{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:2P56SGHDO4XFDIEUKME6PT2PN2","short_pith_number":"pith:2P56SGHD","schema_version":"1.0","canonical_sha256":"d3fbe918e3772e51a0945309e7cf4f6e951c0f3e39e4cb71eab3eb6f447564a4","source":{"kind":"arxiv","id":"1405.7029","version":2},"attestation_state":"computed","paper":{"title":"The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Curto, E. Martinez-Gonzalez, M. Kunz, M. Tucci","submitted_at":"2014-05-27T19:47:57Z","abstract_excerpt":"We characterize the Cosmic Infrared Background (CIB)-lensing bispectrum which is one of the contributions to the three-point functions of Cosmic Microwave Background (CMB) maps in harmonic space. We show that the CIB-lensing bispectrum has a considerable strength and that it can be detected with high significance in the Planck high-frequency maps. We also present forecasts of the contamination on different shapes of the primordial non-Gaussianity $f_{nl}$ parameter produced by the CIB-lensing bispectrum and by the extragalactic point sources bispectrum in the Planck high-resolution CMB anisotr"},"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":"1405.7029","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-05-27T19:47:57Z","cross_cats_sorted":[],"title_canon_sha256":"a6863205dd20c4e420f24d4d625e5c124d02c9977bc8bb705279cc7a3b01ca8e","abstract_canon_sha256":"e86283b3f3b19da08300ce5a8d99d8023d1cb262d375dd582e8b0de429e9233b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:37.714900Z","signature_b64":"WrFtqpIYUWA2UBrxPmju13MXvwHfWZYx7bsZMsWNcK/3PnT8HnLpZ9KH5/MfJi0cooj5iKmBGLdtsLoDhwPgAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3fbe918e3772e51a0945309e7cf4f6e951c0f3e39e4cb71eab3eb6f447564a4","last_reissued_at":"2026-05-18T02:03:37.714139Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:37.714139Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Curto, E. Martinez-Gonzalez, M. Kunz, M. Tucci","submitted_at":"2014-05-27T19:47:57Z","abstract_excerpt":"We characterize the Cosmic Infrared Background (CIB)-lensing bispectrum which is one of the contributions to the three-point functions of Cosmic Microwave Background (CMB) maps in harmonic space. We show that the CIB-lensing bispectrum has a considerable strength and that it can be detected with high significance in the Planck high-frequency maps. We also present forecasts of the contamination on different shapes of the primordial non-Gaussianity $f_{nl}$ parameter produced by the CIB-lensing bispectrum and by the extragalactic point sources bispectrum in the Planck high-resolution CMB anisotr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.7029","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":"1405.7029","created_at":"2026-05-18T02:03:37.714270+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.7029v2","created_at":"2026-05-18T02:03:37.714270+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.7029","created_at":"2026-05-18T02:03:37.714270+00:00"},{"alias_kind":"pith_short_12","alias_value":"2P56SGHDO4XF","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_16","alias_value":"2P56SGHDO4XFDIEU","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_8","alias_value":"2P56SGHD","created_at":"2026-05-18T12:28:11.866339+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2","json":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2.json","graph_json":"https://pith.science/api/pith-number/2P56SGHDO4XFDIEUKME6PT2PN2/graph.json","events_json":"https://pith.science/api/pith-number/2P56SGHDO4XFDIEUKME6PT2PN2/events.json","paper":"https://pith.science/paper/2P56SGHD"},"agent_actions":{"view_html":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2","download_json":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2.json","view_paper":"https://pith.science/paper/2P56SGHD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.7029&json=true","fetch_graph":"https://pith.science/api/pith-number/2P56SGHDO4XFDIEUKME6PT2PN2/graph.json","fetch_events":"https://pith.science/api/pith-number/2P56SGHDO4XFDIEUKME6PT2PN2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2/action/storage_attestation","attest_author":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2/action/author_attestation","sign_citation":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2/action/citation_signature","submit_replication":"https://pith.science/pith/2P56SGHDO4XFDIEUKME6PT2PN2/action/replication_record"}},"created_at":"2026-05-18T02:03:37.714270+00:00","updated_at":"2026-05-18T02:03:37.714270+00:00"}