{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:HCVDG7W3O43U76CZADWMZT67D4","short_pith_number":"pith:HCVDG7W3","schema_version":"1.0","canonical_sha256":"38aa337edb77374ff85900eccccfdf1f144ea82c5c70037ffd96112f2dd8b3df","source":{"kind":"arxiv","id":"1709.01519","version":1},"attestation_state":"computed","paper":{"title":"The distribution of local star formation activity as a function of galaxy stellar mass, environment and morphology","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. J. B. Smith, E. K. Lofthouse, M. J. Hardcastle, S. Kaviraj","submitted_at":"2017-09-05T18:00:03Z","abstract_excerpt":"We present a detailed inventory of star formation in the local Universe, dissecting the cosmic star formation budget as a function of key variables that influence the star formation rate (SFR) of galaxies: stellar mass, local environment and morphology. We use a large homogeneous dataset from the SDSS to first study how the star-formation budget in galaxies with stellar masses greater than $\\log (\\textrm{M}_{*}/\\textrm{M}_{\\odot}) = 10$ splits as a function of each parameter separately. We then explore how the budget behaves as a simultaneous function of these three parameters. We show that 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":"1709.01519","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-09-05T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"3fd9de02abe91fb0c276733440a720fd8b4ba79bc5e54ee2c0525a2e1c38e064","abstract_canon_sha256":"9f4b6126eeca7fce5bbdf0e26b1a406c19ba234b8488b7cd4b8374ca52d5c59e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:32:39.099201Z","signature_b64":"4vHdWlpPjaOBtBChoOIZM6SwkyhTRAhlwJRUaPt75c2ZWJN7BOnH7MY5sNnzXD3FRYnEemaVF0IkcaZemnJ8AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"38aa337edb77374ff85900eccccfdf1f144ea82c5c70037ffd96112f2dd8b3df","last_reissued_at":"2026-05-18T00:32:39.098572Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:32:39.098572Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The distribution of local star formation activity as a function of galaxy stellar mass, environment and morphology","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. J. B. Smith, E. K. Lofthouse, M. J. Hardcastle, S. Kaviraj","submitted_at":"2017-09-05T18:00:03Z","abstract_excerpt":"We present a detailed inventory of star formation in the local Universe, dissecting the cosmic star formation budget as a function of key variables that influence the star formation rate (SFR) of galaxies: stellar mass, local environment and morphology. We use a large homogeneous dataset from the SDSS to first study how the star-formation budget in galaxies with stellar masses greater than $\\log (\\textrm{M}_{*}/\\textrm{M}_{\\odot}) = 10$ splits as a function of each parameter separately. We then explore how the budget behaves as a simultaneous function of these three parameters. We show that th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.01519","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":"1709.01519","created_at":"2026-05-18T00:32:39.098671+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.01519v1","created_at":"2026-05-18T00:32:39.098671+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.01519","created_at":"2026-05-18T00:32:39.098671+00:00"},{"alias_kind":"pith_short_12","alias_value":"HCVDG7W3O43U","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"HCVDG7W3O43U76CZ","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"HCVDG7W3","created_at":"2026-05-18T12:31:18.294218+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/HCVDG7W3O43U76CZADWMZT67D4","json":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4.json","graph_json":"https://pith.science/api/pith-number/HCVDG7W3O43U76CZADWMZT67D4/graph.json","events_json":"https://pith.science/api/pith-number/HCVDG7W3O43U76CZADWMZT67D4/events.json","paper":"https://pith.science/paper/HCVDG7W3"},"agent_actions":{"view_html":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4","download_json":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4.json","view_paper":"https://pith.science/paper/HCVDG7W3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.01519&json=true","fetch_graph":"https://pith.science/api/pith-number/HCVDG7W3O43U76CZADWMZT67D4/graph.json","fetch_events":"https://pith.science/api/pith-number/HCVDG7W3O43U76CZADWMZT67D4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4/action/storage_attestation","attest_author":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4/action/author_attestation","sign_citation":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4/action/citation_signature","submit_replication":"https://pith.science/pith/HCVDG7W3O43U76CZADWMZT67D4/action/replication_record"}},"created_at":"2026-05-18T00:32:39.098671+00:00","updated_at":"2026-05-18T00:32:39.098671+00:00"}