{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:MTZMRKZBHGSIGD5S6I6JCIJBDY","short_pith_number":"pith:MTZMRKZB","schema_version":"1.0","canonical_sha256":"64f2c8ab2139a4830fb2f23c9121211e3e82a3c0e952140d06c9679e61da156b","source":{"kind":"arxiv","id":"1707.06627","version":2},"attestation_state":"computed","paper":{"title":"KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alexander Mead, Alexandra Amon, Ami Choi, Andrew Johnson, Catherine Heymans, Chris Blake, Chris Lidman, Christian Wolf, David Parkinson, Dominik Klaes, Gregory B. Poole, Hendrik Hildebrandt, Henk Hoekstra, Joachim Harnois-Deraps, Karl Glazebrook, Konrad Kuijken, Lance Miller, Marika Asgari, Massimo Viola, Peter Schneider, Shahab Joudaki, Thomas Erben","submitted_at":"2017-07-20T17:37:23Z","abstract_excerpt":"We perform a combined analysis of cosmic shear tomography, galaxy-galaxy lensing tomography, and redshift-space multipole power spectra (monopole and quadrupole) using 450 deg$^2$ of imaging data by the Kilo Degree Survey (KiDS) overlapping with two spectroscopic surveys: the 2-degree Field Lensing Survey (2dFLenS) and the Baryon Oscillation Spectroscopic Survey (BOSS). We restrict the galaxy-galaxy lensing and multipole power spectrum measurements to the overlapping regions with KiDS, and self-consistently compute the full covariance between the different observables using a large suite of $N"},"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":"1707.06627","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-07-20T17:37:23Z","cross_cats_sorted":[],"title_canon_sha256":"cbd6a616ab36712ce927ca33c9f75e28ed2c76de382ef2f8c159b12a1a4be51a","abstract_canon_sha256":"15145c4c880a6ccce509a70eb51b141a9d65a47f438b23c5002c292ede0879ae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:31:02.629464Z","signature_b64":"35AW2UY7bxWpcbcylV//vwXr+Sq+CKaWAehwfzr/Doz3QtczrqhGoHL7YBg44K+b3riLFtpJPQqHaOMzW3q9Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"64f2c8ab2139a4830fb2f23c9121211e3e82a3c0e952140d06c9679e61da156b","last_reissued_at":"2026-05-18T00:31:02.628777Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:31:02.628777Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alexander Mead, Alexandra Amon, Ami Choi, Andrew Johnson, Catherine Heymans, Chris Blake, Chris Lidman, Christian Wolf, David Parkinson, Dominik Klaes, Gregory B. Poole, Hendrik Hildebrandt, Henk Hoekstra, Joachim Harnois-Deraps, Karl Glazebrook, Konrad Kuijken, Lance Miller, Marika Asgari, Massimo Viola, Peter Schneider, Shahab Joudaki, Thomas Erben","submitted_at":"2017-07-20T17:37:23Z","abstract_excerpt":"We perform a combined analysis of cosmic shear tomography, galaxy-galaxy lensing tomography, and redshift-space multipole power spectra (monopole and quadrupole) using 450 deg$^2$ of imaging data by the Kilo Degree Survey (KiDS) overlapping with two spectroscopic surveys: the 2-degree Field Lensing Survey (2dFLenS) and the Baryon Oscillation Spectroscopic Survey (BOSS). We restrict the galaxy-galaxy lensing and multipole power spectrum measurements to the overlapping regions with KiDS, and self-consistently compute the full covariance between the different observables using a large suite of $N"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.06627","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":"1707.06627","created_at":"2026-05-18T00:31:02.628877+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.06627v2","created_at":"2026-05-18T00:31:02.628877+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.06627","created_at":"2026-05-18T00:31:02.628877+00:00"},{"alias_kind":"pith_short_12","alias_value":"MTZMRKZBHGSI","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"MTZMRKZBHGSIGD5S","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"MTZMRKZB","created_at":"2026-05-18T12:31:31.346846+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"1907.04473","citing_title":"CMB-S4 Science Case, Reference Design, and Project Plan","ref_index":170,"is_internal_anchor":true},{"citing_arxiv_id":"2105.13549","citing_title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","ref_index":79,"is_internal_anchor":true},{"citing_arxiv_id":"2510.08339","citing_title":"Probing departures from $\\Lambda$CDM by late-time datasets","ref_index":26,"is_internal_anchor":true},{"citing_arxiv_id":"2602.11093","citing_title":"New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"1807.06209","citing_title":"Planck 2018 results. VI. Cosmological parameters","ref_index":194,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY","json":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY.json","graph_json":"https://pith.science/api/pith-number/MTZMRKZBHGSIGD5S6I6JCIJBDY/graph.json","events_json":"https://pith.science/api/pith-number/MTZMRKZBHGSIGD5S6I6JCIJBDY/events.json","paper":"https://pith.science/paper/MTZMRKZB"},"agent_actions":{"view_html":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY","download_json":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY.json","view_paper":"https://pith.science/paper/MTZMRKZB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.06627&json=true","fetch_graph":"https://pith.science/api/pith-number/MTZMRKZBHGSIGD5S6I6JCIJBDY/graph.json","fetch_events":"https://pith.science/api/pith-number/MTZMRKZBHGSIGD5S6I6JCIJBDY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY/action/storage_attestation","attest_author":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY/action/author_attestation","sign_citation":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY/action/citation_signature","submit_replication":"https://pith.science/pith/MTZMRKZBHGSIGD5S6I6JCIJBDY/action/replication_record"}},"created_at":"2026-05-18T00:31:02.628877+00:00","updated_at":"2026-05-18T00:31:02.628877+00:00"}