{"as_of":"2026-08-16T15:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4d47b0743505ebc5f4475018501cf4922396fdcdfb0fdc8a70bfee5a4fdeb9dd","coverage":[{"denominator":15,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":15,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T15:34:26.153763Z","state":"measured"},{"denominator":15,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":15,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+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/1908.02142/citation-record","integrity":"/paper/1908.02142/integrity","json":"/paper/1908.02142/citation-record.json","paper":"/paper/1908.02142"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.380808Z","title":"Band limited data reconstruction in modulated polarimeters,","venue":null,"work_id":"08792ef7-8f20-4764-983b-cd405e62a16a","year":2011},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.094958Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:53e73a61319a42e386db0f97ff2efcc5faf1d0b4baee0d3fa62ac8d5806c7608","observation_id":"c845a536-659b-410b-a747-72e619917f1c","resolution":{"observed_at":"2026-08-14T15:34:26.385090Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.367836Z","title":"Stokes-vector and Mueller-matrix polarimetry,","venue":null,"work_id":"00d375c2-b621-48f5-b8bb-8b80addd235f","year":2016},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.099605Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:9c106afdd573f44f6b8e4dfce0c7284bb004d00bade1b5f966f2e1a9c6f3f858","observation_id":"11a44e81-9d50-4e85-88a6-235d6151f6c1","resolution":{"observed_at":"2026-08-14T15:34:26.372564Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.355339Z","title":"Collett, Polarized Light: Fundamentals and Applications (Marcel Dekker, New York, 1993)","venue":null,"work_id":"f466433f-ecba-4a75-96ca-dda92a9eb4bb","year":1993},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.103631Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:be592aa9ab932e8fa85c600be5c2ab36e667c51e523f9261726a23c760e1b5f4","observation_id":"b91e6bbc-4fe0-4308-b18b-8e00f334eb3e","resolution":{"observed_at":"2026-08-14T15:34:26.359673Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.342402Z","title":"Single-shot spatially modulated Stokes polarimeter based on a GRIN lens,","venue":null,"work_id":"f4185af9-d1f8-47f4-a25f-03601b85fc9c","year":2014},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.107324Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:bd430a8d91888fa3dd60a848042b0cf4b44a41e264665eb2b892d34aa12b7d14","observation_id":"1602d878-fd10-4260-bc32-20a301e763a2","resolution":{"observed_at":"2026-08-14T15:34:26.346819Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.329670Z","title":"Chapter 22: Polarimetry,","venue":null,"work_id":"38825266-3412-4991-a91e-c9651364cd4e","year":1995},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.111261Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:30e7575d4e98713e645bbec375d1f02581d23402b14511e1238d2e31c8626de0","observation_id":"5894c485-36d8-4227-8a0f-2b19e98e5083","resolution":{"observed_at":"2026-08-14T15:34:26.333685Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.316509Z","title":"Star test polarimetry using stress-engineered optical elements,","venue":null,"work_id":"cf512843-8272-491b-85a1-5754bfdcd699","year":2012},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.115157Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:c3219eb5fe741ad5b5e22e25c49e3310a8b5b12565aee0574f92a527a13f531c","observation_id":"8c9c568b-c919-4a0c-9bf8-a84f27c5e536","resolution":{"observed_at":"2026-08-14T15:34:26.320806Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.303317Z","title":"Imaging the polarization of a light field,","venue":null,"work_id":"17611613-f455-43c3-8b80-45706a7d1707","year":2013},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.119999Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:cba44fdd3c8b7bc592c303cbb8d039f398f4aa73a623ae66eb1089a61d2eef04","observation_id":"cd0cab22-dd5e-4d04-a682-5c8ffe1704bf","resolution":{"observed_at":"2026-08-14T15:34:26.307495Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.290701Z","title":"Single-shotpolarimetry imaging of multicore fiber,","venue":null,"work_id":"8e53cdf3-0885-4d01-b328-27fa2bd871f0","year":2016},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.124464Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:c17e5baedc35f2c3c30137dc5f1d4dd91f08f06bb457244bd3ddc26fba6dbd84","observation_id":"a477c2ca-d7b3-4611-9e4a-4016f178781d","resolution":{"observed_at":"2026-08-14T15:34:26.294554Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.05828","last_updated":"2020-09-06T17:49:32Z","snapshot_observed_at":"2026-08-14T16:06:21.222747Z","submitted_at":"2019-07-12T16:34:57Z","title":"Birefringent Fourier filtering for single molecule Coordinate and Height super-resolution