{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:FA4BDZZDHD4AUHDELEMFZR4QJL","short_pith_number":"pith:FA4BDZZD","schema_version":"1.0","canonical_sha256":"283811e72338f80a1c6459185cc7904ae24b1d7bacf33792fde4703b7fe0c2d8","source":{"kind":"arxiv","id":"1802.07628","version":4},"attestation_state":"computed","paper":{"title":"On the fast quenching of young low-mass galaxies up to z $\\sim$ 0.6: new spotlight on the lead role of environment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anneya Golob, Christophe Adami, Jean Coupon, Marcin Sawicki, Nicola Malavasi, Olivier Ilbert, St\\'ephane Arnouts, Thibaud Moutard","submitted_at":"2018-02-21T15:56:07Z","abstract_excerpt":"We investigate the connection between environment and the different quenching channels that galaxies are prone to follow in the rest-frame NUVrK colour diagram, as identified by Moutard et al. (2016b). Namely, the fast quenching channel followed by $young$ low-mass galaxies and the slow quenching channel followed by $old$ high-mass ones. We make use of the >22 deg$^2$ covered the VIPERS Multi-Lambda Survey (VIPERS-MLS) to select a galaxy sample complete down to stellar masses of $M_* > 10^{9.4} M_\\odot$ at $z < 0.65$ ($M_* > 10^{8.8} M_\\odot$ at $z < 0.5$) and including 33,500 (43,000) quiesce"},"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":"1802.07628","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-02-21T15:56:07Z","cross_cats_sorted":[],"title_canon_sha256":"bf1416d7cc315c56e52eb06b7a2415e413e02ed76d15921d1e77853433b21d47","abstract_canon_sha256":"01a6b91ce231e4b6629a840338e4acbc1a35c23f33f7d56616dfb9d66bd2444d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:18.582974Z","signature_b64":"YI0zZTvqP37xZMB8ptb+pMniUT0R+OY5DY2bhINeEKb+94bmFHmHc7NwkEHD3xQ+RCq4C38eKU05MrhMQ2+MCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"283811e72338f80a1c6459185cc7904ae24b1d7bacf33792fde4703b7fe0c2d8","last_reissued_at":"2026-05-17T23:52:18.582203Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:18.582203Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the fast quenching of young low-mass galaxies up to z $\\sim$ 0.6: new spotlight on the lead role of environment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anneya Golob, Christophe Adami, Jean Coupon, Marcin Sawicki, Nicola Malavasi, Olivier Ilbert, St\\'ephane Arnouts, Thibaud Moutard","submitted_at":"2018-02-21T15:56:07Z","abstract_excerpt":"We investigate the connection between environment and the different quenching channels that galaxies are prone to follow in the rest-frame NUVrK colour diagram, as identified by Moutard et al. (2016b). Namely, the fast quenching channel followed by $young$ low-mass galaxies and the slow quenching channel followed by $old$ high-mass ones. We make use of the >22 deg$^2$ covered the VIPERS Multi-Lambda Survey (VIPERS-MLS) to select a galaxy sample complete down to stellar masses of $M_* > 10^{9.4} M_\\odot$ at $z < 0.65$ ($M_* > 10^{8.8} M_\\odot$ at $z < 0.5$) and including 33,500 (43,000) quiesce"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.07628","kind":"arxiv","version":4},"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":"1802.07628","created_at":"2026-05-17T23:52:18.582341+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.07628v4","created_at":"2026-05-17T23:52:18.582341+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.07628","created_at":"2026-05-17T23:52:18.582341+00:00"},{"alias_kind":"pith_short_12","alias_value":"FA4BDZZDHD4A","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_16","alias_value":"FA4BDZZDHD4AUHDE","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_8","alias_value":"FA4BDZZD","created_at":"2026-05-18T12:32:22.470017+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/FA4BDZZDHD4AUHDELEMFZR4QJL","json":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL.json","graph_json":"https://pith.science/api/pith-number/FA4BDZZDHD4AUHDELEMFZR4QJL/graph.json","events_json":"https://pith.science/api/pith-number/FA4BDZZDHD4AUHDELEMFZR4QJL/events.json","paper":"https://pith.science/paper/FA4BDZZD"},"agent_actions":{"view_html":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL","download_json":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL.json","view_paper":"https://pith.science/paper/FA4BDZZD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.07628&json=true","fetch_graph":"https://pith.science/api/pith-number/FA4BDZZDHD4AUHDELEMFZR4QJL/graph.json","fetch_events":"https://pith.science/api/pith-number/FA4BDZZDHD4AUHDELEMFZR4QJL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL/action/storage_attestation","attest_author":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL/action/author_attestation","sign_citation":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL/action/citation_signature","submit_replication":"https://pith.science/pith/FA4BDZZDHD4AUHDELEMFZR4QJL/action/replication_record"}},"created_at":"2026-05-17T23:52:18.582341+00:00","updated_at":"2026-05-17T23:52:18.582341+00:00"}