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Figure Captions
Fig. 1. (a) Experimental setup. (b) Measured (left) and retrieved (right) SHG-FROG traces
of the gate pulse. (c) Time-domain waveform of the retrieved gate pulse (left) and the
spectrum of the pulse after CM3 (right). Here, CM1: Edmund Optics (highly-dispersive
ultrafast mirror), GDD=−500 fs2 @ 1000–1060 nm; CM2: custom made, GDD ~ −50 fs2 @
725 nm–1325 nm, and CM3: Edmund Optics (ultra-broadband complementary chirped
mirror), GDD=−60 fs2 @ 650–1350 nm.
Fig. 2. (a) Phase-matching conditions in the LGS crystals for DFG (upper panel) and (b)
optical parametric amplification (lower panel). The phase-matching function |sinc(∆kL/2)| is
shown as functions of the phase-matching (PM) angle and the MIR wavelength.
Fig. 3. (a) MIR spectra before (upper panel) and (b) after the two-stage OPA (lower panel).
The red dots in the lower panel show the pulse energy. The inset shows the spatial beam
profile of the MIR beam at 6 m after the LGS (OPA2).
Fig. 4. (a) The time-domain waveform of the MIR pulse after the two-stage OPA. (b) The
Fourier transform of (a). (c) 2D map of 401 time-domain waveforms measured within 20
minutes (left) and the corresponding CEPs (right). (d) 2D map of 21 average time-domain
waveforms measured within 5 hours (left) and their CEPs (right).
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Fig. 1.
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Fig. 2.
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Fig. 3.
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Fig. 4.
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