{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:MHNN66PPRH6CBZGC57JH6TPNTM","short_pith_number":"pith:MHNN66PP","schema_version":"1.0","canonical_sha256":"61dadf79ef89fc20e4c2efd27f4ded9b346b0896a134dfac4bce6542ca1e9794","source":{"kind":"arxiv","id":"1603.03441","version":1},"attestation_state":"computed","paper":{"title":"Distinguishing `disks' from `mergers': tracing the kinematic asymmetries in local (U)LIRGs using `kinemetry'-based criteria","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Enrica Bellocchi, Luis Colina, Santiago Arribas","submitted_at":"2016-03-10T21:00:23Z","abstract_excerpt":"The kinematic characterization of different galaxy populations is a key observational input to distinguish between different galaxy evolutionary scenarios, since it helps to determine the number ratio of rotating disks to mergers at different cosmic epochs. Local (U)LIRGs offer a unique opportunity to study at high linear resolution and S/N extreme star forming events and compare them with those observed at high-z. We obtained Very Large Telescope (VLT) VIMOS optical integral field spectroscopy (IFS) data of a sample of 38 (U)LIRGs. The `unweighted' and `weighted' {kinemetry}-based methods are"},"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":"1603.03441","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-03-10T21:00:23Z","cross_cats_sorted":[],"title_canon_sha256":"36de60b2e48ff4b596137693da50a0e9d219d9b8fc6f245be98186bc9084b572","abstract_canon_sha256":"f927aca40bdad27f373de9e432d99a8fdb1ed1ebdd317551d75680900f97b349"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:04.324916Z","signature_b64":"+xx8HwAKThSSpDi/WdlTcw2UzoMt/H8mLk6eJgR7qTItRY3f+yWzktLWdebgVmgWf7OhpnjYhSm/Xv6A4Y10DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"61dadf79ef89fc20e4c2efd27f4ded9b346b0896a134dfac4bce6542ca1e9794","last_reissued_at":"2026-05-18T01:12:04.324574Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:04.324574Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Distinguishing `disks' from `mergers': tracing the kinematic asymmetries in local (U)LIRGs using `kinemetry'-based criteria","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Enrica Bellocchi, Luis Colina, Santiago Arribas","submitted_at":"2016-03-10T21:00:23Z","abstract_excerpt":"The kinematic characterization of different galaxy populations is a key observational input to distinguish between different galaxy evolutionary scenarios, since it helps to determine the number ratio of rotating disks to mergers at different cosmic epochs. Local (U)LIRGs offer a unique opportunity to study at high linear resolution and S/N extreme star forming events and compare them with those observed at high-z. We obtained Very Large Telescope (VLT) VIMOS optical integral field spectroscopy (IFS) data of a sample of 38 (U)LIRGs. The `unweighted' and `weighted' {kinemetry}-based methods are"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.03441","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":"1603.03441","created_at":"2026-05-18T01:12:04.324633+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.03441v1","created_at":"2026-05-18T01:12:04.324633+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.03441","created_at":"2026-05-18T01:12:04.324633+00:00"},{"alias_kind":"pith_short_12","alias_value":"MHNN66PPRH6C","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_16","alias_value":"MHNN66PPRH6CBZGC","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_8","alias_value":"MHNN66PP","created_at":"2026-05-18T12:30:32.724797+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/MHNN66PPRH6CBZGC57JH6TPNTM","json":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM.json","graph_json":"https://pith.science/api/pith-number/MHNN66PPRH6CBZGC57JH6TPNTM/graph.json","events_json":"https://pith.science/api/pith-number/MHNN66PPRH6CBZGC57JH6TPNTM/events.json","paper":"https://pith.science/paper/MHNN66PP"},"agent_actions":{"view_html":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM","download_json":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM.json","view_paper":"https://pith.science/paper/MHNN66PP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.03441&json=true","fetch_graph":"https://pith.science/api/pith-number/MHNN66PPRH6CBZGC57JH6TPNTM/graph.json","fetch_events":"https://pith.science/api/pith-number/MHNN66PPRH6CBZGC57JH6TPNTM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM/action/storage_attestation","attest_author":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM/action/author_attestation","sign_citation":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM/action/citation_signature","submit_replication":"https://pith.science/pith/MHNN66PPRH6CBZGC57JH6TPNTM/action/replication_record"}},"created_at":"2026-05-18T01:12:04.324633+00:00","updated_at":"2026-05-18T01:12:04.324633+00:00"}