{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:X5XXGSUN7UFEH3ZWPJ2ACNJWNO","short_pith_number":"pith:X5XXGSUN","schema_version":"1.0","canonical_sha256":"bf6f734a8dfd0a43ef367a740135366bab0d098e66ba03eb703eadc758c9b0d9","source":{"kind":"arxiv","id":"1701.01695","version":1},"attestation_state":"computed","paper":{"title":"Star formation driven galactic winds in UGC 10043","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Monreal Ibero, A. V. Moiseev, C. Kehrig, C. L\\'opez-Cob\\'a, C. Morisset, D. J. Bomans, D. V. Oparin, I. Cruz-Gonz\\'alez, J. Bland-Hawthorn, L. Galbany, M. Cano-D\\'iaz, M. M. Roth, R. A. Marino, R.-J. Dettmar, R. M. Gonz\\'alez Delgado, S. F. S\\'anchez, T. Bitsakis, V. Abril-Melgarejo","submitted_at":"2017-01-06T17:06:31Z","abstract_excerpt":"We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of the CALIFA integral field spectroscopy data, scanning Fabry-Perot interferometry (FPI), and multiband photometry. We detect ionized gas in the extraplanar regions reaching a relatively high distance, up to ~ 4 kpc above the galactic disk. The ionized gas line ratios ([N ii]/Ha, [S ii]/Ha and [O i]/Ha) present an enhancement along the semi minor axis, in contrast with the values found at the disk, where they are compatible with ionization due to H ii-regions. These differences, together with the biconic sy"},"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":"1701.01695","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-01-06T17:06:31Z","cross_cats_sorted":[],"title_canon_sha256":"48658b6d76fffd02240044aaaa5fc9b42396249ee44d92473f3bf479afefa110","abstract_canon_sha256":"2df8793a2adbe8824f35c580be97c447bcea5f107abd1769f9dc5c9a81ec95b3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:46.750793Z","signature_b64":"Qwzmn9UgP+YookPbd/hrOsGwNwESFKCOqLzOUUhYAcsiZXua/9KWmzf7YnYcsaIR06iqG/ZY4lsziKNvwY5UCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bf6f734a8dfd0a43ef367a740135366bab0d098e66ba03eb703eadc758c9b0d9","last_reissued_at":"2026-05-18T00:48:46.750364Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:46.750364Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Star formation driven galactic winds in UGC 10043","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Monreal Ibero, A. V. Moiseev, C. Kehrig, C. L\\'opez-Cob\\'a, C. Morisset, D. J. Bomans, D. V. Oparin, I. Cruz-Gonz\\'alez, J. Bland-Hawthorn, L. Galbany, M. Cano-D\\'iaz, M. M. Roth, R. A. Marino, R.-J. Dettmar, R. M. Gonz\\'alez Delgado, S. F. S\\'anchez, T. Bitsakis, V. Abril-Melgarejo","submitted_at":"2017-01-06T17:06:31Z","abstract_excerpt":"We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of the CALIFA integral field spectroscopy data, scanning Fabry-Perot interferometry (FPI), and multiband photometry. We detect ionized gas in the extraplanar regions reaching a relatively high distance, up to ~ 4 kpc above the galactic disk. The ionized gas line ratios ([N ii]/Ha, [S ii]/Ha and [O i]/Ha) present an enhancement along the semi minor axis, in contrast with the values found at the disk, where they are compatible with ionization due to H ii-regions. These differences, together with the biconic sy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01695","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":"1701.01695","created_at":"2026-05-18T00:48:46.750436+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.01695v1","created_at":"2026-05-18T00:48:46.750436+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.01695","created_at":"2026-05-18T00:48:46.750436+00:00"},{"alias_kind":"pith_short_12","alias_value":"X5XXGSUN7UFE","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"X5XXGSUN7UFEH3ZW","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"X5XXGSUN","created_at":"2026-05-18T12:31:53.515858+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/X5XXGSUN7UFEH3ZWPJ2ACNJWNO","json":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO.json","graph_json":"https://pith.science/api/pith-number/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/graph.json","events_json":"https://pith.science/api/pith-number/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/events.json","paper":"https://pith.science/paper/X5XXGSUN"},"agent_actions":{"view_html":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO","download_json":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO.json","view_paper":"https://pith.science/paper/X5XXGSUN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.01695&json=true","fetch_graph":"https://pith.science/api/pith-number/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/graph.json","fetch_events":"https://pith.science/api/pith-number/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/action/storage_attestation","attest_author":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/action/author_attestation","sign_citation":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/action/citation_signature","submit_replication":"https://pith.science/pith/X5XXGSUN7UFEH3ZWPJ2ACNJWNO/action/replication_record"}},"created_at":"2026-05-18T00:48:46.750436+00:00","updated_at":"2026-05-18T00:48:46.750436+00:00"}