{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:EPA7RXLWQZ72DMOD3NTAYJ5KIL","short_pith_number":"pith:EPA7RXLW","schema_version":"1.0","canonical_sha256":"23c1f8dd76867fa1b1c3db660c27aa42e36da33475e73c78949b26d9c0a2a198","source":{"kind":"arxiv","id":"2009.00424","version":1},"attestation_state":"computed","paper":{"title":"From global to spatially resolved in low-redshift galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Camps-Fari\\~na, A. Mejia-Narvaez, C. Espinosa-Ponce, C. J. Walcher, C. Lopez-Coba, J. K. Barrera-Ballesteros, S. F. Sanchez","submitted_at":"2020-09-01T13:53:24Z","abstract_excerpt":"Our understanding of the structure, composition and evolution of galaxies has strongly improved in the last decades, mostly due to new results based on large spectroscopic and imaging surveys. In particular, the nature of ionized gas, its ionization mechanisms, its relation with the stellar properties and chemical composition, the existence of scaling relations that describe the cycle between stars and gas, and the corresponding evolution patterns have been widely explored and described. More recently, the introduction of additional techniques, in particular Integral Field Spectroscopy, and th"},"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":"2009.00424","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-09-01T13:53:24Z","cross_cats_sorted":[],"title_canon_sha256":"42932e2ec9e97c080966e83081369d08234654d7c4381e5c246a4eab4af639f3","abstract_canon_sha256":"a15f228821edc04b2e4a8e315cb0975aae8fe330daee4c511dc57442d714bcbd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:27:25.504857Z","signature_b64":"PHn4m9w0oOp9pTbTvbNySHh5+Nz61hMonPScoDy36H5Me0SdKgXX2UrG2LPBneGhy2MWvua/k7XsPFq2Erv7CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23c1f8dd76867fa1b1c3db660c27aa42e36da33475e73c78949b26d9c0a2a198","last_reissued_at":"2026-07-05T02:27:25.504139Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:27:25.504139Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"From global to spatially resolved in low-redshift galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Camps-Fari\\~na, A. Mejia-Narvaez, C. Espinosa-Ponce, C. J. Walcher, C. Lopez-Coba, J. K. Barrera-Ballesteros, S. F. Sanchez","submitted_at":"2020-09-01T13:53:24Z","abstract_excerpt":"Our understanding of the structure, composition and evolution of galaxies has strongly improved in the last decades, mostly due to new results based on large spectroscopic and imaging surveys. In particular, the nature of ionized gas, its ionization mechanisms, its relation with the stellar properties and chemical composition, the existence of scaling relations that describe the cycle between stars and gas, and the corresponding evolution patterns have been widely explored and described. More recently, the introduction of additional techniques, in particular Integral Field Spectroscopy, and th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.00424","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2009.00424/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2009.00424","created_at":"2026-07-05T02:27:25.504206+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.00424v1","created_at":"2026-07-05T02:27:25.504206+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.00424","created_at":"2026-07-05T02:27:25.504206+00:00"},{"alias_kind":"pith_short_12","alias_value":"EPA7RXLWQZ72","created_at":"2026-07-05T02:27:25.504206+00:00"},{"alias_kind":"pith_short_16","alias_value":"EPA7RXLWQZ72DMOD","created_at":"2026-07-05T02:27:25.504206+00:00"},{"alias_kind":"pith_short_8","alias_value":"EPA7RXLW","created_at":"2026-07-05T02:27:25.504206+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.18347","citing_title":"The PyKOALA python library: a multi-instrument package for IFS data reduction","ref_index":12,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL","json":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL.json","graph_json":"https://pith.science/api/pith-number/EPA7RXLWQZ72DMOD3NTAYJ5KIL/graph.json","events_json":"https://pith.science/api/pith-number/EPA7RXLWQZ72DMOD3NTAYJ5KIL/events.json","paper":"https://pith.science/paper/EPA7RXLW"},"agent_actions":{"view_html":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL","download_json":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL.json","view_paper":"https://pith.science/paper/EPA7RXLW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.00424&json=true","fetch_graph":"https://pith.science/api/pith-number/EPA7RXLWQZ72DMOD3NTAYJ5KIL/graph.json","fetch_events":"https://pith.science/api/pith-number/EPA7RXLWQZ72DMOD3NTAYJ5KIL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL/action/storage_attestation","attest_author":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL/action/author_attestation","sign_citation":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL/action/citation_signature","submit_replication":"https://pith.science/pith/EPA7RXLWQZ72DMOD3NTAYJ5KIL/action/replication_record"}},"created_at":"2026-07-05T02:27:25.504206+00:00","updated_at":"2026-07-05T02:27:25.504206+00:00"}