Dark and bright sides of the Broad Line Region clouds as seen in the FeII emission of SDSS RM 102

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Fig. B.1.

Comparison of the observed Fe II emission from the source with the Fe II model produced from a CLOUDY simulation including mechanical heating (also shown as the red line in Figure 2), assuming 25% covering factor after being convolved with a Gaussian kernel of FWHM = 2500 km s⁻¹.

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