{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:WEWEEP2RW3VC34QAUCQJUVS6WZ","short_pith_number":"pith:WEWEEP2R","schema_version":"1.0","canonical_sha256":"b12c423f51b6ea2df200a0a09a565eb65a170876afc60c8050d45536387646f0","source":{"kind":"arxiv","id":"1505.04705","version":2},"attestation_state":"computed","paper":{"title":"High-resolution imaging of the molecular outflows in two mergers: IRAS17208-0014 and NGC1614","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Alonso-Herrero, A. Labiano, A. Usero, F. Combes, F. Costagliola, L. Colina, L. J. Tacconi, L. K. Hunt, M. Pereira-Santaella, P. P. van der Werf, R. Neri, S. Aalto, S. Arribas, S. Garcia-Burillo","submitted_at":"2015-05-18T16:22:07Z","abstract_excerpt":"Galaxy evolution scenarios predict that the feedback of star formation and nuclear activity (AGN) can drive the transformation of gas-rich spiral mergers into ULIRGs, and, eventually, lead to the build-up of QSO/elliptical hosts. We study the role that star formation and AGN feedback have in launching and maintaining the molecular outflows in two starburst-dominated advanced mergers, NGC1614 and IRAS17208-0014, by analyzing the distribution and kinematics of their molecular gas reservoirs. We have used the PdBI array to image with high spatial resolution (0.5\"-1.2\") the CO(1-0) and CO(2-1) lin"},"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":"1505.04705","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-05-18T16:22:07Z","cross_cats_sorted":[],"title_canon_sha256":"4c99d9635e93f18b60a7636a896bb0fd217d934d987e26697b41f117c9c0a873","abstract_canon_sha256":"1c283645e851540898497f637f518d59327e551c1b4dbc9025062759a9d74d59"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:12.916705Z","signature_b64":"PgzAFvf7th5zPCg1IgjJncI+OoJ+k6m5bbuTh628QCSPKo+ioSOrYG7rnNdBc0otEx+IsCg+1klXcVDZnLX7CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b12c423f51b6ea2df200a0a09a565eb65a170876afc60c8050d45536387646f0","last_reissued_at":"2026-05-18T01:36:12.916125Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:12.916125Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-resolution imaging of the molecular outflows in two mergers: IRAS17208-0014 and NGC1614","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Alonso-Herrero, A. Labiano, A. Usero, F. Combes, F. Costagliola, L. Colina, L. J. Tacconi, L. K. Hunt, M. Pereira-Santaella, P. P. van der Werf, R. Neri, S. Aalto, S. Arribas, S. Garcia-Burillo","submitted_at":"2015-05-18T16:22:07Z","abstract_excerpt":"Galaxy evolution scenarios predict that the feedback of star formation and nuclear activity (AGN) can drive the transformation of gas-rich spiral mergers into ULIRGs, and, eventually, lead to the build-up of QSO/elliptical hosts. We study the role that star formation and AGN feedback have in launching and maintaining the molecular outflows in two starburst-dominated advanced mergers, NGC1614 and IRAS17208-0014, by analyzing the distribution and kinematics of their molecular gas reservoirs. We have used the PdBI array to image with high spatial resolution (0.5\"-1.2\") the CO(1-0) and CO(2-1) lin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.04705","kind":"arxiv","version":2},"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":"1505.04705","created_at":"2026-05-18T01:36:12.916218+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.04705v2","created_at":"2026-05-18T01:36:12.916218+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.04705","created_at":"2026-05-18T01:36:12.916218+00:00"},{"alias_kind":"pith_short_12","alias_value":"WEWEEP2RW3VC","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"WEWEEP2RW3VC34QA","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"WEWEEP2R","created_at":"2026-05-18T12:29:47.479230+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/WEWEEP2RW3VC34QAUCQJUVS6WZ","json":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ.json","graph_json":"https://pith.science/api/pith-number/WEWEEP2RW3VC34QAUCQJUVS6WZ/graph.json","events_json":"https://pith.science/api/pith-number/WEWEEP2RW3VC34QAUCQJUVS6WZ/events.json","paper":"https://pith.science/paper/WEWEEP2R"},"agent_actions":{"view_html":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ","download_json":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ.json","view_paper":"https://pith.science/paper/WEWEEP2R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.04705&json=true","fetch_graph":"https://pith.science/api/pith-number/WEWEEP2RW3VC34QAUCQJUVS6WZ/graph.json","fetch_events":"https://pith.science/api/pith-number/WEWEEP2RW3VC34QAUCQJUVS6WZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ/action/storage_attestation","attest_author":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ/action/author_attestation","sign_citation":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ/action/citation_signature","submit_replication":"https://pith.science/pith/WEWEEP2RW3VC34QAUCQJUVS6WZ/action/replication_record"}},"created_at":"2026-05-18T01:36:12.916218+00:00","updated_at":"2026-05-18T01:36:12.916218+00:00"}