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. 2019 Dec 10;10:5633. doi: 10.1038/s41467-019-13580-w

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© The Author(s) 2019

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

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Fig. 1 — a PL spectra of CsPbBr_2.4Cl_0.6, CsPbBr_2.4Cl_0.6:2%YCl₃, CsPbBr₃:PEACl (1:1), and CsPbBr₃:PEACl:2%YCl₃ films. b CIE coordinates of CsPbBr_2.4Cl_0.6 (1), CsPbBr_2.4Cl_0.6:2%YCl₃ (2), CsPbBr₃:PEACl (1:1) (3), and CsPbBr₃:PEACl:2%YCl₃ (4) films. CIE coordinates of CsPbBr₃:PEACl:2%YCl₃ (5) device and CsPbBr₃:PEACl:10%YCl₃ (6) device. c A photograph of the films under UV lamp. The composition of each film is labeled in the photograph. d Power-dependent PLQEs of the perovskite films with different compositions.