{"as_of":"2026-08-15T11:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:32487031fbcb0a4aa78d297516ad6f7c93754ab40ecb600880f03cb16f339c22","coverage":[{"denominator":140,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:18:26.054084Z","state":"measured"},{"denominator":104,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":104,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T07:18:21.762304Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03690","snapshot_observed_at":"2026-07-14T10:44:26.626236Z","title":", keywords =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10573","last_updated":"2026-07-16T02:37:35Z","snapshot_observed_at":"2026-08-14T18:35:08.958897Z","submitted_at":"2026-07-12T05:03:00Z","title":"Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\\AA\\ Bump","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-14T10:44:26.626236Z"},"links":{"cited_paper":"/paper/2412.03690","citing_paper":"/paper/2607.10573"},"observation_digest":"sha256:56648633e0098511cf5dc835dd5da4adaa45c516cebb7d5c488d870ad583a0fb","observation_id":"36873fa1-e835-40a6-9249-eb0933cbdb91","resolution":{"observed_at":"2026-07-14T10:44:26.626236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"cited_work":{"arxiv_id":"2412.03690","doi":"10.48550/arxiv.2412.03690","metadata_source":"pith","pith_arxiv_id":"2412.03690","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","venue":"astro-ph.GA","work_id":"d198d4f8-e2b1-4f76-8000-aa3ef023695f","year":2024},"citing_paper":{"arxiv_id":"2607.10573","last_updated":"2026-07-16T02:37:35Z","snapshot_observed_at":"2026-08-14T18:35:08.958897Z","submitted_at":"2026-07-12T05:03:00Z","title":"Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\\AA\\ Bump","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-14T10:44:26.626236Z"},"links":{"cited_paper":"/paper/2412.03690","citing_paper":"/paper/2607.10573"},"observation_digest":"sha256:69ffdfb51042441054bcd5c7e0f74c6931fa8b049c8fb21bb4e0beaa93b2e84d","observation_id":"de1d2204-d43a-405c-9dfd-642ab724b38c","resolution":{"observed_at":"2026-07-14T10:50:24.487830Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-14T23:21:08.958037+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T23:21:08.958037+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03690","snapshot_observed_at":"2026-08-02T07:18:14.813249Z","title":", keywords =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10573","last_updated":"2026-07-16T02:37:35Z","snapshot_observed_at":"2026-08-14T18:35:08.958897Z","submitted_at":"2026-07-12T05:03:00Z","title":"Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\\AA\\ Bump","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-02T07:18:14.813249Z"},"links":{"cited_paper":"/paper/2412.03690","citing_paper":"/paper/2607.10573"},"observation_digest":"sha256:fcf7eb3cd740ffdb22d62c3b6788f7ae2db46fd6040cad674f57f695ad2687a3","observation_id":"127e1257-d3dc-405b-969c-678892902cbc","resolution":{"observed_at":"2026-08-02T07:18:14.813249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03690","snapshot_observed_at":"2026-08-02T07:18:21.762304Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10573","last_updated":"2026-07-16T02:37:35Z","snapshot_observed_at":"2026-08-14T18:35:08.958897Z","submitted_at":"2026-07-12T05:03:00Z","title":"Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\\AA\\ Bump","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-02T07:18:21.762304Z"},"links":{"cited_paper":"/paper/2412.03690","citing_paper":"/paper/2607.10573"},"observation_digest":"sha256:2771ea5e22f2d9298cf0d0b759bd7d49049d8856a11474065927d249b639cbe6","observation_id":"f3443f1a-f115-47b3-bee4-9ae1faf92a2f","resolution":{"observed_at":"2026-08-02T07:18:21.762304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2412.03690/citation-record","integrity":"/paper/2412.03690/integrity","json":"/paper/2412.03690/citation-record.json","paper":"/paper/2412.03690"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.235748Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.235748Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:53f4a53fc015e69e84b95f5245c9a9e704889d1afa6a7a56af2755c4da620851","observation_id":"b377bdc9-b8e9-4e80-a540-9f0a4db7dcab","resolution":{"observed_at":"2026-08-11T22:18:24.235748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.240558Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.240558Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:c4e3a048787a73e19932341b39b15daef82b215d315b34b7d9b27ee9d6c0caad","observation_id":"9ab67e4d-9ced-4d69-8fcc-a1a6fd652ff2","resolution":{"observed_at":"2026-08-11T22:18:24.240558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.245439Z","title":"T., Gordon , K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.245439Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:1b06c4b2a742b49f3a1c4de68860ec42e7319d88aa814a70fc25c204aff575ba","observation_id":"bb243247-e536-4ae2-a806-6d01e2763a77","resolution":{"observed_at":"2026-08-11T22:18:24.245439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.249625Z","title":"A., Phillips , M","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.249625Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:32021f47927ce934a14613bb5808b4707b7ae44ebf910a6088eb8023941c5d98","observation_id":"5bdb3263-db08-42cb-b879-73c7a120adb9","resolution":{"observed_at":"2026-08-11T22:18:24.249625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.253578Z","title":"J., Calzetti , D., & Chary , R.