{"as_of":"2026-08-21T10:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:537f709d304736b475c7f5b762f479f2e5523899c4418d36df63892975721e37","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":"2026-08-15T16:35:16.420484Z","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":"2026-08-21T06:32:19.484+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/2509.04427/citation-record","integrity":"/paper/2509.04427/integrity","json":"/paper/2509.04427/citation-record.json","paper":"/paper/2509.04427"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/175557","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.963884Z","title":null,"venue":null,"work_id":"71c4e97f-b953-4296-a0c1-8083bc0214ae","year":1995},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.180966Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:cc326490b6707e0106bcf3afd3d6a7fa27649b08b1215db8d01f1bea6b0803ed","observation_id":"80610cc3-d94c-4579-972a-63a4fcbe7d7b","resolution":{"observed_at":"2026-08-15T16:35:16.967531Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.185337Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.185337Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:f044df8164e967435b3730f1abc900e78e4b75c59a404976ba31103fd4373f67","observation_id":"8150cc3a-06cc-4786-8ac4-4566495c86b1","resolution":{"observed_at":"2026-08-15T16:35:16.185337Z","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":"2026-08-15T16:35:17.257770Z","title":"C., & Savage, B","venue":null,"work_id":"e11ac03a-78f3-4218-84fd-6a568e80e96f","year":1970},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.190088Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:0d2e37179e1bf3df24ba680d28cf63343b6b4c3bbac78c3fb7d5cceedaf6ce36","observation_id":"8ca25266-dd7e-4b45-9772-b4df65a262de","resolution":{"observed_at":"2026-08-15T16:35:17.260880Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.194011Z","title":"A., Clayton, G","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.194011Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:fe06c777f79875dc7120a2ca2dc01f395281733ab5dc50a7cf9d97a3ffe4febe","observation_id":"212049f7-b3db-47a7-9d5f-0670c73e535a","resolution":{"observed_at":"2026-08-15T16:35:16.194011Z","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":"2026-08-15T16:35:16.197688Z","title":"L., Goldsmith, P","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.197688Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:a725ce143c43ad02764a6e837265111ea805ef193a69238fcc23db5bf6b088cf","observation_id":"0a4491cd-9e97-4dd2-8242-45101fb120ad","resolution":{"observed_at":"2026-08-15T16:35:16.197688Z","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":"10.1088/0004-637x/800/2/132","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.935204Z","title":"2015, The Astrophysical Journal, 800, 132, 10.1088/0004-637X/800/2/132","venue":null,"work_id":"6167f16f-0e10-4bd1-a9cf-da6907713971","year":2015},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.201788Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:52655c202136c86566d97bea75309918212f6b8dc8f5c9c2e8825094071a58c8","observation_id":"ad3925bd-025b-497d-8cd5-6a37aaab3f9e","resolution":{"observed_at":"2026-08-15T16:35:16.938802Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/114838","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.924108Z","title":"C., & Cardelli, J","venue":null,"work_id":"01786ad4-a839-4d99-a0b6-041bee21ab75","year":1988},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.205914Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:9f3b15e7dee801729ea52c556ee8077e94cd1666484207614c7189476beb34a3","observation_id":"aa3595f0-9ed8-4a56-ab03-95bdc234e0d0","resolution":{"observed_at":"2026-08-15T16:35:16.927650Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.209434Z","title":"A., Boquien, M., Barnes, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.209434Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:fb08c2f999ec42918695a004958b533fb3a603a392d081bbbf1c78f008aee969","observation_id":"d829346a-3c01-4e76-bcb7-75770d5ddf5b","resolution":{"observed_at":"2026-08-15T16:35:16.209434Z","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":"2026-08-15T16:35:16.212833Z","title":null,"venue":null,"work_id":null,"year":1951},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.212833Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