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Research data for: Halide remixing under device operation imparts stability on mixed-cation mixed-halide perovskite solar cells


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Type

Dataset

Change log

Authors

Anaya Martin, Miguel 
Galkowski, Krzysztof 
Abfalterer, Anna 
Chiang, Yu-Hsien 

Description

This entry contains the data required to reproduce the figures from the main text of the associated manuscript. This includes:

  • GIWAXS diffractograms (calibrated, processed, and extracted to a readily-readable format) and relative extracted peak positions
  • current vs time data
  • current vs voltage data
  • photoluminescence spectra (wavelength-dependent, and eV-dependent) and relative peak positions.

Version

Software / Usage instructions

The data is contained within a .opju file and is readily plottable in OriginPro software.

Keywords

Perovskite, Photovoltaics, Diffraction, Photosegregation, Electrostriction

Publisher

Sponsorship
The authors acknowledge the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (HYPERION, grant agreement No. 756962), and the Engineering and Physical Sciences Research Council (EPSRC) (grant agreement No. EP/R023980/1). E.R. was partially supported by an EPSRC Departmental Graduate Studentship. K.G. appreciates support from the Polish Ministry of Science and Higher Education within the Mobilnosc Plus program (grant agreement No. 1603/MOB/V/2017/0). A.A. acknowledges the Royal Society for funding. Y.-H.C. acknowledges funding from a Taiwan Cambridge Scholarship. K.J. acknowledges funding from the Royal Society (RGFR1180002). Z.A.-G. acknowledges funding from a Winton Studentship, and ICON Studentship from the Lloyd’s Register Foundation. M.A. acknowledges funding from the Marie Skłodowska-Curie actions (grant agreement No. 841386) under the European Union’s Horizon 2020 research and innovation programme, and from the Leverhulme Early Career Fellowship (grant agreement No. ECF-2019-224) funded by the Leverhulme Trust and the Isaac Newton Trust. S.D.S. also acknowledges the Royal Society and Tata Group (UF150033). This work utilized beamline I07 at the Diamond Light Source (Proposal SI17223).
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