{"paper":{"title":"Spurious Shear in Weak Lensing with LSST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Connolly, A. Meert, A. P. Rasmussen, C. Chang, D. Bard, E. Grace, E. Peng, J. Bankert, J. G. Jernigan, J. R. Peterson, K. Gilmore, L. Jones, M. A. Hodge, M. Hannel, M. J. Jee, M. Shmakova, M. Young, N. Sylvestre, N. Todd, P. J. Marshall, R. R. Gibson, S. Krughoff, S. Lorenz, S. Marshall, S. M. Kahn, S. Nagarajan, Y. Alsayyad, Z. Ahmad","submitted_at":"2012-06-07T01:06:44Z","abstract_excerpt":"The complete 10-year survey from the Large Synoptic Survey Telescope (LSST) will image $\\sim$ 20,000 square degrees of sky in six filter bands every few nights, bringing the final survey depth to $r\\sim27.5$, with over 4 billion well measured galaxies. To take full advantage of this unprecedented statistical power, the systematic errors associated with weak lensing measurements need to be controlled to a level similar to the statistical errors.\n  This work is the first attempt to quantitatively estimate the absolute level and statistical properties of the systematic errors on weak lensing shea"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.1378","kind":"arxiv","version":4},"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"}