Oxford diffraction supernova
The Oxford Diffraction SuperNova is a high-performance X-ray diffraction system designed for single-crystal structure determination. It features a microfocus X-ray source and a high-performance CCD or CMOS detector, providing efficient data collection and high-quality results.
Lab products found in correlation
13 protocols using oxford diffraction supernova
Structural Analysis of Crystalline Samples
Crystallization and Structure Determination
Crystallization and Structure Determination of THB4
Crystallization and Diffraction of C6F6:C4H5N
Crystallization and Diffraction of C6F6:C4H5N
Single-Crystal X-Ray Diffraction of Lactones
Crystallization and Structural Characterization of Compound 1
we successfully obtained the colorless orthorhombic crystals of compound
(10:1) at room temperature for several days. The intensity data were
collected on a diffractometer Rigaku Oxford Diffraction SuperNova,
Dual, Cu at zero, equipped with an AtlasS2 CCD using Cu Kα radiation.
The crystal of
collection. The crystallographic data of
deposited in the Cambridge Crystallographic Data Center database (CCDC
2172881).
Single-crystal X-ray Structure of 1-(Sa)
Structural Determination via Single-Crystal X-ray Diffraction
Hydrogen atom parameters were constrained. For full details see Table S1. † CCDC 1557650-1557653. †
Temperature and Pressure X-ray Diffraction
Exploratory high-pressure X-ray diffraction measurements to 7.3 GPa at room temperature were performed on a Stoe IPDS-II single-crystal diffractometer with a Mo Kα X-ray source using a Boehler Almax diamond anvil cell loaded with a CrAs crystal, a ruby chip and a 4:1 methanol–ethanol mixture as a pressure-transmitting medium. The diffraction data were integrated with the X-Area (v1.62; Stoe & Cie, 2011 ▸ ) software.
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