{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:SFOWX6Y4NOWB5JEBJ4T6SW4KCR","short_pith_number":"pith:SFOWX6Y4","schema_version":"1.0","canonical_sha256":"915d6bfb1c6bac1ea4814f27e95b8a147553b5edd0415b50b93a5f659653d754","source":{"kind":"arxiv","id":"1507.05636","version":2},"attestation_state":"computed","paper":{"title":"The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adriano Fontana, A. Grazian, Brett Salmon, Casey Papovich, Emiliano Merlin, Giovanni G. Fazio, Henry C. Ferguson, K. Duncan, Mark Dickinson, Matthew L. N. Ashby, Mimi Song, Nimish Hathi, Rachel S. Somerville, Sandy M. Faber, Seong-Kook Lee, S. P. Willner, Steven L. Finkelstein, Yicheng Guo, Yu Lu","submitted_at":"2015-07-20T20:02:52Z","abstract_excerpt":"We present galaxy stellar mass functions (GSMFs) at $z=$ 4-8 from a rest-frame ultraviolet (UV) selected sample of $\\sim$4500 galaxies, found via photometric redshifts over an area of $\\sim$280 arcmin$^2$ in the CANDELS/GOODS fields and the Hubble Ultra Deep Field. The deepest Spitzer/IRAC data yet-to-date and the relatively large volume allow us to place a better constraint at both the low- and high-mass ends of the GSMFs compared to previous space-based studies from pre-CANDELS observations. Supplemented by a stacking analysis, we find a linear correlation between the rest-frame UV absolute "},"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":"1507.05636","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-07-20T20:02:52Z","cross_cats_sorted":[],"title_canon_sha256":"3313ec341bcc4f25ab9c6da6571298713b1cfc1e6e3ee7bac2fa202c966e298c","abstract_canon_sha256":"f495f91991258fa5b780d40578e3d22933e22983cf8818699950aee961a4aa17"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:33.481010Z","signature_b64":"yJWtISMsFQFQ9fW/JPfuyoXO9AwQOfZIGNDclGlNeTEW3HCmMRh4Uauexub2zwLETIuISWqbSlAp6ZKISiNODA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"915d6bfb1c6bac1ea4814f27e95b8a147553b5edd0415b50b93a5f659653d754","last_reissued_at":"2026-05-18T01:11:33.480611Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:33.480611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adriano Fontana, A. Grazian, Brett Salmon, Casey Papovich, Emiliano Merlin, Giovanni G. Fazio, Henry C. Ferguson, K. Duncan, Mark Dickinson, Matthew L. N. Ashby, Mimi Song, Nimish Hathi, Rachel S. Somerville, Sandy M. Faber, Seong-Kook Lee, S. P. Willner, Steven L. Finkelstein, Yicheng Guo, Yu Lu","submitted_at":"2015-07-20T20:02:52Z","abstract_excerpt":"We present galaxy stellar mass functions (GSMFs) at $z=$ 4-8 from a rest-frame ultraviolet (UV) selected sample of $\\sim$4500 galaxies, found via photometric redshifts over an area of $\\sim$280 arcmin$^2$ in the CANDELS/GOODS fields and the Hubble Ultra Deep Field. The deepest Spitzer/IRAC data yet-to-date and the relatively large volume allow us to place a better constraint at both the low- and high-mass ends of the GSMFs compared to previous space-based studies from pre-CANDELS observations. Supplemented by a stacking analysis, we find a linear correlation between the rest-frame UV absolute "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.05636","kind":"arxiv","version":2},"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":"1507.05636","created_at":"2026-05-18T01:11:33.480675+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.05636v2","created_at":"2026-05-18T01:11:33.480675+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.05636","created_at":"2026-05-18T01:11:33.480675+00:00"},{"alias_kind":"pith_short_12","alias_value":"SFOWX6Y4NOWB","created_at":"2026-05-18T12:29:39.896362+00:00"},{"alias_kind":"pith_short_16","alias_value":"SFOWX6Y4NOWB5JEB","created_at":"2026-05-18T12:29:39.896362+00:00"},{"alias_kind":"pith_short_8","alias_value":"SFOWX6Y4","created_at":"2026-05-18T12:29:39.896362+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2605.21599","citing_title":"JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15310","citing_title":"Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13966","citing_title":"Massive Galaxies Form Early and Gray: Stellar Assembly and Dust Attenuation at $\\mathbf{z>3.5}$ from CAPERS","ref_index":43,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR","json":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR.json","graph_json":"https://pith.science/api/pith-number/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/graph.json","events_json":"https://pith.science/api/pith-number/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/events.json","paper":"https://pith.science/paper/SFOWX6Y4"},"agent_actions":{"view_html":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR","download_json":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR.json","view_paper":"https://pith.science/paper/SFOWX6Y4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.05636&json=true","fetch_graph":"https://pith.science/api/pith-number/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/graph.json","fetch_events":"https://pith.science/api/pith-number/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/action/storage_attestation","attest_author":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/action/author_attestation","sign_citation":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/action/citation_signature","submit_replication":"https://pith.science/pith/SFOWX6Y4NOWB5JEBJ4T6SW4KCR/action/replication_record"}},"created_at":"2026-05-18T01:11:33.480675+00:00","updated_at":"2026-05-18T01:11:33.480675+00:00"}