Title: Inverse Problems in Astronomy
Organizer(s): Ronny Ramlau, Johannes Kepler University
Jean-Luc Starck, CEA/Saclay
Andreas Neubauer, Johannes Kepler University
Speakers: Brent Ellerbroek, TMT project office
Progress in Atmospheric Tomography Methods for Extremely Large Telescopes over the Past Decade

Andreas Neubauer, Johannes Kepler University
Cumulative wavefront reconstructor for the Shack-Hartmann sensor

Simone Esposito, Osservatorio Astrofisico di Arcetri
Wavefront Reconstruction for the AO system FLAO of Large Binocular Telescope (LBT).

Clementine Bechet, ESO, Munich
Algorithms for fast wavefront reconstruction and model update : needs for next generation Adaptive Optics

Ronny Ramlau, Johannes Kepler University
Iterative Reconstructors for Multi Conjugate Adaptive Optics

Curtis Vogel, The Optical Science Company
Modeling and parameter estimation for deformable mirrors used in ground-based astronomical adaptive optics

Francois-Xavier Dupe, Laboratoire de Cosmologie et Statistiques
Recovering the galaxy density

Adrienne Leonard, Pisa
Compressed Sensing for Weak Lensing

Abstract: Efficient solution methods for Inverse Problems are required in astronomy for the image postprocessing as well as for the imaging process itself. Typical examples for postprocessing are image deblurring or the determination of physical parameters, e.g. the density of a galaxy, from the recorded images. The focus of the minisymposium will be in particular on Inverse Problems related to Adaptive Optics, a technique for the correction of degraded images caused by turbulences in the atmosphere. The correction process is based on the reconstruction of wavefronts coming from guide stars and involves inversion of data from different wavefront sensors and an atmospheric tomography. The minisymposium will present several new reconstruction approaches.

Please address administrative questions to Scientific questions should be addressed to the chair of the Scientific Program Committee: rundell AT

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