As we have seen for digital camera market and a sensor resolution increasing
to "megapixels", all the scientific and high-tech imagers (whatever the wave
length - from radio to X-ray range) tends also to always increases the pixels
number. So the constraints on front-end signals transmission increase too. An
almost unavoidable solution to simplify integration of large arrays of pixels
is front-end multiplexing. Moreover, "simple" and "efficient" techniques allow
integration of read-out multiplexers in the focal plane itself. For instance,
CCD (Charge Coupled Device) technology has boost number of pixels in digital
camera. Indeed, this is exactly a planar technology which integrates both the
sensors and a front-end multiplexed readout. In this context, front-end
multiplexing techniques will be discussed for a better understanding of their
advantages and their limits. Finally, the cases of astronomical instruments in
the millimeter and in the X-ray ranges using SQUID (Superconducting QUantum
Interference Device) will be described