XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
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Dorito enables diffraction-limited image reconstruction from JWST AMI observations by deconvolving images or Fourier observables using maximum entropy and total variation regularization.
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A XRISM view of the iron line complex in NGC 1068: Rethinking the prototypical Compton-thick AGN
XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
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Image reconstruction with the JWST Interferometer
Dorito enables diffraction-limited image reconstruction from JWST AMI observations by deconvolving images or Fourier observables using maximum entropy and total variation regularization.