-R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.253578Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:e0348662179731c107fdd31336e2fca1485f9ac787d085a40b04609908d5f937","observation_id":"ab42e1e4-4fa4-425e-ab9d-4cd7f1d61d74","resolution":{"observed_at":"2026-08-11T22:18:24.253578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.257776Z","title":"2017, , 851, 90","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.257776Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:8c5c7ccd608a2ad3ae81bfc0a73737f9863f68238c4ae0ae32b54a7e9cd9227f","observation_id":"f5552506-0bb3-4838-9172-02d029ffe3a1","resolution":{"observed_at":"2026-08-11T22:18:24.257776Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.268661Z","title":"J., da Cunha , E., Shivaei , I., & Calzetti , D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.268661Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:01b057103ad4ca9a0d5bba741d8d4fd3ef6b46f31718f639d45ec9106703275a","observation_id":"821e63e2-dc9a-4996-8f6f-0360d8cbc368","resolution":{"observed_at":"2026-08-11T22:18:24.268661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.311437Z","title":"J., da Cunha , E., Grasha , K., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.311437Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:f34a8eb09b643b3e514bbf34764a3768483ca290f71f1e9cd6aae77458b141f6","observation_id":"643750dc-50c3-47ce-815d-59e08c3e194e","resolution":{"observed_at":"2026-08-11T22:18:24.311437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.369260Z","title":"P., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.369260Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:c1eca503f080938d32ee1c48cb0fc422046ef124978d6e980c078d5e956b2fea","observation_id":"2dce2736-8689-4729-a6ee-fa3fdb188792","resolution":{"observed_at":"2026-08-11T22:18:24.369260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.421681Z","title":"2022, , 134, 054301","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.421681Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:237f21df647de8c1d51adf86284e0607e98837a3a10546b236f80af253a96ebc","observation_id":"3fbe3ec5-9105-43f5-bef4-f0e20fc6ece0","resolution":{"observed_at":"2026-08-11T22:18:24.421681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.443918Z","title":"2010, SWarp: Resampling and Co-adding FITS Images Together , ascl:1010.068","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.443918Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:412e41bb9f7faa93fff3e0009543e0668a875e385ea24e2477331868ec54efd3","observation_id":"ce7a03a1-eff4-444f-acd0-297dc6c616c9","resolution":{"observed_at":"2026-08-11T22:18:24.443918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.448041Z","title":"C., Bohlin , R","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.448041Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:4788cc554e51cac4580955c9d0a15b8fac22b1a3d9beb0d89ff9e1a32c10a716","observation_id":"dde8324b-ed51-4ff5-88c8-b29e4532c1b5","resolution":{"observed_at":"2026-08-11T22:18:24.448041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.452455Z","title":"R., Erni , R., et al","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.452455Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:6b541d5aba95d13725a76646a3a69bac08e7b55b252cc37a226fb458faa21549","observation_id":"ded61faa-8de5-471e-bc87-aab87aa81526","resolution":{"observed_at":"2026-08-11T22:18:24.452455Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.457312Z","title":"2011, , 533, A93","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.457312Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0a423c6df06049c690c3db1e559dd3b7384bc2bf2f8950ac1f61ddb199564cb3","observation_id":"2167b437-d7bb-4b70-8281-d39c878d8a43","resolution":{"observed_at":"2026-08-11T22:18:24.457312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.461161Z","title":"2012, , 545, A141","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.461161Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:1af7715e6aabdebae40750aa360cebeefde599730f255811bfa595e5f594b36f","observation_id":"6058bc8b-d5e8-48ef-94c4-6d21892fb121","resolution":{"observed_at":"2026-08-11T22:18:24.461161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.465181Z","title":"A., Law , D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.465181Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:2d80e9b3201c30ded3d635ca720cddc244415e1aa992a301f3c30e0a2a72c55f","observation_id":"584db105-4797-4baa-86ed-cdfa60c04da9","resolution":{"observed_at":"2026-08-11T22:18:24.465181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.527557Z","title":"2013, Star Formation Rate Indicators , ed","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.527557Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:9873418b0621570d4218f591166bdfb966d7486aa3020630548147c39cc252db","observation_id":"75a0b58a-f745-4868-87de-d2aa6fa77a68","resolution":{"observed_at":"2026-08-11T22:18:24.527557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.555838Z","title":"C., et al","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.555838Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:52a74d39cf497319893517e7cfd2eb338a857ade0e2bb1184c558c9ab4986b5e","observation_id":"1ac4fd14-0e23-49e5-bf0e-1c179a9683c1","resolution":{"observed_at":"2026-08-11T22:18:24.555838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.560585Z","title":"L., & Storchi-Bergmann , T","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.560585Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0082f266e9c4cf2e88cf8f6442a6cf142174470a161fad7bb688d407d94a501e","observation_id":"bedd98cb-e901-4c88-a757-51e426650ba6","resolution":{"observed_at":"2026-08-11T22:18:24.560585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.563526Z","title":"C., Engelbracht , C","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.563526Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:34704d4167e27b4dc2eac3f7fb77dde3e6703a3428e8c8ae60a56f4c83efed70","observation_id":"6c28deda-d0cb-4330-bfc6-ba007c0063f3","resolution":{"observed_at":"2026-08-11T22:18:24.563526Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01831","last_updated":"2024-06-03T22:59:46Z","snapshot_observed_at":"2026-08-12T23:51:03.425220Z","submitted_at":"2024-06-03T22:59:46Z","title":"Feedback in Emerging Extragalactic Star Clusters (JWST--FEAST): Calibration