{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:3KCFTNOFNLATNUQJW7GGWZ2D7Y","short_pith_number":"pith:3KCFTNOF","schema_version":"1.0","canonical_sha256":"da8459b5c56ac136d209b7cc6b6743fe3b59c70a586ff691f39f1cbbcd1931d0","source":{"kind":"arxiv","id":"1307.1712","version":2},"attestation_state":"computed","paper":{"title":"The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Instituto de Fisica de Cantabria, (3) Leibniz-Institute for Astrophysics, (4) Universidad Aut\\'onoma de Madrid, (5) University of Helsinki, (6) Universitat Bielefeld), A. Knebe (4), A. Marcos-Caballero (2), E. Mart\\'inez-Gonz\\'alez (2), G. Yepes (4), I. T. Iliev (1), J. Gonz\\'alez-Nuevo (2), J. M. Diego (2), P. Vielva (2). ((1) University of Sussex, R. B. Barreiro (2), S. Gottl\\\"ober (3), S. Hotchkiss (5), S. Nadathur (6), W. A. Watson (1)","submitted_at":"2013-07-05T20:20:53Z","abstract_excerpt":"We present initial results from the Jubilee ISW project, which models the expected \\LambdaCDM Integrated Sachs-Wolfe (ISW) effect in the Jubilee simulation. The simulation volume is (6 Gpc/h)^3, allowing power on very large-scales to be incorporated into the calculation. Haloes are resolved down to a mass of 1.5x10^12 M_sun/h, which allows us to derive a catalogue of mock Luminous Red Galaxies (LRGs) for cross-correlation analysis with the ISW signal. We find the ISW effect observed on a projected sky to grow stronger at late times with the evolution of the ISW power spectrum matching expectat"},"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":"1307.1712","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-07-05T20:20:53Z","cross_cats_sorted":[],"title_canon_sha256":"6dfe32121d434ce9fdca70b76844d6a1b75826e0fb1c78c5922df3a84f46dcef","abstract_canon_sha256":"2fd834f16232de53afd647ae19eb8dc6002a9d502d3e57fdaaeb4ffa477fac5e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:53:15.175435Z","signature_b64":"ZdllbEhUOyQyEQYZQOU8sjlG5QJgpxYxpD0aWpfzUIp792gqwf/cZOEjMJv+Re0G6Pm51btdDZpCFPckjw4vBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"da8459b5c56ac136d209b7cc6b6743fe3b59c70a586ff691f39f1cbbcd1931d0","last_reissued_at":"2026-05-18T02:53:15.174779Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:53:15.174779Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Instituto de Fisica de Cantabria, (3) Leibniz-Institute for Astrophysics, (4) Universidad Aut\\'onoma de Madrid, (5) University of Helsinki, (6) Universitat Bielefeld), A. Knebe (4), A. Marcos-Caballero (2), E. Mart\\'inez-Gonz\\'alez (2), G. Yepes (4), I. T. Iliev (1), J. Gonz\\'alez-Nuevo (2), J. M. Diego (2), P. Vielva (2). ((1) University of Sussex, R. B. Barreiro (2), S. Gottl\\\"ober (3), S. Hotchkiss (5), S. Nadathur (6), W. A. Watson (1)","submitted_at":"2013-07-05T20:20:53Z","abstract_excerpt":"We present initial results from the Jubilee ISW project, which models the expected \\LambdaCDM Integrated Sachs-Wolfe (ISW) effect in the Jubilee simulation. The simulation volume is (6 Gpc/h)^3, allowing power on very large-scales to be incorporated into the calculation. Haloes are resolved down to a mass of 1.5x10^12 M_sun/h, which allows us to derive a catalogue of mock Luminous Red Galaxies (LRGs) for cross-correlation analysis with the ISW signal. We find the ISW effect observed on a projected sky to grow stronger at late times with the evolution of the ISW power spectrum matching expectat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.1712","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":"1307.1712","created_at":"2026-05-18T02:53:15.174883+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.1712v2","created_at":"2026-05-18T02:53:15.174883+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.1712","created_at":"2026-05-18T02:53:15.174883+00:00"},{"alias_kind":"pith_short_12","alias_value":"3KCFTNOFNLAT","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"3KCFTNOFNLATNUQJ","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"3KCFTNOF","created_at":"2026-05-18T12:27:32.513160+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/3KCFTNOFNLATNUQJW7GGWZ2D7Y","json":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y.json","graph_json":"https://pith.science/api/pith-number/3KCFTNOFNLATNUQJW7GGWZ2D7Y/graph.json","events_json":"https://pith.science/api/pith-number/3KCFTNOFNLATNUQJW7GGWZ2D7Y/events.json","paper":"https://pith.science/paper/3KCFTNOF"},"agent_actions":{"view_html":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y","download_json":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y.json","view_paper":"https://pith.science/paper/3KCFTNOF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.1712&json=true","fetch_graph":"https://pith.science/api/pith-number/3KCFTNOFNLATNUQJW7GGWZ2D7Y/graph.json","fetch_events":"https://pith.science/api/pith-number/3KCFTNOFNLATNUQJW7GGWZ2D7Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y/action/storage_attestation","attest_author":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y/action/author_attestation","sign_citation":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y/action/citation_signature","submit_replication":"https://pith.science/pith/3KCFTNOFNLATNUQJW7GGWZ2D7Y/action/replication_record"}},"created_at":"2026-05-18T02:53:15.174883+00:00","updated_at":"2026-05-18T02:53:15.174883+00:00"}