{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:VA46NEJEP6PJSQMDOO42CIV7PX","short_pith_number":"pith:VA46NEJE","schema_version":"1.0","canonical_sha256":"a839e691247f9e99418373b9a122bf7de66cb68be9bc2a61e70d872f1d40d70b","source":{"kind":"arxiv","id":"1411.0200","version":3},"attestation_state":"computed","paper":{"title":"Recent stellar mass assembly of low-mass star-forming galaxies at redshifts 0.3 < z < 0.9","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Armando Gil de Paz, Camilla Pacifici, Guillermo Barro, Jes\\'us Gallego, Laurence Tresse, Luc\\'ia Rodr\\'iguez-Mu\\~noz, St\\'ephane Charlot, V\\'ictor Villar","submitted_at":"2014-11-02T03:31:41Z","abstract_excerpt":"The epoch when low-mass star forming galaxies (LMSFGs) form the bulk of their stellar mass is uncertain. While some models predict an early formation, others favor a delayed scenario until later ages of the universe. We present constraints on the star formation histories (SFHs) of a sample of LMSFGs obtained through the analysis of their spectral energy distributions using a novel approach that (1) consistently combines photometric (broadband) and spectroscopic (equivalent widths of emission lines) data, and (2) uses physically motivated SFHs with non-uniform variations of the star formation r"},"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":"1411.0200","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-02T03:31:41Z","cross_cats_sorted":[],"title_canon_sha256":"f06b7ea217977c01820021020653345980faa45dde4434c66dfd718f2ba2c156","abstract_canon_sha256":"6b3e4cb2e19ec3c9b294a60bfb7d91400b57259c314144371c039f3a981f9619"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:36.180679Z","signature_b64":"5a7RYNJxUulu8FyFEMuubXLF88vbZHCb++3dpvu4E2NO7C8E1dA1qSjpitMb8SBQptTeRHW0aKpKXATUMxdKCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a839e691247f9e99418373b9a122bf7de66cb68be9bc2a61e70d872f1d40d70b","last_reissued_at":"2026-05-18T01:41:36.179997Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:36.179997Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Recent stellar mass assembly of low-mass star-forming galaxies at redshifts 0.3 < z < 0.9","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Armando Gil de Paz, Camilla Pacifici, Guillermo Barro, Jes\\'us Gallego, Laurence Tresse, Luc\\'ia Rodr\\'iguez-Mu\\~noz, St\\'ephane Charlot, V\\'ictor Villar","submitted_at":"2014-11-02T03:31:41Z","abstract_excerpt":"The epoch when low-mass star forming galaxies (LMSFGs) form the bulk of their stellar mass is uncertain. While some models predict an early formation, others favor a delayed scenario until later ages of the universe. We present constraints on the star formation histories (SFHs) of a sample of LMSFGs obtained through the analysis of their spectral energy distributions using a novel approach that (1) consistently combines photometric (broadband) and spectroscopic (equivalent widths of emission lines) data, and (2) uses physically motivated SFHs with non-uniform variations of the star formation r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.0200","kind":"arxiv","version":3},"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":"1411.0200","created_at":"2026-05-18T01:41:36.180099+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.0200v3","created_at":"2026-05-18T01:41:36.180099+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.0200","created_at":"2026-05-18T01:41:36.180099+00:00"},{"alias_kind":"pith_short_12","alias_value":"VA46NEJEP6PJ","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"VA46NEJEP6PJSQMD","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"VA46NEJE","created_at":"2026-05-18T12:28:52.271510+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/VA46NEJEP6PJSQMDOO42CIV7PX","json":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX.json","graph_json":"https://pith.science/api/pith-number/VA46NEJEP6PJSQMDOO42CIV7PX/graph.json","events_json":"https://pith.science/api/pith-number/VA46NEJEP6PJSQMDOO42CIV7PX/events.json","paper":"https://pith.science/paper/VA46NEJE"},"agent_actions":{"view_html":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX","download_json":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX.json","view_paper":"https://pith.science/paper/VA46NEJE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.0200&json=true","fetch_graph":"https://pith.science/api/pith-number/VA46NEJEP6PJSQMDOO42CIV7PX/graph.json","fetch_events":"https://pith.science/api/pith-number/VA46NEJEP6PJSQMDOO42CIV7PX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX/action/storage_attestation","attest_author":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX/action/author_attestation","sign_citation":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX/action/citation_signature","submit_replication":"https://pith.science/pith/VA46NEJEP6PJSQMDOO42CIV7PX/action/replication_record"}},"created_at":"2026-05-18T01:41:36.180099+00:00","updated_at":"2026-05-18T01:41:36.180099+00:00"}