The Multi-Mission Maximum Likelihood framework (3ML)

Understand

Astrophysical sources are now observed by many different instruments at different wavelengths, from radio to high-energy gamma-rays, with an unprecedented quality.

• Putting all these data together to form a coherent view, however, is a very difficult task.
• Each instrument has its own data format, software and analysis procedure, which are difficult to combine.
• It is for example very challenging to perform a broadband fit of the energy spectrum of the source.