{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:BQ3XGISCUUDHM3TU2NYX6LKJBO","short_pith_number":"pith:BQ3XGISC","schema_version":"1.0","canonical_sha256":"0c37732242a506766e74d3717f2d490ba7da6ffa66a9aceaec935baf22519936","source":{"kind":"arxiv","id":"1011.3391","version":1},"attestation_state":"computed","paper":{"title":"Images of unclassified and supergiant B[e] stars disks with interferometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Adriane Liermann (MPIFR), Anthony Meilland (MPIFR), Florentin Millour (FIZEAU), Gerd Weigelt (MPIFR), Jos\\'e Groh (MPIFR), Marcelo Borges Fernandes, Olivier Chesneau (FIZEAU), Thomas Driebe (DLR)","submitted_at":"2010-11-15T14:18:09Z","abstract_excerpt":"B[e] stars are among the most peculiar objects in the sky. This spectral type, characterised by allowed and forbidden emission lines, and a large infrared excess, does not represent an homogenous class of objects, but instead, a mix of stellar bodies seen in all evolutionary status. Among them, one can find Herbig stars, planetary nebulae central stars, interacting binaries, supermassive stars, and even \"unclassified\" B[e] stars: systems sharing properties of several of the above. Interferometry, by resolving the innermost regions of these stellar systems, enables us to reveal the true nature "},"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":"1011.3391","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-11-15T14:18:09Z","cross_cats_sorted":[],"title_canon_sha256":"ad2c2135a25a4f6f1903a592b4495711c4608015d367052a0a90ae19aca599ab","abstract_canon_sha256":"08609380e62fa2741def4c5ef5b1989d377cae3167be63fbe9fefaa9dcfdfa2f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:47.588753Z","signature_b64":"EgKC1mS8bHTV0Yu81tgjjicuFZlMpEVXlZRS0diPDpKCkhnQeYhHQcjy2dDmd57mMKgkcMkH4SU0eYYrO+iBCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c37732242a506766e74d3717f2d490ba7da6ffa66a9aceaec935baf22519936","last_reissued_at":"2026-05-18T02:04:47.588108Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:47.588108Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Images of unclassified and supergiant B[e] stars disks with interferometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Adriane Liermann (MPIFR), Anthony Meilland (MPIFR), Florentin Millour (FIZEAU), Gerd Weigelt (MPIFR), Jos\\'e Groh (MPIFR), Marcelo Borges Fernandes, Olivier Chesneau (FIZEAU), Thomas Driebe (DLR)","submitted_at":"2010-11-15T14:18:09Z","abstract_excerpt":"B[e] stars are among the most peculiar objects in the sky. This spectral type, characterised by allowed and forbidden emission lines, and a large infrared excess, does not represent an homogenous class of objects, but instead, a mix of stellar bodies seen in all evolutionary status. Among them, one can find Herbig stars, planetary nebulae central stars, interacting binaries, supermassive stars, and even \"unclassified\" B[e] stars: systems sharing properties of several of the above. Interferometry, by resolving the innermost regions of these stellar systems, enables us to reveal the true nature "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.3391","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":"1011.3391","created_at":"2026-05-18T02:04:47.588221+00:00"},{"alias_kind":"arxiv_version","alias_value":"1011.3391v1","created_at":"2026-05-18T02:04:47.588221+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.3391","created_at":"2026-05-18T02:04:47.588221+00:00"},{"alias_kind":"pith_short_12","alias_value":"BQ3XGISCUUDH","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BQ3XGISCUUDHM3TU","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BQ3XGISC","created_at":"2026-05-18T12:26:05.355336+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/BQ3XGISCUUDHM3TU2NYX6LKJBO","json":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO.json","graph_json":"https://pith.science/api/pith-number/BQ3XGISCUUDHM3TU2NYX6LKJBO/graph.json","events_json":"https://pith.science/api/pith-number/BQ3XGISCUUDHM3TU2NYX6LKJBO/events.json","paper":"https://pith.science/paper/BQ3XGISC"},"agent_actions":{"view_html":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO","download_json":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO.json","view_paper":"https://pith.science/paper/BQ3XGISC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1011.3391&json=true","fetch_graph":"https://pith.science/api/pith-number/BQ3XGISCUUDHM3TU2NYX6LKJBO/graph.json","fetch_events":"https://pith.science/api/pith-number/BQ3XGISCUUDHM3TU2NYX6LKJBO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO/action/storage_attestation","attest_author":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO/action/author_attestation","sign_citation":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO/action/citation_signature","submit_replication":"https://pith.science/pith/BQ3XGISCUUDHM3TU2NYX6LKJBO/action/replication_record"}},"created_at":"2026-05-18T02:04:47.588221+00:00","updated_at":"2026-05-18T02:04:47.588221+00:00"}