The final product of galaxy evolution through cosmic time is the population of galaxies in the
local universe. These galaxies are also those that can be studied in most detail, thus …

Context. The spatial variations of stellar population properties within a galaxy are intimately
related to their formation process. Therefore, spatially resolved studies of galaxies are …

We present Chandra and XMM-Newton X-ray observations of the compact group HCG 57,
and optical integral field spectroscopy of the interacting galaxy pair HCG 57A/D. These two …

The Visible Integral-field Replicable Unit Spectrograph (VIRUS) consists of a baseline build
of 150 identical spectrographs (arrayed as 75 units, each with a pair of spectrographs) fed …

VIRUS is the visible, integral-field replicable unit spectrograph for the Hobby-Eberly-
Telescope (HET) consisting of 75 integral-field-units that feed 150 spectrographs. The full …

The Visible Integral-field Replicable Unit Spectrograph (VIRUS) consists of a baseline build
of 150 identical spectrographs (arrayed as 75 units, each with a pair of spectrographs) fed …

Context. We carry out a detailed 2-D study of the ionised gas in the local universe galaxy
UGC 9837. In nearby galaxies, like the galaxy in question here, the spatial distribution of the …

The Mitchell Spectrograph (aka VIRUS‐P) on the 2.7 m Harlan J. Smith telescope at
McDonald Observatory is currently the largest field of view (FOV) integral field unit (IFU) …

The use of deployable fibre-bundles plays an increasing role in the design of future Multi-
Object-Spectrographs (MOS). Within a research and development project for" Enabling …