{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:KI2ATX2YSUOSZ2WELWKUJ2U6KV","short_pith_number":"pith:KI2ATX2Y","schema_version":"1.0","canonical_sha256":"523409df58951d2ceac45d9544ea9e55426820392a6a2c391991a4a11b19a3c8","source":{"kind":"arxiv","id":"2007.08534","version":2},"attestation_state":"computed","paper":{"title":"Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andrea Lapi, Giulio Scelfo, Lumen Boco, Matteo Viel","submitted_at":"2020-07-16T18:00:03Z","abstract_excerpt":"Gravitational waves astronomy has opened a new opportunity to study the Universe. Full exploitation of this window can especially be provided by combining data coming from gravitational waves experiments with luminous tracers of the Large Scale Structure, like galaxies. In this work we investigate the cross-correlation signal between gravitational waves resolved events, as detected by the Einstein Telescope, and actively star-forming galaxies. The galaxies distribution is computed through their UV and IR luminosity functions and the gravitational waves events, assumed to be of stellar origin, "},"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":"2007.08534","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2020-07-16T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"f5bb40ccc3a71f24bfc1c8b22dcf85043be5521a995e180ddd41a81e16b91ffc","abstract_canon_sha256":"1ba9e2a63c6dde2e1de1db55869b3877811b5aba20b26aeabc97de8a1e07b8c1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:44:15.462381Z","signature_b64":"zpU95n6Xgej5Vz6CREgMVTKBF3qLr0J8Zv1WKvQzvRTLsvWk4kLNOaEh2cibAo0S9+eeCmbK0BqjZvF/JnSZDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"523409df58951d2ceac45d9544ea9e55426820392a6a2c391991a4a11b19a3c8","last_reissued_at":"2026-07-05T01:44:15.461940Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:44:15.461940Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andrea Lapi, Giulio Scelfo, Lumen Boco, Matteo Viel","submitted_at":"2020-07-16T18:00:03Z","abstract_excerpt":"Gravitational waves astronomy has opened a new opportunity to study the Universe. Full exploitation of this window can especially be provided by combining data coming from gravitational waves experiments with luminous tracers of the Large Scale Structure, like galaxies. In this work we investigate the cross-correlation signal between gravitational waves resolved events, as detected by the Einstein Telescope, and actively star-forming galaxies. The galaxies distribution is computed through their UV and IR luminosity functions and the gravitational waves events, assumed to be of stellar origin, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.08534","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2007.08534/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2007.08534","created_at":"2026-07-05T01:44:15.461992+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.08534v2","created_at":"2026-07-05T01:44:15.461992+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.08534","created_at":"2026-07-05T01:44:15.461992+00:00"},{"alias_kind":"pith_short_12","alias_value":"KI2ATX2YSUOS","created_at":"2026-07-05T01:44:15.461992+00:00"},{"alias_kind":"pith_short_16","alias_value":"KI2ATX2YSUOSZ2WE","created_at":"2026-07-05T01:44:15.461992+00:00"},{"alias_kind":"pith_short_8","alias_value":"KI2ATX2Y","created_at":"2026-07-05T01:44:15.461992+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2506.10469","citing_title":"Constraining the lensing dispersion from the angular clustering of binary black hole mergers","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2510.21521","citing_title":"Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies","ref_index":128,"is_internal_anchor":false},{"citing_arxiv_id":"2203.06142","citing_title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV","json":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV.json","graph_json":"https://pith.science/api/pith-number/KI2ATX2YSUOSZ2WELWKUJ2U6KV/graph.json","events_json":"https://pith.science/api/pith-number/KI2ATX2YSUOSZ2WELWKUJ2U6KV/events.json","paper":"https://pith.science/paper/KI2ATX2Y"},"agent_actions":{"view_html":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV","download_json":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV.json","view_paper":"https://pith.science/paper/KI2ATX2Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.08534&json=true","fetch_graph":"https://pith.science/api/pith-number/KI2ATX2YSUOSZ2WELWKUJ2U6KV/graph.json","fetch_events":"https://pith.science/api/pith-number/KI2ATX2YSUOSZ2WELWKUJ2U6KV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV/action/storage_attestation","attest_author":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV/action/author_attestation","sign_citation":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV/action/citation_signature","submit_replication":"https://pith.science/pith/KI2ATX2YSUOSZ2WELWKUJ2U6KV/action/replication_record"}},"created_at":"2026-07-05T01:44:15.461992+00:00","updated_at":"2026-07-05T01:44:15.461992+00:00"}