MUSE, a 2nd generation VLT instrument, will become the world's largest integral field spectrograph. It will be an AO assisted instrument which, in a single exposure, covers the wavelength range from 465 to 930 nm with an average resolution of 3000 over a field of view of 1'x1' with 0.2'' spatial sampling. Both the complexity and the rate of the data are a challenge for the data processing of this instrument.
We will give an overview of the data processing scheme that has been designed for MUSE. Specifically, we will use only a single resampling step from the raw data to the reduced data product. This allows us to improve data quality, accurately propagate variance, and minimize spreading of artifacts and correlated noise. This approach necessitates changes to the standard way in which reduction steps like wavelength calibration and sky subtraction are carried out, but can be expanded to include combination of multiple exposures.
PERRY: A Human-in-the-Loop GUI for Precision Alignment of MUSE Data
Australian Astronomical Optics, Faculty of Science and Engineering, Macquarie University（澳大利亚天文光学，麦考瑞大学科学与工程学院）；Astrophysics and Space Technologies Research Centre, Macquarie University（麦考瑞大学天体物理学与空间技术中心）；School of Physics, University of New South Wales（新南威尔士大学物理学院）
Design and optimization of neural networks for multifidelity cosmological emulation
University of California, Riverside（加州大学河滨分校）；Department of Physics & Astronomy, University of California, Riverside（加州大学河滨分校物理与天文系）；Department of Physics, University of Michigan（密歇根大学物理系）；Leinweber Center for Theoretical Physics（莱因韦伯理论物理中心）；The University of Texas at Austin（德克萨斯大学奥斯汀分校）
