We present the data release for Galaxy Zoo 2 (GZ2), a citizen science project with more than
16 million morphological classifications of 304 122 galaxies drawn from the Sloan Digital …

Understanding the processes that trigger morphological transformation is central to
understanding how and why the Universe transitions from being disc-dominated at early …

Abstract We present the Combined Array for Research in Millimeter Astronomy (CARMA)
ATLAS3D molecular gas imaging survey, a systematic study of the distribution and …

We explore how the presence of detectable molecular gas depends on the inferred star
formation histories (SFHs) in eight massive, quiescent galaxies at z∼ 0.7. Half of the sample …

We present a study of the cold gas contents of the Atlas3d early-type galaxies, in the context
of their optical colours, near-ultraviolet colours and Hβ absorption line strengths. Early-type …

This is the fourth paper of a series investigating the AGN fuelling/feedback processes in a
sample of 11 nearby low-excitation radio galaxies (LERGs). In this paper, we present follow …

We present an analysis of optical spectroscopically identified active galactic nuclei (AGN)
down to a cluster magnitude of M⋆+ 1 in a sample of six self-similar Sloan Digital Sky …

Understanding the processes that drive the formation of black holes (BHs) is a key topic in
observational cosmology. While the observed M BH–M Bulge correlation in bulge …

The near-absence of compact massive quiescent galaxies in the local Universe implies a
size evolution since z∼ 2.5. It is often theorized that such 'red nuggets' have evolved into …

We investigate the connection between star formation and molecular gas properties in
galaxy mergers at low redshift (z≤ 0.06). The study we present is based on IRAM 30-m CO …