Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

We review the current knowledge about nuclear star clusters (NSCs), the spectacularly
dense and massive assemblies of stars found at the centers of most galaxies. Recent …

We present the Stage II results from the ongoing Satellites Around Galactic Analogs (SAGA)
Survey. Upon completion, the SAGA Survey will spectroscopically identify satellite galaxies …

We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …

Abstract The Galaxy and Mass Assembly (GAMA) survey has been operating since 2008
February on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed …

Abstract The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary
spectroscopic surveys of low redshift galaxies. Covering an area of∼ 286 deg2 (split among …

We compare the predictions of Horizon-AGN, a hydrodynamical cosmological simulation
that uses an adaptive mesh refinement code, to observational data in the redshift range 0< …

We introduce ProFound, a source finding and image analysis package. ProFound provides
methods to detect sources in noisy images, generate segmentation maps identifying the …

We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01<
z< 0.1 (8399 galaxies in g to K s bands) to derive the stellar mass–half-light radius relations …

New surface photometry of all known elliptical galaxies in the Virgo cluster is combined with
published data to derive composite profiles of brightness, ellipticity, position angle, isophote …