All-fibre pseudo-slit reformatters

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data archive 2477 disk0/00/00/03/98 2017-07-20 09:59:13 2024-07-17 15:09:05 2017-07-20 09:59:13 data_collection show Yerolatsitis Stephanos S.Yerolatsitis@bath.ac.uk 0000-0002-6268-3674 University of Bath TRUE Researcher Harrington Kerrianne kh302@bath.ac.uk 0000-0003-3450-1842 University of Bath Supervisor Birks Tim T.A.Birks@bath.ac.uk 0000-0001-7984-4932 University of Bath All-fibre pseudo-slit reformatters HH0030 dept_physics Collected data and code used for the results presented in the paper All-fibre pseudo-slit reformatters 2017-07 University of Bath restricted RightsHolder University of Bath Seventh Framework Programme https://doi.org/10.13039/501100004963 312430 Optical Infrared Co-ordination Network for Astronomy (OPTICON) Science and Technology Facilities Council https://doi.org/10.13039/501100000271 ST/N000544/1 Precision Astronomical Spectrographs using Single-Mode Photonic Technologies An IR camera (Xenics XEVA -927) used and the near- and far- field intensity patterns were collected. Images were processed using the uploaded code. Matlab code for analysing the NF and FF intensity patterns captured using the IR camera. The code plots the x and y intensity profiles of all NF and FF patterns and calculates the centroid drift for each direction. https://doi.org/10.1364/OE.25.018713 en 1 10.15125/BATH-00398 https://doi.org/10.1364/OE.25.018713 pub