of Star Formation Rates in the Mid-Infrared with NGC 628","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.01831","snapshot_observed_at":"2026-08-11T22:18:24.567503Z","title":"T., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.567503Z"},"links":{"cited_paper":"/paper/2406.01831","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:17784b339e6339e4b0fc33b98f21be7c2dd736faa996b3e4d9095037b0377d30","observation_id":"ea4244fe-54f8-459e-b5ef-62124293ad32","resolution":{"observed_at":"2026-08-11T22:18:24.567503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.571664Z","title":"2015, Astronomy and Computing, 9, 20","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.571664Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:95fe80c1dece51315558e85b8e806ca218e73f9345b82014179626a0e0b0af6d","observation_id":"96a7c4d6-f6fc-4f37-8fc8-0eee308c3cbb","resolution":{"observed_at":"2026-08-11T22:18:24.571664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.575247Z","title":"2020, Astronomy and Computing, 31, 100381","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.575247Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:d8c89e7aacd221983cecd8f4a6d5f4df90790ce726f982c8c4205baf6bd7ef0f","observation_id":"46e9496f-8ad8-40ca-b4b9-fb25c86a84e4","resolution":{"observed_at":"2026-08-11T22:18:24.575247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.579824Z","title":"A., Clayton , G","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.579824Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:beca3992f51eb6e3adcbfbd44072ad1face4d53b71b77970fa7a11b7b73e8a92","observation_id":"ccdd76f0-fdf7-4a05-8554-8156f1c14b3d","resolution":{"observed_at":"2026-08-11T22:18:24.579824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.583697Z","title":"2003, , 115, 763","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.583697Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:805dae234f3d4364d0558deaf7f8bbb5fd49c862f0191ed91b20d28dc7004b8a","observation_id":"f6561c7d-c584-425a-b79c-e36df3593ca4","resolution":{"observed_at":"2026-08-11T22:18:24.583697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.621851Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.621851Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:a538cd30b9afc8599d2b6080b9bb2e0e2a1ae5e6ea54f3a5056c118b9a9e6f9c","observation_id":"33c4828c-e9f3-4bca-9796-bab01ae07671","resolution":{"observed_at":"2026-08-11T22:18:24.621851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.665372Z","title":"2023, , 944, L11","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.665372Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:5b9a3e0405c5eb2b16771ead4c885478712d68d8d7f92fa2c094406e2967864a","observation_id":"87d250fb-e767-4929-b2a7-ffee2ecee925","resolution":{"observed_at":"2026-08-11T22:18:24.665372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.03835","last_updated":"2024-10-04T18:03:21Z","snapshot_observed_at":"2026-08-12T22:30:29.764739Z","submitted_at":"2024-10-04T18:03:21Z","title":"The Resolved Behavior of Dust Mass, Polycyclic Aromatic Hydrocarbon Fraction, and Radiation Field in ~ 800 Nearby Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.03835","snapshot_observed_at":"2026-08-11T22:18:24.722295Z","title":"M., Leroy , A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.722295Z"},"links":{"cited_paper":"/paper/2410.03835","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:ef9cf065956e70efd9c4e053a958ea3490ce9988cc91979a87890b9d36fae8e1","observation_id":"0ea4da70-d14a-4428-ad0b-ad6f71378324","resolution":{"observed_at":"2026-08-11T22:18:24.722295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05397","last_updated":"2025-03-19T16:52:50Z","snapshot_observed_at":"2026-08-14T14:28:46.277997Z","submitted_at":"2024-10-07T18:02:21Z","title":"Polycyclic Aromatic Hydrocarbon and CO(2-1) Emission at 50-150 pc Scales in 70 Nearby Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05397","snapshot_observed_at":"2026-08-11T22:18:24.738952Z","title":"K., Sandstrom , K., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.738952Z"},"links":{"cited_paper":"/paper/2410.05397","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:f010458f83650f5e5cfcecc4fa9a2b456749637095368bd6710aa80add0fcbd6","observation_id":"a46e8713-f55b-4447-a9d5-ae980c4fcccc","resolution":{"observed_at":"2026-08-11T22:18:24.738952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.755326Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.755326Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:5b65f67c0a00aeef6ebaa1d96454e2fd7a3db211dabaa94b2e0f911f4845143e","observation_id":"a1698d7d-d999-4a22-9138-e6d641d64b1c","resolution":{"observed_at":"2026-08-11T22:18:24.755326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.759493Z","title":"C., Gordon , K","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.759493Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:6291c05332c764662844b823126ba090ac4ad6fc396bcb3908b53c4494970942","observation_id":"4d9f9f07-51a1-452d-a37e-f5ab564add90","resolution":{"observed_at":"2026-08-11T22:18:24.759493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.764125Z","title":"C., Gordon , K","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.764125Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:bb863b229de9a1e250c18cf605f0429b5e0223d1ad3dec1125a8b179052dd7f3","observation_id":"6d4d1d73-bede-4f67-b8e4-2c539476d1b1","resolution":{"observed_at":"2026-08-11T22:18:24.764125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.768399Z","title":"C., Gordon , K","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.768399Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:ab8934ac8ea34b3a7b5ba68a2f24cfbdafbeaeeed483908728839abffa57c05c","observation_id":"35c5b4b2-18be-453f-9c57-dd2281545276","resolution":{"observed_at":"2026-08-11T22:18:24.768399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.772628Z","title":"2013, , 