{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:AEVM3BDWTR66LD2NWADAA5ZSQQ","short_pith_number":"pith:AEVM3BDW","schema_version":"1.0","canonical_sha256":"012acd84769c7de58f4db006007732840ed66cf1355d9326a427a29c618e3e28","source":{"kind":"arxiv","id":"astro-ph/0204213","version":1},"attestation_state":"computed","paper":{"title":"The Great Observatories Origins Deep Survey","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"AUI), Boston, Caltech, ESO, for the GOODS team: (2) STScI, Gemini, GSFC, IAP, JPL, Mark Dickinson (1), Mauro Giavalisco (1) ((1) STScI, PSU, Saclay, SSC, ST-ECF, U.Ariz., UCB, UCLA, UCSC, U.Fla., U.Hawaii, U.Wisc., Yale","submitted_at":"2002-04-12T15:58:53Z","abstract_excerpt":"The Great Observatories Origins Deep Survey (GOODS) is designed to gather the best and deepest multiwavelength data for studying the formation and evolution of galaxies and active galactic nuclei, the distribution of dark and luminous matter at high redshift, the cosmological parameters from distant supernovae, and the extragalactic background light. The program uses the most powerful space- and ground-based telescopes to cover two fields, each 10'x16', centered on the Hubble Deep Field North and the Chandra Deep Field South, already the sites of extensive observations from X-ray through radio"},"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/0204213","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-04-12T15:58:53Z","cross_cats_sorted":[],"title_canon_sha256":"839b79c797aa25cfbe441d1f7f047e26b7d542c953d556ed0541c2d451cb6a26","abstract_canon_sha256":"e200b518c30f4c6048feb9e41c5d6913b4a9f817980b38326db0c800eb8517c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:55:49.097885Z","signature_b64":"ZqXNIbIEBpPBczGjJ3e5/jrpmL1VdUHMMJy8HlXtGNVfMIMmRx7oPPw13GMk2nDCJ6bUfZEfXHcrwb+BEj+YDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"012acd84769c7de58f4db006007732840ed66cf1355d9326a427a29c618e3e28","last_reissued_at":"2026-07-04T23:55:49.097414Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:55:49.097414Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Great Observatories Origins Deep Survey","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"AUI), Boston, Caltech, ESO, for the GOODS team: (2) STScI, Gemini, GSFC, IAP, JPL, Mark Dickinson (1), Mauro Giavalisco (1) ((1) STScI, PSU, Saclay, SSC, ST-ECF, U.Ariz., UCB, UCLA, UCSC, U.Fla., U.Hawaii, U.Wisc., Yale","submitted_at":"2002-04-12T15:58:53Z","abstract_excerpt":"The Great Observatories Origins Deep Survey (GOODS) is designed to gather the best and deepest multiwavelength data for studying the formation and evolution of galaxies and active galactic nuclei, the distribution of dark and luminous matter at high redshift, the cosmological parameters from distant supernovae, and the extragalactic background light. The program uses the most powerful space- and ground-based telescopes to cover two fields, each 10'x16', centered on the Hubble Deep Field North and the Chandra Deep Field South, already the sites of extensive observations from X-ray through radio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0204213","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/0204213/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/0204213","created_at":"2026-07-04T23:55:49.097474+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0204213v1","created_at":"2026-07-04T23:55:49.097474+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0204213","created_at":"2026-07-04T23:55:49.097474+00:00"},{"alias_kind":"pith_short_12","alias_value":"AEVM3BDWTR66","created_at":"2026-07-04T23:55:49.097474+00:00"},{"alias_kind":"pith_short_16","alias_value":"AEVM3BDWTR66LD2N","created_at":"2026-07-04T23:55:49.097474+00:00"},{"alias_kind":"pith_short_8","alias_value":"AEVM3BDW","created_at":"2026-07-04T23:55:49.097474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.18504","citing_title":"NOEMA3D: extended CO, [C I] and dust in massive star-forming main sequence galaxies at cosmic noon","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18503","citing_title":"NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ","json":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ.json","graph_json":"https://pith.science/api/pith-number/AEVM3BDWTR66LD2NWADAA5ZSQQ/graph.json","events_json":"https://pith.science/api/pith-number/AEVM3BDWTR66LD2NWADAA5ZSQQ/events.json","paper":"https://pith.science/paper/AEVM3BDW"},"agent_actions":{"view_html":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ","download_json":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ.json","view_paper":"https://pith.science/paper/AEVM3BDW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0204213&json=true","fetch_graph":"https://pith.science/api/pith-number/AEVM3BDWTR66LD2NWADAA5ZSQQ/graph.json","fetch_events":"https://pith.science/api/pith-number/AEVM3BDWTR66LD2NWADAA5ZSQQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ/action/storage_attestation","attest_author":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ/action/author_attestation","sign_citation":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ/action/citation_signature","submit_replication":"https://pith.science/pith/AEVM3BDWTR66LD2NWADAA5ZSQQ/action/replication_record"}},"created_at":"2026-07-04T23:55:49.097474+00:00","updated_at":"2026-07-04T23:55:49.097474+00:00"}