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S. J. Turnbull, M. J. Hudson, H. A. Feldman, M. Hicken, R. P. Kirshner and R. Watkins, Cosmic flows in the nearby universe from Type Ia supernovae
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2012
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C. Park, Y.-Y. Choi, J. Kim, J. R. Gott, III, S. S. Kim and K.-S. Kim, The Challenge of the Largest Structures in the Universe to Cosmology
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2012
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N. Suzuki et. al
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2012
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I. Ben-Dayan, G. Marozzi, F. Nugier and G. Veneziano, The second-order luminosity-redshift relation in a generic inhomogeneous cosmology
Original
2012
Cited alongside, same era.
C. Bonvin, R. Durrer and M. A. Gasparini, Fluctuations of the luminosity distance
2012

Then

A. E. Romano, H.-W. Chiang and P. Chen, A new method to determine large scale structure from the luminosity distance
Original
2014
Later among the works it cites.
G. R. Bengochea and M. E. De Rossi, Dependence on supernovae light-curve processing in void models
Original
2014
Later among the works it cites.
R. B. Tully, H. Courtois, Y. Hoffman and D. Pomarède, The Laniakea supercluster of galaxies
Original
2014
Later among the works it cites.
G. Fanizza and L. Tedesco, Inhomogeneous and anisotropic Universe and apparent acceleration
Original
2015
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R. A. Battye, T. Charnock and A. Moss, Tension between the power spectrum of density perturbations measured on large and small scales

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2017

Probing homogeneity with standard candles

Chiang, Hsu Wen, Romano, Antonio Enea, Nugier, Fabien et al.

Understand

We show that standard candles can provide some valuable information about the density contrast, which could be particularly important at redshifts where other observations are not available.

We use an inversion method to reconstruct the local radial density profile from luminosity distance observations assuming background cosmological parameters obtained from large scale observations.
Using type Ia Supernovae% (SNe) , Cepheids and the cosmological parameters from the Planck mission we reconstruct the radial density profiles along two different directions of the sky.
We compare these profiles to other density maps obtained from luminosity density, in particular Keenan et al.