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Home All issues Volume 665 (September 2022) A&A, 665 (2022) A72 Full HTML
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Fig. 4.

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Best-fit model (Model M1 in Tables 2 and 3) to the RGS spectra of NGC 3227 on 2019-11-15 (top) and 2019-12-05 (bottom). The warm emitter component is shown in red and is identical for both observations, while the continuum is shown in blue. The black curves are the total emission.

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