{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:S373GNFSDK7D2AC4VPA4YMROM4","short_pith_number":"pith:S373GNFS","schema_version":"1.0","canonical_sha256":"96ffb334b21abe3d005cabc1cc322e67161630e33e0a0b85647cbbe3c975a6a8","source":{"kind":"arxiv","id":"2011.06469","version":2},"attestation_state":"computed","paper":{"title":"Consistency of cosmic shear analyses in harmonic and real space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amon, A. A. Plazas, A. Carnero Rosell, A. Choi, A. Fert\\'e, A. Palmese, A. Roodman, B. Jain, C. Chang, C. Doux, C. To, D. Bacon, D. Brooks, DES Collaboration, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. Hollowood, D. W. Gerdes, E. Bertin, E. Gaztanaga, E. Krause, E. Sanchez, E. Suchyta, F. Menanteau, F. Paz-Chinch\\'on, G. Gutierrez, G. Tarle, H. Camacho, I. Ferrero, I. Sevilla-Noarbe, J. Blazek, J. Carretero, J. Garc\\'ia-Bellido, J. Gschwend, J. L. Marshall, J. P. Dietrich, J. Weller, J. Zuntz, K. Kuehn, L. F. Secco, L. N. da Costa, M. A. G. Maia, M. Aguena, M. A. Troxel, M. Carrasco Kind, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Gatti, M. Schubnell, M. Smith, N. Kuropatkin, N. MacCrann, P. Doel, P. Fosalba, R. A. Gruendl, R.D. Wilkinson, R. Miquel, R. Morgan, S. Allam, S. Avila, S. R. Hinton, S. Samuroff, S. Serrano, T. M. Davis, T. N. Varga, W. G. Hartley, X. Fang","submitted_at":"2020-11-12T16:21:03Z","abstract_excerpt":"Recent cosmic shear studies have reported discrepancies of up to $1\\sigma$ on the parameter ${S_{8}=\\sigma_{8}\\sqrt{\\Omega_{\\rm m}/0.3}}$ between the analysis of shear power spectra and two-point correlation functions, derived from the same shear catalogs. It is not a priori clear whether the measured discrepancies are consistent with statistical fluctuations. In this paper, we investigate this issue in the context of the forthcoming analyses from the third year data of the Dark Energy Survey (DES-Y3). We analyze DES-Y3 mock catalogs from Gaussian simulations with a fast and accurate importanc"},"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":"2011.06469","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2020-11-12T16:21:03Z","cross_cats_sorted":[],"title_canon_sha256":"4f6fe43c25c5c31b8344da462ada394f6d5b813231b4cb23c5c27de8cd72e9f2","abstract_canon_sha256":"46b459c9e6c0a8b896be7a257dd5814c967dac6924e1808a69e1989fc38f929d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:33:06.506717Z","signature_b64":"KjTX8I8EshmCWzPMp7BrHmii3avc2UIsCjkbZntKBbRztWNRTDm5czUnxuhxvksCxYPCNVXl4hLR8lU4FSOEDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96ffb334b21abe3d005cabc1cc322e67161630e33e0a0b85647cbbe3c975a6a8","last_reissued_at":"2026-07-05T02:33:06.506197Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:33:06.506197Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Consistency of cosmic shear analyses in harmonic and real space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amon, A. A. Plazas, A. Carnero Rosell, A. Choi, A. Fert\\'e, A. Palmese, A. Roodman, B. Jain, C. Chang, C. Doux, C. To, D. Bacon, D. Brooks, DES Collaboration, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. Hollowood, D. W. Gerdes, E. Bertin, E. Gaztanaga, E. Krause, E. Sanchez, E. Suchyta, F. Menanteau, F. Paz-Chinch\\'on, G. Gutierrez, G. Tarle, H. Camacho, I. Ferrero, I. Sevilla-Noarbe, J. Blazek, J. Carretero, J. Garc\\'ia-Bellido, J. Gschwend, J. L. Marshall, J. P. Dietrich, J. Weller, J. Zuntz, K. Kuehn, L. F. Secco, L. N. da Costa, M. A. G. Maia, M. Aguena, M. A. Troxel, M. Carrasco Kind, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Gatti, M. Schubnell, M. Smith, N. Kuropatkin, N. MacCrann, P. Doel, P. Fosalba, R. A. Gruendl, R.D. Wilkinson, R. Miquel, R. Morgan, S. Allam, S. Avila, S. R. Hinton, S. Samuroff, S. Serrano, T. M. Davis, T. N. Varga, W. G. Hartley, X. Fang","submitted_at":"2020-11-12T16:21:03Z","abstract_excerpt":"Recent cosmic shear studies have reported discrepancies of up to $1\\sigma$ on the parameter ${S_{8}=\\sigma_{8}\\sqrt{\\Omega_{\\rm m}/0.3}}$ between the analysis of shear power spectra and two-point correlation functions, derived from the same shear catalogs. It is not a priori clear whether the measured discrepancies are consistent with statistical fluctuations. In this paper, we investigate this issue in the context of the forthcoming analyses from the third year data of the Dark Energy Survey (DES-Y3). We analyze DES-Y3 mock catalogs from Gaussian simulations with a fast and accurate importanc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2011.06469","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/2011.06469/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":"2011.06469","created_at":"2026-07-05T02:33:06.506265+00:00"},{"alias_kind":"arxiv_version","alias_value":"2011.06469v2","created_at":"2026-07-05T02:33:06.506265+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2011.06469","created_at":"2026-07-05T02:33:06.506265+00:00"},{"alias_kind":"pith_short_12","alias_value":"S373GNFSDK7D","created_at":"2026-07-05T02:33:06.506265+00:00"},{"alias_kind":"pith_short_16","alias_value":"S373GNFSDK7D2AC4","created_at":"2026-07-05T02:33:06.506265+00:00"},{"alias_kind":"pith_short_8","alias_value":"S373GNFS","created_at":"2026-07-05T02:33:06.506265+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2105.13549","citing_title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","ref_index":114,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4","json":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4.json","graph_json":"https://pith.science/api/pith-number/S373GNFSDK7D2AC4VPA4YMROM4/graph.json","events_json":"https://pith.science/api/pith-number/S373GNFSDK7D2AC4VPA4YMROM4/events.json","paper":"https://pith.science/paper/S373GNFS"},"agent_actions":{"view_html":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4","download_json":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4.json","view_paper":"https://pith.science/paper/S373GNFS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2011.06469&json=true","fetch_graph":"https://pith.science/api/pith-number/S373GNFSDK7D2AC4VPA4YMROM4/graph.json","fetch_events":"https://pith.science/api/pith-number/S373GNFSDK7D2AC4VPA4YMROM4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4/action/storage_attestation","attest_author":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4/action/author_attestation","sign_citation":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4/action/citation_signature","submit_replication":"https://pith.science/pith/S373GNFSDK7D2AC4VPA4YMROM4/action/replication_record"}},"created_at":"2026-07-05T02:33:06.506265+00:00","updated_at":"2026-07-05T02:33:06.506265+00:00"}