{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:HENP4WIQKLUY6TEA5D6CFVXJDJ","short_pith_number":"pith:HENP4WIQ","schema_version":"1.0","canonical_sha256":"391afe591052e98f4c80e8fc22d6e91a488136b92f2941d1b51687387c87ab80","source":{"kind":"arxiv","id":"1208.0155","version":1},"attestation_state":"computed","paper":{"title":"Polarimetric coronagraphy of BD+31643","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Djupvik, G. Olofsson, H.-G. Flor\\'en, M. Aberasturi, R. Nilsson","submitted_at":"2012-08-01T09:57:50Z","abstract_excerpt":"Context. The binary B5V star BD+31?643 exhibits a disk-like structure detected at optical wavelengths. Even though the feature is well centered on the star, it has been argued, based on Spitzer observations, that the feature is a filament not directly associated to the binary star. Aims. The purpose of the present paper is to investigate whether polarization imaging may provide evidence either for or against the disk hypothesis. In addition, we aim at clarifying whether there might be any additional close companion to the binary star. Methods. We used the coronagraph PolCor in its polarization"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1208.0155","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-08-01T09:57:50Z","cross_cats_sorted":[],"title_canon_sha256":"4cf94c147440838bfeccbde4a47d2dbc4cf3f9dfd47aa99e86fefa72c0e470f2","abstract_canon_sha256":"5399265b90d0381423358956b9f0ab9a195ca472afea5a39ca45a0ce88b9b21d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:49:36.129830Z","signature_b64":"J0lx7GmwnG9IexRWEDgXWIACUGEjL09Vpt+VuseSeq6dM/B243ekXI2qWStxXqcLlqNgsZZ5zgNbifd7Cs/nCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"391afe591052e98f4c80e8fc22d6e91a488136b92f2941d1b51687387c87ab80","last_reissued_at":"2026-05-18T03:49:36.129102Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:49:36.129102Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Polarimetric coronagraphy of BD+31643","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Djupvik, G. Olofsson, H.-G. Flor\\'en, M. Aberasturi, R. Nilsson","submitted_at":"2012-08-01T09:57:50Z","abstract_excerpt":"Context. The binary B5V star BD+31?643 exhibits a disk-like structure detected at optical wavelengths. Even though the feature is well centered on the star, it has been argued, based on Spitzer observations, that the feature is a filament not directly associated to the binary star. Aims. The purpose of the present paper is to investigate whether polarization imaging may provide evidence either for or against the disk hypothesis. In addition, we aim at clarifying whether there might be any additional close companion to the binary star. Methods. We used the coronagraph PolCor in its polarization"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.0155","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1208.0155","created_at":"2026-05-18T03:49:36.129207+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.0155v1","created_at":"2026-05-18T03:49:36.129207+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.0155","created_at":"2026-05-18T03:49:36.129207+00:00"},{"alias_kind":"pith_short_12","alias_value":"HENP4WIQKLUY","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"HENP4WIQKLUY6TEA","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"HENP4WIQ","created_at":"2026-05-18T12:27:09.501522+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ","json":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ.json","graph_json":"https://pith.science/api/pith-number/HENP4WIQKLUY6TEA5D6CFVXJDJ/graph.json","events_json":"https://pith.science/api/pith-number/HENP4WIQKLUY6TEA5D6CFVXJDJ/events.json","paper":"https://pith.science/paper/HENP4WIQ"},"agent_actions":{"view_html":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ","download_json":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ.json","view_paper":"https://pith.science/paper/HENP4WIQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.0155&json=true","fetch_graph":"https://pith.science/api/pith-number/HENP4WIQKLUY6TEA5D6CFVXJDJ/graph.json","fetch_events":"https://pith.science/api/pith-number/HENP4WIQKLUY6TEA5D6CFVXJDJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ/action/storage_attestation","attest_author":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ/action/author_attestation","sign_citation":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ/action/citation_signature","submit_replication":"https://pith.science/pith/HENP4WIQKLUY6TEA5D6CFVXJDJ/action/replication_record"}},"created_at":"2026-05-18T03:49:36.129207+00:00","updated_at":"2026-05-18T03:49:36.129207+00:00"}