S. Bardelli

The Capodimonte Deep Field

The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy cluster survey

MASSIV: Mass Assembly Survey with SINFONI in VVDS

What is a cool-core cluster? a detailed analysis of the cores of the X-ray flux-limitedHIFLUGCScluster sample

JKCS 041: a colour-detected galaxy cluster at $z_{\mathrm{phot}}$ ~ 1.9 with deep potential well as confirmed by X-ray data

The evolution of the luminosity functions in the FORS Deep Field from low to high redshift

DeepU-B-Vimaging of the Lockman Hole with the LBT

The IllustrisTNG simulations: public data release

A two-solar-mass neutron star measured using Shapiro delay

A 610-MHz survey of the Lockman Hole with the Giant Metrewave Radio Telescope - I. Observations, data reduction and source catalogue for the central 5 deg²

Creation of cosmic structure in the complex galaxy cluster merger Abell 2744

First results from the IllustrisTNG simulations: matter and galaxy clustering

The kinematics and dark matter fractions of TNG50 galaxies at z = 2 from an observational perspective

Plateau de Bure High-z Blue Sequence Survey 2 (PHIBSS2): Search for Secondary Sources, CO Luminosity Functions in the Field, and the Evolution of Molecular Gas Density through Cosmic Time*

The DEEP2 Galaxy Redshift Survey: Spectral Classification of Galaxies at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z\sim 1$ \end{document}

NUCLEAR ACTIVITY IS MORE PREVALENT IN STAR-FORMING GALAXIES

Fueling Low‐Level AGN Activity through Stochastic Accretion of Cold Gas

Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z = 2.26 Galaxy SDSS J0901+1814

MASSIV: Mass Assembly Survey with SINFONI in VVDS - II. Kinematics and close environment classification

THE IMPACT OF COLD GAS ACCRETION ABOVE A MASS FLOOR ON GALAXY SCALING RELATIONS

The physical properties of star-forming galaxies in the low-redshift Universe

Turbulent motions and shocks waves in galaxy clusters simulated with adaptive mesh refinement

VALIDATION OF THE EQUILIBRIUM MODEL FOR GALAXY EVOLUTION TOz∼ 3 THROUGH MOLECULAR GAS AND DUST OBSERVATIONS OF LENSED STAR-FORMING GALAXIES

STAR FORMATION AND DUST OBSCURATION AT z ≈ 2: GALAXIES AT THE DAWN OF DOWNSIZING

[O iii]/[N ii] as an abundance indicator at high redshift

Observational Evidence of Active Galactic Nuclei Feedback

GOYA Survey:UandBNumber Counts in the Groth‐Westphal Strip

Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe

Molecular and atomic gas along and across the main sequence of star-forming galaxies

Enriched haloes at redshift z = 2 with no star formation: implications for accretion and wind scenarios★

A survey of molecular gas in luminous sub-millimetre galaxies

THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROMz= 0-8

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THEWMAPDATA

Stellar population synthesis at the resolution of 2003

High-resolution CO and radio imaging of ULIRGs: extended CO structures and implications for the universal star formation law

The Millennium Run Observatory: first light

Energetic galaxy-wide outflows in high-redshift ultraluminous infrared galaxies hosting AGN activity

AN X-RAY-SELECTED GALAXY CLUSTER IN THE LOCKMAN HOLE AT REDSHIFT 1.753

Galactic star formation and accretion histories from matching galaxies to dark matter haloes

First results from the IllustrisTNG simulations: radio haloes and magnetic fields

The Physics of Neutron Stars

Deep multi-frequency radio imaging in the Lockman Hole using the GMRT and VLA - I. The nature of the sub-mJy radio population

BLOX: The Bonn Lensing, Optical, and X-ray selected galaxy clusters -- I. Cluster catalog construction

THE STAR FORMATION HISTORY OF MASS-SELECTED GALAXIES IN THE COSMOS FIELD

The Velocity Field of the Local Universe from Measurements of Type Ia Supernovae

Self-regulated growth of supermassive black holes by a dual jet-heating active galactic nucleus feedback mechanism: methods, tests and implications for cosmological simulations

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s⁻¹ Mpc⁻¹ Uncertainty from the Hubble Space Telescope and the SH0ES Team

Star formation, metallicity and dust properties derived from the StromloAPM galaxy survey spectra

THE 2MASS REDSHIFT SURVEY—DESCRIPTION AND DATA RELEASE

Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

The DEEP2 Galaxy Redshift Survey: Spectral classification of galaxies at z~1

Weak gravitational lensing

Deriving a multivariate αCO conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations

Simulating galaxy formation with the IllustrisTNG model

Dusty star-forming galaxies at high redshift

GMRT radio halo survey in galaxy clusters atz= 0.2–0.4

The VVDS-VLA deep field

The VIRMOS deep imaging survey

Spectral properties and origin of the radio halo in A3562

Radio-optically selected clusters of galaxies

Optically-selected clusters at 0.8 $\la$ $\mathsfsl z$ $\la$ 1.3 in the EIS clustersurvey

The VIMOS VLT Deep Survey

The ESO-Sculptor Survey: Luminosity functions of galaxies per spectral type at redshifts $0.1{-}0.5$

Shock acceleration as origin of the radio relic in A 521?

GMRT radio halo survey in galaxy clusters atz= 0.2–0.4

A study of the core of the Shapley Concentration - VI. Spectral properties of galaxies^★

Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model

The ESO-Sculptor Survey: Evolution of late-type galaxies \nat redshifts 0.1–0.5

COSMIC EVOLUTION OF RADIO SELECTED ACTIVE GALACTIC NUCLEI IN THE COSMOS FIELD

A study of the core of the Shapley Concentration -- V. The A3528 complex: a young merger event?

A study of the core of the Shapley Concentration - I. The sample