{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:PEREXZOLEIFLFRV2ZI4TN7746O","short_pith_number":"pith:PEREXZOL","schema_version":"1.0","canonical_sha256":"79224be5cb220ab2c6baca3936fffcf3a1227be3d77af3cc6e5b25b486a5c560","source":{"kind":"arxiv","id":"1706.03790","version":1},"attestation_state":"computed","paper":{"title":"The ASTRODEEP Frontier Fields Catalogues III. Multiwavelength photometry and rest frame properties of MACS-J0717 and MACS-J1149","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Fontana, A. Grazian, D. Elbaz, E. M\\'armol-Queralt\\'o, E. Merlin, J.S. Dunlop, K. Boutsia, L. Pentericci, M. Castellano, M. Di Criscienzo, M. J. Michalowski, P. Santini, R. Amorin, R. J. McLure, S. Derriere, S. Mortlock, S. Parsa","submitted_at":"2017-06-12T18:06:45Z","abstract_excerpt":"We present the multiwavelength photometry of two Frontier Fields massive galaxy clusters MACS-J0717 and MACS-J1149 and their parallel fields, ranging from HST to ground based K and Spitzer IRAC bands, and the public release of photometric redshifts and rest frame properties of galaxies found in cluster and parallel pointings. This work was done within ASTRODEEP project and aims to provide a reference for future investigations of the extragalactic populations.\n To fully exploit the depth of the images and detect faint sources we used an accurate procedure which carefully removes the foreground "},"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":"1706.03790","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-12T18:06:45Z","cross_cats_sorted":[],"title_canon_sha256":"aae1636a779c33b2a7f60f3d34a315ad949bac2d72d9e676cfa78457dc292962","abstract_canon_sha256":"c116ab4c4788b635e9f5f9c5c3e2f7e7d81c8e7adb5c4c9686c7677c7f78ce0d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:31:40.870537Z","signature_b64":"tVh5tOxeLnKAn3sqBwLW2pn4T6SLtLiKWmYvmZioXDG0Q+KWWUo2um6BTD0DMjh0oYcj9cdqVZVUC2X0ucEtCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79224be5cb220ab2c6baca3936fffcf3a1227be3d77af3cc6e5b25b486a5c560","last_reissued_at":"2026-05-18T00:31:40.870009Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:31:40.870009Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The ASTRODEEP Frontier Fields Catalogues III. Multiwavelength photometry and rest frame properties of MACS-J0717 and MACS-J1149","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Fontana, A. Grazian, D. Elbaz, E. M\\'armol-Queralt\\'o, E. Merlin, J.S. Dunlop, K. Boutsia, L. Pentericci, M. Castellano, M. Di Criscienzo, M. J. Michalowski, P. Santini, R. Amorin, R. J. McLure, S. Derriere, S. Mortlock, S. Parsa","submitted_at":"2017-06-12T18:06:45Z","abstract_excerpt":"We present the multiwavelength photometry of two Frontier Fields massive galaxy clusters MACS-J0717 and MACS-J1149 and their parallel fields, ranging from HST to ground based K and Spitzer IRAC bands, and the public release of photometric redshifts and rest frame properties of galaxies found in cluster and parallel pointings. This work was done within ASTRODEEP project and aims to provide a reference for future investigations of the extragalactic populations.\n To fully exploit the depth of the images and detect faint sources we used an accurate procedure which carefully removes the foreground "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.03790","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":"1706.03790","created_at":"2026-05-18T00:31:40.870093+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.03790v1","created_at":"2026-05-18T00:31:40.870093+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.03790","created_at":"2026-05-18T00:31:40.870093+00:00"},{"alias_kind":"pith_short_12","alias_value":"PEREXZOLEIFL","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_16","alias_value":"PEREXZOLEIFLFRV2","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_8","alias_value":"PEREXZOL","created_at":"2026-05-18T12:31:37.085036+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/PEREXZOLEIFLFRV2ZI4TN7746O","json":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O.json","graph_json":"https://pith.science/api/pith-number/PEREXZOLEIFLFRV2ZI4TN7746O/graph.json","events_json":"https://pith.science/api/pith-number/PEREXZOLEIFLFRV2ZI4TN7746O/events.json","paper":"https://pith.science/paper/PEREXZOL"},"agent_actions":{"view_html":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O","download_json":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O.json","view_paper":"https://pith.science/paper/PEREXZOL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.03790&json=true","fetch_graph":"https://pith.science/api/pith-number/PEREXZOLEIFLFRV2ZI4TN7746O/graph.json","fetch_events":"https://pith.science/api/pith-number/PEREXZOLEIFLFRV2ZI4TN7746O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O/action/storage_attestation","attest_author":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O/action/author_attestation","sign_citation":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O/action/citation_signature","submit_replication":"https://pith.science/pith/PEREXZOLEIFLFRV2ZI4TN7746O/action/replication_record"}},"created_at":"2026-05-18T00:31:40.870093+00:00","updated_at":"2026-05-18T00:31:40.870093+00:00"}