  We revisit Lyman-alpha bounds on the dark matter mass in Lambda Warm Dark
Matter (Lambda-WDM) models, and derive new bounds in the case of mixed Cold
plus Warm models (Lambda-CWDM), using a set up which is a good approximation
for several theoretically well-motivated dark matter models. We combine WMAP5
results with two different Lyman-alpha data sets, including observations from
the Sloan Digital Sky Survey. We pay a special attention to systematics, test
various possible sources of error, and compare the results of different
statistical approaches. Expressed in terms of the mass of a non-resonantly
produced sterile neutrino, our bounds read m_NRP > 8 keV (frequentist 99.7%
confidence limit) or m_NRP > 12.1 keV (Bayesian 95% credible interval) in the
pure Lambda-WDM limit. For the mixed model, we obtain limits on the mass as a
function of the warm dark matter fraction F_WDM. Within the mass range studied
here (5 keV < m_NRP < infinity), we find that any mass value is allowed when
F_WDM < 0.6 (frequentist 99.7% confidence limit); similarly, the Bayesian joint
probability on (F_WDM, 1/m_NRP) allows any value of the mass at the 95%
confidence level, provided that F_WDM < 0.35.
