{"paper":{"title":"KiDS-450: Tomographic Cross-Correlation of Galaxy Shear with {\\it Planck} Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ami Choi, Catherine Heymans, Hendrik Hildebrandt, Henk Hoekstra, Joachim Harnois-D\\'eraps, Julian Merten, Konrad Kuijken, Lance Miller, Ludovic Van Waerbeke, Maciej Bilicki, Marika Asgari, Massimo Viola, Naomi Robertson, Nora Elisa Chisari, Peter Schneider, Shahab Joudaki, Tilman Tr\\\"oster","submitted_at":"2017-03-09T18:34:32Z","abstract_excerpt":"We present the tomographic cross-correlation between galaxy lensing measured in the Kilo Degree Survey (KiDS-450) with overlapping lensing measurements of the cosmic microwave background (CMB), as detected by Planck 2015. We compare our joint probe measurement to the theoretical expectation for a flat $\\Lambda$CDM cosmology, assuming the best-fitting cosmological parameters from the KiDS-450 cosmic shear and Planck CMB analyses. We find that our results are consistent within $1\\sigma$ with the KiDS-450 cosmology, with an amplitude re-scaling parameter $A_{\\rm KiDS} = 0.86 \\pm 0.19$. Adopting a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.03383","kind":"arxiv","version":1},"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"}