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We derive an observational constraint on a spherical inhomogeneity of the void centered at our position from the angular power spectrum of the cosmic microwave background(CMB) and local measurements of the Hubble parameter.
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The Cosmic Microwave Background
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(2010), arXiv:1009.4193, Observational constraints on the LLTB model
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H. Negishi, K.-i. Nakao, C.-M. Yoo, and R. Nishikawa, · 2015
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(2010), arXiv:1007.3065, Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
T. Biswas, A. Notari, and W. Valkenburg, · 2010
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J. P. Zibin and A. Moss, · 2011
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P. Bull, T. Clifton, and P. G. Ferreira, · 2012
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M. Zumalacarregui, J. Garcia-Bellido, and P. Ruiz-Lapuente, · 2012
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V. Marra, L. Amendola, I. Sawicki, and W. Valkenburg, · 2013
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(2015), arXiv:1502.01589, Planck 2015 results. XIII. Cosmological parameters
Planck, P. A. R. Ade et al · 2015
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K. Ichiki, C.-M. Yoo, and M. Oguri, · 2016
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M. Tokutake and C.-M. Yoo, · 2016
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A. G. Riess et al · 2016
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