Roland Bacon

TL;DR: The ATLAS3D project as discussed by the authors is a multi-wavelength survey combined with a theoretical modelling effort, which provides multicolour imaging, two-dimensional kinematics of the atomic (H i), molecular (CO) and ionized gas (H beta, [O iii] and [N i]), together with the kinematic and population of the stars (H β, Fe5015 and Mg b), for a carefully selected, volume-limited (1.16 x 105 Mpc3) sample of 260 early-type (elliptical E

TL;DR: In this paper, a stellar population analysis of the absorption line strength maps for 48 early-type galaxies from the SAURON sample is presented, where the authors estimate the simple stellar population-equivalent age, metallicity and abundance ratio [alpha/Fe] over a two-dimensional field extending up to approximately one effective radius.

TL;DR: In this paper, the authors reported the detection of extended Ly alpha emission around individual star-forming galaxies at redshifts z = 3-6 in an ultradeep exposure of the Hubble Deep Field South obtained with MUSE on the ESO-VLT.

TL;DR: The MUSE Hubble Ultra Deep Survey (MUSE-UDSS) dataset as discussed by the authors is the most complete dataset of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h exposure in a single 1.15 arcmin 2 field.

TL;DR: In this article, the authors present the rationale for and the observational description of ASPECS: the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (UDF), the cosmological deep field that has the deepest multi-wavelength data available.