:774a23548367518c0a54377ee295a910519ec716967bbc8cc0e93c739f20234e","observation_id":"5c8b35f3-4d60-404c-bbe3-67bfba462dbf","resolution":{"observed_at":"2026-08-15T16:35:16.212833Z","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":"2026-08-15T16:35:16.216571Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.216571Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:0381edf4c498adb5da09b2b2c58e45ac8a36d87227598142485a54dba1bb1afe","observation_id":"6d8bb913-ab7d-4c6c-828a-5e39b39f2809","resolution":{"observed_at":"2026-08-15T16:35:16.216571Z","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":"2026-08-15T16:35:16.220379Z","title":"Z., & Mitrofanov, I","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.220379Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:18d34f4dbf4378425ca83457dba38f8032332af86a448310b9737bf5dbf7f267","observation_id":"bd873e87-2c58-4ad0-8682-01b632b38cd1","resolution":{"observed_at":"2026-08-15T16:35:16.220379Z","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":"10.1086/164694","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.888241Z","title":null,"venue":null,"work_id":"926bf421-8268-4e02-80b7-e1ef733f2f83","year":1986},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.223964Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:15d70d862936f0ca4db8497479ed0086ead9b9f206fa071ea87e737df049a709","observation_id":"cf4fc14f-6a67-4b80-8ec1-9fd12c4cf099","resolution":{"observed_at":"2026-08-15T16:35:16.892772Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09484","last_updated":"2018-02-26T18:03:56Z","snapshot_observed_at":"2026-08-17T20:04:24.859742Z","submitted_at":"2018-02-26T18:03:56Z","title":"Disentangling the independently controllable factors of variation by interacting with the world","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09484","snapshot_observed_at":"2026-08-15T16:35:16.227312Z","title":"2003, Annual Review of Astronomy and Astrophysics, 41, 241, 10.1146/annurev.astro.41.011802.094840","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.227312Z"},"links":{"cited_paper":"/paper/1802.09484","citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:706454aaf30394a7e41bb18fbb5d0a3fdde417431b923b7605caf0e78b477567","observation_id":"91dce8b4-ee5c-4fd0-a9f5-89b13b54d3bb","resolution":{"observed_at":"2026-08-15T16:35:16.227312Z","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":"2026-08-15T16:35:16.230986Z","title":"T., & Weingartner, J","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.230986Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:452816c3fdd40bd4dcfc00ccdd3b449dacffae8309d45824c08f6cbbe33246ac","observation_id":"cec60c00-fbc0-4f2c-bde3-3e36fd3c7320","resolution":{"observed_at":"2026-08-15T16:35:16.230986Z","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":"2026-08-15T16:35:16.234497Z","title":"1997, The Astrophysical Journal, 480, 633, 10.1086/304008","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.234497Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:6c009aac1c463ffdc9af389887509b26ec1d55a438406a24efc721bea3c806f7","observation_id":"bd2e4829-73e9-4c8b-83d0-0cd1aaadc08f","resolution":{"observed_at":"2026-08-15T16:35:16.234497Z","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":"2026-08-15T16:35:16.237999Z","title":"T., Dale, D","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.237999Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:8074e1170c3deaf82479b186bb8348639cb5b56289e925b63fc7628e06910170","observation_id":"1b2e726c-5af5-40c5-80c5-c6115ca9ef79","resolution":{"observed_at":"2026-08-15T16:35:16.237999Z","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":"2026-08-15T16:35:16.241534Z","title":"2024, , 685, A82, 10.1051/0004-6361/202347628","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.241534Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:aab8f9f261b2b3290d2c7309f719e5a5caa9999034b613d19a933f47249fc889","observation_id":"1f2cd559-5e45-44ed-95aa-f2705ab6c7ac","resolution":{"observed_at":"2026-08-15T16:35:16.241534Z","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":"2026-08-15T16:35:16.244902Z","title":"2008, The Astrophysical Journal, 679, 537, 