{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:TN7OQXCW3F5S7Y4RTN2ODUTGHN","short_pith_number":"pith:TN7OQXCW","schema_version":"1.0","canonical_sha256":"9b7ee85c56d97b2fe3919b74e1d2663b41e0831e76086229196f8426180b99a8","source":{"kind":"arxiv","id":"1611.00367","version":1},"attestation_state":"computed","paper":{"title":"The Galaxy End Sequence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chris Duffield, Kiran Appah, Laure Ciesla, Matthew Smith, Pieter De Vis, Simon Schofield, Stephen Eales","submitted_at":"2016-11-01T20:00:03Z","abstract_excerpt":"A common assumption is that galaxies fall in two distinct regions on a plot of specific star-formation rate (SSFR) versus galaxy stellar mass: a star-forming Galaxy Main Sequence (GMS) and a separate region of `passive' or `red and dead galaxies'. Starting from a volume-limited sample of nearby galaxies designed to contain most of the stellar mass in this volume, and thus being a fair representation of the Universe at the end of 12 billion years of galaxy evolution, we investigate the distribution of galaxies in this diagram today. We show that galaxies follow a strongly curved extended GMS wi"},"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":"1611.00367","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-01T20:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"852b2f8836dae02c8e4dbf47db6032318eb8b15784650671a19b6222dd1266ad","abstract_canon_sha256":"2b6a2aba9bd77a0ad1fd16cea6d00842cbc00335d6a1d543333b48d8e13b946f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:14.145356Z","signature_b64":"pPJHQH7cLvO0dubYSQA3Ff6wOVDK3YE81dgYYpqbKmLY+JKOLRHae43PRP8xgc8QY3k+2W0zdN0ih57e6Tp8DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b7ee85c56d97b2fe3919b74e1d2663b41e0831e76086229196f8426180b99a8","last_reissued_at":"2026-05-18T00:52:14.144907Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:14.144907Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Galaxy End Sequence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chris Duffield, Kiran Appah, Laure Ciesla, Matthew Smith, Pieter De Vis, Simon Schofield, Stephen Eales","submitted_at":"2016-11-01T20:00:03Z","abstract_excerpt":"A common assumption is that galaxies fall in two distinct regions on a plot of specific star-formation rate (SSFR) versus galaxy stellar mass: a star-forming Galaxy Main Sequence (GMS) and a separate region of `passive' or `red and dead galaxies'. Starting from a volume-limited sample of nearby galaxies designed to contain most of the stellar mass in this volume, and thus being a fair representation of the Universe at the end of 12 billion years of galaxy evolution, we investigate the distribution of galaxies in this diagram today. We show that galaxies follow a strongly curved extended GMS wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.00367","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":"1611.00367","created_at":"2026-05-18T00:52:14.144967+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.00367v1","created_at":"2026-05-18T00:52:14.144967+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.00367","created_at":"2026-05-18T00:52:14.144967+00:00"},{"alias_kind":"pith_short_12","alias_value":"TN7OQXCW3F5S","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"TN7OQXCW3F5S7Y4R","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"TN7OQXCW","created_at":"2026-05-18T12:30:44.179134+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.19661","citing_title":"COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0