C. Ledoux

V4332 Sagittarii: a circumstellar disc obscuring the main object

A non-LTE study of neutral and singly-ionized calcium in late-type stars

The non-LTE line formation of neutral carbon in late-type stars

Sulphur and zinc abundances in Galactic stars and damped Lyαsystems

A non-LTE study of neutral and singly-ionized iron line spectra in 1D models of the Sun and selected late-type stars

The metal content of bulge field stars from FLAMES-GIRAFFE spectra

Single star progenitors of long gamma-ray bursts

Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly

Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti

The ESO UVES advanced data products quasar sample

Improved stellar parameters of CoRoT-7

Sulphur abundances from the S i near-infrared triplet at 1045 nm

The cosmic microwave background radiation temperature at $\vec{z}_\mathsf{abs} = \mathsf{3.025}$ toward QSO 0347–3819

Probing the time-variation of the fine-structure constant: Resultsbased on Si IV doublets from a UVES sample

High-resolution optical spectroscopy of V838 Monocerotis in 2009

Oxygen, sodium, magnesium, and aluminium as tracers of the galactic bulge formation

A grid of MARCS model atmospheres for late-type stars

Distant radio galaxies and their environments

The Confrontation between General Relativity and Experiment

The Confrontation between General Relativity and Experiment

The IllustrisTNG simulations: public data release

Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants

Cold streams in early massive hot haloes as the main mode of galaxy formation

A test of general relativity using radio links with the Cassini spacecraft

Search for a Variation of the Fine Structure Constant around the Supermassive Black Hole in Our Galactic Center

Properties of galaxies reproduced by a hydrodynamic simulation

Limits on Variations in Fundamental Constants from 21-cm and Ultraviolet Quasar Absorption Lines

Cosmology at low frequencies: The 21cm transition and the high-redshift Universe

PROPER MOTIONS OF THE ARCHES CLUSTER WITH KECK LASER GUIDE STAR ADAPTIVE OPTICS: THE FIRST KINEMATIC MASS MEASUREMENT OF THE ARCHES

First results from the IllustrisTNG simulations: matter and galaxy clustering

The impact of different physical processes on the statistics of Lyman-limit and damped Lyman α absorbers

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 cosmological constant and dark energy

Optical colours and spectral indices of z = 0.1 eagle galaxies with the 3D dust radiative transfer code skirt

Observed versus predicted stellar flux distributions of solar-type stars

Damped Lyman α absorbers as a probe of stellar feedback

DETECTION OF GALACTIC CENTER SOURCE G2 AT 3.8 μm DURING PERIAPSE PASSAGE

The ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass Density

On the evolution of the H i column density distribution in cosmological simulations

A SINFONI integral field spectroscopy survey for galaxy counterparts to damped Lyman α systems - I. New detections and limits for intervening and associated absorbers★

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION

Understanding the H₂/H i ratio in galaxies

Accurate spectroscopic parameters of WASP planet host stars★

THE Pan-STARRS1 PHOTOMETRIC SYSTEM

The Fate of Binaries in the Galactic Center: The Mundane and the Exotic

A model for the metallicity evolution of damped Lyman �� systems

High-Dispersion Spectra Collection of Nearby F–K Stars at Okayama Astrophysical Observatory: A Basis for Spectroscopic Abundance Standards

EVIDENCE FOR A MASSIVE NEUTRON STAR FROM A RADIAL-VELOCITY STUDY OF THE COMPANION TO THE BLACK-WIDOW PULSAR PSR B1957+20

Rotational support of giant clumps in high-z disc galaxies

Lyman-α Emitters and Lyman-Break Galaxies at z = 3–6 in Cosmological SPH Simulations

The Progenitor Stars of Gamma‐Ray Bursts

Observational Evidence of Active Galactic Nuclei Feedback

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

The Lyman α emission of high-z damped Lyman α systems

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

The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations

A survey of molecular gas in luminous sub-millimetre galaxies

MEASURING REDDENING WITH SLOAN DIGITAL SKY SURVEY STELLAR SPECTRA AND RECALIBRATING SFD

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

Directly imaging damped Lyman α galaxies at z > 2 - I. Methodology and first results★

The Constancy of the Constants of Nature: Updates

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

Damped Lyman α systems in galaxy formation simulations

Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate

Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood

THE NATURE OF DAMPED Lyα SYSTEMS AND THEIR HOSTS IN THE STANDARD COLD DARK MATTER UNIVERSE

PHIBSS: exploring the dependence of the CO–H2 conversion factor on total mass surface density at z<1.5

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

Dust-reddening and gravitational lensing of SDSS QSOs due to foreground damped Lymanαsystems

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

Precision measures of the primordial abundance of deuterium

Merging binaries in the Galactic Center: the eccentric Kozai–Lidov mechanism with stellar evolution

f(R,T)gravity

The physics of gamma-ray bursts

Damped Lyα Systems atz < 1.65: The Expanded Sloan Digital Sky SurveyHubble Space TelescopeSample

'Ultimate' Information Content in Solar and Stellar Spectra: Photospheric line asymmetries and wavelength shifts

