Originally posted by Vitalii I donīt care for light ammount -you can argue about that somewhere else.
I was more going in direction of pixel pitch/circle of confusion of the lense - as I understand that determine lvl of detail - since each detail canīt be smaller than the circle or the pixel.
The f/ratio (T stops whatever) is really the effective light gathering power of the lens and I believe you are asking if the total lens projection circle affects the end brightness rather than on a pixel by pixel basis.
f/ratio is the focal length divided by the aperture size and has nothing to do with the sensor, but I suspect the exit pupil of the lens would probably make a difference if it were "condensed" to a smaller sensor.
There was talk that the Sigma 18-35 zoom was really a f/2.8 ff lens with a focal reducer added as a rear element, changing it to a f/1.8 lens. I'm not qualified to answer these questions but thought I'd say a few words to ilicit a response from someone that might help.
PS: Just read a couple of your later posts, which state you aren't interested in what I'm talking about.
Points of light are not the same as pictures of objects. The main thing affecting points of light in pictures is diffraction rings, coma and spherical aberrations etc.. Diffraction rings ARE the COC and the more rings you get, the less the contrast of the image and the larger the star images will be.
You can leave a lens wide open (or one stop down) and get decent Astro shots whereas you may prefer that lens stopped down 2 - 3 stops for landscapes.