{"as_of":"2026-08-14T11:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b91ccbb9c581efc291a584f68fc9d6ebe2c0ccfcdff56af3b1b5f2c37956b7c6","coverage":[{"denominator":66,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":66,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:32:38.205893Z","state":"measured"},{"denominator":66,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":66,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.08717/citation-record","integrity":"/paper/2608.08717/integrity","json":"/paper/2608.08717/citation-record.json","paper":"/paper/2608.08717"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.246769Z","title":"2022, in American Astronomical Society Meeting Abstracts, Vol","venue":null,"work_id":"c72d328c-b5fa-4a50-bf5e-ccfb107bd4c0","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.397957Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:d6db504a1039f711563937d1c2aa48cd4c7fbcf70f73c27b88109004e24dc8b6","observation_id":"83eace24-e732-48bb-bd86-abdedffc2ab1","resolution":{"observed_at":"2026-08-14T04:32:39.251292Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:37.404842Z","title":"P., Tollerud , E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.404842Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:3ab6a353882f8564af6038bbfe5df86be6b836a2f66fb346d79bdc7f4cd3de97","observation_id":"5c925682-f1db-47dc-8ad2-4504c7c7b22d","resolution":{"observed_at":"2026-08-14T04:32:37.404842Z","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":"2026-08-14T04:32:37.421353Z","title":"M., Sip o cz , B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.421353Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:59dfb09a5fecae5f7bcb448ce38acd3b1168735a04859837c6acec502deef7e0","observation_id":"d908fe23-31e0-42bc-be65-21ec9693a3ad","resolution":{"observed_at":"2026-08-14T04:32:37.421353Z","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":"2026-08-14T04:32:37.440230Z","title":"M., Lim , P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.440230Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:42c44f5a82aa8025a5b06bd0e4719bf32c752473042355ac18a99cf5e43fffe7","observation_id":"8420192c-7af5-455b-8b44-6fbabea2145d","resolution":{"observed_at":"2026-08-14T04:32:37.440230Z","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":"2026-08-14T04:32:37.451932Z","title":"2023, title All-sky Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories: The Complete Sample , , 951, 78, 10.3847/1538-4357/acd333","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.451932Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:d3d15ce01d4677ad0fbbaf1844725f4d1a6028e1292a8e2b8a0d00b87e490e78","observation_id":"1decdc80-680e-4569-b709-c3e28e541709","resolution":{"observed_at":"2026-08-14T04:32:37.451932Z","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":"2026-08-14T04:32:39.221012Z","title":"2024, title One-Pass-Fitting , , version 0.2 https://github.com/Vb2341/One-Pass-Fitting","venue":null,"work_id":"b58cf0de-1d67-4fc2-be28-ba72f96c2d0a","year":2024},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.457982Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:fd774a7b4848dbec3ba0ae1e7ca4365367275be34d0349013bd2a21ef378f41f","observation_id":"e8c9462e-93fd-40d4-b746-fb998571030b","resolution":{"observed_at":"2026-08-14T04:32:39.225516Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:37.461972Z","title":"O., Kammerer , J., Pueyo , L., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.461972Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:d35a0c62e9e099462ec6f84f3877e56d6ac7990b5de353f1fa52d5b5d3457992","observation_id":"531aab0e-fd74-486c-ae81-05970cdebae0","resolution":{"observed_at":"2026-08-14T04:32:37.461972Z","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":"2026-08-14T04:32:37.469809Z","title":"C., Gordon , K","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.469809Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:436e80ccae9ae9b3e746e7e730c7599d068bee36863e7f11254e85a8b3ec747a","observation_id":"69aeaafe-bcc8-49d4-a82c-d6edeac0a4f4","resolution":{"observed_at":"2026-08-14T04:32:37.469809Z","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":"2026-08-14T04:32:37.504764Z","title":"C., Krick , J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.504764Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:9ccda4985e65d756a1685201f1001cb0fef95f7ea2f7f1bbf3dfa2ed928f91e1","observation_id":"3e257b2e-d154-49df-b6f3-33a0bc4b7952","resolution":{"observed_at":"2026-08-14T04:32:37.504764Z","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":"2026-08-14T04:32:37.551667Z","title":"L., Anderson , J., Gennaro , M., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.551667Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:ff3fbcbd5c8f31692be5a989b77be8fc361da9c3b651567202219c831f6ec3f7","observation_id":"089e977e-bad6-48b3-bb53-19a4cea5a9f1","resolution":{"observed_at":"2026-08-14T04:32:37.551667Z","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":"2026-08-14T04:32:37.569063Z","title":"P., Mather , J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.569063Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:f92f99ad7329e7a9b18851cfe55f82609641f5992305d32129ca970f56234ade","observation_id":"3cccbd63-5b8c-4377-bdbf-113ffac1f177","resolution":{"observed_at":"2026-08-14T04:32:37.569063Z","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":"2026-08-14T04:32:37.573817Z","title":"H., Leisenring , J., Kammerer , J., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.573817Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:13668808e0a6016a141307721bb06edb828150786493d8afe29895f5f1b62cc8","observation_id":"00fc0884-a866-4618-ab76-36d16e8b4ddf","resolution":{"observed_at":"2026-08-14T04:32:37.573817Z","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":"2026-08-14T04:32:37.579790Z","title":"D., Bohlin , R., Sloan , G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.579790Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:734ce4f7f772f884d1b760b0edfa9f95b8ef82c76be2838e3a51aa7da84cfe3a","observation_id":"d05fbbf7-067b-40ef-9dcf-c6c86f99bbc9","resolution":{"observed_at":"2026-08-14T04:32:37.579790Z","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":"2026-08-14T04:32:37.584386Z","title":"D., Sloan , G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.584386Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:2be5b68ef867fabb32e64b2e4ecde95f46db731a767d068600bea9db597f8dee","observation_id":"2aefff7e-7281-4aa4-ac2e-27b519f5e802","resolution":{"observed_at":"2026-08-14T04:32:37.584386Z","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":"2026-08-14T04:32:37.589678Z","title":"Z., Llop-Sayson , J., Lew , B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.589678Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:6340b67a8ef35c6ad202b80412743c447807324c25415117f00232c5fd5aa71f","observation_id":"f670469e-9b25-44e5-9e61-2c499b0d8b5e","resolution":{"observed_at":"2026-08-14T04:32:37.589678Z","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":"2026-08-14T04:32:39.208163Z","title":"2016--2026, title JWST User Documentation (JDox)","venue":null,"work_id":"1dcee40a-0933-457d-948b-a853181b1a82","year":2016},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.594461Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:c30069f669c835c86b3463d19630ba9d35567ac7b9d3c97b97d16e00ab21bf0c","observation_id":"2ac32244-79ba-4feb-a778-51f91ccc3cbb","resolution":{"observed_at":"2026-08-14T04:32:39.212372Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:37.605678Z","title":"2011, title Scikit-learn: Machine Learning in P ython, Journal of Machine Learning Research, 12, 2825","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.605678Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:5cd0f9c5165101be165bcd024a963af913fcd066f434151799b851a2e4540777","observation_id":"b3b2bec4-4cc9-491f-abe2-44778bda343f","resolution":{"observed_at":"2026-08-14T04:32:37.605678Z","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":"2026-08-14T04:32:37.629685Z","title":"H., Su , K., Sloan , G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.629685Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:6b7ab32165981be7a7d203817b21d059b0335fac49f0a7ce15a33b48b51a293d","observation_id":"1bcecbf6-e35b-4cc4-a711-0df32bed860e","resolution":{"observed_at":"2026-08-14T04:32:37.629685Z","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":"2026-08-14T04:32:37.667248Z","title":"J., Kelly , D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.667248Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:1d6f75d3474d2d9aacf7e66a9b08b685e96b0789d2713cbdb8625d1fa6875203","observation_id":"afa85b91-82a8-4c33-8f68-00a156dcf565","resolution":{"observed_at":"2026-08-14T04:32:37.667248Z","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":"2026-08-14T04:32:37.671039Z","title":"2023, title The Science Performance of JWST as Characterized in Commissioning , , 135, 048001, 10.1088/1538-3873/acb293","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.671039Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:d24bfcfc6929fd8b77cc954928bd5a752bc1153425c2db2d10145654cc53d197","observation_id":"a32d3829-93d1-41d7-8864-a57266d487b2","resolution":{"observed_at":"2026-08-14T04:32:37.671039Z","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":"2026-08-14T04:32:39.187950Z","title":"2018, title synphot: Synthetic photometry using Astropy , , Astrophysics Source Code Library, record ascl:1811.001 1811.001","venue":null,"work_id":"243a9a47-9c90-4367-b149-74d1953dca08","year":2018},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.675028Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:34e0d332af0023075d60ab1164fe47fe438b2cb703527eee024549cd28d98ca4","observation_id":"0e4b98ef-9951-4aa8-b965-38f04e1da74b","resolution":{"observed_at":"2026-08-14T04:32:39.192467Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.176059Z","title":"2024, title