{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:LP7ZCQCPLYPV2L5N6PIJ4TPDGT","short_pith_number":"pith:LP7ZCQCP","schema_version":"1.0","canonical_sha256":"5bff91404f5e1f5d2fadf3d09e4de334d31a5981c87adfb5eca58aa83cd60e60","source":{"kind":"arxiv","id":"2409.00169","version":3},"attestation_state":"computed","paper":{"title":"ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"A. Calabr\\`o, A. Fontana, A. Grazian, A. Kirkpatrick, A. M. Koekemoer, B. Vulcani, C. Papovich, C. T. Donnan, D. D. Kocevski, D. J. McLeod, D. K. Magee, D. Marchesini, D. Paris, E. Merlin, F. Fortuni, G. Leung, G. Roberts-Borsani, G. Yang, H. C. Ferguson, J. M. Lotz, J. R. Trump, J. S. Dunlop, J. S. Kartaltepe, K. Boyett, K. Davis, K. Glazebrook, L. J. Kewley, L. Napolitano, L. Pentericci, L. Y. A. Yung, M. Bagley, M. Castellano, M. Correnti, M. Dickinson, M. Giavalisco, M. Hirschmann, M. Nonino, M. Trenti, N. A. Grogin, N. Hathi, N. Pirzkal, P. Arrabal Haro, P. G. P\\'erez-Gonz\\'alez, P. J. Watson, P. Santini, R. A. Lucas, R. J. McLure, R. S. Somerville, S. L. Finkelstein, S. Mascia, S. M. Wilkins, S. Ravindranath, T. Nanayakkara, T. Treu, X. Wang","submitted_at":"2024-08-30T18:00:00Z","abstract_excerpt":"We present a set of photometric catalogs primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the high redshift Universe. The set gathers data from eight JWST NIRCam observational programs, targeting the Abell 2744 (GLASS-JWST, UNCOVER, DDT2756 and GO3990), EGS (CEERS), COSMOS and UDS (PRIMER), and GOODS North and South (JADES and NGDEEP) deep fields, for a total area of $\\sim$0.2 sq. degrees. Photometric estimates are obtained by means of well-established techniques, including tailored improvements designed to enhance the performance "},"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":"2409.00169","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-08-30T18:00:00Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"267456c35caf02f8861ba66156055da61be4f49bb0f034ff68c783053f45fb0e","abstract_canon_sha256":"6256244072322f12d8eb9daead154147f96f61ebe796f724247b0b596797c61d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:37:40.275534Z","signature_b64":"aRyS/TSSn84H9Jhp1IQ/umHN8RONpcSW2fLSqY2FMh0AYYhYkrlOgm9jHVDQvR1YSSiE31AJEjGqTBKViIcoBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5bff91404f5e1f5d2fadf3d09e4de334d31a5981c87adfb5eca58aa83cd60e60","last_reissued_at":"2026-07-05T09:37:40.275027Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:37:40.275027Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"A. Calabr\\`o, A. Fontana, A. Grazian, A. Kirkpatrick, A. M. Koekemoer, B. Vulcani, C. Papovich, C. T. Donnan, D. D. Kocevski, D. J. McLeod, D. K. Magee, D. Marchesini, D. Paris, E. Merlin, F. Fortuni, G. Leung, G. Roberts-Borsani, G. Yang, H. C. Ferguson, J. M. Lotz, J. R. Trump, J. S. Dunlop, J. S. Kartaltepe, K. Boyett, K. Davis, K. Glazebrook, L. J. Kewley, L. Napolitano, L. Pentericci, L. Y. A. Yung, M. Bagley, M. Castellano, M. Correnti, M. Dickinson, M. Giavalisco, M. Hirschmann, M. Nonino, M. Trenti, N. A. Grogin, N. Hathi, N. Pirzkal, P. Arrabal Haro, P. G. P\\'erez-Gonz\\'alez, P. J. Watson, P. Santini, R. A. Lucas, R. J. McLure, R. S. Somerville, S. L. Finkelstein, S. Mascia, S. M. Wilkins, S. Ravindranath, T. Nanayakkara, T. Treu, X. Wang","submitted_at":"2024-08-30T18:00:00Z","abstract_excerpt":"We present a set of photometric catalogs primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the high redshift Universe. The set gathers data from eight JWST NIRCam observational programs, targeting the Abell 2744 (GLASS-JWST, UNCOVER, DDT2756 and GO3990), EGS (CEERS), COSMOS and UDS (PRIMER), and GOODS North and South (JADES and NGDEEP) deep fields, for a total area of $\\sim$0.2 sq. degrees. Photometric estimates are obtained by means of well-established techniques, including tailored improvements designed to enhance the performance "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2409.00169","kind":"arxiv","version":3},"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/2409.00169/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":"2409.00169","created_at":"2026-07-05T09:37:40.275083+00:00"},{"alias_kind":"arxiv_version","alias_value":"2409.00169v3","created_at":"2026-07-05T09:37:40.275083+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2409.00169","created_at":"2026-07-05T09:37:40.275083+00:00"},{"alias_kind":"pith_short_12","alias_value":"LP7ZCQCPLYPV","created_at":"2026-07-05T09:37:40.275083+00:00"},{"alias_kind":"pith_short_16","alias_value":"LP7ZCQCPLYPV2L5N","created_at":"2026-07-05T09:37:40.275083+00:00"},{"alias_kind":"pith_short_8","alias_value":"LP7ZCQCP","created_at":"2026-07-05T09:37:40.275083+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.02773","citing_title":"Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2502.02637","citing_title":"Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS","ref_index":90,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT","json":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT.json","graph_json":"https://pith.science/api/pith-number/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/graph.json","events_json":"https://pith.science/api/pith-number/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/events.json","paper":"https://pith.science/paper/LP7ZCQCP"},"agent_actions":{"view_html":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT","download_json":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT.json","view_paper":"https://pith.science/paper/LP7ZCQCP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2409.00169&json=true","fetch_graph":"https://pith.science/api/pith-number/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/graph.json","fetch_events":"https://pith.science/api/pith-number/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/action/storage_attestation","attest_author":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/action/author_attestation","sign_citation":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/action/citation_signature","submit_replication":"https://pith.science/pith/LP7ZCQCPLYPV2L5N6PIJ4TPDGT/action/replication_record"}},"created_at":"2026-07-05T09:37:40.275083+00:00","updated_at":"2026-07-05T09:37:40.275083+00:00"}