10.1086/587479","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.244902Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:84525ff25981b10048f4f3cf0c637c0d1b6fc238d3560a04e358f8721891d089","observation_id":"534d6979-8c96-4879-aa84-52abe6ac686a","resolution":{"observed_at":"2026-08-15T16:35:16.244902Z","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":"2026-08-15T16:35:16.248477Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.248477Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:669190be2ba0d7d2bfb5abc8a3e442d6b9fafda508e65ec9f785a38427f35cee","observation_id":"d8cafb7b-cc98-4eeb-aa1e-e3d972ddd197","resolution":{"observed_at":"2026-08-15T16:35:16.248477Z","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":"2026-08-15T16:35:16.251925Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.251925Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:b46e4b0386e64df113699569c593439cfc7df620d36cd750f5352772088b3c50","observation_id":"f8c52123-c8ac-4c23-83f4-8cc65e8f3467","resolution":{"observed_at":"2026-08-15T16:35:16.251925Z","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":"2026-08-15T16:35:16.255318Z","title":"L., & Massa, D","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.255318Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:908136f067054d272f07a14b6edde374db975d7c0c8165be8ce07b92831ab562","observation_id":"a4e21bc9-43be-413c-968f-5e162f9d03f2","resolution":{"observed_at":"2026-08-15T16:35:16.255318Z","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":"2026-08-15T16:35:16.258712Z","title":"L., Massa, D., Gordon, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.258712Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:e13466f8bf20431a2100fc38a3d2587d3314097659a8645376e79b433f2e0ef0","observation_id":"8665f8c5-63f2-4108-b177-432ebf365049","resolution":{"observed_at":"2026-08-15T16:35:16.258712Z","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":"2026-08-15T16:35:16.261981Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.261981Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:6f296530d1dd3c086bddcafa4067729e9c856c0673fbe26199dfb596ff0ac5fa","observation_id":"c7f849be-73f9-408c-91b8-157422d9d246","resolution":{"observed_at":"2026-08-15T16:35:16.261981Z","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":"2026-08-15T16:35:16.265334Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.265334Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:dd2831e2666eb16ddccc353f9c28806ba41100babc2768d7a7e79b50dee835ae","observation_id":"72626548-8c65-46b4-b8d9-695a04648243","resolution":{"observed_at":"2026-08-15T16:35:16.265334Z","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":"2026-08-15T16:35:16.268730Z","title":"A., & Mosenkov, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.268730Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:995145a040e75648ce7f5db0cc766ab0a55b2918c460f102426a7cae858a4d37","observation_id":"78ddf62e-0567-43c8-9f07-3f438efa55a6","resolution":{"observed_at":"2026-08-15T16:35:16.268730Z","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":"2026-08-15T16:35:16.272242Z","title":"D., Clayton, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.272242Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:0f03dfa487d0e7d0e4addc9a4218c405b68e36c5dca923261b6d5948bde9d10a","observation_id":"3dbbd8cc-d577-425e-806b-f53fe6a1b3fe","resolution":{"observed_at":"2026-08-15T16:35:16.272242Z","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":"2026-08-15T16:35:16.276019Z","title":"M., Schlafly, E., Zucker, C., Speagle, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.276019Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:3648ba334ba2595ed7a80e95c2409697c8af3645f09f2ddfdbf302e081cc735c","observation_id":"1b822b08-003a-4b63-8dd0-1637a8949826","resolution":{"observed_at":"2026-08-15T16:35:16.276019Z","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":"2026-08-15T16:35:16.280219Z","title":null,"venue":null,"work_id":null,"year":1949},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.280219Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:d9c74cf5c0b9963488c0d7b6c2eed3e3c65b5a1d7c9c7351e377866e4e6986b6","observation_id":"dd6589c6-29ff-489c-8d21-99276bf6f6ed","resolution":{"observed_at":"2026-08-15T16:35:16.280219Z","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":"2026-08-15T16:35:16.283744Z","title":"H., Kirby, L., Dotson, J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.283744Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:862be7171a40fd546b500bcfe118b3f164b1db636b2341a1a0af749cfc7a96a8","observation_id":"c8193705-31d6-4524-b798-a7f932e9a640","resolution":{"observed_at":"2026-08-15T16:35:16.283744Z","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":"2026-08-15T16:35:16.288113Z","title":null,"venue":null,"work_id":null,"year":1949},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.288113Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:1bcd80e1b34bc717e46f25357ce8c087daba8751760a8f14738f90e7bb8dc4f4","observation_id":"be46b2c4-ea98-4f63-ab39-e9a6c2d65ee2","resolution":{"observed_at":"2026-08-15T16:35:16.288113Z","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":"2026-08-15T16:35:16.291577Z","title":"2012, , 