{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AU7QN2PJOTPLJ7DZVPTGS63C6U","short_pith_number":"pith:AU7QN2PJ","schema_version":"1.0","canonical_sha256":"053f06e9e974deb4fc79abe6697b62f5058421e0c7e5b54c15f16e8887c5d465","source":{"kind":"arxiv","id":"1707.05293","version":1},"attestation_state":"computed","paper":{"title":"The PyCASSO database: Spatially resolved stellar population properties for CALIFA galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. L. de Amorim, C. Cortijo-Ferrero, E. A. D. Lacerda, E. P\\'erez, N. Vale Asari, R. Cid Fernandes, R. Garc\\'ia-Benito, R. L\\'opez Fern\\'andez, R. M. Gonz\\'alez Delgado","submitted_at":"2017-07-17T17:41:09Z","abstract_excerpt":"The Calar Alto Legacy Integral Field Area (CALIFA) survey, a pioneer in integral field spectroscopy legacy projects, has fostered many studies exploring the information encoded on the spatially resolved data on gaseous and stellar features in the optical range of galaxies. We describe a value-added catalogue of stellar population properties for CALIFA galaxies analysed with the spectral synthesis code STARLIGHT and processed with the PyCASSO platform. Our public data base (http://pycasso.ufsc.br/, mirror at http://pycasso.iaa.es/) comprises 445 galaxies from the CALIFA Data Release 3 with COMB"},"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":"1707.05293","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-07-17T17:41:09Z","cross_cats_sorted":[],"title_canon_sha256":"647794b0b819ed27f675bacf95bddb1b59b40213b266d21d681c613a6436edc2","abstract_canon_sha256":"92bf38fd49e2f289cefd80bf85a4893f20e8879f5c24c771fcf4878fb9b14df7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:08.995879Z","signature_b64":"5espjHLy2k45NKHGJMOw6gFwOj6oY16mO7HaXWoNvMVQd7rhKhxTQqLezs7xbg8gsb1wB3FIgC3Dmki1UyJ7DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"053f06e9e974deb4fc79abe6697b62f5058421e0c7e5b54c15f16e8887c5d465","last_reissued_at":"2026-05-18T00:40:08.995218Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:08.995218Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The PyCASSO database: Spatially resolved stellar population properties for CALIFA galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. L. de Amorim, C. Cortijo-Ferrero, E. A. D. Lacerda, E. P\\'erez, N. Vale Asari, R. Cid Fernandes, R. Garc\\'ia-Benito, R. L\\'opez Fern\\'andez, R. M. Gonz\\'alez Delgado","submitted_at":"2017-07-17T17:41:09Z","abstract_excerpt":"The Calar Alto Legacy Integral Field Area (CALIFA) survey, a pioneer in integral field spectroscopy legacy projects, has fostered many studies exploring the information encoded on the spatially resolved data on gaseous and stellar features in the optical range of galaxies. We describe a value-added catalogue of stellar population properties for CALIFA galaxies analysed with the spectral synthesis code STARLIGHT and processed with the PyCASSO platform. Our public data base (http://pycasso.ufsc.br/, mirror at http://pycasso.iaa.es/) comprises 445 galaxies from the CALIFA Data Release 3 with COMB"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.05293","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":"1707.05293","created_at":"2026-05-18T00:40:08.995308+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.05293v1","created_at":"2026-05-18T00:40:08.995308+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.05293","created_at":"2026-05-18T00:40:08.995308+00:00"},{"alias_kind":"pith_short_12","alias_value":"AU7QN2PJOTPL","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_16","alias_value":"AU7QN2PJOTPLJ7DZ","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_8","alias_value":"AU7QN2PJ","created_at":"2026-05-18T12:31:08.081275+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/AU7QN2PJOTPLJ7DZVPTGS63C6U","json":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U.json","graph_json":"https://pith.science/api/pith-number/AU7QN2PJOTPLJ7DZVPTGS63C6U/graph.json","events_json":"https://pith.science/api/pith-number/AU7QN2PJOTPLJ7DZVPTGS63C6U/events.json","paper":"https://pith.science/paper/AU7QN2PJ"},"agent_actions":{"view_html":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U","download_json":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U.json","view_paper":"https://pith.science/paper/AU7QN2PJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.05293&json=true","fetch_graph":"https://pith.science/api/pith-number/AU7QN2PJOTPLJ7DZVPTGS63C6U/graph.json","fetch_events":"https://pith.science/api/pith-number/AU7QN2PJOTPLJ7DZVPTGS63C6U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U/action/storage_attestation","attest_author":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U/action/author_attestation","sign_citation":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U/action/citation_signature","submit_replication":"https://pith.science/pith/AU7QN2PJOTPLJ7DZVPTGS63C6U/action/replication_record"}},"created_at":"2026-05-18T00:40:08.995308+00:00","updated_at":"2026-05-18T00:40:08.995308+00:00"}