{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KALC4H5OKUCPPWR5YPXLA3HPE3","short_pith_number":"pith:KALC4H5O","schema_version":"1.0","canonical_sha256":"50162e1fae5504f7da3dc3eeb06cef26feb8f743062271cb82262407ceaa123e","source":{"kind":"arxiv","id":"1711.01839","version":1},"attestation_state":"computed","paper":{"title":"Measuring Stellar Atmospheric Parameters with ARES+MOOG","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Daniel T. Andreasen, Sergio G. Sousa","submitted_at":"2017-11-06T11:23:51Z","abstract_excerpt":"The technical aspects in the use of an Equivalent Width (EW) method are described for the derivation of spectroscopic stellar parameters with ARES+MOOG. While the science description behind this method can be found in many references, here the goal is to provide a user manual approach for the codes and scripts presented in for the tutorial. All the required data is available online (https://github.com/sousasag/school_codes)."},"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":"1711.01839","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-11-06T11:23:51Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"84b74f0ada0f32935dfefeda6b4bc1742b79fa44f635c607ce405b058721e036","abstract_canon_sha256":"b7a2bd7ddee20167143e0be4b2ea80fa4ee630f2113bcb4e63e2aac2a352de26"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:29:24.386538Z","signature_b64":"rqdAQCV7gMy+5t+Hh86x03iHoOmrK39siGu0KIeTARobDEFi2frYS5DEiW4GBFd3F+qFjyP2JZKHSnqA0GNMBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50162e1fae5504f7da3dc3eeb06cef26feb8f743062271cb82262407ceaa123e","last_reissued_at":"2026-05-18T00:29:24.385808Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:29:24.385808Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measuring Stellar Atmospheric Parameters with ARES+MOOG","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Daniel T. Andreasen, Sergio G. Sousa","submitted_at":"2017-11-06T11:23:51Z","abstract_excerpt":"The technical aspects in the use of an Equivalent Width (EW) method are described for the derivation of spectroscopic stellar parameters with ARES+MOOG. While the science description behind this method can be found in many references, here the goal is to provide a user manual approach for the codes and scripts presented in for the tutorial. All the required data is available online (https://github.com/sousasag/school_codes)."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01839","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":"1711.01839","created_at":"2026-05-18T00:29:24.385932+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.01839v1","created_at":"2026-05-18T00:29:24.385932+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.01839","created_at":"2026-05-18T00:29:24.385932+00:00"},{"alias_kind":"pith_short_12","alias_value":"KALC4H5OKUCP","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"KALC4H5OKUCPPWR5","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"KALC4H5O","created_at":"2026-05-18T12:31:24.725408+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/KALC4H5OKUCPPWR5YPXLA3HPE3","json":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3.json","graph_json":"https://pith.science/api/pith-number/KALC4H5OKUCPPWR5YPXLA3HPE3/graph.json","events_json":"https://pith.science/api/pith-number/KALC4H5OKUCPPWR5YPXLA3HPE3/events.json","paper":"https://pith.science/paper/KALC4H5O"},"agent_actions":{"view_html":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3","download_json":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3.json","view_paper":"https://pith.science/paper/KALC4H5O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.01839&json=true","fetch_graph":"https://pith.science/api/pith-number/KALC4H5OKUCPPWR5YPXLA3HPE3/graph.json","fetch_events":"https://pith.science/api/pith-number/KALC4H5OKUCPPWR5YPXLA3HPE3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3/action/storage_attestation","attest_author":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3/action/author_attestation","sign_citation":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3/action/citation_signature","submit_replication":"https://pith.science/pith/KALC4H5OKUCPPWR5YPXLA3HPE3/action/replication_record"}},"created_at":"2026-05-18T00:29:24.385932+00:00","updated_at":"2026-05-18T00:29:24.385932+00:00"}