We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …

We present an analysis of the host properties of 85 224 emission-line galaxies selected from
the Sloan Digital Sky Survey. We show that Seyferts and low-ionization narrow emission-line …

We analyze star formation in the nuclei of nine Seyfert galaxies at spatial resolutions down
to 0.085'', corresponding to length scales of order 10 pc in most objects. Our data were taken …

Type II quasars are the long-sought luminous analogs of type 2 (narrow emission line)
Seyfert galaxies, suggested by unification models of active galactic nuclei (AGNs) and …

A new stellar library at the near-IR spectral region developed for the empirical calibration of
the Ca ii triplet and stellar population synthesis modelling is presented. The library covers …

Using the latest stellar evolution models, theoretical stellar spectra, and a compilation of
observed emission line strengths from Wolf-Rayet (WR) stars, we construct evolutionary …

The mass of supermassive black holes at the centre of galaxies is tightly correlated with the
mass of the galaxy bulges which host them. This observed correlation implies a mechanism …

We demonstrate that the evolution of the QSO luminosity density with epoch displays a
striking similarity to the cosmological evolution of the field galaxy star formation rate, recently …

We present a study of the stellar populations in the central∼ 200 pc of a large and
homogeneous sample comprising 79 nearby galaxies, most of which are Seyfert 2s. The star …

Abstract We report R~ 4300 VLT SINFONI adaptive optics integral field K-band spectroscopy
of the nucleus of the Seyfert 1 galaxy NGC 3227 at a spatial resolution of 0 farcs 085 (7 pc) …