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The DESI Experiment Part II: Instrument Design
DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290
DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…
The DESI Experiment Part I: Science,Targeting, and Survey Design
DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…
The E-ELT Multi-Object Spectrograph: latest news from MOSAIC
F. Hammer, S. Morris, L. Kaper +9
There are 8000 galaxies, including 1600 at z larger than 1.6, which could be simultaneously observed in an E-ELT field of view of 40 sq. arcmin. A considerable fraction of astrophy…
Science Requirements and Trade-offs for the MOSAIC Instrument for the European ELT
C. J. Evans, M. Puech, M. Rodrigues +9
Building on the comprehensive White Paper on the scientific case for multi-object spectroscopy on the European ELT, we present the top-level instrument requirements that are being…
Properties of galaxies at the faint end of the H luminosity function at
Carlos Gómez-Guijarro, Jesús Gallego, Víctor Villar +3
Studies measuring the star formation rate density, luminosity function, and properties of star-forming galaxies are numerous. However, it exists a gap at in H-based…
MUSE observations of the lensing cluster Abell 1689
D. Bina, R. Pelló, J. Richard +14
We present the results obtained with MUSE on the core of the lensing cluster A1689. Integral-field observations with MUSE provide a unique view of the central region, allowing us t…