Figure 5 from A Statistical Inference Method for Interpreting the CLASP Observations

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A Statistical Inference Method for Interpreting the CLASP Observations

Authors: J. Štěpán, J. Trujillo Bueno, L. Belluzzi, A. Asensio Ramos, R. Manso Sainz, T. del Pino Alemán, R. Casini, R. Kano, A. Winebarger, F. Auchère, R. Ishikawa, N. Narukage, K. Kobayashi, T. Bando, Y. Katsukawa, M. Kubo, S. Ishikawa, G. Giono, H. Hara, Y. Suematsu, T. Shimizu, T. Sakao, S. Tsuneta, K. Ichimoto, J. Cirtain, P. Champey, B. De Pontieu, and M. Carlsson

2018 The Astrophysical Journal 865 48.

Provider: AAS Journals

Caption: Figure 5.

Maps of the likelihood ratios (see Equation (13)) corresponding to the three particular data realizations of Figure 4. From top to bottom, the number of observed points is 10, 50, and 200. The white dot at a = 5, ﹩\bar{B}=50﹩ G (b ≈ 0.5) indicates the true model parameters. For N = 200, the estimator, i.e., the point of maximum likelihood, is already very close to the true value.

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