{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:G76JCKL73BKLKSWVSLI3ZNFBEM","short_pith_number":"pith:G76JCKL7","schema_version":"1.0","canonical_sha256":"37fc91297fd854b54ad592d1bcb4a123001623e977d539f43766bf5cf0922fdd","source":{"kind":"arxiv","id":"2503.17519","version":1},"attestation_state":"computed","paper":{"title":"Interstellar gas motions around massive star formation regions in the nearby dwarf galaxy DDO 43","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'as P\\'eter Jo\\'o, Bendeg\\'uz Koncz, Enik\\H{o} Pichler, Krisztina \\'E. Gab\\'anyi, L. Viktor T\\'oth","submitted_at":"2025-03-21T20:06:01Z","abstract_excerpt":"Areas of massive star formation are strongly influenced by stellar winds and supernovae, therefore, enhanced turbulent flows are expected. We analyse high-quality Karl G. Jansky Very Large Array observations of the neutral hydrogen gas content of DDO 43, a relatively nearby irregular dwarf galaxy. The line wings of neutral hydrogen spectral lines, which provide insights into local enhanced velocity dispersion, are investigated together with far-ultraviolet data, tracing emissions from massive star-forming regions. We find very weak correlations with both higher and lower velocity areas."},"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":"2503.17519","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-03-21T20:06:01Z","cross_cats_sorted":[],"title_canon_sha256":"0716e622dfaacfb4196692e1c65dfa0e06d8f3bfede6c91fdf7095b20de92f52","abstract_canon_sha256":"4ce7e0907a9dfb375456814a21700503eeb3964795ef6de5281616d72eefe965"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:37:11.255275Z","signature_b64":"NoZuqjn1LLfHPoI9ViUKH1ZRwNVleVlYZ3bKw1ZQhAItVyJnB/zdlWxbG3ZuDsa6gZ7xGdVkaexCXxhushUuBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"37fc91297fd854b54ad592d1bcb4a123001623e977d539f43766bf5cf0922fdd","last_reissued_at":"2026-07-05T10:37:11.254211Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:37:11.254211Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interstellar gas motions around massive star formation regions in the nearby dwarf galaxy DDO 43","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'as P\\'eter Jo\\'o, Bendeg\\'uz Koncz, Enik\\H{o} Pichler, Krisztina \\'E. Gab\\'anyi, L. Viktor T\\'oth","submitted_at":"2025-03-21T20:06:01Z","abstract_excerpt":"Areas of massive star formation are strongly influenced by stellar winds and supernovae, therefore, enhanced turbulent flows are expected. We analyse high-quality Karl G. Jansky Very Large Array observations of the neutral hydrogen gas content of DDO 43, a relatively nearby irregular dwarf galaxy. The line wings of neutral hydrogen spectral lines, which provide insights into local enhanced velocity dispersion, are investigated together with far-ultraviolet data, tracing emissions from massive star-forming regions. We find very weak correlations with both higher and lower velocity areas."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.17519","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2503.17519/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2503.17519","created_at":"2026-07-05T10:37:11.254384+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.17519v1","created_at":"2026-07-05T10:37:11.254384+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.17519","created_at":"2026-07-05T10:37:11.254384+00:00"},{"alias_kind":"pith_short_12","alias_value":"G76JCKL73BKL","created_at":"2026-07-05T10:37:11.254384+00:00"},{"alias_kind":"pith_short_16","alias_value":"G76JCKL73BKLKSWV","created_at":"2026-07-05T10:37:11.254384+00:00"},{"alias_kind":"pith_short_8","alias_value":"G76JCKL7","created_at":"2026-07-05T10:37:11.254384+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/G76JCKL73BKLKSWVSLI3ZNFBEM","json":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM.json","graph_json":"https://pith.science/api/pith-number/G76JCKL73BKLKSWVSLI3ZNFBEM/graph.json","events_json":"https://pith.science/api/pith-number/G76JCKL73BKLKSWVSLI3ZNFBEM/events.json","paper":"https://pith.science/paper/G76JCKL7"},"agent_actions":{"view_html":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM","download_json":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM.json","view_paper":"https://pith.science/paper/G76JCKL7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.17519&json=true","fetch_graph":"https://pith.science/api/pith-number/G76JCKL73BKLKSWVSLI3ZNFBEM/graph.json","fetch_events":"https://pith.science/api/pith-number/G76JCKL73BKLKSWVSLI3ZNFBEM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM/action/storage_attestation","attest_author":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM/action/author_attestation","sign_citation":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM/action/citation_signature","submit_replication":"https://pith.science/pith/G76JCKL73BKLKSWVSLI3ZNFBEM/action/replication_record"}},"created_at":"2026-07-05T10:37:11.254384+00:00","updated_at":"2026-07-05T10:37:11.254384+00:00"}