{"references": ["de la Cruz Rodr\u00edguez, J., L\u00f6fdahl, M. G., S\u00fctterlin, P., Hillberg, T., & Rouppe van der Voort, L. (2014). CRISPRED: A data pipeline for the CRISP imaging spectropolarimeter. Astronomy & Astrophysics, 573, A40. https://doi.org/10.1051/0004-6361/201424319", "Scharmer G. B., Kiselman D., Lofdahl M. G., Rouppe van der Voort L. H. M., 2003, ASPC..307, 3, ASPC..307", "Scharmer, G. B. (2006). Comments on the optimization of high resolution Fabry-P\u00e9rot filtergraphs. Astronomy & Astrophysics, 447(3), 1111\u20131120. https://doi.org/10.1051/0004-6361:20052981", "Scharmer, G. B., Narayan, G., Hillberg, T., de la Cruz Rodriguez, J., L\u00f6fdahl, M. G., Kiselman, D., \u2026 Lagg, A. (2008). CRISP Spectropolarimetric Imaging of Penumbral Fine Structure. The Astrophysical Journal, 689(1), L69\u2013L72. https://doi.org/10.1086/595744", "Van Noort, M., Der Voort, L. R. V., & L\u00f6fdahl, M. G. (2005). Solar Image Restoration By Use Of Multi-frame Blind De-convolution With Multiple Objects And Phase Diversity. Solar Physics, 228(1\u20132), 191\u2013215. https://doi.org/10.1007/s11207-005-5782-z"]}

CRISP Python code