{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:KDOGDIWPLPONTMWTUY6WIZJVXY","short_pith_number":"pith:KDOGDIWP","schema_version":"1.0","canonical_sha256":"50dc61a2cf5bdcd9b2d3a63d646535be11b71138ab679ea459bc9de76e53a281","source":{"kind":"arxiv","id":"1502.03020","version":1},"attestation_state":"computed","paper":{"title":"GLACE survey: OSIRIS/GTC Tuneable Filter H$\\alpha$ imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alessandro Ederoclite, Alfonso Arag\\'on-Salamanca, Ana L. Chies-Santos, Ana L. Serra, Ana M. P\\'erez Garc\\'ia, Andrea Biviano, \\'Angel Bongiovanni, Antonaldo Diaferio, Bianca Poggianti, Brian McBreen, Bruno Altieri, Chantal Balkowski, Chris. P. Haines, Daniela Coia, Emilio Alfaro, Francisco Castander, Graham P. Smith, H\\'ector Casta\\~neda, Helena Dom\\'inguez-S\\'anchez, Ian Smail, Ignacio Gonz\\'alez-Serrano, Irene Pintos-Castro, Ismael P\\'erez-Fourn\\'on, Iv\\'an Oteo, Ivan Valtchanov, James Geach, Jana Polednikova, Joana S. Santos, Jordi Cepa, Jos\\'e M. Rodr\\'iguez-Espinosa, Leo Metcalfe, Malcom Bremer, Marina Ram\\'on-P\\'erez, Miguel S\\'anchez-Portal, Nieves Castro-Rodr\\'iguez, Pierre-Alain Duc, Ricardo P\\'erez-Mart\\'inez, Sonia Temporin","submitted_at":"2015-02-10T18:01:07Z","abstract_excerpt":"The cores of clusters at 0 $\\lesssim$ z $\\lesssim$ 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type ones. Galaxy properties, notably the star formation (SF) ability, are altered as they fall into overdense regions. The critical issues to understand this evolution are how the truncation of SF is connected to the morphological transformation and the responsible physical mechanism. The GaLAxy Cluster Evolution Survey (GLACE) is conducting a study on the variation of galaxy properties (SF, AGN, morphology) as a function of environment in a "},"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":"1502.03020","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-02-10T18:01:07Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"a5d386df9923261569b9e9e19c0569f939bf2154a836027859f1ac1316bab5b2","abstract_canon_sha256":"eac4ab31a12ef63527a5227247c4a7be4268a14e3f26d3d1c9fd00cae58ff7d5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:34.387699Z","signature_b64":"ar3Di/tZRQqeKWQ3mQdjZ2LCU86cojG6Nch2a+lB7OMScjaq8f4fwt+YqvWTuJ9DZPEVoV/Eplwl4sNI/fPSDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50dc61a2cf5bdcd9b2d3a63d646535be11b71138ab679ea459bc9de76e53a281","last_reissued_at":"2026-05-18T02:03:34.387163Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:34.387163Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GLACE survey: OSIRIS/GTC Tuneable Filter H$\\alpha$ imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alessandro Ederoclite, Alfonso Arag\\'on-Salamanca, Ana L. Chies-Santos, Ana L. Serra, Ana M. P\\'erez Garc\\'ia, Andrea Biviano, \\'Angel Bongiovanni, Antonaldo Diaferio, Bianca Poggianti, Brian McBreen, Bruno Altieri, Chantal Balkowski, Chris. P. Haines, Daniela Coia, Emilio Alfaro, Francisco Castander, Graham P. Smith, H\\'ector Casta\\~neda, Helena Dom\\'inguez-S\\'anchez, Ian Smail, Ignacio Gonz\\'alez-Serrano, Irene Pintos-Castro, Ismael P\\'erez-Fourn\\'on, Iv\\'an Oteo, Ivan Valtchanov, James Geach, Jana Polednikova, Joana S. Santos, Jordi Cepa, Jos\\'e M. Rodr\\'iguez-Espinosa, Leo Metcalfe, Malcom Bremer, Marina Ram\\'on-P\\'erez, Miguel S\\'anchez-Portal, Nieves Castro-Rodr\\'iguez, Pierre-Alain Duc, Ricardo P\\'erez-Mart\\'inez, Sonia Temporin","submitted_at":"2015-02-10T18:01:07Z","abstract_excerpt":"The cores of clusters at 0 $\\lesssim$ z $\\lesssim$ 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type ones. Galaxy properties, notably the star formation (SF) ability, are altered as they fall into overdense regions. The critical issues to understand this evolution are how the truncation of SF is connected to the morphological transformation and the responsible physical mechanism. The GaLAxy Cluster Evolution Survey (GLACE) is conducting a study on the variation of galaxy properties (SF, AGN, morphology) as a function of environment in a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.03020","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":"1502.03020","created_at":"2026-05-18T02:03:34.387247+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.03020v1","created_at":"2026-05-18T02:03:34.387247+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.03020","created_at":"2026-05-18T02:03:34.387247+00:00"},{"alias_kind":"pith_short_12","alias_value":"KDOGDIWPLPON","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"KDOGDIWPLPONTMWT","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"KDOGDIWP","created_at":"2026-05-18T12:29:27.538025+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/KDOGDIWPLPONTMWTUY6WIZJVXY","json":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY.json","graph_json":"https://pith.science/api/pith-number/KDOGDIWPLPONTMWTUY6WIZJVXY/graph.json","events_json":"https://pith.science/api/pith-number/KDOGDIWPLPONTMWTUY6WIZJVXY/events.json","paper":"https://pith.science/paper/KDOGDIWP"},"agent_actions":{"view_html":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY","download_json":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY.json","view_paper":"https://pith.science/paper/KDOGDIWP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.03020&json=true","fetch_graph":"https://pith.science/api/pith-number/KDOGDIWPLPONTMWTUY6WIZJVXY/graph.json","fetch_events":"https://pith.science/api/pith-number/KDOGDIWPLPONTMWTUY6WIZJVXY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY/action/storage_attestation","attest_author":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY/action/author_attestation","sign_citation":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY/action/citation_signature","submit_replication":"https://pith.science/pith/KDOGDIWPLPONTMWTUY6WIZJVXY/action/replication_record"}},"created_at":"2026-05-18T02:03:34.387247+00:00","updated_at":"2026-05-18T02:03:34.387247+00:00"}