  Multi-messenger astronomy is becoming the key to understanding the Universe
from a comprehensive perspective. In most cases, the data and the technology
are already in place, therefore it is important to provide an easily-accessible
package that combines datasets from multiple telescopes at different
wavelengths. In order to achieve this, we are working to produce a data
analysis pipeline that allows the data reduction from different instruments
without needing detailed knowledge of each observation. Ideally, the specifics
of each observation are automatically dealt with, while the necessary
information on how to handle the data in each case is provided by a tutorial
that is included in the program. We first focus our project on the study of
pulsars and their wind nebulae (PWNe) at radio and gamma-ray frequencies. In
this way, we aim to combine time-domain and imaging datasets at two extremes of
the electromagnetic spectrum. In addition, the emission has the same
non-thermal origin in pulsars at radio and gamma-ray frequencies, and the
population of electrons is believed to be the same at these energies in PWNe.
The final goal of the project will be to unveil the properties of these objects
by tracking their behaviour using all of the available multi-wavelength data.
