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0210098","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/0210098","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:4f96e0d4369ca1fc8debfceaab123d358fc0fa71c4075de7971f175eee25fcf6","observation_id":"e5e6c737-a7b5-4485-9688-aaf488fcf5a5","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":"Modelling of the circumstellar dust shells","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:4072b8c36e9bed77285197334b348a4b940ebaf22feb5c977372fd9078028baf","observation_id":"c0e4ba04-43c3-4fc6-a985-9492163c7fcb","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15704","last_updated":"2024-06-13T19:14:27Z","snapshot_observed_at":"2026-08-16T15:12:25.708861Z","submitted_at":"2023-07-28T17:51:43Z","title":"A JWST/MIRI and NIRCam Analysis of the Young Stellar Object Population in the Spitzer I region of NGC 6822","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15704","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2307.15704","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:257898301e7bb3d4467b146cb9604be1c84c3da2431be50160f902c207fdd7c5","observation_id":"341eb3f6-742e-41e6-bbe5-9665f2373d2e","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.4450","last_updated":"2012-04-19T20:00:02Z","snapshot_observed_at":"2026-08-15T04:12:30.967258Z","submitted_at":"2012-04-19T20:00:02Z","title":"Spectral Types of Red Supergiants in NGC 6822 and the Wolf-Lundmark-Melotte Galaxy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.4450","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1204.4450","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:917cb83aa5c884249c216bb77dfea2cc37260a6a258cacf362d591342458673c","observation_id":"e00dfb23-ef43-4b78-aa22-572607ab3851","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:36bef368417dc29045b20be6bb3e52607d5b1061ebc7f01deea0159271d1aaf1","observation_id":"fce37888-438b-4255-8f1a-fc6d9726882b","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9901235","last_updated":"1999-01-18T17:31:43Z","snapshot_observed_at":"2026-07-07T01:24:08.224353Z","submitted_at":"1999-01-18T17:31:43Z","title":"The third dredge-up and the carbon star luminosity functions in the Magellanic Clouds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9901235","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/9901235","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:0fe42175c40c3a29be6fe2bf820773049fd67a594e59bebe5681943b64722120","observation_id":"153ba67d-9d6f-4404-9507-b80cbb98c4df","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4922","last_updated":"2008-02-11T13:35:47Z","snapshot_observed_at":"2026-08-17T16:17:16.907561Z","submitted_at":"2007-11-30T13:01:45Z","title":"Evolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.4922","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/0711.4922","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:aaf81cd26736fe9e40c593a9564f1c1149d11099c634b6d0d9a1aae18b0127c2","observation_id":"4c2fc146-1ebc-4e68-9ae5-c16a8cae2618","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:dea5447cc79499f24278422b3d9762c2ef1ac9098d86279794c02ef9a9b55680","observation_id":"9576ca58-695d-4a0e-8364-2d83968211c4","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9810070","last_updated":"1998-10-05T21:32:43Z","snapshot_observed_at":"2026-08-18T10:36:24.253252Z","submitted_at":"1998-10-05T21:32:43Z","title":"Dwarf Galaxies of the Local Group","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9810070","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/astro-ph/9810070","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:782ce7b28ffa7bc49f5c515e22c72795ec796f8cd6ef0f43d2e4a029300c5483","observation_id":"b5b52e30-4fc5-403a-9ca1-2d73b495c4a9","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","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":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:3308e7fde7584bc6f11903aa283fcc29f3f0de327d46493a82caa9e16e6c043b","observation_id":"74a1e727-1803-4c33-9b62-4b3c70bed2f3","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1562","last_updated":"2012-05-05T00:11:37Z","snapshot_observed_at":"2026-08-18T02:46:18.511722Z","submitted_at":"2012-04-06T20:54:59Z","title":"The observed properties of dwarf galaxies in and around the Local Group","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.1562","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/1204.1562","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:0713034f635e508b8f25ef7e7330916a52bd02540a0da638afcd8efb65e8310a","observation_id":"8d7627e1-e47e-4786-9d32-b5d1afccbadd","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.01586","last_updated":"2020-12-14T19:14:09Z","snapshot_observed_at":"2026-08-16T19:01:24.768793Z","submitted_at":"2020-12-02T22:53:26Z","title":"Solo dwarfs III: Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.01586","snapshot_observed_at":"2026-07-14T03:55:10.305506Z","title":"Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-07-14T03:55:10.305506Z"},"links":{"cited_paper":"/paper/2012.01586","citing_paper":"/paper/2607.11682"},"observation_digest":"sha256:858de8d481bb9de1864808c1ca1cedfa7c202dbf1e4c5c97ab765faa668f55e8","observation_id":"e24cc5d8-d0c3-4723-a434-bd566db268ba","resolution":{"observed_at":"2026-07-14T03:55:10.305506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.11682","last_updated":"2026-07-13T15:20:16Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-17T06:02:51.024997Z","submitted_at":"2026-07-13T15:20:16Z","title":"JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":163},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 100 of 163 outbound references and 1 inbound Pith citation observation for arXiv:2607.11682."}