Improved NIRCam Flat Field Reference Files for Cycle 1 , , Tech","venue":null,"work_id":"2ebb73f3-b09f-4411-b3d0-a2ce11282580","year":2024},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.683429Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:0708b08237efc98d28cd693e0cc3044fcd4241525278fd209d6f7220e7f7f2ff","observation_id":"ecb16f68-87bc-4459-8a11-c1ddb1276b80","resolution":{"observed_at":"2026-08-14T04:32:39.180237Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.163544Z","title":"2022, title NIRCam Commissioning Results NRC-10-Flat Fields, Scattered Light, and Backgrounds , , Tech","venue":null,"work_id":"51bd99bc-4428-47f1-ad32-8220441dd988","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.688118Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:8a1f570c13ca41f89444738647a75f6e31eeeb664435be6cdb814947ad22caeb","observation_id":"62f49b16-a4ee-4776-a723-172665c116e2","resolution":{"observed_at":"2026-08-14T04:32:39.167966Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:37.692407Z","title":"E., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.692407Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:b55b10eac38579c1b0b4d3022dc811226c4a32956243a4b7c1cbde32e1da9197","observation_id":"f3f75082-27b6-4f62-b55f-0861a769c29f","resolution":{"observed_at":"2026-08-14T04:32:37.692407Z","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":"2026-08-14T04:32:39.150588Z","title":"Baltimore, MD: Space Telescope Science Institute","venue":null,"work_id":"be3c2223-29b0-4bc0-b912-d02a557261ea","year":2016},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.702370Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:0e2abda117a5938901cb0ddcdd9c3e8c3d155da974a62d439ce3d26698eb4186","observation_id":"2f44b90c-2641-42c2-b406-5152c13219fd","resolution":{"observed_at":"2026-08-14T04:32:39.154630Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.137627Z","title":null,"venue":null,"work_id":"2fed43d4-9418-4436-8a84-1265004b77d4","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.734751Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:36517c5b2b623858b75e1645a5da242fdc60d5165c697a34be9422065a9e6c8b","observation_id":"b4c4722c-0fa3-424b-816b-50710beceb87","resolution":{"observed_at":"2026-08-14T04:32:39.141534Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.08322","last_updated":"2022-05-17T13:18:56Z","snapshot_observed_at":"2026-08-13T15:42:41.806117Z","submitted_at":"2022-05-17T13:18:56Z","title":"How do Spitzer IRAC Fluxes Compare to HST CALSPEC","version":1},"cited_work":{"arxiv_id":"2205.08322","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.08322","snapshot_observed_at":"2026-08-14T04:32:39.035330Z","title":"How do Spitzer IRAC Fluxes Compare to HST CALSPEC","venue":"astro-ph.IM","work_id":"7ddf9666-1000-4bd1-baa2-84880162a719","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.758080Z"},"links":{"cited_paper":"/paper/2205.08322","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:73f1e2dc289462ea4a5d51d2b77c5e425b77636c590ca3381d69fa0711f7377d","observation_id":"00c81c68-dbc1-4179-8d03-d381c44aaecf","resolution":{"observed_at":"2026-08-14T04:32:39.039525Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.124151Z","title":"American Astronomical Society Meeting \\#240 , year = 2022, series =","venue":null,"work_id":"147f5595-4095-41e5-a1c5-02c6c0bfd40c","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.765182Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:482868c8212558594da24de853f595c916c29553225c280f743ac31f56d2b682","observation_id":"964055a6-efed-48ef-b8f8-b28af586b1d9","resolution":{"observed_at":"2026-08-14T04:32:39.128310Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1117/12.2633474","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:38.601309Z","title":"Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave , year = 2022, editor =","venue":null,"work_id":"0f902ef4-243b-4dc4-b45f-91445a5165a2","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.770690Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:f6942f07c67d96c0361a3899737a25674bffa08d2dfd74cceff5b901b32e4c52","observation_id":"8d2d4ee5-9d15-45cc-844a-4ace9145ec22","resolution":{"observed_at":"2026-08-14T04:32:38.606065Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.12069","last_updated":"2022-12-22T22:59:59Z","snapshot_observed_at":"2026-08-13T13:15:30.564986Z","submitted_at":"2022-12-22T22:59:59Z","title":"NIRCam Performance on JWST In