{"paper":{"title":"Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas, A. A. Stark, A. Carnero Rosell, A. E. Evrard, A. Gilbert, A. G. Kim, A. J. Anderson, A. Kovacs, A. K. Romer, A. Nadolski, A. N. Bender, A. T. Crites, A. T. Lee, B. A. Benson, B. Flaugher, B. Hoyle, B. R. Saliwanchik, C. Davis, C. E. Cunha, C. J. Miller, C. L. Chang, C. L. Reichardt, C. Pryke, C. Tucker, D. Brooks, D. Gruen, D. J. James, D. L. Burke, D. L. Hollowood, D. Rapetti, D. Thomas, E. Baxter, E. Bertin, E. Gaztanaga, E. M. George, E. Rozo, E. Sanchez, E. Suchyta, F. Bianchini, F. Menanteau, F. Sobreira, G. Bernstein, G. C. Hilton, G. Gutierrez, G. P. Holder, G. Smecher, G. Tarle, G. Wang, H. C. Chiang, H-M. Cho, H. T. Diehl, I. Sevilla-Noarbe, J. A. Beall, J. Annis, J. Carretero, J. De Vicente, J. D. Hrubes, J. D. Vieira, J. E. Austermann, J. E. Carlstrom, J. E. Ruhl, J. Frieman, J. Gallicchio, J. Garc\\'ia-Bellido, J. Gschwend, J. Hubmayr, J. J. McMahon, J. L. Marshall, J. Montgomery, J. P. Dietrich, J. P. Nibarger, J.T. Sayre, J. W. Henning, K. Bechtol, K. D. Irwin, K. Honscheid, K. K. Schaffer, K. Kuehn, K. T. Story, K. Vanderlinde, L. Bleem, L. E. Bleem, L. Knox, L. Mocanu, L. N. da Costa, M. A. Dobbs, M. A. G. Maia, M. Carrasco Kind, M. E. C. Swanson, M. Lima, M. Schubnell, M. Soares-Santos, N. Gupta, N. Harrington, N. Huang, N. Kuropatkin, N. W. Halverson, N. Whitehorn, P. A. R. Ade, P. Doel, P. Fosalba, P. Melchior, R. A. Gruendl, R. Citron, R. C. Smith, R. Miquel, S. Allam, S. Avila, S. Desai, S. Padin, S. Patil, S. Raghunathan, S. Serrano, S. S. Meyer, T. de Haan, T. F. Eifler, T. Jeltema, T. L. Chou, T. M. C. Abbott, T. McClintock, T. M. Crawford, T. Natoli, T. N. Varga, T. S. Li, V. Novosad, V. Scarpine, W. Everett, W. G. Hartley, W. L. Holzapfel, W. L. K. Wu, Y. Zhang, Z. Hou","submitted_at":"2018-10-25T17:43:15Z","abstract_excerpt":"We use cosmic microwave background (CMB) temperature maps from the 500 deg$^{2}$ SPTpol survey to measure the stacked lensing convergence of galaxy clusters from the Dark Energy Survey (DES) Year-3 redMaPPer (RM) cluster catalog. The lensing signal is extracted through a modified quadratic estimator designed to be unbiased by the thermal Sunyaev-Zel{'}dovich (tSZ) effect. The modified estimator uses a tSZ-free map, constructed from the SPTpol 95 and 150 GHz datasets, to estimate the background CMB gradient. For lensing reconstruction, we employ two versions of the RM catalog: a flux-limited sa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.10998","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"}