The INDI AHP Telescope Array correlator driver permits the usage of multiple flux collectors, both in radio and optical frequencies, and gives the possibility to plot a sky correlation of the visibilities of each baseline obtained. The result is stored into an image and can be post-processed.
Once you're connected, You can enable and power-up each line (flux collector) of the array and read directly its pulsing rate, and start the integration like a common CCD.
The delay between each line is calculated automatically and the result will be a Fourier plane filled with the correlation ratios been read during the observation.
It is important the Flux collectors location to be precise at most, so the best usage would be custom GPS drivers snooped by this driver.
All flux collector should point at the same object, so each mount snooped on each line should be linked to others.