Joachimi_Bridle_alpha ================================================ Calculate the gradient of the galaxy luminosity function at the limiting magnitude of the survey. +-------------+--------------------------------------------------------+ | File | luminosity_function/Joachimi_Bridle_alpha/interface.py | +-------------+--------------------------------------------------------+ | Attribution | CosmoSIS team | +-------------+--------------------------------------------------------+ | | Simon Samuroff | +-------------+--------------------------------------------------------+ | URL | | +-------------+--------------------------------------------------------+ The gradient of the cumulative galaxy luminosity function \alpha is sensitive to both redshift and magnitude limit of the survey considered. Joachimi & Bridle (2010) extend the fitting function of Blake & Bridle (2005) to obtain a polynomial \alpha(z, r_lim) at a range of redshifts, where z_i is the median in redshift bin i and r_lim is the r-band magnitude limit. Note that the fitting is based on ground-based data from the COMBO-17 survey. See Joachimi & Bridle (2010) for discussion of its applicability. Assumptions ----------- - The galaxy luminosity function is well approximated by the fitting function of Blake & Bridle (2005). - The limiting r-band magnitude r_lim>16.9 Setup Parameters ---------------- .. list-table:: :header-rows: 1 * - Name - Type - Default - Description * - magnitude_limit - real - 24.0 - Limiting r-band magnitude of the survey considered. * - binned_alpha - bool - True - Compute alpha in the survey redshift bins, rather than as a continuous funtion of redshift. Input values ---------------- .. list-table:: :header-rows: 1 * - Section - Name - Type - Default - Description * - wl_num_density - Nz - int - - Number of points used to evaluate the distribution in each redshift bin. * - - nzbin - int - - Number of survey redshift bins. * - - zmax - real - - Maximum redshift of the redshift distributions. * - - bin_{i} - real 1d - - An array of Nz points evenly sampled from the galaxy redshift distribution in bin i in the range z={0...zmax}. The index ranges i={0, 1, ..., nzbin}. Output values ---------------- .. list-table:: Output values :header-rows: 1 * - Section - Name - Type - Description * - galaxy_luminosity_function - z - real 1d - Redshift values of alpha(z) samples * - - alpha - real 1d - Gradient of the logarithmic cumulative galaxy luminosity function at the limiting magnitude. * - - z_binned - real 1d - Median values of the n(z) in the survey redshift bins. * - - alpha_binned - real 1d - Gradient of the logarithmic cumulative galaxy luminosity function at the limiting magnitude, evaluated at the median redshift of each bin.