The High Energy Density Scientific Instrument at the European XFEL

Zastrau, U.; Appel, K.; Baehtz, C.; Baehr, O.; Batchelor, L.; Berghäuser, A.; Banjafar, M.; Brambrink, E.; Cerantola, V.; Cowan, T.E.; Damker, H.; Dietrich, S.; Di Dio Cafiso, S.; Dreyer, J.; Engel, H.-O.; Feldmann, T.; Findeisen, S.; Foese, M.; Fulla-Marsa, D.; Göde, S.; Hassan, M.; Hauser, J.; Herrmannsdörfer, T.; Höppner, H.; Kaa, J.; Kaever, P.; Knöfel, K.; Konôpková, Z.; Laso García, A.; Liermann, H.-P.; Mainberger, J.; Makita, M.; Martens, E.-C.; McBride, E.E.; Möller, D.; Nakatsutsumi, M.; Pelka, A.; Plueckthun, C.; Prescher, C.; Preston, T.R.; Röper, M.; Schmidt, A.; Seidel, W.; Schwinkendorf, J.-P.; Schoelmerich, M.O.; Schramm, U.; Schropp, A.; Strohm, C.; Sukharnikov, K.; Talkovski, P.; Thorpe, I.; Toncian, M.; Toncian, T.; Wollenweber, L.; Yamamoto, Sh.; Tschentscher, T.

doi:10.1107/S1600577521007335

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Figure 24
HED focusing optics. The X-rays enter from the left. The coordinate system starts at the center of U33. On the right, in red, are the achievable best focus conditions for 5–25 keV for monochromatic (seeded) beam.

JOURNAL OF
SYNCHROTRON
RADIATION

ISSN: 1600-5775

Volume 28| Part 5| September 2021| Pages 1393-1416

https://doi.org/10.1107/S1600577521007335

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