2 code implementations • 19 Nov 2020 • T. Liaudat, J. Bonnin, J. -L. Starck, M. A. Schmitz, A. Guinot, M. Kilbinger, S. D. J. Gwyn
We present, and share the code of, a new PSF modelling algorithm that models the PSF field on all the focal plane that is mature enough to handle real data.
Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics
1 code implementation • 17 Jun 2019 • M. A. Schmitz, J. -L. Starck, F. Ngole Mboula, N. Auricchio, J. Brinchmann, R. I. Vito Capobianco, R. Clédassou, L. Conversi, L. Corcione, N. Fourmanoit, M. Frailis, B. Garilli, F. Hormuth, D. Hu, H. Israel, S. Kermiche, T. D. Kitching, B. Kubik, M. Kunz, S. Ligori, P. B. Lilje, I. Lloro, O. Mansutti, O. Marggraf, R. J. Massey, F. Pasian, V. Pettorino, F. Raison, J. D. Rhodes, M. Roncarelli, R. P. Saglia, P. Schneider, S. Serrano, A. N. Taylor, R. Toledo-Moreo, L. Valenziano, C. Vuerli, J. Zoubian
Firstly, we took steps toward a nonparametric method to address the issue of recovering the PSF field, namely that of finding the correct PSF at the position of any galaxy in the field, applicable to Euclid.
Instrumentation and Methods for Astrophysics