Question rephrased
OK, the QM world is admittedly unintuitive to macro-particles like me

So can I try a re-phrase of the question?
I think, but am not sure, this statement is true: The more you try and 'pin down' the location of a QM particle, the more it tends to 'spread out'. So as the resolving power of your locating instrument increases, you find that you can detect the particle less often within a given bounding box.
That means, I think, that as resolving power of the instrument increases, a point will be reached at which the particle is detected exactly 99.00% of the time within the limits of resolution of the instrument.
So if I am looking at photons streaming in from a 'perfectly' collimated laser beam source, and using the Palomar telescope to do so, I will observe the photons a very high percentage of the time. As I shrink the aperture of the telescope, at some point I will only observe the photons 99.0% of the time, not because the beam isn't perfect, but because Heisenberg says I can't know the position of the photons that accurately.
If the above is true, then the question about size becomes something like:
A) For light of a specific frequency in the range of, say, visible red, what is the 2-D size of the aperture (3-D bounding box?) in meters, that will enclose the position of the photons 99.00% of the time?
If this question makes any more sense than the original one, then:
B)Is this aperture (bounding box?) different in size than that of photons of a different frequency, say visible blue light?
And for a somewhat related question about quantities in photons:
A photon is a wave of EM energy, oscillating at a given frequency. How many oscillations does a photon consist of?