The co-evolution between supermassive black holes and their environment is most directly
traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere …

Contrary to many stereotypes about massive galaxies, observed brightest group galaxies
(BGGs) are diverse in their star formation rates, kinematic properties, and morphologies …

Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …

Abstract The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-
object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey …

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 …

The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2
Southern Survey and Full Release of eBOSS Spectra - IOPscience This site uses cookies. By …

We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled
independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey …

The role of the cosmic web in shaping galaxy properties is investigated in the Galaxy And
Mass Assembly (GAMA) spectroscopic survey in the redshift range 0.03≤ z≤ 0.25. The …

ABSTRACT The Galaxy And Mass Assembly (GAMA) survey furnishes a deep redshift
catalog that, when combined with the Wide-field Infrared Survey Explorer (WISE), allows us …

We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The
GAMA survey is a spectroscopic redshift and multiwavelength photometric survey in three …