Diffraction supernova
The Diffraction SuperNova is a high-performance X-ray diffraction system designed for advanced materials analysis. It features a micro-focus X-ray source and a high-efficiency detector, providing exceptional data quality and resolution. The system is capable of performing a wide range of X-ray diffraction experiments, including phase identification, structural analysis, and in-situ studies.
Lab products found in correlation
5 protocols using diffraction supernova
Structural Determination by X-ray Diffraction
Powder X-ray Diffraction Measurements
X-ray Crystallographic Structural Analysis
Synthesis and Characterization of Rhenium Complexes
Single-Crystal X-Ray Diffraction Analysis
of all compounds
suitable for X-ray analyses were grown via the liquid–vapor
diffusion method using dichloromethane and n-hexane
as solvents. The X-ray diffraction measurements were carried out on
a Rigaku Oxford Diffraction SuperNova instrument equipped with a microfocus
Cu X-ray source. During the measurements, crystals were maintained
at low temperature with the use of a Oxford Cryosystems nitrogen gas-flow
device. Unit-cell parameter determination and raw diffraction image
processing were performed with the native diffractometer software.53 All structures were solved using an intrinsic
phasing method implemented in the SHELXT program54 (link) and refined with the SHELXL module of the SHELX package55 (link) (with an aid of the OLEX2 suite56 (link)) within the independent atom model approximation. Scattering
factors, in their analytical form, were taken from the International
Tables for Crystallography.57 Final crystal,
data collection, and refinement parameters for all compounds are summarized
in the associated CIF files, which are present in the
the Cambridge Structural Database58 (link),59 (link) (deposition
numbers: CCDC 2004139-43).
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