{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:CWVQM6DA2KWAHLMMMD7I6IKGGC","short_pith_number":"pith:CWVQM6DA","schema_version":"1.0","canonical_sha256":"15ab067860d2ac03ad8c60fe8f214630b11f9aad79442972eedbb06bcd6323c2","source":{"kind":"arxiv","id":"1910.09517","version":2},"attestation_state":"computed","paper":{"title":"The ALPINE-ALMA [CII] survey: Survey strategy, observations and sample properties of 118 star-forming galaxies at $4<z<6$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Faisst, D. Schaerer, G. Jones, J.D. Silverman, L. Yan, M. B\\'ethermin, O. Le F\\`evre, P. Capak, P. Cassata, the ALPINE team","submitted_at":"2019-10-21T17:16:17Z","abstract_excerpt":"The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) features 118 galaxies observed in the [CII]-158$\\mu$m line and far infrared (FIR) continuum emission during the period of rapid mass assembly, right after the end of the HI reionization, at redshifts of 4<z<6. We present the survey science goals, the observational strategy, and the sample selection of the 118 galaxies observed with ALMA, with an average beam minor axis of about 0.85 arcsec, or $\\sim$5 kpc at the median redshif"},"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":"1910.09517","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-10-21T17:16:17Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"d091c6cfe2d7f63ed1b730af2c6a402100f394bed94f013bb47fb42817f1f021","abstract_canon_sha256":"ec83a0d9af8d053a0a8377049adad0512a140eb54bfca4296dfb225dd08f11dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:46:43.596902Z","signature_b64":"JC5iBRY4PhvDpgu7ot8bn6tWTcH52W4vOgzJa0iPS8Yu/4WqVvCmi2Djnu49zILVEOH3y8TBfWWlnVKBoqoFDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15ab067860d2ac03ad8c60fe8f214630b11f9aad79442972eedbb06bcd6323c2","last_reissued_at":"2026-07-05T01:46:43.596407Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:46:43.596407Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The ALPINE-ALMA [CII] survey: Survey strategy, observations and sample properties of 118 star-forming galaxies at $4<z<6$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Faisst, D. Schaerer, G. Jones, J.D. Silverman, L. Yan, M. B\\'ethermin, O. Le F\\`evre, P. Capak, P. Cassata, the ALPINE team","submitted_at":"2019-10-21T17:16:17Z","abstract_excerpt":"The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) features 118 galaxies observed in the [CII]-158$\\mu$m line and far infrared (FIR) continuum emission during the period of rapid mass assembly, right after the end of the HI reionization, at redshifts of 4<z<6. We present the survey science goals, the observational strategy, and the sample selection of the 118 galaxies observed with ALMA, with an average beam minor axis of about 0.85 arcsec, or $\\sim$5 kpc at the median redshif"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.09517","kind":"arxiv","version":2},"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/1910.09517/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":"1910.09517","created_at":"2026-07-05T01:46:43.596466+00:00"},{"alias_kind":"arxiv_version","alias_value":"1910.09517v2","created_at":"2026-07-05T01:46:43.596466+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1910.09517","created_at":"2026-07-05T01:46:43.596466+00:00"},{"alias_kind":"pith_short_12","alias_value":"CWVQM6DA2KWA","created_at":"2026-07-05T01:46:43.596466+00:00"},{"alias_kind":"pith_short_16","alias_value":"CWVQM6DA2KWAHLMM","created_at":"2026-07-05T01:46:43.596466+00:00"},{"alias_kind":"pith_short_8","alias_value":"CWVQM6DA","created_at":"2026-07-05T01:46:43.596466+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05523","citing_title":"BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\\simeq5.23$","ref_index":94,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC","json":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC.json","graph_json":"https://pith.science/api/pith-number/CWVQM6DA2KWAHLMMMD7I6IKGGC/graph.json","events_json":"https://pith.science/api/pith-number/CWVQM6DA2KWAHLMMMD7I6IKGGC/events.json","paper":"https://pith.science/paper/CWVQM6DA"},"agent_actions":{"view_html":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC","download_json":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC.json","view_paper":"https://pith.science/paper/CWVQM6DA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1910.09517&json=true","fetch_graph":"https://pith.science/api/pith-number/CWVQM6DA2KWAHLMMMD7I6IKGGC/graph.json","fetch_events":"https://pith.science/api/pith-number/CWVQM6DA2KWAHLMMMD7I6IKGGC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC/action/storage_attestation","attest_author":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC/action/author_attestation","sign_citation":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC/action/citation_signature","submit_replication":"https://pith.science/pith/CWVQM6DA2KWAHLMMMD7I6IKGGC/action/replication_record"}},"created_at":"2026-07-05T01:46:43.596466+00:00","updated_at":"2026-07-05T01:46:43.596466+00:00"}