{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:Q22SZNXOXPLLZZQKJXQXB6ODQY","short_pith_number":"pith:Q22SZNXO","schema_version":"1.0","canonical_sha256":"86b52cb6eebbd6bce60a4de170f9c38613cac39592edbfaceb9001e8d7d1074a","source":{"kind":"arxiv","id":"1805.06496","version":1},"attestation_state":"computed","paper":{"title":"Herschel Planetary Nebula Survey (HerPlaNS): Hydrogen Recombination Laser Lines in Mz 3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. G. G. M. Tielens, Albert Zijlstra, Edgar Mendoza, Eva Villaver, Isabel Aleman, Jacques D. R. Lepine, Katrina Exter, Marcelo L. Leal-Ferreira, Masaaki Otsuka, Pedro P. B. Beaklini, Peter A. M. van Hoof, Rodolfo Montez Jr., Samuel Walton, Toshiya Ueta, Zulema Abraham","submitted_at":"2018-05-16T19:14:01Z","abstract_excerpt":"The bipolar nebula Menzel 3 (Mz 3) was observed as part of the \\textit{Herschel} Planetary Nebula Survey (\\textit{HerPlaNS}), which used the PACS and SPIRE instruments aboard the \\textit{Herschel Space Observatory} to study a sample of planetary nebulae (PNe). In this paper, one of the series describing \\textit{HerPlaNS} results, we report the detection of H I recombination lines (HRLs) in the spectrum of Mz 3. Inspection of the spectrum reveals the presence of 12 HRLs in the 55 to 680 $\\mu$m range covered by the PACS and SPIRE instruments (H11$\\alpha$ to H21$\\alpha$ and H14$\\beta$). The prese"},"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":"1805.06496","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-05-16T19:14:01Z","cross_cats_sorted":[],"title_canon_sha256":"ca33ae63c64ec3cd8f85dbebc35adf3a72a0b7cb894100de820f709a5c2e83a4","abstract_canon_sha256":"4c362afd0d115b532b4247799ba1f5853a8674b153f00c6333a27a50c73662f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:15:46.132424Z","signature_b64":"54yXVEppWc+gCBDN5pwrP33WudEK6CTUE3AqjeN3QjdNps8WFx9eVJP0osNBhX79RnuPoZ35GpJYwZ3kQt1nDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"86b52cb6eebbd6bce60a4de170f9c38613cac39592edbfaceb9001e8d7d1074a","last_reissued_at":"2026-05-18T00:15:46.131771Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:15:46.131771Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel Planetary Nebula Survey (HerPlaNS): Hydrogen Recombination Laser Lines in Mz 3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. G. G. M. Tielens, Albert Zijlstra, Edgar Mendoza, Eva Villaver, Isabel Aleman, Jacques D. R. Lepine, Katrina Exter, Marcelo L. Leal-Ferreira, Masaaki Otsuka, Pedro P. B. Beaklini, Peter A. M. van Hoof, Rodolfo Montez Jr., Samuel Walton, Toshiya Ueta, Zulema Abraham","submitted_at":"2018-05-16T19:14:01Z","abstract_excerpt":"The bipolar nebula Menzel 3 (Mz 3) was observed as part of the \\textit{Herschel} Planetary Nebula Survey (\\textit{HerPlaNS}), which used the PACS and SPIRE instruments aboard the \\textit{Herschel Space Observatory} to study a sample of planetary nebulae (PNe). In this paper, one of the series describing \\textit{HerPlaNS} results, we report the detection of H I recombination lines (HRLs) in the spectrum of Mz 3. Inspection of the spectrum reveals the presence of 12 HRLs in the 55 to 680 $\\mu$m range covered by the PACS and SPIRE instruments (H11$\\alpha$ to H21$\\alpha$ and H14$\\beta$). The prese"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.06496","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":"1805.06496","created_at":"2026-05-18T00:15:46.131862+00:00"},{"alias_kind":"arxiv_version","alias_value":"1805.06496v1","created_at":"2026-05-18T00:15:46.131862+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1805.06496","created_at":"2026-05-18T00:15:46.131862+00:00"},{"alias_kind":"pith_short_12","alias_value":"Q22SZNXOXPLL","created_at":"2026-05-18T12:32:46.962924+00:00"},{"alias_kind":"pith_short_16","alias_value":"Q22SZNXOXPLLZZQK","created_at":"2026-05-18T12:32:46.962924+00:00"},{"alias_kind":"pith_short_8","alias_value":"Q22SZNXO","created_at":"2026-05-18T12:32:46.962924+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/Q22SZNXOXPLLZZQKJXQXB6ODQY","json":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY.json","graph_json":"https://pith.science/api/pith-number/Q22SZNXOXPLLZZQKJXQXB6ODQY/graph.json","events_json":"https://pith.science/api/pith-number/Q22SZNXOXPLLZZQKJXQXB6ODQY/events.json","paper":"https://pith.science/paper/Q22SZNXO"},"agent_actions":{"view_html":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY","download_json":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY.json","view_paper":"https://pith.science/paper/Q22SZNXO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1805.06496&json=true","fetch_graph":"https://pith.science/api/pith-number/Q22SZNXOXPLLZZQKJXQXB6ODQY/graph.json","fetch_events":"https://pith.science/api/pith-number/Q22SZNXOXPLLZZQKJXQXB6ODQY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY/action/storage_attestation","attest_author":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY/action/author_attestation","sign_citation":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY/action/citation_signature","submit_replication":"https://pith.science/pith/Q22SZNXOXPLLZZQKJXQXB6ODQY/action/replication_record"}},"created_at":"2026-05-18T00:15:46.131862+00:00","updated_at":"2026-05-18T00:15:46.131862+00:00"}