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Preface
Reconstructing images in astrophysics, an inverse problem point of view
Reconstruction of the solar subsurface through helioseismology with SDO
Imaging surface spots from space-borne photometry
Reconstruction of Thermal and Magnetic Field Structure of the Solar Subsurface through Helioseismology
Physical processes leading to surface inhomogeneities: the case of rotation
Interferometry to determine stellar shapes: application to Achernar
Interferometry to image surface spots
Interferometric Surface Mapping of RapidlyRotating Stars.
Application to the Be star Achernar
Doppler and Zeeman Doppler Imaging of Stars.

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