{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:FLYFO5H54YIRHCURWT432BQASZ","short_pith_number":"pith:FLYFO5H5","schema_version":"1.0","canonical_sha256":"2af05774fde611138a91b4f9bd060096510d1b3b4010d8261a98aad01a6c6d11","source":{"kind":"arxiv","id":"2206.14908","version":1},"attestation_state":"computed","paper":{"title":"The Prime Focus Spectrograph Galaxy Evolution Survey","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jenny Greene, John Silverman, Masami Ouchi, Rachel Bezanson, the PFS Galaxy Evolution Working Group","submitted_at":"2022-06-29T20:51:22Z","abstract_excerpt":"We present the Prime Focus Spectrograph (PFS) Galaxy Evolution pillar of the 360-night PFS Subaru Strategic Program. This 130-night program will capitalize on the wide wavelength coverage and massive multiplexing capabilities of PFS to study the evolution of typical galaxies from cosmic dawn to the present. From Lyman alpha emitters at z~7 to probe reionization, drop-outs at z~3 to map the inter-galactic medium in absorption, and a continuum-selected sample at z~1.5, we will chart the physics of galaxy evolution within the evolving cosmic web. This article is dedicated to the memory of Olivier"},"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":"2206.14908","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-06-29T20:51:22Z","cross_cats_sorted":[],"title_canon_sha256":"728396ec72dbd7cb509d5aec587e918bb06a43889a19f15d76b7d97d9db55524","abstract_canon_sha256":"7fcd7b4c745108f243f0c15a21b853a12d16034f6350dd2ff55ee10e8922aa9b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:36:11.577527Z","signature_b64":"L2XbS2l86O4axQIlzAxbanV+xcpnZ0Sftf1S5FHoSTAPRHJ8+bI4gl9aeeg7Dd06bOTka/VKBrynUHx9y+b6Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2af05774fde611138a91b4f9bd060096510d1b3b4010d8261a98aad01a6c6d11","last_reissued_at":"2026-07-05T04:36:11.577074Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:36:11.577074Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Prime Focus Spectrograph Galaxy Evolution Survey","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jenny Greene, John Silverman, Masami Ouchi, Rachel Bezanson, the PFS Galaxy Evolution Working Group","submitted_at":"2022-06-29T20:51:22Z","abstract_excerpt":"We present the Prime Focus Spectrograph (PFS) Galaxy Evolution pillar of the 360-night PFS Subaru Strategic Program. This 130-night program will capitalize on the wide wavelength coverage and massive multiplexing capabilities of PFS to study the evolution of typical galaxies from cosmic dawn to the present. From Lyman alpha emitters at z~7 to probe reionization, drop-outs at z~3 to map the inter-galactic medium in absorption, and a continuum-selected sample at z~1.5, we will chart the physics of galaxy evolution within the evolving cosmic web. This article is dedicated to the memory of Olivier"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.14908","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/2206.14908/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":"2206.14908","created_at":"2026-07-05T04:36:11.577150+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.14908v1","created_at":"2026-07-05T04:36:11.577150+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.14908","created_at":"2026-07-05T04:36:11.577150+00:00"},{"alias_kind":"pith_short_12","alias_value":"FLYFO5H54YIR","created_at":"2026-07-05T04:36:11.577150+00:00"},{"alias_kind":"pith_short_16","alias_value":"FLYFO5H54YIRHCUR","created_at":"2026-07-05T04:36:11.577150+00:00"},{"alias_kind":"pith_short_8","alias_value":"FLYFO5H5","created_at":"2026-07-05T04:36:11.577150+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26234","citing_title":"Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level","ref_index":81,"is_internal_anchor":false},{"citing_arxiv_id":"2606.11089","citing_title":"MusE GAs FLOw and Wind (MEGAFLOW) XIV: Background-Galaxy Absorption Reveals Kiloparsec-Scale Structure in the Cool Circumgalactic Medium","ref_index":31,"is_internal_anchor":false},{"citing_arxiv_id":"2606.24744","citing_title":"Unlocking the Full Potential of SKAO Extra-galactic Science with High-multiplex Optical Spectroscopy","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2507.16115","citing_title":"Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2509.07453","citing_title":"Cross-correlations between the CLAMATO Lyman-alpha forest and galaxies within the COSMOS field","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2509.23549","citing_title":"Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman","ref_index":51,"is_internal_anchor":false},{"citing_arxiv_id":"2601.10709","citing_title":"Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06791","citing_title":"Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon","ref_index":267,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09875","citing_title":"Galactic Archaeology with the Subaru `\\=Onohi`ula Prime Focus Spectrograph Strategic Program","ref_index":121,"is_internal_anchor":false},{"citing_arxiv_id":"2604.16792","citing_title":"The Role of Cluster Environments in Quiescent Galaxy Stellar Halo Assembly","ref_index":74,"is_internal_anchor":false},{"citing_arxiv_id":"2605.01994","citing_title":"Baryons in the Darkest Sites of the Universe","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ","json":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ.json","graph_json":"https://pith.science/api/pith-number/FLYFO5H54YIRHCURWT432BQASZ/graph.json","events_json":"https://pith.science/api/pith-number/FLYFO5H54YIRHCURWT432BQASZ/events.json","paper":"https://pith.science/paper/FLYFO5H5"},"agent_actions":{"view_html":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ","download_json":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ.json","view_paper":"https://pith.science/paper/FLYFO5H5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.14908&json=true","fetch_graph":"https://pith.science/api/pith-number/FLYFO5H54YIRHCURWT432BQASZ/graph.json","fetch_events":"https://pith.science/api/pith-number/FLYFO5H54YIRHCURWT432BQASZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ/action/storage_attestation","attest_author":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ/action/author_attestation","sign_citation":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ/action/citation_signature","submit_replication":"https://pith.science/pith/FLYFO5H54YIRHCURWT432BQASZ/action/replication_record"}},"created_at":"2026-07-05T04:36:11.577150+00:00","updated_at":"2026-07-05T04:36:11.577150+00:00"}