22 July 2014 Current status and future plans for the Maunakea Spectroscopic Explorer (MSE)
Author Affiliations +
Abstract
The Maunakea Spectroscopic Explorer (MSE; formerly ngCFHT) will be a large format wide field spectroscopic facility that replaces the existing 3.6 m Canada-France-Hawaii Telescope. Capable of recording tens of thousands of spectra on faint targets each night, and sustain that pace for years, MSE will be an ideal complement to emerging space- and ground-based imaging survey facilities. The combination of aperture, spectral resolution, and dedicated access to support large surveys makes MSE distinct from any other facilities under development or being planned. We provide an overview of the MSE technical design, organization of the project office, and the core science goals that will help drive MSE for decades.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Doug A. Simons, Doug A. Simons, David Crampton, David Crampton, Pat Côté, Pat Côté, Alan McConnachie, Alan McConnachie, Kei Szeto, Kei Szeto, Derrick Salmon, Derrick Salmon, Daniel Devost, Daniel Devost, Richard Murowinski, Richard Murowinski, "Current status and future plans for the Maunakea Spectroscopic Explorer (MSE)", Proc. SPIE 9145, Ground-based and Airborne Telescopes V, 914515 (22 July 2014); doi: 10.1117/12.2056389; https://doi.org/10.1117/12.2056389
PROCEEDINGS
11 PAGES


SHARE
RELATED CONTENT

Keck 1 deployable tertiary mirror (K1DM3)
Proceedings of SPIE (September 16 2012)
Development of the single fibres and IFUs of WEAVE
Proceedings of SPIE (September 12 2012)
Project management at a university
Proceedings of SPIE (June 26 2006)

Back to Top