The Materials Science beamline upgrade at the Swiss Light Source

Willmott, P.R.; Meister, D.; Leake, S.J.; Lange, M.; Bergamaschi, A.; Böge, M.; Calvi, M.; Cancellieri, C.; Casati, N.; Cervellino, A.; Chen, Q.; David, C.; Flechsig, U.; Gozzo, F.; Henrich, B.; Jäggi-Spielmann, S.; Jakob, B.; Kalichava, I.; Karvinen, P.; Krempasky, J.; Lüdeke, A.; Lüscher, R.; Maag, S.; Quitmann, C.; Reinle-Schmitt, M.L.; Schmidt, T.; Schmitt, B.; Streun, A.; Vartiainen, I.; Vitins, M.; Wang, X.; Wullschleger, R.

doi:10.1107/S0909049513018475

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Figure 21
(a) UHV cryostat chamber for experiments in which the sample needs to be cooled to as low as 4.2 K. (b) UHV `baby chamber' for experiments requiring vacuum below 10⁻⁹ mbar.

JOURNAL OF
SYNCHROTRON
RADIATION

ISSN: 1600-5775

Volume 20| Part 5| July 2013| Pages 667-682

doi:10.1107/S0909049513018475

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