{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:OIX7A5C6HE3GREKKE2FPE5HO77","short_pith_number":"pith:OIX7A5C6","schema_version":"1.0","canonical_sha256":"722ff0745e393668914a268af274eeffc4b17b5b06d24c410310aecc7f456cb3","source":{"kind":"arxiv","id":"1807.00820","version":1},"attestation_state":"computed","paper":{"title":"The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Gabriel W. Pratt, Hakon Dahle, Herve Aussel, Monique Arnaud, Remco F. J. van der Burg, Sean McGee","submitted_at":"2018-07-02T18:00:00Z","abstract_excerpt":"We study the abundance of star-forming and quiescent galaxies in a sample of 21 massive clusters at 0.5<z<0.7, detected with the Planck satellite. We measure the cluster galaxy stellar mass function (SMF), which is a fundamental observable to study and constrain the formation and evolution of galaxies. Our measurements are based on homogeneous and deep multi-band photometry spanning u- to the Ks-band for each cluster and are supported by spectroscopic data from different programs. The galaxy population is separated between quiescent and star-forming galaxies based on their rest-frame U-V and V"},"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":"1807.00820","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-07-02T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"2fb9dfda63994220da0cbde26ffbb350d1f430af9f3af65bf391d28b64fad392","abstract_canon_sha256":"139b032e32d2714f7c3a60094e9d7d31554c4faefdbff714d98cbe4bf36df516"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:01:29.143231Z","signature_b64":"MCnzXXVjT0i0OTq3IosNDUZl0r3Cr+SMw/j4/JKK/ksdrkX2zPBe6TOqjN8futtNeqt5cRcWOBjL6e45KIu5AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"722ff0745e393668914a268af274eeffc4b17b5b06d24c410310aecc7f456cb3","last_reissued_at":"2026-05-18T00:01:29.142687Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:01:29.142687Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Gabriel W. Pratt, Hakon Dahle, Herve Aussel, Monique Arnaud, Remco F. J. van der Burg, Sean McGee","submitted_at":"2018-07-02T18:00:00Z","abstract_excerpt":"We study the abundance of star-forming and quiescent galaxies in a sample of 21 massive clusters at 0.5<z<0.7, detected with the Planck satellite. We measure the cluster galaxy stellar mass function (SMF), which is a fundamental observable to study and constrain the formation and evolution of galaxies. Our measurements are based on homogeneous and deep multi-band photometry spanning u- to the Ks-band for each cluster and are supported by spectroscopic data from different programs. The galaxy population is separated between quiescent and star-forming galaxies based on their rest-frame U-V and V"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.00820","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":"1807.00820","created_at":"2026-05-18T00:01:29.142765+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.00820v1","created_at":"2026-05-18T00:01:29.142765+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.00820","created_at":"2026-05-18T00:01:29.142765+00:00"},{"alias_kind":"pith_short_12","alias_value":"OIX7A5C6HE3G","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_16","alias_value":"OIX7A5C6HE3GREKK","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_8","alias_value":"OIX7A5C6","created_at":"2026-05-18T12:32:43.782077+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/OIX7A5C6HE3GREKKE2FPE5HO77","json":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77.json","graph_json":"https://pith.science/api/pith-number/OIX7A5C6HE3GREKKE2FPE5HO77/graph.json","events_json":"https://pith.science/api/pith-number/OIX7A5C6HE3GREKKE2FPE5HO77/events.json","paper":"https://pith.science/paper/OIX7A5C6"},"agent_actions":{"view_html":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77","download_json":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77.json","view_paper":"https://pith.science/paper/OIX7A5C6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.00820&json=true","fetch_graph":"https://pith.science/api/pith-number/OIX7A5C6HE3GREKKE2FPE5HO77/graph.json","fetch_events":"https://pith.science/api/pith-number/OIX7A5C6HE3GREKKE2FPE5HO77/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77/action/storage_attestation","attest_author":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77/action/author_attestation","sign_citation":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77/action/citation_signature","submit_replication":"https://pith.science/pith/OIX7A5C6HE3GREKKE2FPE5HO77/action/replication_record"}},"created_at":"2026-05-18T00:01:29.142765+00:00","updated_at":"2026-05-18T00:01:29.142765+00:00"}