LePHARE: Photometric Analysis for Redshift Estimate

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The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme (2015, methodology): “A complementary effort uses large-area sky surveys designed to support the Dark Energy Survey (DES, Annis et al. 2005).”
Dark Energy Survey Year 1 Results: The Photometric Data Set for Cosmology (2017, methodology): “The flat SED was chosen to represent the wide range of stellar SEDs from the Pickles ATLAS (Pickles 1998) and SEDs of galaxies over the range of redshifts probed by DES (Arnouts & Ilbert 2011).”
The VIMOS Public Extragalactic Redshift Survey (VIPERS) - an unprecedented view of galaxies and large-scale structure at 0.5 < z < 1.2 (2013, methodology): “Photometric redshifts have been derived using Le Phare (Ilbert et al. 2006; Arnouts & Ilbert 2011), a code that provides us, on top of the best redshift solution, zphot, with a specific 68% confidence interval [ẑph−min, ẑph−max] for each galaxy.”
The VIMOS Public Extragalactic Survey (VIPERS) - First Data Release of 57 204 spectroscopic measurements (2013, methodology): “An automatic algorithm cross-correlates the spectroscopic measurement (zspec) with the corresponding photometric redshift (zphot), estimated from the five-band CFHTLS photometry using the Le Phare code (Ilbert et al. 2006; Arnouts & Ilbert 2011).”