Brand: Agilent
Model: Oxford Supernova
Brief description 1. 4-circle kappa goniometer 2. Hi-flux dual wavelength micro-focus Mo & Cu X-ray sources 3. Small, compact cabinet 4. 135 mm Atlas, CCD detector 5. CrysAlisPro - Data collection & processing software 6. AutoChem - Fully automatic structure solution and refinement software 7. Optional nitrogen or helium cryo-device
The SuperNova has been designed around two low power consumption yet high intensity X-ray microsources. Built in-house by Oxford Diffraction, the Nova (Cu) and Mova (Mo) X-ray sources combine the latest in micro-focus tube technology with specially designed multi-layer X-ray optics
X-ray Laboratory C14 B
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1. Must have a single, robust (stable) sample, generally between 50-250 microns in size
2. Optically clear sample
3. For a typical crystal, a pre-experiment lasting less than 5minutes is recorded to evaluate the crystal quality. From the first frame of data, CrysAlisPro automatically evaluates the crystal quality and provides the user with information regarding the unit cell, angular resolution and suggested frame exposure time.
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Last Update: 11/09/2023