.. _book_fig_chapter8_fig_nonlinear_mu_z:


Nonlinear cosmology fit to mu vs z
----------------------------------
Figure 8.5

Cosmology fit to the standard cosmological integral. Errors in mu are a factor
of ten smaller than for the sample used in figure 8.2. Contours are 1-sigma,
2-sigma, and 3-sigma for the posterior (uniform prior in :math:`\Omega_M` and
:math:`\Omega_\Lambda`). The dashed line shows flat cosmology. The dotted lines
show the input values.



.. image:: ../images/chapter8/fig_nonlinear_mu_z_1.png
    :scale: 100
    :align: center


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