Optical output coupling mirror was set to ∼9.7%.
Other tips: Request that a mirror be set up so you can watch the painter in progress and that you be allowed periodic peeks at the unfinished work.
The integration time was set at the minimal stable integration time of this spectrograph, τ = 6 ms. To meet the sampling frequency requirement (Section 2.2), the velocity of the reference mirror was set at vR = 12 µm/s (frequency fR = 0.3 Hz, scanning range ΔR = 20 µm).
Some paid an extra four hundred and fifty dollars to attend the Beauty Academy, where rows of vanity mirrors were set up for seminars.
The collection mirrors were set to the front facing setting, and the samples were scanned at 450 to 600 nm for emission (3 nm slit widths, integration times of 0.2 seconds at 5 nm increments) and from 400 to 550 nm for excitation (3 nm slit width, 10 nm increments).
Two mirrors were set behind the cylinder to view all directions.
The difference in the OPD between the two mirrors was set about 11 mm, which was used to place the zero-delay lines of the two images on the top and the bottom of the anterior segment.
A removable mirror, M3, is set either to image the spatial modal structure onto a CCD camera, or to send the output beam to the Optical Spectrum Analyzer, OSA, through a × 20 microscope objective, Obj3, and a multimode fiber, MMF.
The programmable mask, using Digital Micro-mirror Device, is set on the second image plane to implement the function of spectral domain encoding.
