{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:7PWTOYZPWW23ZXW47YTYDJIH6C","short_pith_number":"pith:7PWTOYZP","schema_version":"1.0","canonical_sha256":"fbed37632fb5b5bcdedcfe2781a507f09bf64109d9afbe2a58d9136fbbbc1f33","source":{"kind":"arxiv","id":"1404.1933","version":2},"attestation_state":"computed","paper":{"title":"Cross-correlation of cosmic far-infrared background anisotropies with large scale structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Anthony Pullen, Guilaine Lagache, Martin White, Olivier Dor\\'e, Paolo Serra","submitted_at":"2014-04-07T20:03:57Z","abstract_excerpt":"We measure the cross-power spectra between luminous red galaxies (LRGs) from the Sloan Digital Sky Survey (SDSS)-III Data Release Eight (DR8) and cosmic infrared background (CIB) anisotropies from Planck and data from the Improved Reprocessing (IRIS) of the Infrared Astronomical Satellite (IRAS) at 353, 545, 857, and 3000 GHz, corresponding to 850, 550, 350 and 100 micron, respectively, in the multipole range 100<l<1000. Using approximately 6.5 10^5 photometrically determined LRGs in 7760 deg^2 of the northern hemisphere in the redshift range 0.45 < z < 0.65, we model the far-infrared backgrou"},"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":"1404.1933","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-04-07T20:03:57Z","cross_cats_sorted":[],"title_canon_sha256":"5fe93b861701cb70ee344da2d4bba600687f12f6223dd4d36e8d625d2b397f53","abstract_canon_sha256":"67491ee3937ec4c816dac3d5515660f04a9763d0fbb2cb7fd31522f9c418d688"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:38:44.262048Z","signature_b64":"apaZClWBxiJzJMAPUYhngNzEKnSe5engg2ojjAbOoaSHrd98wFhdjQIw+4ny6/GxGhLvkgSL/3X5//dPAV9iCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fbed37632fb5b5bcdedcfe2781a507f09bf64109d9afbe2a58d9136fbbbc1f33","last_reissued_at":"2026-05-18T02:38:44.261649Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:38:44.261649Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cross-correlation of cosmic far-infrared background anisotropies with large scale structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Anthony Pullen, Guilaine Lagache, Martin White, Olivier Dor\\'e, Paolo Serra","submitted_at":"2014-04-07T20:03:57Z","abstract_excerpt":"We measure the cross-power spectra between luminous red galaxies (LRGs) from the Sloan Digital Sky Survey (SDSS)-III Data Release Eight (DR8) and cosmic infrared background (CIB) anisotropies from Planck and data from the Improved Reprocessing (IRIS) of the Infrared Astronomical Satellite (IRAS) at 353, 545, 857, and 3000 GHz, corresponding to 850, 550, 350 and 100 micron, respectively, in the multipole range 100<l<1000. Using approximately 6.5 10^5 photometrically determined LRGs in 7760 deg^2 of the northern hemisphere in the redshift range 0.45 < z < 0.65, we model the far-infrared backgrou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1933","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":"1404.1933","created_at":"2026-05-18T02:38:44.261706+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.1933v2","created_at":"2026-05-18T02:38:44.261706+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1933","created_at":"2026-05-18T02:38:44.261706+00:00"},{"alias_kind":"pith_short_12","alias_value":"7PWTOYZPWW23","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_16","alias_value":"7PWTOYZPWW23ZXW4","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_8","alias_value":"7PWTOYZP","created_at":"2026-05-18T12:28:19.803747+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/7PWTOYZPWW23ZXW47YTYDJIH6C","json":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C.json","graph_json":"https://pith.science/api/pith-number/7PWTOYZPWW23ZXW47YTYDJIH6C/graph.json","events_json":"https://pith.science/api/pith-number/7PWTOYZPWW23ZXW47YTYDJIH6C/events.json","paper":"https://pith.science/paper/7PWTOYZP"},"agent_actions":{"view_html":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C","download_json":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C.json","view_paper":"https://pith.science/paper/7PWTOYZP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.1933&json=true","fetch_graph":"https://pith.science/api/pith-number/7PWTOYZPWW23ZXW47YTYDJIH6C/graph.json","fetch_events":"https://pith.science/api/pith-number/7PWTOYZPWW23ZXW47YTYDJIH6C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/action/storage_attestation","attest_author":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/action/author_attestation","sign_citation":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/action/citation_signature","submit_replication":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/action/replication_record"}},"created_at":"2026-05-18T02:38:44.261706+00:00","updated_at":"2026-05-18T02:38:44.261706+00:00"}