{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:WTRDMSSM3YE2SLDTP6TBF5466T","short_pith_number":"pith:WTRDMSSM","schema_version":"1.0","canonical_sha256":"b4e2364a4cde09a92c737fa612f79ef4ee43c9101f4249a98769dd0c42002203","source":{"kind":"arxiv","id":"1011.6226","version":2},"attestation_state":"computed","paper":{"title":"Spatial distribution of stellar populations in the Magellanic Clouds: Implementation to Gaia","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2), (2) Sofia University St.Kliment Ohridski, (3) National Observatory of Athens), E. Kontizas (3) ((1) National, E. Livanou (1), G. B. Nikolov (1, Kapodistrian University of Athens, M. K. Belcheva (1), M. Kontizas (1)","submitted_at":"2010-11-29T13:49:04Z","abstract_excerpt":"The main goal of our project is to investigate the spatial distribution of different stellar populations in the Magellanic Clouds. The results from modelling the Magellanic Clouds can be useful, among others, for simulations during the Gaia mission preparation. Isodensity contour maps have been used in order to trace the morphology of the different stellar populations and estimate the size of these structures. Moreover, star density maps are constructed through star counts and projected radial density profiles are obtained. Fitting exponential disk and King law curves to the spatial distributi"},"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":"1011.6226","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-11-29T13:49:04Z","cross_cats_sorted":[],"title_canon_sha256":"6a41bf4ba1515f1994ee984287e79d3549afc1d9bd6d5992b069fb6c7b261df4","abstract_canon_sha256":"c402cd839ab08d337bd531283919226f4defb71271c824349f640a0e1207dee7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:37.991487Z","signature_b64":"1Bysgi6x065plOAuz3Pyo+6jRmPC6nPUjC7qPXGJe0S5w3KX7JGtC42DDlRDX2B6PRIa0DWXYcCA2P41aONcAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b4e2364a4cde09a92c737fa612f79ef4ee43c9101f4249a98769dd0c42002203","last_reissued_at":"2026-05-18T02:04:37.990766Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:37.990766Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spatial distribution of stellar populations in the Magellanic Clouds: Implementation to Gaia","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2), (2) Sofia University St.Kliment Ohridski, (3) National Observatory of Athens), E. Kontizas (3) ((1) National, E. Livanou (1), G. B. Nikolov (1, Kapodistrian University of Athens, M. K. Belcheva (1), M. Kontizas (1)","submitted_at":"2010-11-29T13:49:04Z","abstract_excerpt":"The main goal of our project is to investigate the spatial distribution of different stellar populations in the Magellanic Clouds. The results from modelling the Magellanic Clouds can be useful, among others, for simulations during the Gaia mission preparation. Isodensity contour maps have been used in order to trace the morphology of the different stellar populations and estimate the size of these structures. Moreover, star density maps are constructed through star counts and projected radial density profiles are obtained. Fitting exponential disk and King law curves to the spatial distributi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.6226","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":"1011.6226","created_at":"2026-05-18T02:04:37.990875+00:00"},{"alias_kind":"arxiv_version","alias_value":"1011.6226v2","created_at":"2026-05-18T02:04:37.990875+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.6226","created_at":"2026-05-18T02:04:37.990875+00:00"},{"alias_kind":"pith_short_12","alias_value":"WTRDMSSM3YE2","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"WTRDMSSM3YE2SLDT","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"WTRDMSSM","created_at":"2026-05-18T12:26:17.028572+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/WTRDMSSM3YE2SLDTP6TBF5466T","json":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T.json","graph_json":"https://pith.science/api/pith-number/WTRDMSSM3YE2SLDTP6TBF5466T/graph.json","events_json":"https://pith.science/api/pith-number/WTRDMSSM3YE2SLDTP6TBF5466T/events.json","paper":"https://pith.science/paper/WTRDMSSM"},"agent_actions":{"view_html":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T","download_json":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T.json","view_paper":"https://pith.science/paper/WTRDMSSM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1011.6226&json=true","fetch_graph":"https://pith.science/api/pith-number/WTRDMSSM3YE2SLDTP6TBF5466T/graph.json","fetch_events":"https://pith.science/api/pith-number/WTRDMSSM3YE2SLDTP6TBF5466T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T/action/storage_attestation","attest_author":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T/action/author_attestation","sign_citation":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T/action/citation_signature","submit_replication":"https://pith.science/pith/WTRDMSSM3YE2SLDTP6TBF5466T/action/replication_record"}},"created_at":"2026-05-18T02:04:37.990875+00:00","updated_at":"2026-05-18T02:04:37.990875+00:00"}