51, 393","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.772628Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:e9166236f291bbd2bc0c854285c27a5984e95dc0b738159b244a47db367b5ad4","observation_id":"5dc1d1d6-11e7-41e2-99e7-a543386f9f15","resolution":{"observed_at":"2026-08-11T22:18:24.772628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.779534Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.779534Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:45221c50e0e402ede0247eeb671015401ba8f518fe98d0d8931145175b73bcca","observation_id":"7e0c7b6e-6c46-45b0-af82-ecd7aa97aa57","resolution":{"observed_at":"2026-08-11T22:18:24.779534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.831439Z","title":"M., Skrutskie , M","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.831439Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0493a1770a543329ff9cc36ebb06f1d874c19bb2aa1bdd97ef0fb0bd0dcff2fa","observation_id":"79aa85ed-2ec6-43bc-96da-14e677e46140","resolution":{"observed_at":"2026-08-11T22:18:24.831439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.886325Z","title":"2008, , 388, 1595","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.886325Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:10e53831d91ad8c24ab89b563861d6f9f613b7563094cf898d5f1cd0f96cd438","observation_id":"49d95570-d075-4933-8136-d4572d455094","resolution":{"observed_at":"2026-08-11T22:18:24.886325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.908034Z","title":"2019, PhD thesis, Ghent University, Belgium","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.908034Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:2e25a2f83ba4ece3d1d63e11ddbdecf4bbb71b4b7fa37229515374afce3ab284","observation_id":"28f5b488-3bcb-4ea1-9095-82a7ab1a7f57","resolution":{"observed_at":"2026-08-11T22:18:24.908034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.912600Z","title":"2019, , 486, 743","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.912600Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:928e53bdbf0549cc886b5f300b501dbe23f62d509e72b91918bc190e011761d6","observation_id":"ec4816b7-4d22-4c6d-9c3f-dbb1dc10d901","resolution":{"observed_at":"2026-08-11T22:18:24.912600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.916965Z","title":"D., Andrews , J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.916965Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:cae007ddd022a455b14561840a6520863f687a49dc14cce41de82aa9ce9edb75","observation_id":"a146ae94-8d96-4b9f-bc22-c7077874556e","resolution":{"observed_at":"2026-08-11T22:18:24.916965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.920580Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.920580Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:55e036381f1d26adc2c66cd15ded53e50b1dd9aeef01e8354da577995ffc6174","observation_id":"e95f30ab-8025-446a-9911-3f47532ec918","resolution":{"observed_at":"2026-08-11T22:18:24.920580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.925205Z","title":"T., & Li , A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.925205Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:048ff846d226cdb0458f49aae9bc782a78c295b7ae999fa9c8ff00a785c4bb0f","observation_id":"d55007a6-bff8-408c-9f69-87532df1ba36","resolution":{"observed_at":"2026-08-11T22:18:24.925205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.929546Z","title":"T., Li , A., Hensley , B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.929546Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:575bc07e531e052e1be3136e91f1bfa431803229e7921877d85a3b618260853f","observation_id":"4e0a9ccd-96fc-4d9f-a6f4-a050137550f8","resolution":{"observed_at":"2026-08-11T22:18:24.929546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.933810Z","title":"T., Dale , D","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.933810Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:35062f95ba441069386dac046f3f8ac43abbd3ca8b15df17529c3d431a64de0e","observation_id":"8cef7274-cea9-4c5f-a5f4-d8f0f41d0896","resolution":{"observed_at":"2026-08-11T22:18:24.933810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.937933Z","title":"V., Kreckel , K., Sandstrom , K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.937933Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:663c30db5089c3c8842b45d4c293ba214c722f31d1e578d42a32ddccb062f8cc","observation_id":"4a5bd6cc-9c55-4913-9cc0-d0a2575cdf2b","resolution":{"observed_at":"2026-08-11T22:18:24.937933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.942264Z","title":"2022, , 659, A191","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.942264Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0679979f008f169568ea9d736eef957363b51f5fe8c26049a6b99fd3de88551a","observation_id":"8397a048-b031-4c68-9f5c-3580deebec10","resolution":{"observed_at":"2026-08-11T22:18:24.942264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.946417Z","title":"2024, arXiv e-prints, arXiv:2405.13491","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.946417Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:aeebe5e5bd26e87748d5fb6e9c134027736e498a14d208915e4ddfdeffb855f5","observation_id":"6d2170b2-1d4d-4a39-9067-09e5589bef61","resolution":{"observed_at":"2026-08-11T22:18:24.946417Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:24.991441Z","title":"2021, , 505, 283","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:24.991441Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:56b5c54a0a8845aee450b709dd6bd407d821dda63c7704fbe8b92b9b46bda281","observation_id":"40666a8d-121b-49b7-afb7-3fdbbed654f2","resolution":{"observed_at":"2026-08-11T22:18:24.991441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.038490Z","title":"2011, , 