Keck Segment Surface Artifacts: Impacts on Segment Phasing and Image Quality

We show that the segments of the Keck telescopes su er from small but signi cant surface artifacts that limit
segment phasing accuracy. Both the segment surface artifacts themselves and the limits they place on segment
phasing have important implications for adaptive optics, high contrast imaging, and seeing limited observations.
These surface artifacts are likely by-products of the segment polishing, most likely the Ion Beam Figuring (IBF)
process that constitutes the nal step of the segment surface guring. The surface artifacts di ract a signi cant
amount of light out past 3.5 arcseconds and generate chromatic e ects that limit segment phasing accuracy.
We present on-sky measurements of the di racted intensity. Segment surface roughness measurements are also
presented, which show that surface roughness is not the source of the problem. These results have direct relevance
to segment manufacturing for the Thirty Meter Telescope (TMT) and other segmented mirror telescopes.