GALACSI is part of the Adaptive Optics Facility (AOF), and associated with the Deformable Secondary Mirror (DSM) and the 4 Laser Guide Star Facility (4LGSF). It defines an AO system developed to increase the performance of the MUSE instrument in Wide Field Mode, dubbed MUSE/AOF. Commissioning is proceeding and Science Verification is planned for August 2017, for which applications are invited.
MUSE Wide Field Mode Adaptive Optics Science Verification
An integral part of the commissioning of a new instrument at the VLT is the Science Verification (SV) phase. SV programmes include a set of typical scientific observations that should verify and demonstrate to the community the capabilities of the new instrument in the operational framework of the VLT Observatory. ESO encourages the community to submit highly challenging or risky science observations that will push MUSE/AOF and the VLT to its limits in order to better understand the performance parameter space and its envelope.
The call for proposals for MUSE WFM/AO can be found at here. The deadline for proposal submission is 14 June 2017, 18:00 CEST.