422, 1263, 10.1111/j.1365-2966.2012.20702.x","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.291577Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:c7afca03d0d0ae59bb30c63e168d3219a8d5e6fc7ddd8059609239d7c0da47f1","observation_id":"4847d3ca-9c80-49da-bad7-464b181ef223","resolution":{"observed_at":"2026-08-15T16:35:16.291577Z","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":"10.1086/146063","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.771107Z","title":"L., & Morgan, W","venue":null,"work_id":"ca8cc281-7d0d-4c48-9277-1b07fe906f45","year":1955},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.294830Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:1d68285b3d7ea642aebca993d91dc813093b949215462c3cd288e81999c0ee29","observation_id":"d5cdd5a9-7cf6-4dd7-a1c9-11be15d82c04","resolution":{"observed_at":"2026-08-15T16:35:16.774395Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.298331Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.298331Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:0c482aa01d1a155b8addd3f415ab825c674b463de38697d1c715c53b65dad468","observation_id":"6ed0af9b-2a0c-4693-94a2-840f4de1f4ca","resolution":{"observed_at":"2026-08-15T16:35:16.298331Z","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":"10.1088/0004-6256/135/4/1318","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.755145Z","title":"J., Stark, D., Woodward, C","venue":null,"work_id":"7712ce0c-405b-4bc7-b3bf-e1b46b0d89ff","year":2008},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.302323Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:132284dbef1a90d652d6d4a36c86d0b79efe374b3177f0c43df4d7110a97e4ab","observation_id":"1210a927-1bb9-414a-b3e2-221cc0ef502b","resolution":{"observed_at":"2026-08-15T16:35:16.758699Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.307076Z","title":"Y., Vergely, J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.307076Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:68664b15471ea2a1e6b326d8e495a993cb47df90f68fe1de05f149326e32fccd","observation_id":"5c81f06e-b4cf-411e-94e0-27d7099ba670","resolution":{"observed_at":"2026-08-15T16:35:16.307076Z","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":"10.1086/308619","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.739660Z","title":"A., Wolff, M","venue":null,"work_id":"adbb144a-5a34-4079-8e65-003beb477db5","year":2000},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.310507Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:ada29b29ac265bfced047c6997386660d8e518089be8e889b0a9fcb989ccd04e","observation_id":"00dbbaf1-e4f8-4f36-9fc0-c45e0391c3ef","resolution":{"observed_at":"2026-08-15T16:35:16.743018Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.313915Z","title":"2007, Monthly Notices of the Royal Astronomical Society, 378, 910, 10.1111/j.1365-2966.2007.11817.x","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.313915Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:456153f65b2c8652e77117c1743cdacd5de4ff4c59af73daec21eaf9a4d7e741","observation_id":"2426c540-cb5c-421f-9540-ed339a5ea47c","resolution":{"observed_at":"2026-08-15T16:35:16.313915Z","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":"2026-08-15T16:35:17.247848Z","title":null,"venue":null,"work_id":"ce0840dc-2c7b-4ca1-8cc7-25c3843a6420","year":1999},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.317855Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:86b9fbb32e9035eab95d104fcbc9f4c1b8cb826ee3c7befcff8ad3cf2f42ce70","observation_id":"36a16d53-e950-4c40-9b6f-6871d1bb77e4","resolution":{"observed_at":"2026-08-15T16:35:17.251069Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:200810905","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.729523