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Gutierrez, G. Tarle, H. T. Diehl, I. Sevilla-Noarbe, J. Annis, J. Carretero, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\\'ia-Bellido, J. Marshall, J. Mohr, J. Weller, K. Honscheid, K. Kuehn, K. Romer, L. N. da Costa, M. Carrasco Kind, M. Crocce, M. Lima, M. Maia, M. March, M. Schubnell, M. Smith, M. Soares-Santos, M. Swanson, N. Hamaus, N. Kuropatkin, O. Lahav, P. Doel, P. Fosalba, P. Melchior, R. Cawthon, R. C. Smith, R. Gruendl, R. Miquel, R. Schindler, S. Avila, S. Desai, S. Nadathur, T. Abbott, V. Miranda, V. Scarpine, V. Vikram, W. Hartley","submitted_at":"2018-11-19T17:16:34Z","abstract_excerpt":"The largest structures in the cosmic web probe the dynamical nature of dark energy through their integrated Sachs-Wolfe imprints. In the strength of the signal, typical cosmic voids have shown good consistency with expectation $A_{\\rm ISW}=\\Delta T^{\\rm data} / \\Delta T^{\\rm theory}=1$, given the substantial cosmic variance. 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