Explore projects

reports on the progress of the Toolkit for Adaptive Optics

Development of the base features of Lenstool using HPC techniques for modern CPU and GPU clusters.

Reproduction pipeline for MUSE UDF photometry and astrometry (Section 4 of Bacon et al. 2017, A&A, 608, A1).

Reproduction pipeline to generate HST broad-band magnitudes for ORIGIN-only detected objects within MUSE 3D datacube (Section 7.3 of Bacon et al. 2017, A&A, 608, A1)

Make narrow band images of muse cube in command line

PampelMuse analysis plots

based on mpdaf, this script can produce narrow band images in command line