The major science driver of the Very Wide component of the CFHTLS is to study the populations of Small Bodies of the Outer Solar System. In this respect, the main products of the Ecliptic Survey is to provide an unbiased orbital database, and a mean to compare the really observed population to a set of theoretical populations. In the near future, we will provide two services to the scientific community., The first will be a web accessible orbital database containing all astrometric measurements and orbital determinations of TNOs discovered in the CFHTLS-VW. In particular, we will select the subset of such objects for which we have determined good orbits, without introducing unknown biases, such as selected follow-up based on provisional orbits., The second will be a survey simulator which will be accessible as a web service. Given a model describing the current population of Small Bodies of the Outer Solar System, this service will give the set of objects that would have been detected and followed by CFHTLS-VW, had this model been the truth. The interested scientist will then be able to compare the distribution of simulated detected objects to the real ones. In the next version of the Survey Simulator, we will also include some Bayesian test to compare the model to the real detections.