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1by Soergel, B., Flender, S., Story, K. T., Bleem, L., Giannantonio, T., Efstathiou, G., Rykoff, E., Benson, B. A., Crawford, T., Dodelson, S., Habib, S., Heitmann, K., Holder, G., Jain, B., Rozo, E., Saro, A., Weller, J., Abdalla, F. B., Allam, S., Annis, J., Armstrong, R., Benoit-Lévy, A., Bernstein, G. M., Carlstrom, J. E., Carnero Rosell, A., Carrasco Kind, M., Castander, F. J., Chiu, I., Chown, R., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., de Haan, T., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Holzapfel, W. L., Honscheid, K., James, D. J., Keisler, R., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Marshall, J. L., McDonald, M., Melchior, P., Miller, C. J., Miquel, R., Nord, B., Ogando, R., Omori, Y., Plazas, A. A., Rapetti, D., Reichardt, C. L., Romer, A. K., Roodman, A., Saliwanchik, B. R., Sanchez, E., Schubnell, M., Sevilla-Noarbe, I., Sheldon, E., Smith, R. C., Soares-Santos, M., Sobreira, F., Stark, A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Vieira, J. D., Walker, A. R., Whitehorn, N.“... optical depth of the cluster sample, (tau) over bar (e) = (3.75 +/- 0.89) x 10(-3). We compare...”
Published in Monthly Notices of the Royal Astronomical Society (2016)
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2by Baxter, E J, Raghunathan, S, Crawford, T M, Fosalba, P, Hou, Z, Holder, G P, Omori, Y, Patil, S, Rozo, E, Abbott, T M C, Annis, J, Aylor, K, Benoit-Lévy, A, Benson, B A, Bertin, E, Bleem, L, Buckley-Geer, E, Burke, D L, Carlstrom, J, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Chang, C L, Cho, H-M, Crites, A T, Crocce, M, Cunha, C E, da Costa, L N, D'Andrea, C B, Davis, C, de Haan, T, Desai, S, Dietrich, J P, Dobbs, M A, Dodelson, S, Doel, P, Drlica-Wagner, A, Estrada, J, Everett, W B, Fausti Neto, A, Flaugher, B, Frieman, J, García-Bellido, J, George, E M, Gaztanaga, E, Giannantonio, T, Gruen, D, Gruendl, R A, Gschwend, J, Gutierrez, G, Halverson, N W, Harrington, N L, Hartley, W G, Holzapfel, W L, Honscheid, K, Hrubes, J D, Jain, B, James, D J, Jarvis, M, Jeltema, T, Knox, L, Krause, E, Kuehn, K, Kuhlmann, S, Kuropatkin, N, Lahav, O, Lee, A T, Leitch, E M, Li, T S, Lima, M, Luong-Van, D, Manzotti, A, March, M, Marrone, D P, Marshall, J L, Martini, P, McMahon, J J, Melchior, P, Menanteau, F, Meyer, S S, Miller, C J, Miquel, R, Mocanu, L M, Mohr, J J, Natoli, T, Nord, B, Ogando, R L C, Padin, S, Plazas, A A, Pryke, C, Rapetti, D, Reichardt, C L, Romer, A K, Roodman, A, Ruhl, J E, Rykoff, E, Sako, M, Sanchez, E, Sayre, J T, Scarpine, V, Schaffer, K K, Schindler, R, Schubnell, M, Sevilla-Noarbe, I, Shirokoff, E, Smith, M, Smith, R C, Soares-Santos, M, Sobreira, F, Staniszewski, Z, Stark, A, Story, K, Suchyta, E, Tarle, G, Thomas, D, Troxel, M A, Vanderlinde, K, Vieira, J D, Walker, A R, Williamson, R, Zhang, Y, Zuntz, J“... bar = 0.45. We detect lensing of the CMB by the galaxy clusters at 8.1 sigma significance. Using...”
Published in Monthly Notices of the Royal Astronomical Society (2018)
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