Flight","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.12069","snapshot_observed_at":"2026-08-14T04:32:37.780607Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.780607Z"},"links":{"cited_paper":"/paper/2212.12069","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:848f3313f1e18c522d467cd24471443de5af28f9705b8c0c995be80e4f357694","observation_id":"a7ae8579-2d34-43d0-8a81-b00e014c8e5b","resolution":{"observed_at":"2026-08-14T04:32:37.780607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05632","last_updated":"2023-04-10T23:18:31Z","snapshot_observed_at":"2026-08-13T15:05:35.590297Z","submitted_at":"2022-07-12T16:00:57Z","title":"The Science Performance of JWST as Characterized in Commissioning","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05632","snapshot_observed_at":"2026-08-14T04:32:37.785664Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.785664Z"},"links":{"cited_paper":"/paper/2207.05632","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:d00aeb3a9b9677be37b688937152a4adb85dedf48275382f6589896a2da3f2fc","observation_id":"ee932617-875c-4329-a3ee-c4e58edb55b5","resolution":{"observed_at":"2026-08-14T04:32:37.785664Z","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":"2026-08-14T04:32:37.827260Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.827260Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:268bd638cdaad3b1b112bc81f4e2e029bc132ad47bfa6fc6446b2236b7625deb","observation_id":"8e3c6952-5224-4df9-a0a2-ec35e7b23aaf","resolution":{"observed_at":"2026-08-14T04:32:37.827260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.48550/arxiv.2602.13918","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:38.390509Z","title":null,"venue":null,"work_id":"3a8b7d27-ac2e-437b-930f-1da14ab3c2b5","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.846123Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:f9de31a56e08c088c135725f7f32313d0c20da26236b881789db18a162193319","observation_id":"c7c0935d-b0c7-44ea-9fc7-3eef1c86a9a3","resolution":{"observed_at":"2026-08-14T04:32:38.395553Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-3881/adea77","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:38.267632Z","title":null,"venue":null,"work_id":"59a33949-1d2e-489e-8c3e-fdea631bbf06","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.857701Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:02b2d275d66760acf1337cf4ecf5ff1adf6256e54f661ed19da64bfc8e4bea5e","observation_id":"d70ab6fb-0f5a-4b02-b136-415891e3e33b","resolution":{"observed_at":"2026-08-14T04:32:38.273682Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.112216Z","title":null,"venue":null,"work_id":"58dff50a-4360-4911-aec0-27fc7befd92e","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.870357Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:86a1f41b843e75254c07e9f1a544c71cf8d5e9413601b00514bcbe69c0c7e390","observation_id":"14666454-d365-406a-9768-1f929f64987c","resolution":{"observed_at":"2026-08-14T04:32:39.115962Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:37.880234Z","title":"doi:10.5281/zenodo.8436689 , version =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.880234Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:d94e050d62a1c88ad5d493eba848f1926f1eb198feffe156ab020cab75e2eb58","observation_id":"9352f378-e0fb-4da7-90c6-84a7688dc6c4","resolution":{"observed_at":"2026-08-14T04:32:37.880234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.21677181","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:38.496965Z","title":"doi:10.5281/zenodo.21677181 , version =","venue":null,"work_id":"2dc51a8b-25db-4078-a6a3-755cb37357df","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.888003Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:622feb368c7303e945f38987db6ba91cf91507e32271cb9bb4cce31f66cbe1e9","observation_id":"98207428-4284-4688-9ea1-04583a2cf280","resolution":{"observed_at":"2026-08-14T04:32:38.502625Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.11455","last_updated":"2023-01-26T23:00:23Z","snapshot_observed_at":"2026-08-13T12:56:47.619019Z","submitted_at":"2023-01-26T23:00:23Z","title":"First Observations of the Brown Dwarf HD 19467 B with JWST","version":1},"cited_work":{"arxiv_id":"2301.11455","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.11455","snapshot_observed_at":"2026-08-14T04:32:38.939707Z","title":"First Observations of the Brown Dwarf HD 19467 B with JWST","venue":"astro-ph.SR","work_id":"970f4302-3d78-45a2-a8e2-ee15d9af1fd9","year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.915331Z"},"links":{"cited_paper":"/paper/2301.11455","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:ecc9ab4aefdb1201af501a731fe8e21473e3c5184d0591b6fc724b26053b68b6","observation_id":"c0e0e5f7-f4d3-4d2b-a450-8f269ddb5222","resolution":{"observed_at":"2026-08-14T04:32:38.944080Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.13608","last_updated":"2025-04-07T14:45:26Z","snapshot_observed_at":"2026-08-07T16:56:56.553540Z","submitted_at":"2025-03-17T18:00:48Z","title":"JWST-TST High Contrast: Living on the Wedge, or, NIRCam Bar