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The Data Processing Pipeline for the MUSE Instrument
Peter M. Weilbacher, Ralf Palsa, Ole Streicher +12
Processing of raw data from modern astronomical instruments is nowadays often carried out using dedicated software, so-called "pipelines" which are largely run in automated operati…
The MUSE Hubble Ultra Deep Field Survey XIV. The evolution of the Lya emitter fraction from z=3 to z=6
Haruka Kusakabe, Jeremy Blaizot, Thibault Garel +19
The Lya emitter (LAE) fraction, X_LAE, is a potentially powerful probe of the evolution of the intergalactic neutral hydrogen gas fraction. However, uncertainties in the measuremen…
Reconstruction of the ground-layer adaptive-optics point spread function for MUSE Wide Field Mode observations
Thierry Fusco, R. Bacon, S. Kamann +7
Here we describe a simple, efficient, and most importantly fully operational point-spread-function(PSF)-reconstruction approach for laser-assisted ground layer adaptive optics (GLA…
The MUSE Hubble Ultra Deep Field Survey XIII. Spatially resolved spectral properties of Lyman alpha haloes around star-forming galaxies at z > 3
Floriane Leclercq, Roland Bacon, Anne Verhamme +18
We present spatially resolved maps of six individually-detected Lyman alpha haloes (LAHs) as well as a first statistical analysis of the Lyman alpha (Lya) spectral signature in the…
ORIGIN: Blind detection of faint emission line galaxies in MUSE datacubes
David Mary, Roland Bacon, Simon Conseil +2
One of the major science cases of the MUSE integral field spectrograph is the detection of Lyman-alpha emitters at high redshifts. The on-going and planned deep fields observations…