{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:CAGJHVWFJUIYMAAAHQN3QWRQJG","short_pith_number":"pith:CAGJHVWF","schema_version":"1.0","canonical_sha256":"100c93d6c54d118600003c1bb85a3049b53a0daf874f5a3882c20a4999278102","source":{"kind":"arxiv","id":"1404.7656","version":2},"attestation_state":"computed","paper":{"title":"Large-scale environment of z~5.7 CIV absorption systems I: projected distribution of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"(2) NAOJ, (3) University of Tokyo, (4) Subaru, C. Gonzalo D\\'iaz (1), Emma V. Ryan-Weber (1), Fumiaki Nakata (4) ((1) Swinburne, Jeff Cooke (1), Kazuhiro Shimasaku (3), Masami Ouchi (3), NOAJ), Yusei Koyama (2)","submitted_at":"2014-04-30T09:47:15Z","abstract_excerpt":"Metal absorption systems are products of star formation. They are believed to be associated with massive star forming galaxies, which have significantly enriched their surroundings. To test this idea with high column density CIV absorption systems at z~5.7, we study the projected distribution of galaxies and characterise the environment of CIV systems in two independent quasar lines-of-sight: J103027.01+052455.0 and J113717.73+354956.9. Using wide field photometry (~80x60h$^{-1}$ comoving Mpc), we select bright (Muv(1350\\AA)<-21.0 mag.) Lyman break galaxies (LBGs) at z~5.7 in a redshift slice "},"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":"1404.7656","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-30T09:47:15Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4e4817035e5fb668395af3ddda14c4188e2cfd2922b8946da2a3a671397d9148","abstract_canon_sha256":"cb02d8dd25945bb78c988bd13c5b2f7c685fb7db9fb82cbe3d652dcc3ecd157c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:49:04.318679Z","signature_b64":"6vJOIQIpCYyfoC75DkRixtfdPFVkmrQN/SfFl4AS8yhooHeY0G9KwhWY4m7PICQTxaL5V9T+Nsv3FCHG54c/Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"100c93d6c54d118600003c1bb85a3049b53a0daf874f5a3882c20a4999278102","last_reissued_at":"2026-05-18T02:49:04.318265Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:49:04.318265Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large-scale environment of z~5.7 CIV absorption systems I: projected distribution of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"(2) NAOJ, (3) University of Tokyo, (4) Subaru, C. Gonzalo D\\'iaz (1), Emma V. Ryan-Weber (1), Fumiaki Nakata (4) ((1) Swinburne, Jeff Cooke (1), Kazuhiro Shimasaku (3), Masami Ouchi (3), NOAJ), Yusei Koyama (2)","submitted_at":"2014-04-30T09:47:15Z","abstract_excerpt":"Metal absorption systems are products of star formation. They are believed to be associated with massive star forming galaxies, which have significantly enriched their surroundings. To test this idea with high column density CIV absorption systems at z~5.7, we study the projected distribution of galaxies and characterise the environment of CIV systems in two independent quasar lines-of-sight: J103027.01+052455.0 and J113717.73+354956.9. Using wide field photometry (~80x60h$^{-1}$ comoving Mpc), we select bright (Muv(1350\\AA)<-21.0 mag.) Lyman break galaxies (LBGs) at z~5.7 in a redshift slice "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.7656","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":""},"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":"1404.7656","created_at":"2026-05-18T02:49:04.318328+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.7656v2","created_at":"2026-05-18T02:49:04.318328+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.7656","created_at":"2026-05-18T02:49:04.318328+00:00"},{"alias_kind":"pith_short_12","alias_value":"CAGJHVWFJUIY","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"CAGJHVWFJUIYMAAA","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"CAGJHVWF","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.20622","citing_title":"Connecting CGM enrichment with Lyman alpha emitters at 2.9 < z < 6.7","ref_index":94,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG","json":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG.json","graph_json":"https://pith.science/api/pith-number/CAGJHVWFJUIYMAAAHQN3QWRQJG/graph.json","events_json":"https://pith.science/api/pith-number/CAGJHVWFJUIYMAAAHQN3QWRQJG/events.json","paper":"https://pith.science/paper/CAGJHVWF"},"agent_actions":{"view_html":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG","download_json":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG.json","view_paper":"https://pith.science/paper/CAGJHVWF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.7656&json=true","fetch_graph":"https://pith.science/api/pith-number/CAGJHVWFJUIYMAAAHQN3QWRQJG/graph.json","fetch_events":"https://pith.science/api/pith-number/CAGJHVWFJUIYMAAAHQN3QWRQJG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG/action/storage_attestation","attest_author":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG/action/author_attestation","sign_citation":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG/action/citation_signature","submit_replication":"https://pith.science/pith/CAGJHVWFJUIYMAAAHQN3QWRQJG/action/replication_record"}},"created_at":"2026-05-18T02:49:04.318328+00:00","updated_at":"2026-05-18T02:49:04.318328+00:00"}