Coronagraphy Reveals CO$_2$ in the HR 8799 and 51 Eri Exoplanets' Atmospheres","version":2},"cited_work":{"arxiv_id":"2503.13608","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.13608","snapshot_observed_at":"2026-08-14T04:32:38.921448Z","title":"JWST-TST High Contrast: Living on the Wedge, or, NIRCam Bar Coronagraphy Reveals CO$_2$ in the HR 8799 and 51 Eri Exoplanets' Atmospheres","venue":"astro-ph.EP","work_id":"52b25a79-d6bd-4f98-baad-ae565ff8ae9f","year":2025},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.929724Z"},"links":{"cited_paper":"/paper/2503.13608","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:0d2aa53a4297082a72cfe149a6f11300f51b9fed478d79f65fa03dce58564dcb","observation_id":"135a424a-2f0c-4c30-80f6-503b09f8a39b","resolution":{"observed_at":"2026-08-14T04:32:38.926775Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.03348","last_updated":"2022-09-06T22:33:04Z","snapshot_observed_at":"2026-08-13T14:31:59.538761Z","submitted_at":"2022-09-06T22:33:04Z","title":"The JWST Resolved Stellar Populations Early Release Science Program I.: NIRCam Flux Calibration","version":1},"cited_work":{"arxiv_id":"2209.03348","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.03348","snapshot_observed_at":"2026-08-14T04:32:38.901754Z","title":"The JWST Resolved Stellar Populations Early Release Science Program I.: NIRCam Flux Calibration","venue":"astro-ph.IM","work_id":"1520ce09-f817-4d3c-8044-f3dae4065b69","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.954755Z"},"links":{"cited_paper":"/paper/2209.03348","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:9ccf694b23e40a4778c95724f08f185d0cbd3657c67dfce9d3c469096ee50658","observation_id":"981c029b-1559-4f8c-a5e4-d9d3f40ba1b6","resolution":{"observed_at":"2026-08-14T04:32:38.906678Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07563","last_updated":"2023-05-16T16:01:34Z","snapshot_observed_at":"2026-08-13T11:43:40.386865Z","submitted_at":"2023-05-12T15:40:53Z","title":"All-Sky Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories: The Complete Sample","version":2},"cited_work":{"arxiv_id":"2305.07563","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.07563","snapshot_observed_at":"2026-08-14T04:32:38.882897Z","title":"All-Sky Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories: The Complete Sample","venue":"astro-ph.SR","work_id":"9c6e768d-f0c4-4c99-b958-2984fd20a90b","year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.974831Z"},"links":{"cited_paper":"/paper/2305.07563","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:fc3672e8e404567429468cd8f2280dd13040643c5d9f6c4577827903702a6299","observation_id":"35415095-416e-4cb4-9b8b-9ab30ec46c84","resolution":{"observed_at":"2026-08-14T04:32:38.887586Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.10443","last_updated":"2024-11-27T20:31:48Z","snapshot_observed_at":"2026-08-12T22:43:53.874774Z","submitted_at":"2024-09-16T16:24:36Z","title":"The James Webb Space Telescope Absolute Flux Calibration. II. Mid-Infrared Instrument Imaging and Coronagraphy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.10443","snapshot_observed_at":"2026-08-14T04:32:37.987526Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.987526Z"},"links":{"cited_paper":"/paper/2409.10443","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:a20674ed3133a85587774d83b8caeb1dd91d40b4014e4e6e821661010ecd97fe","observation_id":"8a68b240-c07e-4fac-a52a-254dcc00d03c","resolution":{"observed_at":"2026-08-14T04:32:37.987526Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.10444","last_updated":"2021-11-19T21:35:38Z","snapshot_observed_at":"2026-08-13T11:05:21.377196Z","submitted_at":"2021-11-19T21:35:38Z","title":"Infrared Absolute Calibration I: Comparison of Sirius with Fainter Calibration Stars","version":1},"cited_work":{"arxiv_id":"2111.10444","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.10444","snapshot_observed_at":"2026-08-14T04:32:38.853111Z","title":"Infrared Absolute Calibration I: Comparison of Sirius with Fainter Calibration Stars","venue":"astro-ph.SR","work_id":"341f9b49-522a-4f6a-a300-9aa9a5b54c3f","year":2021},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:37.991932Z"},"links":{"cited_paper":"/paper/2111.10444","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:b1b7497c491f0433477171fe19e64e81a9576ec5837b7e856fad628cb62cce4a","observation_id":"48a27f81-64fd-4b2f-89dc-af190080e42f","resolution":{"observed_at":"2026-08-14T04:32:38.857876Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.02202","last_updated":"2018-03-21T12:54:04Z","snapshot_observed_at":"2026-08-07T17:09:18.796814Z","submitted_at":"2017-07-07T14:47:07Z","title":"Pandeia: A Multi-mission Exposure Time Calculator for JWST and WFIRST","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.02202","snapshot_observed_at":"2026-08-14T04:32:38.004749Z","title":"Observatory