We present the constraints on inflationary parameters in a flat ΛCDM universe obtained from the Wilkinson Microwave Anisotropy Probe (WMAP) three-year data release, plus smaller scale cosmic microwave background (CMB) and two large scale structure (LSS) data sets, 2dF and the Sloan Digital Sky Survey (SDSS) (treated separately). We use a Markov chain Monte Carlo (MCMC) technique combined with an analytic description of the inflationary spectra in terms of the horizon flow functions (HFF). By imposing a consistency condition for the tensor-to-scalar ratio, we study the constraints on both single field standard inflation and on inflation with the violation of the null energy condition, which leads to a blue spectrum for gravitational waves. For standard inflation, the constraint on the tensor-to-scalar ratio we obtain from CMB data and 2dF05 is r_0.01<0.26 at 2σ confidence level. Without the consistency condition between the tensor-to-scalar ratio and the tensor slope, the constraint on the tensor amplitude is not significantly changed, but the constraints on the HFFs are significantly relaxed. We then show that when the third HFF ₃ is allowed to be non-zero and to be of order unity, a large negative (at 2σ) value for the running of the scalar spectral index in standard inflation is found in any set of data we consider.