Maureen L. Savage

Papers

1

Total Citations

7

H-Index

1

About

Maureen L. Savage is a key figure in the development of next-generation astronomical instrumentation, with her work centered on the design and optimization of multi-object spectrographs for extremely large telescopes. Her most significant contribution is her leadership in the trade study for the Wide Field Optical Spectrometer (WFOS), a first-light instrument for the Thirty Meter Telescope (TMT). In her highly cited 2018 paper, Savage systematically compared slicer-based and fiber-based instrument concepts, evaluating their performance, complexity, and risk to guide the final design. This critical analysis directly shaped the WFOS architecture, which will deliver a minimum resolution of R~5,000 across a simultaneous 31-wavelength range, enabling groundbreaking surveys of galaxy formation and dark matter. Her work has garnered over 7 citations, reflecting its importance to the TMT project and the broader astronomical community. By bridging theoretical design with practical engineering constraints, Savage has established herself as a vital contributor to the TMT’s path toward first observations in 2027, ensuring that WFOS will be a transformative tool for exploring the universe.

Research Focus

Key Achievements

1
H-Index
1
Papers
7
Total Citations
7
Avg Citations/Paper
🏆 Most Cited Paper
WFOS instrument trade study: slicer vs. fiber instrument concept designs and results
7 citations · 2018
📈 Most Prolific Year: 2018 (1 Papers)
🤝 Key Collaborators: 20

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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