Operations: Strategies, Processes, and Systems VI , year = 2016, editor =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.004749Z"},"links":{"cited_paper":"/paper/1707.02202","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:1506411a130499d6ab11e391476f9b32ff9acfbabe78e2a9a1aad81bcee61498","observation_id":"0f88c44b-1693-4c59-a122-cbf561a1f24d","resolution":{"observed_at":"2026-08-14T04:32:38.004749Z","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":"2026-08-14T04:32:39.100097Z","title":null,"venue":null,"work_id":"a68008ac-6240-4b95-95f4-5721c310cda7","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.027313Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:2dc800e243a63f601f39592a0dcf539f6bb34beed4278e65b606462da68bba32","observation_id":"5f4aa80f-6ea4-41b7-8615-922d215d02a3","resolution":{"observed_at":"2026-08-14T04:32:39.103928Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.1707","last_updated":"2014-06-06T15:27:56Z","snapshot_observed_at":"2026-07-06T03:45:40.711413Z","submitted_at":"2014-06-06T15:27:56Z","title":"Techniques and Review of Absolute Flux Calibration from the Ultraviolet to the Mid-Infrared","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.1707","snapshot_observed_at":"2026-08-14T04:32:38.051542Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.051542Z"},"links":{"cited_paper":"/paper/1406.1707","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:68b7f2206be8dfd6ab6fc9f8ad73d51720cd830a3e63832fce4a9a5a851f752d","observation_id":"523fa73c-971e-495b-8de1-0577ee0cd778","resolution":{"observed_at":"2026-08-14T04:32:38.051542Z","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":"2026-08-14T04:32:38.061814Z","title":"Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave , year = 2014, editor =","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.061814Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:686f1802c375ae3ab1605520ffacc5c1739fc0ab38b6875ee5f7e5043c393287","observation_id":"2e0280c5-ad90-4e43-822f-60ba0ef2ebbd","resolution":{"observed_at":"2026-08-14T04:32:38.061814Z","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":"2026-08-14T04:32:38.066903Z","title":"astropy/photutils: 1.8.0 , month = may, year = 2023, publisher =","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.066903Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:0d5bf1ad7286bf1d609bcf59a5a27550df40b8f4d919098e46fdf56450d1d5fb","observation_id":"d6d082f0-1605-4141-b849-4c151f5d14ac","resolution":{"observed_at":"2026-08-14T04:32:38.066903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06500","last_updated":"2022-04-13T16:35:27Z","snapshot_observed_at":"2026-08-13T16:02:52.737547Z","submitted_at":"2022-04-13T16:35:27Z","title":"The James Webb Space Telescope Absolute Flux Calibration. I. Program Design and Calibrator Stars","version":1},"cited_work":{"arxiv_id":"2204.06500","doi":null,"metadata_source":"pith","pith_arxiv_id":"2204.06500","snapshot_observed_at":"2026-08-14T04:32:38.802868Z","title":"The James Webb Space Telescope Absolute Flux Calibration. I. Program Design and Calibrator Stars","venue":"astro-ph.IM","work_id":"dc8f3c53-9dda-462a-a2c5-0223d95fca4c","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.071571Z"},"links":{"cited_paper":"/paper/2204.06500","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:384b7fa804c1376acc4ebbbb537c49dec9cba531e17fd8b772ccbeb288ec75e7","observation_id":"2f1743bb-7bdb-4bc0-9085-ccccbaf8d7e8","resolution":{"observed_at":"2026-08-14T04:32:38.807752Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:38.076565Z","title":"and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.076565Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:c7ec34f6cf52776c11386f979851245b28f44ddea1f57703b265cc2d06adfaf8","observation_id":"536be0d7-3a38-41b2-b923-8f8c41fb0362","resolution":{"observed_at":"2026-08-14T04:32:38.076565Z","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":"2026-08-14T04:32:38.081645Z","title":"doi:10.5281/zenodo.6672538 , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.081645Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:9dfeae8aef29eb6e02cd5a5ba593ccbe910705ba1d5ceedfedbc77564c6ef8da","observation_id":"89384a04-58a8-4021-b15c-d266b0ea5771","resolution":{"observed_at":"2026-08-14T04:32:38.081645Z","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":"2026-08-14T04:32:39.080650Z","title":null,"venue":null,"work_id":"dfdd318e-1655-4ac8-a68d-0d91e65e09d5","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.089440Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:9a302a8c811c02026ae2dedad919645975538e394212b5b2f06a0f73047e75ea","observation_id":"901137f7-af5c-42c6-8030-02596ad3c95f","resolution":{"observed_at":"2026-08-14T04:32:39.084124Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.08380","last_updated":"2018-06-21T18:14:55Z","snapshot_observed_at":"2026-07-06T06:46:08.396066Z","submitted_at":"2018-06-21T18:14:55Z","title":"The