Z","title":"S., Pety, J., & Tachihara, K","venue":null,"work_id":"81a9a11c-e8bb-4657-b132-f1758fe26578","year":2009},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.321485Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:02930cf4134ec86bf7e268e684b4c8d312e4b9721a86f7e56dedebbef4ae3a9b","observation_id":"bf1817a4-4ba2-4385-af27-014268c4ab34","resolution":{"observed_at":"2026-08-15T16:35:16.732941Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/191088","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.719748Z","title":null,"venue":null,"work_id":"25c06e9d-deff-4f44-8279-1fc74bd2237a","year":1986},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.324800Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:1dd6bcb8afe91d72cf632927d5da4bb22a24ccae489bc3fb4a36bb5fffaf47bf","observation_id":"720c4525-ae68-4464-9894-6cf6931871b5","resolution":{"observed_at":"2026-08-15T16:35:16.723217Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.328443Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.328443Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:5bcdfd01608ff478d3e7c5817c9c694ddc3d5eefc0dc004431d5355fdd0d26f4","observation_id":"2b2da5e1-811f-4092-918a-6a46f08db1b8","resolution":{"observed_at":"2026-08-15T16:35:16.328443Z","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":"2026-08-15T16:35:16.331916Z","title":"S., Rumpl, W., & Nordsieck, K","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.331916Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:4f563c7e825e46bb7ed375e53933bba7ebe3abc81a6144e3aed8815e13252e58","observation_id":"977b3a12-df8e-46ba-b60c-81779faa2aee","resolution":{"observed_at":"2026-08-15T16:35:16.331916Z","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":"2026-08-15T16:35:16.336579Z","title":"2018, , 478, 2851, 10.1093/mnras/sty1248","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.336579Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:d097cdd6c6201dc8a9631910d1a106884bd2682ea9fb2b8c8457c8ea2aa44cb8","observation_id":"6d82e22f-75b4-4406-ac87-afadc0005e15","resolution":{"observed_at":"2026-08-15T16:35:16.336579Z","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":"2026-08-15T16:35:16.340467Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.340467Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:f361bd292724fe1cc59abdab0820923f441c93cb16acf4e2edf85deff5f1175a","observation_id":"45626219-32c8-4b95-baa4-53ee45a066d5","resolution":{"observed_at":"2026-08-15T16:35:16.340467Z","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":"2026-08-15T16:35:16.343811Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.343811Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:9469fd0cc8d0daef8929e04ab74658ad4c7d1c956024c3f9da519b85e40d4d55","observation_id":"c5b6877c-deb8-4144-b05d-1193561ebb09","resolution":{"observed_at":"2026-08-15T16:35:16.343811Z","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":"2026-08-15T16:35:16.347519Z","title":"J., Zucker, C., Goodman, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.347519Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:186fd19f1e7316dd80bd91b52b23c05699db5f2e3bb206b8ab84acd114437881","observation_id":"0791d972-4ab9-4f2d-8b67-81348d449206","resolution":{"observed_at":"2026-08-15T16:35:16.347519Z","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":"2026-08-15T16:35:16.350971Z","title":"V., Hensley, B","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.350971Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:17c7b415530dbed09a734bb19ed12bf896330d6f6a51dcffc046e83725584a0c","observation_id":"abe74e30-4e83-4259-b0bc-9ada8476c6cb","resolution":{"observed_at":"2026-08-15T16:35:16.350971Z","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":"2026-08-15T16:35:16.354672Z","title":"2020, Astronomy and Astrophysics, 636, A17, 