{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:UMU2F5LNUTMBWGSVH4P6ZKHT7A","short_pith_number":"pith:UMU2F5LN","schema_version":"1.0","canonical_sha256":"a329a2f56da4d81b1a553f1feca8f3f83d7e849ddbdb098e5fa28bb5f1e83782","source":{"kind":"arxiv","id":"2505.19844","version":1},"attestation_state":"computed","paper":{"title":"Magnetic fields in the massive star-forming region NGC 6334 and their relationship with the properties of dust filaments probed by [CII] and PAH emissions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akiko Yasuda, Devendra Ojha, Hayata Tsuji, Hidehiro Kaneda, Joe P. Ninan, Koshvendra Singh, Shinki Oyabu, Swarna K. Ghosh, Takayoshi Kusune, Toyoaki Suzuki","submitted_at":"2025-05-26T11:28:00Z","abstract_excerpt":"We carried out the near-infrared ($JHK_{\\rm s}$) imaging polarimetric observation with the polarimeter SIRPOL on the Infrared Survey Facility (IRSF) 1.4 m telescope and [CII] line mapping observation with a Fabry-P\\'{e}rot spectrometer on board a 100-cm TIFR balloon-borne far-infrared telescope toward NGC 6334, and revealed the relationship between the plane-of-sky (POS) magnetic fields and [CII] emission lines to investigate the star formation in the molecular cloud. The polarization vector map shows that the POS magnetic fields are approximately perpendicular to the main filament elongation "},"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":"2505.19844","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-05-26T11:28:00Z","cross_cats_sorted":[],"title_canon_sha256":"a80bd9bc7b8823331e73c475880b50836944d7d75622b107c5caa027a330fa3c","abstract_canon_sha256":"1ab187df91202c3cc62913bb31aafa9e1aaee73de5ee42b14337c7b1dfddad89"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:09:48.843346Z","signature_b64":"spmLiw3VChEFI04fkzTjzEV7ds1BZrdNROgoU5Ba6bA/3uIo2M8mKUJKzLcIcAxQqmt7L2DuHriGMl4dpHh8Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a329a2f56da4d81b1a553f1feca8f3f83d7e849ddbdb098e5fa28bb5f1e83782","last_reissued_at":"2026-07-05T11:09:48.842815Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:09:48.842815Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetic fields in the massive star-forming region NGC 6334 and their relationship with the properties of dust filaments probed by [CII] and PAH emissions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akiko Yasuda, Devendra Ojha, Hayata Tsuji, Hidehiro Kaneda, Joe P. Ninan, Koshvendra Singh, Shinki Oyabu, Swarna K. Ghosh, Takayoshi Kusune, Toyoaki Suzuki","submitted_at":"2025-05-26T11:28:00Z","abstract_excerpt":"We carried out the near-infrared ($JHK_{\\rm s}$) imaging polarimetric observation with the polarimeter SIRPOL on the Infrared Survey Facility (IRSF) 1.4 m telescope and [CII] line mapping observation with a Fabry-P\\'{e}rot spectrometer on board a 100-cm TIFR balloon-borne far-infrared telescope toward NGC 6334, and revealed the relationship between the plane-of-sky (POS) magnetic fields and [CII] emission lines to investigate the star formation in the molecular cloud. The polarization vector map shows that the POS magnetic fields are approximately perpendicular to the main filament elongation "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.19844","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/2505.19844/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":"2505.19844","created_at":"2026-07-05T11:09:48.842886+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.19844v1","created_at":"2026-07-05T11:09:48.842886+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.19844","created_at":"2026-07-05T11:09:48.842886+00:00"},{"alias_kind":"pith_short_12","alias_value":"UMU2F5LNUTMB","created_at":"2026-07-05T11:09:48.842886+00:00"},{"alias_kind":"pith_short_16","alias_value":"UMU2F5LNUTMBWGSV","created_at":"2026-07-05T11:09:48.842886+00:00"},{"alias_kind":"pith_short_8","alias_value":"UMU2F5LN","created_at":"2026-07-05T11:09:48.842886+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/UMU2F5LNUTMBWGSVH4P6ZKHT7A","json":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A.json","graph_json":"https://pith.science/api/pith-number/UMU2F5LNUTMBWGSVH4P6ZKHT7A/graph.json","events_json":"https://pith.science/api/pith-number/UMU2F5LNUTMBWGSVH4P6ZKHT7A/events.json","paper":"https://pith.science/paper/UMU2F5LN"},"agent_actions":{"view_html":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A","download_json":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A.json","view_paper":"https://pith.science/paper/UMU2F5LN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.19844&json=true","fetch_graph":"https://pith.science/api/pith-number/UMU2F5LNUTMBWGSVH4P6ZKHT7A/graph.json","fetch_events":"https://pith.science/api/pith-number/UMU2F5LNUTMBWGSVH4P6ZKHT7A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A/action/storage_attestation","attest_author":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A/action/author_attestation","sign_citation":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A/action/citation_signature","submit_replication":"https://pith.science/pith/UMU2F5LNUTMBWGSVH4P6ZKHT7A/action/replication_record"}},"created_at":"2026-07-05T11:09:48.842886+00:00","updated_at":"2026-07-05T11:09:48.842886+00:00"}