{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:ENJZ2D6BBLA5XF5YHT46THQ624","short_pith_number":"pith:ENJZ2D6B","schema_version":"1.0","canonical_sha256":"23539d0fc10ac1db97b83cf9e99e1ed72004277f33286ab5c025b063f87d14f6","source":{"kind":"arxiv","id":"2004.00718","version":1},"attestation_state":"computed","paper":{"title":"The properties of inside-out assembled galaxies at $z<0.1$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Asrate Gaulle, Dejene Zewdie, Manuel Aravena, Mirjana Povi\\'c, Roberto J. Assef","submitted_at":"2020-04-01T21:58:10Z","abstract_excerpt":"In this work, we study the properties of galaxies that are showing the inside-out assembly (which we call inside-out assembled galaxies; IOAGs), with the main aim to understand better their properties and morphological transformation. We analysed a sample of galaxies from the Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8), with stellar masses in the range $\\log M_{\\star}=10.73-11.03$ $M_{\\odot{}}$ at $z < 0.1$, and analyze their location in the stellar mass-SFR and the color-stellar mass diagram. We found that IOAGs have different spectroscopic properties, most of them being classified e"},"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":"2004.00718","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-04-01T21:58:10Z","cross_cats_sorted":[],"title_canon_sha256":"de257238d586da477b35675c077753c2fdd112f56c12a984706dcefe3e633009","abstract_canon_sha256":"474dee8e715fda63be3672d6f7e43254575669f4864ac29cfb1fa351b8b9edfa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:57:06.999499Z","signature_b64":"wf7kTggblCE0SL8G+JocI2RBq8Gm/6LFObHgwJydA98He2iAKqQ77p6UfOx8Sj5JUfMR+2fNcu5+CIq9nk5bAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23539d0fc10ac1db97b83cf9e99e1ed72004277f33286ab5c025b063f87d14f6","last_reissued_at":"2026-07-05T02:57:06.999131Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:57:06.999131Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The properties of inside-out assembled galaxies at $z<0.1$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Asrate Gaulle, Dejene Zewdie, Manuel Aravena, Mirjana Povi\\'c, Roberto J. Assef","submitted_at":"2020-04-01T21:58:10Z","abstract_excerpt":"In this work, we study the properties of galaxies that are showing the inside-out assembly (which we call inside-out assembled galaxies; IOAGs), with the main aim to understand better their properties and morphological transformation. We analysed a sample of galaxies from the Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8), with stellar masses in the range $\\log M_{\\star}=10.73-11.03$ $M_{\\odot{}}$ at $z < 0.1$, and analyze their location in the stellar mass-SFR and the color-stellar mass diagram. We found that IOAGs have different spectroscopic properties, most of them being classified e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2004.00718","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/2004.00718/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":"2004.00718","created_at":"2026-07-05T02:57:06.999186+00:00"},{"alias_kind":"arxiv_version","alias_value":"2004.00718v1","created_at":"2026-07-05T02:57:06.999186+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2004.00718","created_at":"2026-07-05T02:57:06.999186+00:00"},{"alias_kind":"pith_short_12","alias_value":"ENJZ2D6BBLA5","created_at":"2026-07-05T02:57:06.999186+00:00"},{"alias_kind":"pith_short_16","alias_value":"ENJZ2D6BBLA5XF5Y","created_at":"2026-07-05T02:57:06.999186+00:00"},{"alias_kind":"pith_short_8","alias_value":"ENJZ2D6B","created_at":"2026-07-05T02:57:06.999186+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/ENJZ2D6BBLA5XF5YHT46THQ624","json":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624.json","graph_json":"https://pith.science/api/pith-number/ENJZ2D6BBLA5XF5YHT46THQ624/graph.json","events_json":"https://pith.science/api/pith-number/ENJZ2D6BBLA5XF5YHT46THQ624/events.json","paper":"https://pith.science/paper/ENJZ2D6B"},"agent_actions":{"view_html":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624","download_json":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624.json","view_paper":"https://pith.science/paper/ENJZ2D6B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2004.00718&json=true","fetch_graph":"https://pith.science/api/pith-number/ENJZ2D6BBLA5XF5YHT46THQ624/graph.json","fetch_events":"https://pith.science/api/pith-number/ENJZ2D6BBLA5XF5YHT46THQ624/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624/action/storage_attestation","attest_author":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624/action/author_attestation","sign_citation":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624/action/citation_signature","submit_replication":"https://pith.science/pith/ENJZ2D6BBLA5XF5YHT46THQ624/action/replication_record"}},"created_at":"2026-07-05T02:57:06.999186+00:00","updated_at":"2026-07-05T02:57:06.999186+00:00"}