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Two component XSTAR model fit to the 800 ks Chandra HETG observation of NGC 3783. Model fit performed in xspec11 using the warmabs analytic model. |
XSTAR model fit to the HST/COS combined emission and absorption line spectrum of Mrk 290. Top panel: data and model fit; lower panels: emission and absorption model components (Zhang et al. 2014). |
XSTAR model fit to the Hitomi observation of the Perseus cluster. |
An older release of warmabs, which used a simpler system of saved quantities, is here