{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:2ZJEGFQN5A54VUAUHTSLZFLYLB","short_pith_number":"pith:2ZJEGFQN","schema_version":"1.0","canonical_sha256":"d65243160de83bcad0143ce4bc95785848e5c59f23ccf0583359ee45308ab9ab","source":{"kind":"arxiv","id":"astro-ph/0612291","version":1},"attestation_state":"computed","paper":{"title":"zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Bongiorno, A. Cimatti, A. Iovino, A. Leauthaud, A. Renzini, B. Garilli, C. Maier, C. Marinoni, C.M. Carollo, C. Scarlata, D. Bottini, D. B. Sanders, D. Vergani, E. Daddi, E. Ricciardelli, E. Schinnerer, F. Lamareille, G. Hasinger, G. Zamorani, H. J. McCracken, J.-F. Le Borgne, J.-P. Kneib, J. Silverman, K. Caputi, K. Kovac, L.A.M. Tasca, L. Guzzo, M. Bolzonella, M. Mignoli, M. Scodeggio, N. Scoville, O. Cucciati, O. Ilbert, O. Le Fevre, other zCOSMOS team members, P. Capak, P. Franzetti, P. Kampczyk, R. Feldmann, R. Pello, S.J. Lilly, T. Contini, V. Le Brun, V. Mainieri, Y. Taniguchi","submitted_at":"2006-12-11T21:44:34Z","abstract_excerpt":"zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to characterise the environments of COSMOS galaxies from the 100 kpc scales of galaxy groups up to the 100 Mpc scale of the cosmic web and to produce diagnostic information on galaxies and active galactic nuclei. The zCOSMOS survey consists of two parts: (a) zCOSMOS-bright, a magnitude-limited I-band IAB < 22.5 sample of about 20,000 galaxies with 0.1 < z < 1.2 covering the whole 1.7 deg2 COSMOS ACS field and designed "},"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":"astro-ph/0612291","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-11T21:44:34Z","cross_cats_sorted":[],"title_canon_sha256":"6bdd610f9ead9660a6bcff020e7988857518ab3129a64e3debb60237ab82cc86","abstract_canon_sha256":"2f9149190043b3998434cadab8eee3b1e0eb45717b6ece9eb5175c6bf80cdf28"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:59:45.176660Z","signature_b64":"bcHi3MWpiW4Y2kSNEUyTAj1mQzUaPzWeHgLbNh4gCrIAhdlopzyH936ivLeiIvCZ1T+TO9J9CFDLD8zgcZk/CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d65243160de83bcad0143ce4bc95785848e5c59f23ccf0583359ee45308ab9ab","last_reissued_at":"2026-07-04T16:59:45.176218Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:59:45.176218Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Bongiorno, A. Cimatti, A. Iovino, A. Leauthaud, A. Renzini, B. Garilli, C. Maier, C. Marinoni, C.M. Carollo, C. Scarlata, D. Bottini, D. B. Sanders, D. Vergani, E. Daddi, E. Ricciardelli, E. Schinnerer, F. Lamareille, G. Hasinger, G. Zamorani, H. J. McCracken, J.-F. Le Borgne, J.-P. Kneib, J. Silverman, K. Caputi, K. Kovac, L.A.M. Tasca, L. Guzzo, M. Bolzonella, M. Mignoli, M. Scodeggio, N. Scoville, O. Cucciati, O. Ilbert, O. Le Fevre, other zCOSMOS team members, P. Capak, P. Franzetti, P. Kampczyk, R. Feldmann, R. Pello, S.J. Lilly, T. Contini, V. Le Brun, V. Mainieri, Y. Taniguchi","submitted_at":"2006-12-11T21:44:34Z","abstract_excerpt":"zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to characterise the environments of COSMOS galaxies from the 100 kpc scales of galaxy groups up to the 100 Mpc scale of the cosmic web and to produce diagnostic information on galaxies and active galactic nuclei. The zCOSMOS survey consists of two parts: (a) zCOSMOS-bright, a magnitude-limited I-band IAB < 22.5 sample of about 20,000 galaxies with 0.1 < z < 1.2 covering the whole 1.7 deg2 COSMOS ACS field and designed "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612291","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0612291/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0612291","created_at":"2026-07-04T16:59:45.176275+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612291v1","created_at":"2026-07-04T16:59:45.176275+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612291","created_at":"2026-07-04T16:59:45.176275+00:00"},{"alias_kind":"pith_short_12","alias_value":"2ZJEGFQN5A54","created_at":"2026-07-04T16:59:45.176275+00:00"},{"alias_kind":"pith_short_16","alias_value":"2ZJEGFQN5A54VUAU","created_at":"2026-07-04T16:59:45.176275+00:00"},{"alias_kind":"pith_short_8","alias_value":"2ZJEGFQN","created_at":"2026-07-04T16:59:45.176275+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2606.30757","citing_title":"Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys","ref_index":295,"is_internal_anchor":true},{"citing_arxiv_id":"2606.28489","citing_title":"pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web","ref_index":155,"is_internal_anchor":true},{"citing_arxiv_id":"2606.11308","citing_title":"pop-cosmos: Disentangling galaxy properties from observables using data-driven approaches","ref_index":153,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB","json":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB.json","graph_json":"https://pith.science/api/pith-number/2ZJEGFQN5A54VUAUHTSLZFLYLB/graph.json","events_json":"https://pith.science/api/pith-number/2ZJEGFQN5A54VUAUHTSLZFLYLB/events.json","paper":"https://pith.science/paper/2ZJEGFQN"},"agent_actions":{"view_html":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB","download_json":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB.json","view_paper":"https://pith.science/paper/2ZJEGFQN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0612291&json=true","fetch_graph":"https://pith.science/api/pith-number/2ZJEGFQN5A54VUAUHTSLZFLYLB/graph.json","fetch_events":"https://pith.science/api/pith-number/2ZJEGFQN5A54VUAUHTSLZFLYLB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB/action/storage_attestation","attest_author":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB/action/author_attestation","sign_citation":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB/action/citation_signature","submit_replication":"https://pith.science/pith/2ZJEGFQN5A54VUAUHTSLZFLYLB/action/replication_record"}},"created_at":"2026-07-04T16:59:45.176275+00:00","updated_at":"2026-07-04T16:59:45.176275+00:00"}