To carry out serious autocollimation, you need a mirror with a diameter equal to or greater than that of the mirror you are doing, so for 1 meter it takes a floor of one 1 metro, with hole in the center and with surface precision 1/10 wavelength. Unfortunately I cannot have such a thing and therefore I have to do differently.
For the primary
1) hyperbola generation with measurements made with Foucault using the Texerau formulin
2) I also use the Ronchi reticle
a lot of patience and a good dose of luck !!!
For the secondary
1) generation of the shape with verification of the fringes on a spherical mirror (as for the Cassegrain)
2) once the primary is well done, continue to work on the secondary, checking with mirrors mounted on a distant point source (artificial star)
and here too much luck !
Or a nice Zygo interferometer and let's solve the story
This is basically what I think I am doing …… then there will certainly be variations during construction, as always
However I also have a home made Bath Interferometer which helps in more serious cases …………..