We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field
spectrograph at the ESO VLT to map 19 massive (9.4< log (M⋆/M⊙)< 11.0) nearby (D≲ 20 …

It is now 16 years since the first data release from the Sloan Digital Sky Survey (SDSS; York
et al. 2000). This Early Data Release, or EDR, occurred in 2001 June (Stoughton et al …

We study the spatially resolved excitation properties of the ionized gas in a sample of 646
galaxies using integral field spectroscopy data from the Sloan Digital Sky Survey IV Mapping …

We investigate how star formation quenching proceeds within central and satellite galaxies
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …

The Sloan Digital Sky Survey (SDSS) has been observing the universe using the 2.5 m
Sloan Foundation Telescope (Gunn et al. 2006) at Apache Point Observatory (APO) for over …

We present an analysis of the quenching of star formation in galaxies, bulges, and disks
throughout the bulk of cosmic history, from z= 2− 0. We utilise observations from the Sloan …

This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral
Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public …

We present the characterization of the main properties of a sample of 98 AGN host galaxies,
both type-II and type-I, in comparison with those of≈ 2700 non-active galaxies observed by …

Aims. The complexity of star formation at the physical scale of molecular clouds is not yet
fully understood. We investigate the mechanisms regulating the formation of stars in different …

We present interferometric CO observations, made with the Combined Array for Millimeter-
wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for …