{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:UOPYM4UDPWGS633WDAGRMR5IL7","short_pith_number":"pith:UOPYM4UD","schema_version":"1.0","canonical_sha256":"a39f8672837d8d2f6f76180d1647a85fc9627a9b595936df59361353773ece03","source":{"kind":"arxiv","id":"2509.25166","version":1},"attestation_state":"computed","paper":{"title":"Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Halder, C. MacMahon-Gell\\'er, C. T. Davies, C. Uhlemann, J. Armijo, J. Blazek, J. Harnois-D\\'eraps, J. Liu, K. Heitmann, L. Castiblanco, L. Linke, L. Medina Varela, L. Porth, N. van Alfen, N. \\v{S}ar\\v{c}evi\\'c, P. Larsen, S. Rangel, The LSST Dark Energy Science Collaboration","submitted_at":"2025-09-29T17:58:19Z","abstract_excerpt":"Intrinsic alignments (IA) of galaxies is one of the key secondary signals to cosmic shear measurements, and must be modeled to interpret weak lensing data and infer the correct cosmology. There are large uncertainties in the physical description of IA, and analytical calculations are often out of reach for weak lensing statistics beyond two-point functions. We present here a set of six flexible IA models infused directly into weak lensing simulations, constructed from the mass shells, the projected tidal fields and, optionally, dark matter halo catalogues. We start with the non-linear linear a"},"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":"2509.25166","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-09-29T17:58:19Z","cross_cats_sorted":[],"title_canon_sha256":"2db00c0619368f32c449e3f1d7f24501dc15d4e7cefb9191d10589e4b6946db1","abstract_canon_sha256":"d2440ecd142ca40058d8bf3f68f019c64f7d0dd6169a96acbc232e2eb8793720"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-22T14:23:26.879626Z","signature_b64":"a3+6i3FidG7XhpqkeFOBiYF31pSGPFnb/VbvaQEEiu3UKND86wBrQAqRtf3cG1iSGKFsTfqfBH+VAyA/YuZPBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a39f8672837d8d2f6f76180d1647a85fc9627a9b595936df59361353773ece03","last_reissued_at":"2026-07-22T14:23:26.878708Z","signature_status":"signed_v1","first_computed_at":"2026-07-22T14:23:26.878708Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Halder, C. MacMahon-Gell\\'er, C. T. Davies, C. Uhlemann, J. Armijo, J. Blazek, J. Harnois-D\\'eraps, J. Liu, K. Heitmann, L. Castiblanco, L. Linke, L. Medina Varela, L. Porth, N. van Alfen, N. \\v{S}ar\\v{c}evi\\'c, P. Larsen, S. Rangel, The LSST Dark Energy Science Collaboration","submitted_at":"2025-09-29T17:58:19Z","abstract_excerpt":"Intrinsic alignments (IA) of galaxies is one of the key secondary signals to cosmic shear measurements, and must be modeled to interpret weak lensing data and infer the correct cosmology. There are large uncertainties in the physical description of IA, and analytical calculations are often out of reach for weak lensing statistics beyond two-point functions. We present here a set of six flexible IA models infused directly into weak lensing simulations, constructed from the mass shells, the projected tidal fields and, optionally, dark matter halo catalogues. We start with the non-linear linear a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2509.25166","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/2509.25166/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":"2509.25166","created_at":"2026-07-22T14:23:26.879127+00:00"},{"alias_kind":"arxiv_version","alias_value":"2509.25166v1","created_at":"2026-07-22T14:23:26.879127+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2509.25166","created_at":"2026-07-22T14:23:26.879127+00:00"},{"alias_kind":"pith_short_12","alias_value":"UOPYM4UDPWGS","created_at":"2026-07-22T14:23:26.879127+00:00"},{"alias_kind":"pith_short_16","alias_value":"UOPYM4UDPWGS633W","created_at":"2026-07-22T14:23:26.879127+00:00"},{"alias_kind":"pith_short_8","alias_value":"UOPYM4UD","created_at":"2026-07-22T14:23:26.879127+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.00818","citing_title":"$4\\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback","ref_index":76,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7","json":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7.json","graph_json":"https://pith.science/api/pith-number/UOPYM4UDPWGS633WDAGRMR5IL7/graph.json","events_json":"https://pith.science/api/pith-number/UOPYM4UDPWGS633WDAGRMR5IL7/events.json","paper":"https://pith.science/paper/UOPYM4UD"},"agent_actions":{"view_html":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7","download_json":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7.json","view_paper":"https://pith.science/paper/UOPYM4UD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2509.25166&json=true","fetch_graph":"https://pith.science/api/pith-number/UOPYM4UDPWGS633WDAGRMR5IL7/graph.json","fetch_events":"https://pith.science/api/pith-number/UOPYM4UDPWGS633WDAGRMR5IL7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7/action/storage_attestation","attest_author":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7/action/author_attestation","sign_citation":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7/action/citation_signature","submit_replication":"https://pith.science/pith/UOPYM4UDPWGS633WDAGRMR5IL7/action/replication_record"}},"created_at":"2026-07-22T14:23:26.879127+00:00","updated_at":"2026-07-22T14:23:26.879127+00:00"}