Dissipative systems play a very important role in several physical models, most notably in Celestial Mechanics, where the dissipation drives the motion of natural and artificial satellites, leading them to migration of orbits, resonant states, etc. Hence the need to develop theories that ensure the existence of structures such as invariant tori or periodic orbits and device efficient computational methods. The point of view that we adopt is that we are dealing with real problems and that we will have to use a very wide variety of methods. From the applications, to numerical studies to rigorous mathematics. As we will see, all of these methods feed on each other. The rigorous mathematics leads to efficient algorithms (and allows us to believe the results), the numerical experiments lead to deep mathematical conjectures, the applications benefit from all this tools, and set meaningful goals that prevent from doing things just because they are easy. Of course, the road towards this lofty goal is not rosy and there are many false starts, complications, etc. After several years, we can erase the false starts from the story, but we hope to provide some flavor. Given the rather wide scope is unavoidable that some arguments have different standards (rigorous proofs, numerical efficiency, conjectures). We have strived to make all those very explicit, but may be it would be hard to keep this present. Of course, similar programs can be applied to many problems, but in this paper we will deal with a rather concrete set of problems.In this work we concentrate on the existence of invariant tori for the specific case of dissipative systems known as conformally symplectic systems, which have the property that they transform the symplectic form into a multiple of itself. To give explicit examples of conformally symplectic systems, we will present two different models: a discrete system known as the standard map and a continuous system known as the spin-orbit problem. In both cases we will consider the conservative and dissipative