{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:RHV5YMI3LHJAGUVUUF5LDHJQMS","short_pith_number":"pith:RHV5YMI3","schema_version":"1.0","canonical_sha256":"89ebdc311b59d20352b4a17ab19d3064b00913dccb1706bc7b6e3b32b5b0d405","source":{"kind":"arxiv","id":"1901.06723","version":1},"attestation_state":"computed","paper":{"title":"Hidden or missing outflows in highly obscured galaxy nuclei?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. S. Evans, C. Henkel, E. Gonz\\'alez-Alfonso, F. Combes, F. Hallqvist, G. A. Fuller, G. C. Privon, J. G. Mangum, J. S. Gallagher, K. Sakamoto, M. Imanishi, N. Falstad, P. P. van der Werf, R. Aladro, S. Aalto, S. Garc\\'ia-Burillo, S. K\\\"onig, S. Mart\\'in, S. Muller, S. Veilleux, T. Izumi, T. R. Greve","submitted_at":"2019-01-20T20:13:36Z","abstract_excerpt":"Understanding the nuclear growth and feedback processes in galaxies requires investigating their often obscured central regions. One way to do this is to use (sub)millimeter line emission from vibrationally excited HCN (HCN-vib). It has been suggested that the most intense HCN-vib emission from a galaxy is connected to a phase of nuclear growth that occurs before the nuclear feedback processes have been fully developed. We aim to investigate if there is a connection between the presence of strong HCN-vib emission and the development of feedback in (U)LIRGs. We collected literature and archival"},"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":"1901.06723","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-01-20T20:13:36Z","cross_cats_sorted":[],"title_canon_sha256":"7e0d58519917eaa76e5bb9f6fd5650f7a21f0711261d87aeeb6a7c96db2a5e50","abstract_canon_sha256":"83ad3c04b2b0147901ace2a5c1cd5ed18af8dffa488b501050cb05f785150778"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:38.341621Z","signature_b64":"9FX5P5gZCNeLZqUE9wqeFd/XEgapkK6gsy92aky11l2ju30dPNaF3M/o3ETJigOf94xazE8Rxi5BNUta52VxDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"89ebdc311b59d20352b4a17ab19d3064b00913dccb1706bc7b6e3b32b5b0d405","last_reissued_at":"2026-05-17T23:52:38.340870Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:38.340870Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hidden or missing outflows in highly obscured galaxy nuclei?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. S. Evans, C. Henkel, E. Gonz\\'alez-Alfonso, F. Combes, F. Hallqvist, G. A. Fuller, G. C. Privon, J. G. Mangum, J. S. Gallagher, K. Sakamoto, M. Imanishi, N. Falstad, P. P. van der Werf, R. Aladro, S. Aalto, S. Garc\\'ia-Burillo, S. K\\\"onig, S. Mart\\'in, S. Muller, S. Veilleux, T. Izumi, T. R. Greve","submitted_at":"2019-01-20T20:13:36Z","abstract_excerpt":"Understanding the nuclear growth and feedback processes in galaxies requires investigating their often obscured central regions. One way to do this is to use (sub)millimeter line emission from vibrationally excited HCN (HCN-vib). It has been suggested that the most intense HCN-vib emission from a galaxy is connected to a phase of nuclear growth that occurs before the nuclear feedback processes have been fully developed. We aim to investigate if there is a connection between the presence of strong HCN-vib emission and the development of feedback in (U)LIRGs. We collected literature and archival"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.06723","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":"1901.06723","created_at":"2026-05-17T23:52:38.340993+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.06723v1","created_at":"2026-05-17T23:52:38.340993+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.06723","created_at":"2026-05-17T23:52:38.340993+00:00"},{"alias_kind":"pith_short_12","alias_value":"RHV5YMI3LHJA","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_16","alias_value":"RHV5YMI3LHJAGUVU","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_8","alias_value":"RHV5YMI3","created_at":"2026-05-18T12:33:27.125529+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/RHV5YMI3LHJAGUVUUF5LDHJQMS","json":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS.json","graph_json":"https://pith.science/api/pith-number/RHV5YMI3LHJAGUVUUF5LDHJQMS/graph.json","events_json":"https://pith.science/api/pith-number/RHV5YMI3LHJAGUVUUF5LDHJQMS/events.json","paper":"https://pith.science/paper/RHV5YMI3"},"agent_actions":{"view_html":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS","download_json":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS.json","view_paper":"https://pith.science/paper/RHV5YMI3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.06723&json=true","fetch_graph":"https://pith.science/api/pith-number/RHV5YMI3LHJAGUVUUF5LDHJQMS/graph.json","fetch_events":"https://pith.science/api/pith-number/RHV5YMI3LHJAGUVUUF5LDHJQMS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS/action/storage_attestation","attest_author":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS/action/author_attestation","sign_citation":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS/action/citation_signature","submit_replication":"https://pith.science/pith/RHV5YMI3LHJAGUVUUF5LDHJQMS/action/replication_record"}},"created_at":"2026-05-17T23:52:38.340993+00:00","updated_at":"2026-05-17T23:52:38.340993+00:00"}