{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:TAC2ASSLXDBJEOPBJ5BTIUSKZI","short_pith_number":"pith:TAC2ASSL","schema_version":"1.0","canonical_sha256":"9805a04a4bb8c29239e14f4334524aca34dcf861224c55c38d9587d01b8e7243","source":{"kind":"arxiv","id":"1409.6869","version":2},"attestation_state":"computed","paper":{"title":"CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Kavilan Moodley, Simon Muya Kasanda","submitted_at":"2014-09-24T09:25:33Z","abstract_excerpt":"We forecast how current ({\\planck}) and future ({\\prism}) cosmic microwave background (CMB) experiments constrain the adiabatic mode and its admixtures with primordial isocurvature modes, using measurements of the reconstructed CMB lensing potential and lensing-induced CMB B-mode polarization anisotropies in combination with the CMB temperature and E-mode polarization anisotropies. We first study the characteristic features of the CMB temperature, polarization and lensing spectra for adiabatic and isocurvature modes. We then consider how lensing-induced B-mode polarization and lensing potentia"},"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":"1409.6869","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-09-24T09:25:33Z","cross_cats_sorted":[],"title_canon_sha256":"264ff776fcf7a1c4e7de1189d848585d827694c6bf65aaaf66533a9bceec2cc0","abstract_canon_sha256":"fe2885e86a2eea013ae5411de70543d5bc497198c4815876936b284d561c856a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:57.290426Z","signature_b64":"MMOljIH4f0YAYmE/LNU4NUqqOTKa2aGlriUmmIcRjaHIQd7kMTwz38l84v2gtIWZwHlKzzkEm/k40Ett6IWdCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9805a04a4bb8c29239e14f4334524aca34dcf861224c55c38d9587d01b8e7243","last_reissued_at":"2026-05-18T01:41:57.289831Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:57.289831Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Kavilan Moodley, Simon Muya Kasanda","submitted_at":"2014-09-24T09:25:33Z","abstract_excerpt":"We forecast how current ({\\planck}) and future ({\\prism}) cosmic microwave background (CMB) experiments constrain the adiabatic mode and its admixtures with primordial isocurvature modes, using measurements of the reconstructed CMB lensing potential and lensing-induced CMB B-mode polarization anisotropies in combination with the CMB temperature and E-mode polarization anisotropies. We first study the characteristic features of the CMB temperature, polarization and lensing spectra for adiabatic and isocurvature modes. We then consider how lensing-induced B-mode polarization and lensing potentia"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.6869","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":"1409.6869","created_at":"2026-05-18T01:41:57.289932+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.6869v2","created_at":"2026-05-18T01:41:57.289932+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.6869","created_at":"2026-05-18T01:41:57.289932+00:00"},{"alias_kind":"pith_short_12","alias_value":"TAC2ASSLXDBJ","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"TAC2ASSLXDBJEOPB","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"TAC2ASSL","created_at":"2026-05-18T12:28:49.207871+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/TAC2ASSLXDBJEOPBJ5BTIUSKZI","json":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI.json","graph_json":"https://pith.science/api/pith-number/TAC2ASSLXDBJEOPBJ5BTIUSKZI/graph.json","events_json":"https://pith.science/api/pith-number/TAC2ASSLXDBJEOPBJ5BTIUSKZI/events.json","paper":"https://pith.science/paper/TAC2ASSL"},"agent_actions":{"view_html":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI","download_json":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI.json","view_paper":"https://pith.science/paper/TAC2ASSL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.6869&json=true","fetch_graph":"https://pith.science/api/pith-number/TAC2ASSLXDBJEOPBJ5BTIUSKZI/graph.json","fetch_events":"https://pith.science/api/pith-number/TAC2ASSLXDBJEOPBJ5BTIUSKZI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI/action/storage_attestation","attest_author":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI/action/author_attestation","sign_citation":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI/action/citation_signature","submit_replication":"https://pith.science/pith/TAC2ASSLXDBJEOPBJ5BTIUSKZI/action/replication_record"}},"created_at":"2026-05-18T01:41:57.289932+00:00","updated_at":"2026-05-18T01:41:57.289932+00:00"}