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Figure 1
Calculated (using Mercury; Macrae et al., 2020BB19) powder diffraction patterns (Cu Kα radiation) for CPO-27-Co [FEGBEB (Gen, 2017BB16), VOFJIM (Rosnes et al., 2019BB23) and VOFJIM01 (Ayoub et al., 2019BB2)]. The differences in peak positions result from the different temperatures of the diffraction studies. Image generated using JADE Pro (MDI, 2022BB21).

ISSN: 2056-9890
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