10.1051/0004-6361/201937157","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.354672Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:7b3c7d224450566adbc27374f854e3e283ccaf11fc6dfb879e7d8455061d2564","observation_id":"ad95c314-2687-46f9-9969-d747ab4731d7","resolution":{"observed_at":"2026-08-15T16:35:16.354672Z","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":"10.3847/1538-4357/ac36d8","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.668326Z","title":"N., & Kobulnicky, H","venue":null,"work_id":"2badbfb7-de33-49d1-95f8-526e70cdde94","year":2022},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.358491Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:89c3b9641e65079b01ab35b3178caf9519f2ed3b52baddeed59d8145c885743c","observation_id":"82928869-508f-4540-9b0c-ae93006572ea","resolution":{"observed_at":"2026-08-15T16:35:16.672082Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.362531Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.362531Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:cb2b7a9c485ee88fa28dac5290d1da46588d86e635b4bead22abc89a418c86f6","observation_id":"d91bdc64-eeb6-4cf1-8df6-4dc5a21210bd","resolution":{"observed_at":"2026-08-15T16:35:16.362531Z","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":"2026-08-15T16:35:16.367347Z","title":"D., & Mathis, J","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.367347Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:1a4b849396dc7ef582d312dc3b3cdff1d80b69f941df275c2739f08882189066","observation_id":"afacb24e-34e4-4913-bb5e-9c0442fa9150","resolution":{"observed_at":"2026-08-15T16:35:16.367347Z","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":"2026-08-15T16:35:16.370695Z","title":"F., Meisner, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.370695Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:80a7462500e984e2d51619bfba938664289ba630854f076304d6e7949b810a6e","observation_id":"f7029164-b1e4-4273-8924-11c1df058c77","resolution":{"observed_at":"2026-08-15T16:35:16.370695Z","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":"2026-08-15T16:35:16.374128Z","title":"D., Elston, R., & Lupie, O","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.374128Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:b54d8c133459c394fa3304de8a0d111b78489d0b4e4b7608891a8fdf1e5df89c","observation_id":"5d62d15d-2231-452b-9115-6fa38dab90cb","resolution":{"observed_at":"2026-08-15T16:35:16.374128Z","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":"2026-08-15T16:35:16.377522Z","title":"L., & Ford, V","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.377522Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:ee401548067aea93cc159444e170ac705b46d22915fda7ca1348935547313f75","observation_id":"61816d46-7050-4b6a-bc84-f929e79979f0","resolution":{"observed_at":"2026-08-15T16:35:16.377522Z","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":"2026-08-15T16:35:16.381454Z","title":"2020, Astronomy & Astrophysics, 641, A35, 10.1051/0004-6361/202037511","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.381454Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:d31c6e407c5c3d0f9a516c2498f1008d726f20edc0a83a293bfafb4ff3a24486","observation_id":"10bd2c78-3b5a-4ff4-819b-ccdc5c1eb8b6","resolution":{"observed_at":"2026-08-15T16:35:16.381454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08971","last_updated":"2024-11-13T19:03:43Z","snapshot_observed_at":"2026-08-16T16:16:50.554647Z","submitted_at":"2024-11-13T19:03:43Z","title":"Challenges in constraining dust properties from starlight polarization","version":1},"cited_work":{"arxiv_id":"2411.08971","doi":"10.48550/arxiv.2411.08971","metadata_source":"pith","pith_arxiv_id":"2411.08971","snapshot_observed_at":"2026-08-15T18:16:14.067578Z","title":"Challenges in constraining dust properties from starlight polarization","venue":"astro-ph.GA","work_id":"0bc57837-0a34-4300-9a30-aa83d51cb24a","year":2024},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.384974Z"},"links":{"cited_paper":"/paper/2411.08971","citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:18acc7ff6718246cf3d10b8601f4467a838a22f3c48af9291268571087c59a7f","observation_id":"8aa425bc-a33c-4d82-9dbc-efa4a9343062","resolution":{"observed_at":"2026-08-15T16:35:16.629753Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/pasj/52.6.1147","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:35:16.608456Z","title":"2000, Publications of the Astronomical Society of Japan, 52, 1147, 10.1093/pasj/52.6.1147","venue":null,"work_id":"fa7825a7-ac32-4d9e-b8de-0453703e615d","year":2000},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.388347Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:ad13e91fe175d2b45107cfa660e09e9839dd5e9a5a410468ca228e644e199872","observation_id":"901768b1-53de-4989-bf5c-6f0ac8dd86cf","resolution":{"observed_at":"2026-08-15T16:35:16.613822Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:17.237884Z","title":"2005, Astronomical