{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:AGABYA2TOOIIZIDJTMG4EKP5QH","short_pith_number":"pith:AGABYA2T","schema_version":"1.0","canonical_sha256":"01801c035373908ca0699b0dc229fd81f7adec51eefe4235f749507935378368","source":{"kind":"arxiv","id":"1502.02041","version":1},"attestation_state":"computed","paper":{"title":"NGC 1266: Characterization of the Nuclear Molecular Gas in an Unusual SB0 Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jason Glenn, Julia R. Kamenetzky, Naseem Rangwala, Philip R. Maloney","submitted_at":"2015-02-06T21:00:59Z","abstract_excerpt":"With a substantial nuclear molecular gas reservoir and broad, high-velocity CO molecular line wings previously interpreted as an outflow, NGC 1266 is a rare SB$0$ galaxy. Previous analyses of interferometry, spectrally resolved low-$J$ CO emission lines, and unresolved high-$J$ emission lines have established basic properties of the molecular gas and the likely presence of an AGN. Here, new spectrally resolved CO $J = 5 - 4$ to $J = 8 - 7$ lines from {\\it Herschel Space Observatory} HIFI observations are combined with ground-based observations and high-$J$ {\\it Herschel} SPIRE observations to "},"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":"1502.02041","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-02-06T21:00:59Z","cross_cats_sorted":[],"title_canon_sha256":"4980b43304a1decb9dbea0b81689417120eb8fb679b825ba3bc8c1c7b32dc9e9","abstract_canon_sha256":"5e4005ef9bc634bb18858b27437c65450e1442f1a4c519bbfbd25cf59f69c566"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:04.346955Z","signature_b64":"McMbh5u4yWjCG6GwBSAA48cuI/BDajJadZlsfqUrac/c7Za8ukWC9gdtYWDsvKefrn5KUI1mHIPyWrzFW+T0Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"01801c035373908ca0699b0dc229fd81f7adec51eefe4235f749507935378368","last_reissued_at":"2026-05-18T01:41:04.346371Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:04.346371Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"NGC 1266: Characterization of the Nuclear Molecular Gas in an Unusual SB0 Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jason Glenn, Julia R. Kamenetzky, Naseem Rangwala, Philip R. Maloney","submitted_at":"2015-02-06T21:00:59Z","abstract_excerpt":"With a substantial nuclear molecular gas reservoir and broad, high-velocity CO molecular line wings previously interpreted as an outflow, NGC 1266 is a rare SB$0$ galaxy. Previous analyses of interferometry, spectrally resolved low-$J$ CO emission lines, and unresolved high-$J$ emission lines have established basic properties of the molecular gas and the likely presence of an AGN. Here, new spectrally resolved CO $J = 5 - 4$ to $J = 8 - 7$ lines from {\\it Herschel Space Observatory} HIFI observations are combined with ground-based observations and high-$J$ {\\it Herschel} SPIRE observations to "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.02041","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":"1502.02041","created_at":"2026-05-18T01:41:04.346460+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.02041v1","created_at":"2026-05-18T01:41:04.346460+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.02041","created_at":"2026-05-18T01:41:04.346460+00:00"},{"alias_kind":"pith_short_12","alias_value":"AGABYA2TOOII","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_16","alias_value":"AGABYA2TOOIIZIDJ","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_8","alias_value":"AGABYA2T","created_at":"2026-05-18T12:29:10.953037+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/AGABYA2TOOIIZIDJTMG4EKP5QH","json":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH.json","graph_json":"https://pith.science/api/pith-number/AGABYA2TOOIIZIDJTMG4EKP5QH/graph.json","events_json":"https://pith.science/api/pith-number/AGABYA2TOOIIZIDJTMG4EKP5QH/events.json","paper":"https://pith.science/paper/AGABYA2T"},"agent_actions":{"view_html":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH","download_json":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH.json","view_paper":"https://pith.science/paper/AGABYA2T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.02041&json=true","fetch_graph":"https://pith.science/api/pith-number/AGABYA2TOOIIZIDJTMG4EKP5QH/graph.json","fetch_events":"https://pith.science/api/pith-number/AGABYA2TOOIIZIDJTMG4EKP5QH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH/action/storage_attestation","attest_author":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH/action/author_attestation","sign_citation":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH/action/citation_signature","submit_replication":"https://pith.science/pith/AGABYA2TOOIIZIDJTMG4EKP5QH/action/replication_record"}},"created_at":"2026-05-18T01:41:04.346460+00:00","updated_at":"2026-05-18T01:41:04.346460+00:00"}