Imaging with Dithering and Orientation","version":3},"cited_work":{"arxiv_id":"1907.05828","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.05828","snapshot_observed_at":"2026-08-14T15:34:26.208541Z","title":"Birefringent Fourier filtering for single molecule Coordinate and Height super-resolution Imaging with Dithering and Orientation","venue":"physics.optics","work_id":"ae9575dc-e706-468b-aaf2-1365f5ebe7df","year":2019},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.128535Z"},"links":{"cited_paper":"/paper/1907.05828","citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:610996a0623cea803b133ddccd690711e6d168dcff82235832c7a6bea5a5b374","observation_id":"767e191b-a3f4-4e79-bf5a-7c0e8472529e","resolution":{"observed_at":"2026-08-14T15:34:26.213510Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.278372Z","title":"Pinhole array implementation of star test polarimetry,","venue":null,"work_id":"afdbe7a3-9e84-40c8-aa0d-5b5ece60d8b9","year":2014},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.133281Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:6e3aa20a9be2e731a90a9e1be3c3ce1a7dd14f61ac935a65f293d935b1bcbaef","observation_id":"3d6830f0-f6b5-48b1-b2cf-bc6ad159cfef","resolution":{"observed_at":"2026-08-14T15:34:26.282235Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.264946Z","title":"Star test image-sampling polarimeter,","venue":null,"work_id":"2f227dff-628b-4ee5-991b-0ab961e19794","year":2016},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.137474Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:ad38e411ba0a11d38a62668526ab8a1b0c59c79948ac0acdead2d9588681659b","observation_id":"fd6c3ff3-eaad-4117-aec8-f17729953ad6","resolution":{"observed_at":"2026-08-14T15:34:26.269481Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.251452Z","title":"Poincaré sphere representation for spatially varying birefringence,","venue":null,"work_id":"2493e29c-7617-4cb9-8b28-689af31e55e2","year":2018},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.141594Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:a773626a63d74d699ddd43d2edaf629ecf0901bbc0faf2cde43db1dedaaa072a","observation_id":"872530a9-f6ed-43a4-ba9e-0a2ac9add803","resolution":{"observed_at":"2026-08-14T15:34:26.255811Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.238083Z","title":"Description and applications of space-variant polarization states and elements,","venue":null,"work_id":"447b4528-fb3e-4ee1-be62-f691b354c7b5","year":2018},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.145826Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:14aa13ebef703c625d4b35c9df93f81a5f81ba88a484559b0cc83b9711f024ad","observation_id":"022d7351-83b1-4540-be63-c86610de0d93","resolution":{"observed_at":"2026-08-14T15:34:26.242588Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:34:26.223498Z","title":"Review of passive imaging polarimetry for remote sensing applications,","venue":null,"work_id":"64c09c9c-9672-4da8-ba56-579fb6f7886e","year":2006},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.149797Z"},"links":{"citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:7d31957673b053c3b5f1d31bc3ad9d00926f7ef90deb3c5ec0f6c57b15892dbf","observation_id":"37d84429-890b-494b-8fcc-13c2f01ce4a1","resolution":{"observed_at":"2026-08-14T15:34:26.228629Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04503","last_updated":"2018-11-29T22:13:11Z","snapshot_observed_at":"2026-08-14T19:06:13.036860Z","submitted_at":"2018-06-08T06:36:34Z","title":"Tutorial: Maximum likelihood estimation in the context of an optical measurement","version":3},"cited_work":{"arxiv_id":"1806.04503","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.04503","snapshot_observed_at":"2026-08-14T15:34:26.187375Z","title":"Tutorial: Maximum likelihood estimation in the context of an optical measurement","venue":"physics.data-an","work_id":"9db7e672-4469-4444-ac5f-96842fca4416","year":2018},"citing_paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T15:34:26.153763Z"},"links":{"cited_paper":"/paper/1806.04503","citing_paper":"/paper/1908.02142"},"observation_digest":"sha256:d287778143ddc17fb0fd647441fae40ec2c0f59a2395e27ee0ea966c084636b5","observation_id":"051e44bb-3320-406e-b8c9-65d295a524a5","resolution":{"observed_at":"2026-08-14T15:34:26.194006Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.02142","last_updated":"2019-08-03T01:47:19Z","latest_version":1,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-08-15T02:56:48.055016Z","submitted_at":"2019-08-03T01:47:19Z","title":"Optimal birefringence distributions for star test polarimetry"},"reference_resolution":{"displayed":15,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":2,"verified_fuzzy":13},"total_outbound_references":15},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 15 of 15 outbound references and 0 inbound Pith citation observations for arXiv:1908.02142."}