{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:NJSI32H3VRWD2LACDZHJMQVEZ7","short_pith_number":"pith:NJSI32H3","schema_version":"1.0","canonical_sha256":"6a648de8fbac6c3d2c021e4e9642a4cfd4bcaf2b8027bd0eb5ca417e315ded0a","source":{"kind":"arxiv","id":"2208.08516","version":3},"attestation_state":"computed","paper":{"title":"The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission Line Galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Aaron M. Meisner, A. Berti, A. Carr, Adam D. Myers, A. de la Macorra, A. Dey, A. Edge, A. Font-Ribera, A. Glanville, A. J. Ross, A. Kovacs, A. Kremin, A.P. Cooper, A. Raichoor, A. Rocher, B. A. Weaver, Biprateep Dey, B. Weiner, C. Balland, C. G. Sabiu, C. Hahn, C. Howlett, Christophe Yeche, C. Magneville, C. Poppett, C. Saulder, David M. Alexander, D. Brooks, D. Parkinson, D. Sierra-Porta, E. Armengaud, E. Gaztanaga, F. Prada, G. Dhungana, Gregory Tarle, H. Chittenden, Ho Seong Hwang, H. Zou, J.D.Nie, Jeffrey A. Newman, J. Guy, J. Moustakas, J. Xavier Prochaska, J. Yu, K. Dawson, K. Douglass, K. Fanning, K. Said, K. Zhang, L. Garrison, L. Jiang, L. Le Guillou, M.-C. Cousinou, Michael E. Levi, M. Landriau, M. Mezcua, M. Oh, M. Schubnell, N. Palanque-Delabrouille, P. Doel, P. Zarrouk, R. Canning, R. Kehoe, R. Miquel, Rongpu Zhou, R. Tojeiro, S. Ahlen, S. Bailey, S. BenZvi, S. Cole, S. Eftekharzadeh, S. Escoffier, S. Gontcho A Gontcho, S. Moore, S. Nadathur, Ting-Wen Lan, T. Kisner, T. M. Davis, V. Ruhlmann-Kleider, W.J. Percival, Y. Zhang, Zhimin Zhou","submitted_at":"2022-08-17T20:11:49Z","abstract_excerpt":"The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections. To assist in these tasks, we visually inspect (VI) DESI spectra of approximately 2,500 bright galaxies, 3,500 luminous red galaxies (LRGs), and 10,000 emission line galaxies (ELGs), to obtain robust redshift identifications. We then utilize the VI redshift information to characterize the performance of the DESI operation. Based on the VI catalogs, our results show that the final survey design yields samples of bright gala"},"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":"2208.08516","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-08-17T20:11:49Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"099fda067f1509b64d5dc318c0e6a3f3631ad9646cfbcc25890c2c3f9e6416db","abstract_canon_sha256":"dfcdf35ca9f1b5d591e7ffc19ad0856748b55207e41071a4ab0cf72a674cb2da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:17:31.220282Z","signature_b64":"Vonrb8E8ywRu1aAwO+mNfX0twfb2U+cQDkWUELq9teb6TaKoqkZUUDpw8AzwcT3HAi1E6gPc4Lx4L0HKk/ynBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6a648de8fbac6c3d2c021e4e9642a4cfd4bcaf2b8027bd0eb5ca417e315ded0a","last_reissued_at":"2026-07-05T09:17:31.219773Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:17:31.219773Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission Line Galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Aaron M. Meisner, A. Berti, A. Carr, Adam D. Myers, A. de la Macorra, A. Dey, A. Edge, A. Font-Ribera, A. Glanville, A. J. Ross, A. Kovacs, A. Kremin, A.P. Cooper, A. Raichoor, A. Rocher, B. A. Weaver, Biprateep Dey, B. Weiner, C. Balland, C. G. Sabiu, C. Hahn, C. Howlett, Christophe Yeche, C. Magneville, C. Poppett, C. Saulder, David M. Alexander, D. Brooks, D. Parkinson, D. Sierra-Porta, E. Armengaud, E. Gaztanaga, F. Prada, G. Dhungana, Gregory Tarle, H. Chittenden, Ho Seong Hwang, H. Zou, J.D.Nie, Jeffrey A. Newman, J. Guy, J. Moustakas, J. Xavier Prochaska, J. Yu, K. Dawson, K. Douglass, K. Fanning, K. Said, K. Zhang, L. Garrison, L. Jiang, L. Le Guillou, M.-C. Cousinou, Michael E. Levi, M. Landriau, M. Mezcua, M. Oh, M. Schubnell, N. Palanque-Delabrouille, P. Doel, P. Zarrouk, R. Canning, R. Kehoe, R. Miquel, Rongpu Zhou, R. Tojeiro, S. Ahlen, S. Bailey, S. BenZvi, S. Cole, S. Eftekharzadeh, S. Escoffier, S. Gontcho A Gontcho, S. Moore, S. Nadathur, Ting-Wen Lan, T. Kisner, T. M. Davis, V. Ruhlmann-Kleider, W.J. Percival, Y. Zhang, Zhimin Zhou","submitted_at":"2022-08-17T20:11:49Z","abstract_excerpt":"The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections. To assist in these tasks, we visually inspect (VI) DESI spectra of approximately 2,500 bright galaxies, 3,500 luminous red galaxies (LRGs), and 10,000 emission line galaxies (ELGs), to obtain robust redshift identifications. We then utilize the VI redshift information to characterize the performance of the DESI operation. Based on the VI catalogs, our results show that the final survey design yields samples of bright gala"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.08516","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/2208.08516/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":"2208.08516","created_at":"2026-07-05T09:17:31.219840+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.08516v3","created_at":"2026-07-05T09:17:31.219840+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.08516","created_at":"2026-07-05T09:17:31.219840+00:00"},{"alias_kind":"pith_short_12","alias_value":"NJSI32H3VRWD","created_at":"2026-07-05T09:17:31.219840+00:00"},{"alias_kind":"pith_short_16","alias_value":"NJSI32H3VRWD2LAC","created_at":"2026-07-05T09:17:31.219840+00:00"},{"alias_kind":"pith_short_8","alias_value":"NJSI32H3","created_at":"2026-07-05T09:17:31.219840+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07875","citing_title":"Alcock-Paczynski Blinding Scheme for the Ly-$\\alpha$ Forest Analysis","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2503.14744","citing_title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape","ref_index":90,"is_internal_anchor":false},{"citing_arxiv_id":"2404.03002","citing_title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","ref_index":101,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7","json":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7.json","graph_json":"https://pith.science/api/pith-number/NJSI32H3VRWD2LACDZHJMQVEZ7/graph.json","events_json":"https://pith.science/api/pith-number/NJSI32H3VRWD2LACDZHJMQVEZ7/events.json","paper":"https://pith.science/paper/NJSI32H3"},"agent_actions":{"view_html":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7","download_json":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7.json","view_paper":"https://pith.science/paper/NJSI32H3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.08516&json=true","fetch_graph":"https://pith.science/api/pith-number/NJSI32H3VRWD2LACDZHJMQVEZ7/graph.json","fetch_events":"https://pith.science/api/pith-number/NJSI32H3VRWD2LACDZHJMQVEZ7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7/action/storage_attestation","attest_author":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7/action/author_attestation","sign_citation":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7/action/citation_signature","submit_replication":"https://pith.science/pith/NJSI32H3VRWD2LACDZHJMQVEZ7/action/replication_record"}},"created_at":"2026-07-05T09:17:31.219840+00:00","updated_at":"2026-07-05T09:17:31.219840+00:00"}