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