533, A117","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.038490Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:d84871691ba84e5f28fd4fa4fa44923b3e3445bfdea41564e8333c4c68eaa062","observation_id":"11e26ebd-b554-46b9-9b25-f91c278c5fa9","resolution":{"observed_at":"2026-08-11T22:18:25.038490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.052362Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.052362Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:f1eb9953310fa582121395102e93572a810b04a7fa41502d7a63304b0729d1ea","observation_id":"65caf789-c54b-4102-8682-c2e539a48589","resolution":{"observed_at":"2026-08-11T22:18:25.052362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.058710Z","title":"L., & Massa , D","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.058710Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:304a29fc813da4317da4c14c033c32a4322c51058890404696a63149bf9700bf","observation_id":"da0db92b-38fc-480b-9635-0503cf3ba624","resolution":{"observed_at":"2026-08-11T22:18:25.058710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.062685Z","title":"1990, , 72, 163","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.062685Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:16482860484ace698b3c21e75ab6e4d9f5889cc810cece22fc95c5f0c0731d2e","observation_id":"47fe71a8-03ab-47ae-8baa-76f466641ca4","resolution":{"observed_at":"2026-08-11T22:18:25.062685Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.067135Z","title":"L., Massa , D., Gordon , K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.067135Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:669a28d1dabff80cae2124cf4066a4defcaf28e3f37086f3623e5e0b160a0fda","observation_id":"cd2bd61c-985e-48d2-ae16-ca943c31063c","resolution":{"observed_at":"2026-08-11T22:18:25.067135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.071170Z","title":"2010, , 523, A85","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.071170Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:2b2bb3ad1d704e2086a19782a15b75d79f7ee2e00d7e92f57ae7ed162740f9c7","observation_id":"44fa9f66-cb0b-43cd-864e-b07693138f9c","resolution":{"observed_at":"2026-08-11T22:18:25.071170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.075494Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.075494Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:5e24ecea1cce9eb07b968411e06127946d22fc681f162b0022cf2c5f4619b0e9","observation_id":"f1c1cd52-1448-48c6-8f4f-c3ecd80800e7","resolution":{"observed_at":"2026-08-11T22:18:25.075494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.127646Z","title":"2004, , 611, 1005","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.127646Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:e58995bbbd970adb02805224b47cc4927a8e1526bc5a4c5453e34f4470c72ec4","observation_id":"e461c2f3-1029-412b-9d47-24a910b82549","resolution":{"observed_at":"2026-08-11T22:18:25.127646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.132282Z","title":"D., Calzetti , D., & Witt , A","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.132282Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:f45b0af014cc4849acd6e5531741d7d253921518bafbfa3bbc73663a53f165cd","observation_id":"4e97bd18-9b61-4b29-a69e-645c764cebac","resolution":{"observed_at":"2026-08-11T22:18:25.132282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.135739Z","title":"D., Cartledge , S., & Clayton , G","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.135739Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:b7addb05c7ec03fcc7193f866f294ce06cbed1ef3b3ac685b854b33fbc56c75a","observation_id":"4b4ceeb7-095a-429c-bec2-60757482895e","resolution":{"observed_at":"2026-08-11T22:18:25.135739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.190210Z","title":"D., Clayton , G","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.190210Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:05f822bd03bb693b27c649bb214d325d47b592241299985e9773dc75d91e57bd","observation_id":"5fbefccf-8191-48a2-b04f-c667dca6d168","resolution":{"observed_at":"2026-08-11T22:18:25.190210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.264962Z","title":"D., Misselt , K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.264962Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:db6bea4fe7b9fc088f508cdfc7ef0add49f20962f0dc378b88f7d627c982773d","observation_id":"5fe2519d-a3ee-4542-8626-2c600c45c5f6","resolution":{"observed_at":"2026-08-11T22:18:25.264962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12792","last_updated":"2024-05-21T13:42:35Z","snapshot_observed_at":"2026-08-13T00:02:58.301973Z","submitted_at":"2024-05-21T13:42:35Z","title":"Expanded Sample of Small Magellanic Cloud Ultraviolet Dust Extinction Curves: Correlations between the 2175 A bump, q_pah, UV extinction shape, and N(HI)/A(V)","version":1},"cited_work":{"arxiv_id":"2405.12792","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.12792","snapshot_observed_at":"2026-08-11T22:18:26.967158Z","title":"Expanded Sample of Small Magellanic Cloud Ultraviolet Dust Extinction Curves: Correlations between the 2175 A bump, q_pah, UV extinction shape, and N(HI)/A(V)","venue":"astro-ph.GA","work_id":"9da5bc8f-0024-453e-aca7-ce04b13e72dd","year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.347921Z"},"links":{"cited_paper":"/paper/2405.12792","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:465f0fa5565e2f5c8f26d099fdc3406944e881abeca58e239b4067b74d154c61","observation_id":"e46e6ee5-6b89-430f-a147-4b454c6963e7","resolution":{"observed_at":"2026-08-11T22:18:26.989904Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.09667","last_updated":"2024-05-15T19:10:29Z","snapshot_observed_at":"2026-08-13T00:06:56.273791Z","submitted_at":"2024-05-15T19:10:29Z","title":"Feedback in emerging extragalactic star clusters, FEAST: The relation between 3.3 $\\mu$m PAH emission and Star Formation Rate traced by ionized gas in NGC 628","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.09667","snapshot_observed_at":"2026-08-11T22:18:25.353431Z","title":"2024, arXiv