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Two sources of geometric information are encoded in the galaxy power spectrum: the sound horizon at recombination and the horizon at matter-radiation equality.
1902
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A. de Mattia and V. Ruhlmann-Kleider, Integral constraints in spectroscopic surveys , JCAP 2019
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N. Schöneberg, J. Lesgourgues and D. C. Hooper, The BAO+BBN take on the Hubble tension , JCAP 2019
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L. Verde, T. Treu and A. G. Riess, Tensions between the early and late Universe , Nature Astronomy 3
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C. Alcock and B. Paczynski, An evolution free test for non-zero cosmological constant , Nature 281
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M. Tegmark, Measuring Cosmological Parameters with Galaxy Surveys , Phys. Rev. Lett. 79
1997
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D. J. Eisenstein and W. Hu, Baryonic Features in the Matter Transfer Function , ApJ 496
1998
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A. G. Riess, The expansion of the Universe is faster than expected , Nature Reviews Physics 2
2001
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W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole et al., The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe , MNRAS 327
2001
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S. L. Bridle, R. Crittenden, A. Melchiorri, M. P. Hobson, R. Kneissl and A. N. Lasenby, Analytic marginalization over CMB calibration and beam uncertainty , MNRAS 335
2002
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2003
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2004
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J. Schombert, S. McGaugh and F. Lelli, Using the Baryonic Tully-Fisher Relation to Measure H o
2006
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J. Lesgourgues and S. Pastor, Massive neutrinos and cosmology , Phys. Rep. 429
2006
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O. H. E. Philcox, M. M. Ivanov, M. Zaldarriaga, M. Simonović and M. M. Schmittfull, Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections , in prep. (2020)
2020
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