Polarimetry","venue":null,"work_id":"f4be5bbd-b7fd-476b-bc81-d439419e9e8e","year":2005},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.391599Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:0517df75447ddad32e3544b9c0cc8232f8ffe6082720f689c73c66e4a5de1d76","observation_id":"3b0ec6ea-3509-4148-8f5c-318d4acff813","resolution":{"observed_at":"2026-08-15T16:35:17.241271Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+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":"2026-08-15T16:35:16.395386Z","title":"1986, 627, 733, 10.1117/12.968154","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.395386Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:3ff0b216f10ede527455266d435380582c8d73eaa2ffc8fcda06e267b40268b4","observation_id":"d68663c3-f003-4113-a286-757efde7d372","resolution":{"observed_at":"2026-08-15T16:35:16.395386Z","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":"2026-08-15T16:35:16.398553Z","title":"A., Bohlin, R","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.398553Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:c1280593ee4b8e6653a56cf6f231964f4fee3773919c6b0cb07d8a74c32f48b1","observation_id":"5e21f23a-3a0b-41f9-ae99-947fc77b11b6","resolution":{"observed_at":"2026-08-15T16:35:16.398553Z","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":"2026-08-15T16:35:16.402602Z","title":"2007, Astronomy & Astrophysics, 474, 653, 10.1051/0004-6361:20078357","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.402602Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:166d833250e49c20dfa551d1c1758a03f24c2edb6c06202b7cacfbed0db4311a","observation_id":"8caf3142-0081-42d8-9698-549faabd1c9f","resolution":{"observed_at":"2026-08-15T16:35:16.402602Z","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":"2026-08-15T16:35:16.405886Z","title":"C., & Draine, B","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.405886Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:144cc9f073b2bbafcf1a7b7059feac95eb2696a368bbfad7623a762e5538d593","observation_id":"78b83128-0b7f-4111-a8c5-64bbdd959711","resolution":{"observed_at":"2026-08-15T16:35:16.405886Z","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":"2026-08-15T16:35:16.409527Z","title":"W., Roellig, T","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.409527Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:7ccb557c41fbf81ffd0c1f471dfa625ecda35db51d59d4fb0752082364f6977d","observation_id":"f35a406b-c8aa-47eb-a8a5-30d95035abdc","resolution":{"observed_at":"2026-08-15T16:35:16.409527Z","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":"2026-08-15T16:35:16.412945Z","title":"L., Eisenhardt, P","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.412945Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:51ea68f4148e5bb72abe05e6d3369ccc256ac7836e47b1ea4118d9d2fc578b72","observation_id":"fb5a9ece-a633-49db-84ae-1fe1a6e31c53","resolution":{"observed_at":"2026-08-15T16:35:16.412945Z","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":"2026-08-15T16:35:16.416434Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.416434Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:c57680da2109bf8a0c3875049291ae49ae40f67878ec559c0d262536bb2fa793","observation_id":"089623b1-78af-4039-a1fe-a5f6123a983c","resolution":{"observed_at":"2026-08-15T16:35:16.416434Z","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":"2026-08-15T16:35:16.420484Z","title":"K., Speagle , J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-15T16:35:16.420484Z"},"links":{"citing_paper":"/paper/2509.04427"},"observation_digest":"sha256:ec8fe489d4ea03c02f531978b74d6a3d1bac6db828090f66f671f25fcd05015c","observation_id":"ccf132ef-0d01-48d3-a901-4b1c1470357e","resolution":{"observed_at":"2026-08-15T16:35:16.420484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.04427","last_updated":"2025-09-04T17:47:11Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-19T05:49:16.983933Z","submitted_at":"2025-09-04T17:47:11Z","title":"Extreme Starlight Polarization Efficiency Toward $\\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction"},"reference_resolution":{"displayed":66,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":52,"verified_exact":12,"verified_fuzzy":2},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 66 of 66 outbound references and 0 inbound Pith citation observations for arXiv:2509.04427."}