e-prints, arXiv:2405.09667","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.353431Z"},"links":{"cited_paper":"/paper/2405.09667","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:009094158f3d08c77dba1697175f3b0612f8bb10c50bd72f95bc6d92a1e83128","observation_id":"de2f62d0-e95f-4a03-b6c8-d738c9f950cf","resolution":{"observed_at":"2026-08-11T22:18:25.353431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.358304Z","title":"2023, , 520, 4902","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.358304Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0456a99bbb4af3db086f6f35ee352d420aec55a53b6d49807230b486ff16f2b7","observation_id":"ad1311f4-8cd2-4f85-85f5-a26fb7bb339a","resolution":{"observed_at":"2026-08-11T22:18:25.358304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.361534Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.361534Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:8ed938885e91216f668b437331e388424066f9139eec3348c5d8780b84939dc0","observation_id":"4fd3e380-ccee-49d7-b526-3be86b07cf26","resolution":{"observed_at":"2026-08-11T22:18:25.361534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.365317Z","title":"S., & Draine , B","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.365317Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:d7064a38da40a93127fcd60181d587b55dc26ea40f7f1c604621277e8a5ad83e","observation_id":"0747f469-f43d-4872-bfa4-bf0c7f3dea48","resolution":{"observed_at":"2026-08-11T22:18:25.365317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.369631Z","title":"2021, , 906, 73","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.369631Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:9c1e4bdce61ec7c9496e132be2dc70bc939f95359ee95caa288b064fa6e2c8d3","observation_id":"4c25f8c4-0cce-4ff6-b880-7a0832113087","resolution":{"observed_at":"2026-08-11T22:18:25.369631Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:29.040984Z","title":"2023, , 948, 55","venue":null,"work_id":"cbf81cc0-732d-4254-a4af-18e36da8719a","year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.374451Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:2c2defe3edb5b2febea9176962c95a35103230ae4e94d94277933c2aa239b6db","observation_id":"128af69f-2f70-41ce-a483-1039afd3f424","resolution":{"observed_at":"2026-08-11T22:18:29.044881Z","resolver_source":"raw_fallback","status":"parse_uncertain"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:29.027545Z","title":"F., Strauss , M","venue":null,"work_id":"f202930c-1c6c-4468-be2e-5beaa9d332eb","year":2004},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.378044Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:f2a1f0c256d6b25d98e7b48f3600e78f1a096244288ce7525c5cce44629d1c60","observation_id":"6bd71aa1-2632-42e7-9800-0258eb537de4","resolution":{"observed_at":"2026-08-11T22:18:29.032281Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:29.013987Z","title":"A., Gronwall , C., Vanden Berk , D","venue":null,"work_id":"cfcc211f-1db3-46f5-b5a5-052e0cf4edd0","year":2011},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.443690Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:1d87b941e7dc7c77138751edf4ed1f393fb08a56b5f6d0fdca66cbff79912ae2","observation_id":"53c67933-d564-4b7b-8637-9cee0ac035d8","resolution":{"observed_at":"2026-08-11T22:18:29.018251Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.944436Z","title":"J., Silverman , J","venue":null,"work_id":"46a1d348-b73c-4046-9dff-c6d6318efd9e","year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.536286Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:ab7ff7e5eafa16a5efe2fa70cba28f0c3eda371b82e86918b7923e045e1a6b53","observation_id":"77733ed2-9751-44a1-a5b5-46aae438ac78","resolution":{"observed_at":"2026-08-11T22:18:29.004047Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.572330Z","title":"M., Tremonti , C., et al","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.572330Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:e6554d2c12fc77d5fa475e767b893544bc95b9d470bb621b686a131a612c1edb","observation_id":"c4166861-7c96-4592-966f-09223987537f","resolution":{"observed_at":"2026-08-11T22:18:25.572330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.782434Z","title":null,"venue":null,"work_id":"93291e17-6e43-4b4d-8bf9-963437c24498","year":1942},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.585081Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:a0ff72ce71ebaeef336566ba3cb201b173a9516f978df0cf5040ab175744745a","observation_id":"0fdcea2e-0be0-4c1d-8a32-5c900447a814","resolution":{"observed_at":"2026-08-11T22:18:28.857634Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.594314Z","title":"C., & Evans , N","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.594314Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:dcfa5575a390e6ee0ac408ab214c370c49a34ec1e4abb7b51d15c4bf98df1d46","observation_id":"86aa71bd-256c-487e-a156-317ed8eeaba3","resolution":{"observed_at":"2026-08-11T22:18:25.594314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.599338Z","title":"J., Dopita , M","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.599338Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0679861f05ba9f319705064461bd14e69f6ede1b9e4e2d83e367e82f4d5caf55","observation_id":"93f5e943-a0ce-4a3e-9c84-09eb449472ac","resolution":{"observed_at":"2026-08-11T22:18:25.599338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.603459Z","title":"J., Nicholls , D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.603459Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:5fbd95a1ceecfb31baa3bae9b7fba206f6323abfce1aad63072823dd4f6f8d07","observation_id":"1f294acd-e1ec-4dff-9397-791c4e0205dc","resolution":{"observed_at":"2026-08-11T22:18:25.603459Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.732460Z","title":"2013, , 771, 62","venue":null,"work_id":"f5486dcf-30fb-4b03-b6ee-e21b0c7a4a57","year":2013},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.607455Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:654264d0a5863c4e4979ca0e797d12bcc89de5419f172ae41dd2e94ed428e9d3","observation_id":"d8e5e2ed-2f2b-41fd-95df-7b8801c143e9","resolution":{"observed_at":"2026-08-11T22:18:28.736821Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.611207Z","title":"T., Blanc , G","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.611207Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:4fe4c03ae66e0b9c2c8843442cecbc79bcf00a8c30cc9b7e002a0e51b9543c5c","observation_id":"9a93ee25-5e70-41c9-8f12-32c5a82ad7aa","resolution":{"observed_at":"2026-08-11T22:18:25.611207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.713212Z","title":"2013, , 775, L16","venue":null,"work_id":"24b213d6-c88f-48e4-bfbf-7b5ee843a19b","year":2013},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.615115Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:ec8325d243d25577c8a61fe2f9878bcc064b14e2e55cc602bcc2b8008da22932","observation_id":"00c50d21-e8cb-48da-9ef7-79d184ba4414","resolution":{"observed_at":"2026-08-11T22:18:28.717186Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.619206Z","title":"2001, , 322, 231","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.619206Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:1044ace4d8c62941ddc5f75f12e0c14e23f6e64503ac2f6408194173b7d60f5b","observation_id":"8f98a4e9-5e98-44a7-9346-0ddbe8d7f270","resolution":{"observed_at":"2026-08-11T22:18:25.619206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.15608","last_updated":"2023-01-18T00:46:55Z","snapshot_observed_at":"2026-08-13T17:24:39.380477Z","submitted_at":"2021-11-30T17:58:57Z","title":"Science with the Ultraviolet Explorer (UVEX)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.15608","snapshot_observed_at":"2026-08-11T22:18:25.623280Z","title":"R., Harrison , F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.623280Z"},"links":{"cited_paper":"/paper/2111.15608","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:8cb20902b4b7673abb06edb3219a16b50b4affd475a7de2b2c85cff8dd4cbdc7","observation_id":"a56288f4-c50e-4a36-96a7-bcc54cd66d52","resolution":{"observed_at":"2026-08-11T22:18:25.623280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.711754Z","title":"E., Rosolowsky , E., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.711754Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:efe9b5586c1b08fe13656e34f813ff5a6ccedce7e94cbe0494f140f1a446275e","observation_id":"0ff6e29d-c89f-40c5-913a-c00cef495f98","resolution":{"observed_at":"2026-08-11T22:18:25.711754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.799240Z","title":"C., Sandstrom , K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.799240Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:74c188a0351ae9bba8726e504ca495c583d8a61a8f0c515526dfe13a59436556","observation_id":"89b2e4a7-08ad-4d39-ad41-dfa55989092d","resolution":{"observed_at":"2026-08-11T22:18:25.799240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.856216Z","title":"D., et al","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.856216Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:beeb179eb9f2bfb2151173479fa40871b16e46ef3db5c2162bfccf824588ce4e","observation_id":"3051a3f0-00c8-475d-9124-a797bb530e3d","resolution":{"observed_at":"2026-08-11T22:18:25.856216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.863510Z","title":"K., Sandstrom , K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.863510Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:e339d48ce9033771ca0945c0302b3a3bb403aae0bfc20c348d98937353ffb6f9","observation_id":"8dfc9ecf-ef26-42cf-a317-751a73d92303","resolution":{"observed_at":"2026-08-11T22:18:25.863510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.867633Z","title":"K., Schinnerer , E., Hughes , A., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.867633Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:35a5e3f5ad3d29b24c6f87736eeca0b7015112bae0f51a96ef110763d3d5fef9","observation_id":"8342e0f2-b216-4778-ba6f-fe20272506c8","resolution":{"observed_at":"2026-08-11T22:18:25.867633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.872189Z","title":"K., Schinnerer , E., Liu , D., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.872189Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:798c2760bbee1c4f9bbe9bc9791d4dd16cc69820c91e6d92b7672637b12f75b4","observation_id":"fa794ee0-590f-4d53-a19c-774f70645d60","resolution":{"observed_at":"2026-08-11T22:18:25.872189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.651124Z","title":"2020, Nature Astronomy, 4, 339","venue":null,"work_id":"d663ac3a-b1b6-40a7-b985-275d3fcfa380","year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.876008Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:695252ec6ca7dde8b759916dae937b7f49f136fc7daecb816eb4ce361ac0ae40","observation_id":"2afc3a13-1485-423f-8493-042b42172207","resolution":{"observed_at":"2026-08-11T22:18:28.655510Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.880238Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.880238Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:92a0d76d8be8b6b331d4d3d03cf3eb441c93d59077c8eca2b48ebf85ea9327a8","observation_id":"a17b04bd-c144-4056-bb21-d91f809ee203","resolution":{"observed_at":"2026-08-11T22:18:25.880238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:25.884063Z","title":"J., & Li , A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.884063Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:70565fa8f3ecaa1b7bad595a36ae4690161d40d837ffe5e96d10d24c161488f1","observation_id":"3e980b79-d136-4c04-bec5-ddec51e6fee7","resolution":{"observed_at":"2026-08-11T22:18:25.884063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.623473Z","title":"2017, , 472, 2196","venue":null,"work_id":"c8836410-1b63-44a9-a589-d9bef3da67ac","year":2017},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.887404Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:67e8c0c41ebb1b90f53673f7a80843c7f50a7e3e5f743c117c576702bbf453c8","observation_id":"e7582d6c-71e9-41bf-8cba-90e60b13ec09","resolution":{"observed_at":"2026-08-11T22:18:28.627736Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.611543Z","title":"R., Engelbracht , C","venue":null,"work_id":"d56fd5ec-8bce-4740-ad6b-18f48d09a45d","year":2010},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.891290Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:d92d7d6133ca536280479b0bde2c7b9c68133555db4358690d74f8dd5827c678","observation_id":"4b77cf45-2477-48b1-8d40-4882b25c8d0e","resolution":{"observed_at":"2026-08-11T22:18:28.615278Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05996","last_updated":"2025-08-18T15:22:02Z","snapshot_observed_at":"2026-08-13T04:23:05.116984Z","submitted_at":"2024-02-08T19:00:01Z","title":"Dust attenuation evolution in $z \\sim 2$-$12$ JWST galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05996","snapshot_observed_at":"2026-08-11T22:18:25.963183Z","title":"2024, arXiv e-prints, arXiv:2402.05996","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:25.963183Z"},"links":{"cited_paper":"/paper/2402.05996","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:42155930ba8886138fb3ec7259c2280384eaf41da300430e129cd487f77479eb","observation_id":"ca44aa6c-0169-4d4a-ae0f-6e6c70a4f4fe","resolution":{"observed_at":"2026-08-11T22:18:25.963183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:26.021895Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.021895Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:194b3bb3de638af2f9c3ca04d687a54972dd8c0e3ec8c67b0303fcebda693405","observation_id":"67e0730f-36e0-4289-9a8c-768c1c734610","resolution":{"observed_at":"2026-08-11T22:18:26.021895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.561360Z","title":"J., Cullen , F., et al","venue":null,"work_id":"62a80673-24f2-421a-8c07-0f3745c615c8","year":2016},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.026750Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:66dc632bb0848e41774b5071b7850a99f345af2815ccd1f78322ecbbf95a274b","observation_id":"a95cd54c-bc90-430f-9afa-33fff623273f","resolution":{"observed_at":"2026-08-11T22:18:28.592007Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.442006Z","title":"D., & Fitzpatrick , E","venue":null,"work_id":"cc25b9bd-11fc-4655-81e5-3797ebcfbbb2","year":2022},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.030896Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:d5b632406b6a7fedf4dcbf1e19c084222658a5ad3ff127a5274609fdf0d29e9f","observation_id":"012d48b6-20e1-4508-94a7-92f041256804","resolution":{"observed_at":"2026-08-11T22:18:28.489283Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15093","last_updated":"2024-07-21T08:41:08Z","snapshot_observed_at":"2026-08-12T23:17:53.653011Z","submitted_at":"2024-07-21T08:41:08Z","title":"Ultraviolet Extinction Sky Survey (UVESS): A mission concept for probing the interstellar medium in the Milky Way and Local Group galaxies","version":1},"cited_work":{"arxiv_id":"2407.15093","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.15093","snapshot_observed_at":"2026-08-11T22:18:26.857413Z","title":"Ultraviolet Extinction Sky Survey (UVESS): A mission concept for probing the interstellar medium in the Milky Way and Local Group galaxies","venue":"astro-ph.IM","work_id":"ebc941a6-a46e-44dc-8349-a39c23c5594a","year":2024},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.035165Z"},"links":{"cited_paper":"/paper/2407.15093","citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:a172e23fa65ffdd4e6befe05c0174e44768ea73faae34087e520b45acecfa8d9","observation_id":"e29be16e-ce30-4043-8674-2a6ab91813d6","resolution":{"observed_at":"2026-08-11T22:18:26.864294Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.423790Z","title":null,"venue":null,"work_id":"0946fbf6-2a1f-4a07-aaf7-759e33b160a2","year":1994},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.040320Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:c2f98ef81ad4398866d3a9f1394bd321f2f4cccfb1933143bf6c8b7e1d784a63","observation_id":"7c966d0b-3c1e-425b-b346-15c441b3e60e","resolution":{"observed_at":"2026-08-11T22:18:28.427690Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.410167Z","title":"2020, , 251, 11","venue":null,"work_id":"7a7bd037-2220-4ea9-92e6-b8335acad204","year":2020},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.045239Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:391478bd3b7e5d69cab9b4361c46cfd6ba855031b65d60f218c089610f18a959","observation_id":"c6206895-c03b-4649-abd2-56e63086de05","resolution":{"observed_at":"2026-08-11T22:18:28.414768Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:28.397510Z","title":"2009, , 499, 69","venue":null,"work_id":"53a320ad-5e2a-4361-83a2-7baf58abdaa6","year":2009},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.049858Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:45f23de2db65bcf84ca6c955668732fba574e021de1b88fe30aaae65c7021dd0","observation_id":"1d8585ae-ecd9-47de-87d3-67f869393165","resolution":{"observed_at":"2026-08-11T22:18:28.401903Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:18:26.054084Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-11T22:18:26.054084Z"},"links":{"citing_paper":"/paper/2412.03690"},"observation_digest":"sha256:0498eefb2c071b46a64441bcbee8625fb473c071a970cb0e041fe38e1afee895","observation_id":"61d34625-3899-4b42-becb-f0fd7d53f6a6","resolution":{"observed_at":"2026-08-11T22:18:26.054084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.03690","last_updated":"2024-12-04T20:02:57Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T21:24:21.749514Z","submitted_at":"2024-12-04T20:02:57Z","title":"Constraining the link between the 2175{\\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":4,"unresolved":82,"verified_exact":1,"verified_fuzzy":12},"total_outbound_references":140},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 100 of 140 outbound references and 4 inbound Pith citation observations for arXiv:2412.03690."}