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The AMIDAS website has been established as an online interactive tool forrunning simulations and analyzing data in direct Dark Matter detectionexperiments. At the first phase of the website building, only some commonlyused WIMP velocity distribution functions and elastic nuclear form factors havebeen involved in the AMIDAS code. In order to let the options for velocitydistribution as well as for nuclear form factors be more flexible, we haveextended the AMIDAS code to be able to include user-uploaded files with theirown functions. In this article, I describe the preparation of files ofuser-defined functions onto the AMIDAS website. Some examples will also begiven.

Uploading User-Defined Functions onto the AMIDAS Website