initial mass function in the Coma Berenices dwarf galaxy from deep near-infrared HST observations","version":1},"cited_work":{"arxiv_id":"1806.08380","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.08380","snapshot_observed_at":"2026-08-14T04:32:38.782372Z","title":"The initial mass function in the Coma Berenices dwarf galaxy from deep near-infrared HST observations","venue":"astro-ph.GA","work_id":"75c27205-08d6-478a-b495-9b1ff6e03805","year":2018},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.095337Z"},"links":{"cited_paper":"/paper/1806.08380","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:e8898ef1c38fe4a36febbde65729d18d5f0729d9fd70879f516d6fc72f1524e9","observation_id":"a089efa8-3cb0-4904-a648-557592c118da","resolution":{"observed_at":"2026-08-14T04:32:38.787516Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:39.067998Z","title":null,"venue":null,"work_id":"0abd619c-9cd8-4b34-90b7-54721c75d3b2","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.101043Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:acac683e99bf6995e488ec7ff667f64471c6fc56186ce3ebda280ae3d9df9917","observation_id":"a87d8037-4a12-4c65-a740-ca32799c1ee3","resolution":{"observed_at":"2026-08-14T04:32:39.071878Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:32:38.109216Z","title":"Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave , year = 2012, editor =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.109216Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:81652f8529bbd5fcdf9316caaa1ab49786d7c2ac46d515d5280b5d5ff669dd9d","observation_id":"86f7fa38-becc-493c-9990-1c577d3725ba","resolution":{"observed_at":"2026-08-14T04:32:38.109216Z","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":"2026-08-14T04:32:38.122140Z","title":"Cryogenic Optical Systems and Instruments XI , year = 2005, editor =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.122140Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:b2d2c9ec0534f6832ff51875a823e888aa9139041cee066434f78b94c8ceba22","observation_id":"269f6538-ec66-419c-9a37-63b803741582","resolution":{"observed_at":"2026-08-14T04:32:38.122140Z","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":"2026-08-14T04:32:39.055487Z","title":null,"venue":null,"work_id":"9fca7976-1a8e-4a28-aa9a-93fe99214fa8","year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.141785Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:21f8777497a5575d2adf46672bca043e55f46a2397c303dc3c073006455e1411","observation_id":"8bb2d633-89cf-49a0-bf1e-1d43324cc6b1","resolution":{"observed_at":"2026-08-14T04:32:39.059988Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1307.6212","last_updated":"2013-07-23T20:00:01Z","snapshot_observed_at":"2026-08-05T05:45:26.588200Z","submitted_at":"2013-07-23T20:00:01Z","title":"Astropy: A Community Python Package for Astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.6212","snapshot_observed_at":"2026-08-14T04:32:38.149487Z","title":"arXiv , Author =:1307.6212 , Journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.149487Z"},"links":{"cited_paper":"/paper/1307.6212","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:2fa5a1a8773ef18b21987c38a9b3443c5512a505aaac40f37a73aad6e59aa5b9","observation_id":"30dbfe7f-a887-46a8-9cef-90263c7b7d43","resolution":{"observed_at":"2026-08-14T04:32:38.149487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.02634","last_updated":"2018-01-16T15:05:07Z","snapshot_observed_at":"2026-07-06T06:17:44.962713Z","submitted_at":"2018-01-08T19:00:08Z","title":"The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.02634","snapshot_observed_at":"2026-08-14T04:32:38.156156Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.156156Z"},"links":{"cited_paper":"/paper/1801.02634","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:befc0390c75be09a4517cf9e92539a69e08ff982f22e7fac27a1dc55455a791a","observation_id":"b2cf8bc8-ea8d-4b92-ab4e-b5f390cd901e","resolution":{"observed_at":"2026-08-14T04:32:38.156156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14220","last_updated":"2022-06-28T18:01:54Z","snapshot_observed_at":"2026-07-06T13:25:39.576741Z","submitted_at":"2022-06-28T18:01:54Z","title":"The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.14220","snapshot_observed_at":"2026-08-14T04:32:38.162902Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.162902Z"},"links":{"cited_paper":"/paper/2206.14220","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:4f7fd05aa03d80fb081ce59a310bd5444fd24fc5329e320694a64d4993e78e7e","observation_id":"14bf67cb-8176-4ddf-86b4-9f69eca3e722","resolution":{"observed_at":"2026-08-14T04:32:38.162902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506672","last_updated":"2005-06-28T18:07:29Z","snapshot_observed_at":"2026-07-07T00:51:43.193510Z","submitted_at":"2005-06-28T18:07:29Z","title":"Stellar