Abstract
We report on two types of dispersive mirrors. The first one is an ultrabroadband chirped mirror with controlled reflectivity and dispersion of up to 1.5 octaves. A pair of such mirrors allows one to compensate a chirp of the corresponding spectrum, resulting in 2.6-fs pulses. The second type consists of two high-dispersive mirrors for kHz Ti:Sa oscillator-amplifier system and Ti:Sa CPO compressors. These mirrors have dispersion of -400 fs2 (in the range 730–860 nm) and -1300 fs2 (770–820 nm), consequently.
© 2007 Optical Society of America
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