{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:VEQJNER6NHR5T7XUUWEDY7XGRT","short_pith_number":"pith:VEQJNER6","schema_version":"1.0","canonical_sha256":"a92096923e69e3d9fef4a5883c7ee68ccc7fc9c266e5a3582d201a657376b7a9","source":{"kind":"arxiv","id":"1408.7080","version":1},"attestation_state":"computed","paper":{"title":"Dynamical evolution of V-type photometric candidates in the outer Main-belt","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Mariela E. Huaman, Rita Cassia Domingos, Valerio Carruba","submitted_at":"2014-08-29T17:27:18Z","abstract_excerpt":"V-type asteroids, characterized by two absorption bands at 1.0 and 2.0 $\\mu m$, are usually thought to be portions of the crust of differentiated or partially differentiated bodies. Most V-type asteroids are found in the inner main belt and are thought to be current or past members of the Vesta dynamical family. Recently, several V-type photometric candidates have been identified in the central and outer main belt.\n  While the dynamical evolution of V-type photometric candidates in the central main belt has been recently investigated, less attention has been given to the orbital evolution of b"},"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":"1408.7080","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-08-29T17:27:18Z","cross_cats_sorted":[],"title_canon_sha256":"48128e107647a14c1419d3e056d4ab35bc2771b6f1a44d82f1138813c7e98d66","abstract_canon_sha256":"67d6499b694ccb20ca63610eaf634958161de73f50832598755fb4dd96f355dd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:11.687263Z","signature_b64":"moIFpcYBe75U6rld+DbFhmwmdeqY6r7/oX5p7/4EyjHSPPbRDLjfRu5j9TZ/UmgTow35o60JJiJoQYP3rtgzBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a92096923e69e3d9fef4a5883c7ee68ccc7fc9c266e5a3582d201a657376b7a9","last_reissued_at":"2026-05-18T01:42:11.686716Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:11.686716Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamical evolution of V-type photometric candidates in the outer Main-belt","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Mariela E. Huaman, Rita Cassia Domingos, Valerio Carruba","submitted_at":"2014-08-29T17:27:18Z","abstract_excerpt":"V-type asteroids, characterized by two absorption bands at 1.0 and 2.0 $\\mu m$, are usually thought to be portions of the crust of differentiated or partially differentiated bodies. Most V-type asteroids are found in the inner main belt and are thought to be current or past members of the Vesta dynamical family. Recently, several V-type photometric candidates have been identified in the central and outer main belt.\n  While the dynamical evolution of V-type photometric candidates in the central main belt has been recently investigated, less attention has been given to the orbital evolution of b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.7080","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":"1408.7080","created_at":"2026-05-18T01:42:11.686792+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.7080v1","created_at":"2026-05-18T01:42:11.686792+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.7080","created_at":"2026-05-18T01:42:11.686792+00:00"},{"alias_kind":"pith_short_12","alias_value":"VEQJNER6NHR5","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"VEQJNER6NHR5T7XU","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"VEQJNER6","created_at":"2026-05-18T12:28:52.271510+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/VEQJNER6NHR5T7XUUWEDY7XGRT","json":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT.json","graph_json":"https://pith.science/api/pith-number/VEQJNER6NHR5T7XUUWEDY7XGRT/graph.json","events_json":"https://pith.science/api/pith-number/VEQJNER6NHR5T7XUUWEDY7XGRT/events.json","paper":"https://pith.science/paper/VEQJNER6"},"agent_actions":{"view_html":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT","download_json":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT.json","view_paper":"https://pith.science/paper/VEQJNER6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.7080&json=true","fetch_graph":"https://pith.science/api/pith-number/VEQJNER6NHR5T7XUUWEDY7XGRT/graph.json","fetch_events":"https://pith.science/api/pith-number/VEQJNER6NHR5T7XUUWEDY7XGRT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT/action/storage_attestation","attest_author":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT/action/author_attestation","sign_citation":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT/action/citation_signature","submit_replication":"https://pith.science/pith/VEQJNER6NHR5T7XUUWEDY7XGRT/action/replication_record"}},"created_at":"2026-05-18T01:42:11.686792+00:00","updated_at":"2026-05-18T01:42:11.686792+00:00"}