{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:TRE3CRCBXHMVF4XHNAO2L6I33E","short_pith_number":"pith:TRE3CRCB","schema_version":"1.0","canonical_sha256":"9c49b14441b9d952f2e7681da5f91bd93045d4c5317bb0f219c491f166c4880f","source":{"kind":"arxiv","id":"1809.09111","version":1},"attestation_state":"computed","paper":{"title":"Unique Tracks Drive the Scatter of the Spatially-Resolved Star Formation Main Sequence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Christine Hall, Claude Carignan, Fiona Audcent-Ross, Gerhardt Meurer, Michelle Cluver, Stephane Courteau, Thomas Jarrett","submitted_at":"2018-09-24T18:00:01Z","abstract_excerpt":"The scatter of the spatially resolved star formation main sequence (SFMS) is investigated in order to reveal signatures about the processes of galaxy formation and evolution. We have assembled a sample of 355 nearby galaxies with spatially resolved H{\\alpha} and mid-infrared fluxes from the Survey for Ionized Neutral Gas in Galaxies and the Wide-field Infrared Survey Explorer, respectively. We examine the impact of various star formation rate (SFR) and stellar mass transformations on the SFMS. Ranging from 10^6 to 10^11.5 M_sun and derived from color to mass-to-light ratio methods for mid-infr"},"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":"1809.09111","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-09-24T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"364d6dc41b1efcc5ac7881f101cd8c246c7b195c31d6ce390a3f20e45517310d","abstract_canon_sha256":"50da9a5411a6a506f2672487fe243edb70e317bb79c9be10d874ded1415c5fd6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:03:14.795378Z","signature_b64":"d+Xu0nm7t5ra50F2Kk72xhaP7rhE/blYDeobKmXdeJSwg68Eow5vQ+GjYro7s91xO/XyYzwMFfoqjRUTFXSLDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c49b14441b9d952f2e7681da5f91bd93045d4c5317bb0f219c491f166c4880f","last_reissued_at":"2026-05-18T00:03:14.794844Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:03:14.794844Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Unique Tracks Drive the Scatter of the Spatially-Resolved Star Formation Main Sequence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Christine Hall, Claude Carignan, Fiona Audcent-Ross, Gerhardt Meurer, Michelle Cluver, Stephane Courteau, Thomas Jarrett","submitted_at":"2018-09-24T18:00:01Z","abstract_excerpt":"The scatter of the spatially resolved star formation main sequence (SFMS) is investigated in order to reveal signatures about the processes of galaxy formation and evolution. We have assembled a sample of 355 nearby galaxies with spatially resolved H{\\alpha} and mid-infrared fluxes from the Survey for Ionized Neutral Gas in Galaxies and the Wide-field Infrared Survey Explorer, respectively. We examine the impact of various star formation rate (SFR) and stellar mass transformations on the SFMS. Ranging from 10^6 to 10^11.5 M_sun and derived from color to mass-to-light ratio methods for mid-infr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.09111","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":"1809.09111","created_at":"2026-05-18T00:03:14.794923+00:00"},{"alias_kind":"arxiv_version","alias_value":"1809.09111v1","created_at":"2026-05-18T00:03:14.794923+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.09111","created_at":"2026-05-18T00:03:14.794923+00:00"},{"alias_kind":"pith_short_12","alias_value":"TRE3CRCBXHMV","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_16","alias_value":"TRE3CRCBXHMVF4XH","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_8","alias_value":"TRE3CRCB","created_at":"2026-05-18T12:32:56.356000+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/TRE3CRCBXHMVF4XHNAO2L6I33E","json":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E.json","graph_json":"https://pith.science/api/pith-number/TRE3CRCBXHMVF4XHNAO2L6I33E/graph.json","events_json":"https://pith.science/api/pith-number/TRE3CRCBXHMVF4XHNAO2L6I33E/events.json","paper":"https://pith.science/paper/TRE3CRCB"},"agent_actions":{"view_html":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E","download_json":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E.json","view_paper":"https://pith.science/paper/TRE3CRCB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1809.09111&json=true","fetch_graph":"https://pith.science/api/pith-number/TRE3CRCBXHMVF4XHNAO2L6I33E/graph.json","fetch_events":"https://pith.science/api/pith-number/TRE3CRCBXHMVF4XHNAO2L6I33E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E/action/storage_attestation","attest_author":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E/action/author_attestation","sign_citation":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E/action/citation_signature","submit_replication":"https://pith.science/pith/TRE3CRCBXHMVF4XHNAO2L6I33E/action/replication_record"}},"created_at":"2026-05-18T00:03:14.794923+00:00","updated_at":"2026-05-18T00:03:14.794923+00:00"}