{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:7PWTOYZPWW23ZXW47YTYDJIH6C","short_pith_number":"pith:7PWTOYZP","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"},"canonical_sha256":"fbed37632fb5b5bcdedcfe2781a507f09bf64109d9afbe2a58d9136fbbbc1f33","source":{"kind":"arxiv","id":"1404.1933","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1404.1933","created_at":"2026-05-18T02:38:44Z"},{"alias_kind":"arxiv_version","alias_value":"1404.1933v2","created_at":"2026-05-18T02:38:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1933","created_at":"2026-05-18T02:38:44Z"},{"alias_kind":"pith_short_12","alias_value":"7PWTOYZPWW23","created_at":"2026-05-18T12:28:19Z"},{"alias_kind":"pith_short_16","alias_value":"7PWTOYZPWW23ZXW4","created_at":"2026-05-18T12:28:19Z"},{"alias_kind":"pith_short_8","alias_value":"7PWTOYZP","created_at":"2026-05-18T12:28:19Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:7PWTOYZPWW23ZXW47YTYDJIH6C","target":"record","payload":{"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"},"canonical_sha256":"fbed37632fb5b5bcdedcfe2781a507f09bf64109d9afbe2a58d9136fbbbc1f33","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"},"source_kind":"arxiv","source_id":"1404.1933","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:38:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Ft9OvCKG0zaaHF/EVJuX4DFawHApdxmRw3tVvGmDUvougtUD7UW9APp39AQrB67HZWzETLFcp2KoOpM+OBBJBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T17:36:59.660847Z"},"content_sha256":"7c690e510d1c3f891fad506917251c0fce1270e6fddd5529324be9a9bbee4079","schema_version":"1.0","event_id":"sha256:7c690e510d1c3f891fad506917251c0fce1270e6fddd5529324be9a9bbee4079"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:7PWTOYZPWW23ZXW47YTYDJIH6C","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:38:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"t3JrhshUo3swMMOENlhwpr8Dr7arVRrBmBS/EnfO/7A6yPkaBUNoQfxws5JUdkzCmbdtB+zyA9IIvuPX7EOJCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T17:36:59.661487Z"},"content_sha256":"3b5d09da82f083d465eef12622adff0481aa2bfc484faed11fdba22185c9525e","schema_version":"1.0","event_id":"sha256:3b5d09da82f083d465eef12622adff0481aa2bfc484faed11fdba22185c9525e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/bundle.json","state_url":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-28T17:36:59Z","links":{"resolver":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C","bundle":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/bundle.json","state":"https://pith.science/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/state.json","well_known_bundle":"https://pith.science/.well-known/pith/7PWTOYZPWW23ZXW47YTYDJIH6C/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:7PWTOYZPWW23ZXW47YTYDJIH6C","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"67491ee3937ec4c816dac3d5515660f04a9763d0fbb2cb7fd31522f9c418d688","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-04-07T20:03:57Z","title_canon_sha256":"5fe93b861701cb70ee344da2d4bba600687f12f6223dd4d36e8d625d2b397f53"},"schema_version":"1.0","source":{"id":"1404.1933","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1404.1933","created_at":"2026-05-18T02:38:44Z"},{"alias_kind":"arxiv_version","alias_value":"1404.1933v2","created_at":"2026-05-18T02:38:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1933","created_at":"2026-05-18T02:38:44Z"},{"alias_kind":"pith_short_12","alias_value":"7PWTOYZPWW23","created_at":"2026-05-18T12:28:19Z"},{"alias_kind":"pith_short_16","alias_value":"7PWTOYZPWW23ZXW4","created_at":"2026-05-18T12:28:19Z"},{"alias_kind":"pith_short_8","alias_value":"7PWTOYZP","created_at":"2026-05-18T12:28:19Z"}],"graph_snapshots":[{"event_id":"sha256:3b5d09da82f083d465eef12622adff0481aa2bfc484faed11fdba22185c9525e","target":"graph","created_at":"2026-05-18T02:38:44Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"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","authors_text":"Anthony Pullen, Guilaine Lagache, Martin White, Olivier Dor\\'e, Paolo Serra","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-04-07T20:03:57Z","title":"Cross-correlation of cosmic far-infrared background anisotropies with large scale structures"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1933","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:7c690e510d1c3f891fad506917251c0fce1270e6fddd5529324be9a9bbee4079","target":"record","created_at":"2026-05-18T02:38:44Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"67491ee3937ec4c816dac3d5515660f04a9763d0fbb2cb7fd31522f9c418d688","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-04-07T20:03:57Z","title_canon_sha256":"5fe93b861701cb70ee344da2d4bba600687f12f6223dd4d36e8d625d2b397f53"},"schema_version":"1.0","source":{"id":"1404.1933","kind":"arxiv","version":2}},"canonical_sha256":"fbed37632fb5b5bcdedcfe2781a507f09bf64109d9afbe2a58d9136fbbbc1f33","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"fbed37632fb5b5bcdedcfe2781a507f09bf64109d9afbe2a58d9136fbbbc1f33","first_computed_at":"2026-05-18T02:38:44.261649Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:38:44.261649Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"apaZClWBxiJzJMAPUYhngNzEKnSe5engg2ojjAbOoaSHrd98wFhdjQIw+4ny6/GxGhLvkgSL/3X5//dPAV9iCw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:38:44.262048Z","signed_message":"canonical_sha256_bytes"},"source_id":"1404.1933","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:7c690e510d1c3f891fad506917251c0fce1270e6fddd5529324be9a9bbee4079","sha256:3b5d09da82f083d465eef12622adff0481aa2bfc484faed11fdba22185c9525e"],"state_sha256":"7444502b1b46ad4da0c643202c1f4e4a078c8873a58186afcec26772a0fcdb4a"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"06BcM8gv3CB9mdEHXHrjlDqnnYFdiSpjZMl4s1yHuHCnR+FRggIN2yN9ROrZtgjO4HXyxYk53E+a79G+czrdCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T17:36:59.664512Z","bundle_sha256":"1d7d7fe4d041fb94b0e94d0cd8e82aeeb0309a7e26dff2c62d51116e03f87add"}}