“…The L1 Allegra laser is sent from the L1 hall, located above E1, and can be directed to one of two types of secondary sources -an HHG source for XUV radiation (Hort et al, 2019(Hort et al, , 2020 or plasma X-ray sources (Nejdl et al, 2019). The HHG source serves two stations for XUV science: 'MAC' for atomic, molecular and optical science and coherent diffractive imaging (Klimesova ´et al, 2021), and 'ELIps' for XUV materials science applications (Espinoza et al, 2020). Complementary methods for ultrafast optical spectroscopy are also available (using support lasers): transient optical absorption (Naumova et al, 2018), stimulated Raman scattering (Andrikopoulos et al, 2020), time-resolved spectroscopic ellipsometry (Richter et al, 2021) and IR (1D and 2D) spectroscopy.…”