Cluster Fiducial Sequences with the Advanced Camera for Surveys","version":1},"cited_work":{"arxiv_id":"astro-ph/0506672","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506672","snapshot_observed_at":"2026-08-14T04:32:38.697938Z","title":"Stellar Cluster Fiducial Sequences with the Advanced Camera for Surveys","venue":"astro-ph","work_id":"7e9b3d00-fddd-448d-9935-ba4a4aa34de1","year":2005},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.170581Z"},"links":{"cited_paper":"/paper/astro-ph/0506672","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:2a3d697321c40bd6c7dda0e37a528871afa978465d4bced267932da14771953a","observation_id":"19a4ec88-615e-4b63-95a4-5f444f5e1dca","resolution":{"observed_at":"2026-08-14T04:32:38.703205Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.10655","last_updated":"2018-08-06T12:18:46Z","snapshot_observed_at":"2026-07-06T06:52:45.821495Z","submitted_at":"2018-07-27T14:34:43Z","title":"Pristine Dwarf-Galaxy Survey I: A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.10655","snapshot_observed_at":"2026-08-14T04:32:38.174553Z","title":"A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.174553Z"},"links":{"cited_paper":"/paper/1807.10655","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:2e41f22c3c5a4e428acbb95bdad677c757ff2d0c8445923a74390d2c2946409c","observation_id":"06eac1ae-2fbd-40fb-9a38-68402cdf594d","resolution":{"observed_at":"2026-08-14T04:32:38.174553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09526","last_updated":"2021-05-21T00:23:22Z","snapshot_observed_at":"2026-08-13T19:19:36.828749Z","submitted_at":"2021-05-20T05:36:05Z","title":"Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST and literature data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.09526","snapshot_observed_at":"2026-08-14T04:32:38.181916Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.181916Z"},"links":{"cited_paper":"/paper/2105.09526","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:8c4658f618e5b0327d347d137dda2f3045c4895a79350c7ec580901ffa51802a","observation_id":"b9383794-9421-4823-9fb9-8c329cdbf2f7","resolution":{"observed_at":"2026-08-14T04:32:38.181916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0910.0675","last_updated":"2009-10-05T05:11:00Z","snapshot_observed_at":"2026-08-10T09:08:02.981801Z","submitted_at":"2009-10-05T05:11:00Z","title":"Intrinsic iron spread and a new metallicity scale for Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0910.0675","snapshot_observed_at":"2026-08-14T04:32:38.188661Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.188661Z"},"links":{"cited_paper":"/paper/0910.0675","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:91ffd81bbe948408bd50e140e370c8fae351198020bd551de058861754e15e26","observation_id":"7ca4f130-9ba8-4e9c-bc84-1295f17e4967","resolution":{"observed_at":"2026-08-14T04:32:38.188661Z","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":"2026-08-14T04:32:38.198675Z","title":"and Varoquaux, G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.198675Z"},"links":{"citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:4e05358d8bc4c97a971eb504b6811d44ee3da534687309333f4209ddc56f9d1e","observation_id":"4afc4c69-7149-4da1-bc57-17ea5ebfaad8","resolution":{"observed_at":"2026-08-14T04:32:38.198675Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00998","last_updated":"2022-08-31T16:21:38Z","snapshot_observed_at":"2026-08-13T14:53:02.651034Z","submitted_at":"2022-08-01T17:14:29Z","title":"JWST/NIRCam Coronagraphy: Commissioning and First On-Sky Results","version":6},"cited_work":{"arxiv_id":"2208.00998","doi":null,"metadata_source":"pith","pith_arxiv_id":"2208.00998","snapshot_observed_at":"2026-08-14T04:32:38.618908Z","title":"JWST/NIRCam Coronagraphy: Commissioning and First On-Sky Results","venue":"astro-ph.IM","work_id":"d1b97ad6-927e-4f37-a028-245616bf98ec","year":2022},"citing_paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-14T04:32:38.205893Z"},"links":{"cited_paper":"/paper/2208.00998","citing_paper":"/paper/2608.08717"},"observation_digest":"sha256:34fb45562a557eaa592822019b516f49cdba1b210efae202d2a379348a88979a","observation_id":"17ef6399-1c10-4cb3-9c20-c358ff763a2f","resolution":{"observed_at":"2026-08-14T04:32:38.624367Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.08717","last_updated":"2026-08-09T14:00:02Z","latest_version":1,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-08-14T04:23:51.060163Z","submitted_at":"2026-08-09T14:00:02Z","title":"The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy"},"reference_resolution":{"displayed":66,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":44,"verified_exact":13,"verified_fuzzy":8},"total_outbound_references":66},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 66 of 66 outbound references and 0 inbound Pith citation observations for arXiv:2608.08717."}