{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:CIBCNTEWDQ4LP6DI3WKAZM2BJN","short_pith_number":"pith:CIBCNTEW","schema_version":"1.0","canonical_sha256":"120226cc961c38b7f868dd940cb3414b5505e200614197ecb87344c8934628f4","source":{"kind":"arxiv","id":"1105.3628","version":2},"attestation_state":"computed","paper":{"title":"Non-Gaussian Halo Bias Re-examined: Mass-dependent Amplitude from the Peak-Background Split and Thresholding","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Donghui Jeong, Fabian Schmidt, Vincent Desjacques","submitted_at":"2011-05-18T13:44:12Z","abstract_excerpt":"Recent results of N-body simulations have shown that current theoretical models are not able to correctly predict the amplitude of the scale-dependent halo bias induced by primordial non-Gaussianity, for models going beyond the simplest, local quadratic case. Motivated by these discrepancies, we carefully examine three theoretical approaches based on (1) the statistics of thresholded regions, (2) a peak-background split method based on separation of scales, and (3) a peak-background split method using the conditional mass function. We first demonstrate that the statistics of thresholded region"},"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":"1105.3628","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-05-18T13:44:12Z","cross_cats_sorted":[],"title_canon_sha256":"fbd62da86d413d38c233ba146bc6f14d8988dc05f32361293b2ba01826544a4b","abstract_canon_sha256":"8f18e2a52024e4f698c44e919c90b36b7533a8b08966095920305ce22022bd86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:23:34.008455Z","signature_b64":"aItngMnbR8XXwz6c20gew5kjBMiEZR7APZM4PDvoBfDU1+0xlekMoCryXOYdh2Cj21KoHhFwgfaso6RgtI/7BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"120226cc961c38b7f868dd940cb3414b5505e200614197ecb87344c8934628f4","last_reissued_at":"2026-05-18T03:23:34.007768Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:23:34.007768Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-Gaussian Halo Bias Re-examined: Mass-dependent Amplitude from the Peak-Background Split and Thresholding","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Donghui Jeong, Fabian Schmidt, Vincent Desjacques","submitted_at":"2011-05-18T13:44:12Z","abstract_excerpt":"Recent results of N-body simulations have shown that current theoretical models are not able to correctly predict the amplitude of the scale-dependent halo bias induced by primordial non-Gaussianity, for models going beyond the simplest, local quadratic case. Motivated by these discrepancies, we carefully examine three theoretical approaches based on (1) the statistics of thresholded regions, (2) a peak-background split method based on separation of scales, and (3) a peak-background split method using the conditional mass function. We first demonstrate that the statistics of thresholded region"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.3628","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":"1105.3628","created_at":"2026-05-18T03:23:34.007892+00:00"},{"alias_kind":"arxiv_version","alias_value":"1105.3628v2","created_at":"2026-05-18T03:23:34.007892+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1105.3628","created_at":"2026-05-18T03:23:34.007892+00:00"},{"alias_kind":"pith_short_12","alias_value":"CIBCNTEWDQ4L","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"CIBCNTEWDQ4LP6DI","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"CIBCNTEW","created_at":"2026-05-18T12:26:26.731475+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.02882","citing_title":"Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias","ref_index":46,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN","json":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN.json","graph_json":"https://pith.science/api/pith-number/CIBCNTEWDQ4LP6DI3WKAZM2BJN/graph.json","events_json":"https://pith.science/api/pith-number/CIBCNTEWDQ4LP6DI3WKAZM2BJN/events.json","paper":"https://pith.science/paper/CIBCNTEW"},"agent_actions":{"view_html":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN","download_json":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN.json","view_paper":"https://pith.science/paper/CIBCNTEW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1105.3628&json=true","fetch_graph":"https://pith.science/api/pith-number/CIBCNTEWDQ4LP6DI3WKAZM2BJN/graph.json","fetch_events":"https://pith.science/api/pith-number/CIBCNTEWDQ4LP6DI3WKAZM2BJN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN/action/storage_attestation","attest_author":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN/action/author_attestation","sign_citation":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN/action/citation_signature","submit_replication":"https://pith.science/pith/CIBCNTEWDQ4LP6DI3WKAZM2BJN/action/replication_record"}},"created_at":"2026-05-18T03:23:34.007892+00:00","updated_at":"2026-05-18T03:23:34.007892+00:00"}