The raw image from a OSC (colour camera) will be monochrome (grey shades). After processing the filter values are then used with the picture to create a colour image by the computer software - this process is called 'debayering'.
My 383L mono not connected to anything - needs a small gap to allow the light through to create a grey shade image. If you place this on a scope at night - you will need to experiment to find the exposure time that best suits the astronomical target and the camera.
For example - I find that M42 and Planets are too bright for my 383L with my scope, however adding a 2x or 5x telecoverter dims the image so it's not saturated.
ArtemisCapture has a histogram of the image - the idea exposure time should be adjusted so that the image does not saturate (i.e. lots of pixels with the maximum value) or under-exposes. The best exposure allows you to get the histogram in the range - usually 1/2 to 3/4 pixel value.