{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:N33DXGBDNAQ6WFQSH2ORVQKG3Q","short_pith_number":"pith:N33DXGBD","schema_version":"1.0","canonical_sha256":"6ef63b98236821eb16123e9d1ac146dc2a793fd8a9e390c4b592c94a4ae765a8","source":{"kind":"arxiv","id":"1411.6331","version":1},"attestation_state":"computed","paper":{"title":"The mass-metallicity relation of Lyman-break analogues and its dependence on galaxy properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. H. Lian, J. R. Li, W. Yan, X. Kong","submitted_at":"2014-11-24T02:38:21Z","abstract_excerpt":"We investigate the mass-metallicity relation and its dependence on galaxy physical properties with a sample of 703 Lyman-break analogues (LBAs) in local Universe, which have similar properties to high redshift star-forming galaxies. The sample is selected according to $\\ha$ luminosity, $L(\\ha)>10^{41.8}\\,{\\rm erg\\,s^{-1}}$, and surface brightness, $I(\\ha)>10^{40.5}\\,{\\rm erg\\,s^{-1}\\,kpc^{-2}}$, criteria. The mass-metallicity relation of LBAs harmoniously agrees with that of star-forming galaxies at $z \\sim$ 1.4-1.7 in stellar mass range of $10^{8.5}M_{\\odot}<M_{*}<10^{11}M_{\\odot}$. The relat"},"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":"1411.6331","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-24T02:38:21Z","cross_cats_sorted":[],"title_canon_sha256":"c6d139bebef34a2f050798caaa6220f9119efcff7a53ef8b3b4dcf188d9e3e93","abstract_canon_sha256":"d9c617f6bb87f990356f872aca022d56bb7b4825e889a9cdcfb0381c48efe9c1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:33:00.256997Z","signature_b64":"vwlkAJNHPwt2h6AFhy4rI9AhGZQvCtxexvJPFwSlFP5H5pfdePEgCrMeaPTV2+x2oM2l7HdaEL07tlOgOoOpDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ef63b98236821eb16123e9d1ac146dc2a793fd8a9e390c4b592c94a4ae765a8","last_reissued_at":"2026-05-18T02:33:00.256659Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:33:00.256659Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The mass-metallicity relation of Lyman-break analogues and its dependence on galaxy properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. H. Lian, J. R. Li, W. Yan, X. Kong","submitted_at":"2014-11-24T02:38:21Z","abstract_excerpt":"We investigate the mass-metallicity relation and its dependence on galaxy physical properties with a sample of 703 Lyman-break analogues (LBAs) in local Universe, which have similar properties to high redshift star-forming galaxies. The sample is selected according to $\\ha$ luminosity, $L(\\ha)>10^{41.8}\\,{\\rm erg\\,s^{-1}}$, and surface brightness, $I(\\ha)>10^{40.5}\\,{\\rm erg\\,s^{-1}\\,kpc^{-2}}$, criteria. The mass-metallicity relation of LBAs harmoniously agrees with that of star-forming galaxies at $z \\sim$ 1.4-1.7 in stellar mass range of $10^{8.5}M_{\\odot}<M_{*}<10^{11}M_{\\odot}$. The relat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.6331","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":"1411.6331","created_at":"2026-05-18T02:33:00.256713+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.6331v1","created_at":"2026-05-18T02:33:00.256713+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.6331","created_at":"2026-05-18T02:33:00.256713+00:00"},{"alias_kind":"pith_short_12","alias_value":"N33DXGBDNAQ6","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"N33DXGBDNAQ6WFQS","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"N33DXGBD","created_at":"2026-05-18T12:28:41.024544+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/N33DXGBDNAQ6WFQSH2ORVQKG3Q","json":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q.json","graph_json":"https://pith.science/api/pith-number/N33DXGBDNAQ6WFQSH2ORVQKG3Q/graph.json","events_json":"https://pith.science/api/pith-number/N33DXGBDNAQ6WFQSH2ORVQKG3Q/events.json","paper":"https://pith.science/paper/N33DXGBD"},"agent_actions":{"view_html":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q","download_json":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q.json","view_paper":"https://pith.science/paper/N33DXGBD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.6331&json=true","fetch_graph":"https://pith.science/api/pith-number/N33DXGBDNAQ6WFQSH2ORVQKG3Q/graph.json","fetch_events":"https://pith.science/api/pith-number/N33DXGBDNAQ6WFQSH2ORVQKG3Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q/action/storage_attestation","attest_author":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q/action/author_attestation","sign_citation":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q/action/citation_signature","submit_replication":"https://pith.science/pith/N33DXGBDNAQ6WFQSH2ORVQKG3Q/action/replication_record"}},"created_at":"2026-05-18T02:33:00.256713+00:00","updated_at":"2026-05-18T02:33:00.256713+00:00"}