The Galaxy in Context: Structural, Kinematic, and Integrated Properties

QUASARS PROBING QUASARS. III. NEW CLUES TO FEEDBACK, QUENCHING, AND THE PHYSICS OF MASSIVE GALAXY FORMATION

Deuterium abundance in the most metal-poor damped Lyman alpha system: converging on Ω_b,0h²

Implications for Cosmic Reionization from the Optical Afterglow Spectrum of the Gamma-Ray Burst 050904 at z = 6.3

THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS

The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects in Dark Energy Surveys from SNe Ia atz > 2

Searching for Low Surface Brightness Galaxies in the Hubble Ultra Deep Field: Implications for the Star Formation Efficiency in Neutral Gas 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 $z\sim 3$ \end{document}

A combined analysis of 3D weak lensing, Lyman-α forest and WMAP year three data

THE PROPAGATION OF UNCERTAINTIES IN STELLAR POPULATION SYNTHESIS MODELING. I. THE RELEVANCE OF UNCERTAIN ASPECTS OF STELLAR EVOLUTION AND THE INITIAL MASS FUNCTION TO THE DERIVED PHYSICAL PROPERTIES OF GALAXIES

THE STRUCTURE OF GRAVITATIONALLY UNSTABLE GAS-RICH DISK GALAXIES

MOST SUBMILLIMETER GALAXIES ARE MAJOR MERGERS

Gravity-driven Lyα blobs from cold streams into galaxies

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS

Modified gravity with negative and positive powers of curvature: Unification of inflation and cosmic acceleration

THE PROPAGATION OF UNCERTAINTIES IN STELLAR POPULATION SYNTHESIS MODELING. II. THE CHALLENGE OF COMPARING GALAXY EVOLUTION MODELS TO OBSERVATIONS

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations

mufasa: the assembly of the red sequence

THE STAR FORMATION HISTORY OF THE MILKY WAY'S NUCLEAR STAR CLUSTER

STECMAP: STEllar Content from high-resolution galactic spectra via Maximum A Posteriori

Galactic winds in cosmological simulations of the circumgalactic medium

CODATA recommended values of the fundamental physical constants: 2010

The Chemical Composition of the Sun

THE CHEMICAL EVOLUTION OF STAR-FORMING GALAXIES OVER THE LAST 11 BILLION YEARS

Hubble Space TelescopeObservations of Element Abundances in Low‐Redshift Damped Lyα Galaxies and Implications for the Global Metallicity‐Redshift Relation

First results from the IllustrisTNG simulations: the galaxy colour bimodality

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

Evolution of the fine-structure constant in the non-linear regime

MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS

A DEFINITIVE SURVEY FOR LYMAN LIMIT SYSTEMS AT z ∼ 3.5 WITH THE SLOAN DIGITAL SKY SURVEY

Probing Post-Newtonian Physics near the Galactic Black Hole with Stellar Redshift Measurements

DAMPED LYα SYSTEMS

Dust formation in Milky Way-like galaxies

Cosmic evolution of the atomic and molecular gas contents of galaxies

Simulating galaxy formation with the IllustrisTNG model

An improved measurement of the flux distribution of the Ly  forest in QSO absorption spectra: the effect of continuum fitting, metal contamination and noise properties

The large programme "Cosmic Evolution of the IGM"

Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II – Data Release 7

C IV absorption in damped and sub-damped Lyman-α systems

Dust-to-metal ratios in damped Lyman-αabsorbers

Excitation mechanisms in newly discovered H₂-bearing damped Lyman-αclouds: systems with low molecular fractions

Kinematics and star formation activity in the z$\mathsf{_{abs}}$ = 2.03954damped Lyman-$\mathsf{\alpha}$ system towards PKS 0458–020

On the Lyα emission from gamma-ray burst host galaxies: Evidence for low metallicities

Physical conditions in high-redshift GRB-DLA absorbers observed with VLT/UVES: implications for molecular hydrogen searches

HD molecules at high redshift

The most metal-poor damped Lyman $\mathsf{\alpha}$ system atz$\mathsf{<3}$: constraints on early nucleosynthesis

A Lyman-α blob in the GOODSSouth field: evidence for cold accretion onto a dark matter halo

Metal-enriched plasma in protogalactic halos

Hot halos around high redshift protogalaxies

Velocity-metallicity correlation for high-zDLA galaxies: evidence of a mass-metallicity relation?

The sub-damped Ly α system toward HE 0001-2340: galaxy formation at z ≈ 2

A multi-wavelength study ofz= 3.15 Lyman-$\mathsf{\alpha}$ emitters in the GOODS South Field

High-ion absorption in the proximate damped Ly-αsystem toward Q0841+129

Detection of molecular hydrogen in a near Solar-metallicity dampedLyman-α system at $z_\mathsf{abs}$ ≈ 2 towardQ 0551-366

Uncovering strong MgII absorbing galaxies

Time dependence of the proton-to-electron mass ratio

The cosmic microwave background radiation temperature at a redshift of 2.34

Multiphase Plasma in Sub-Damped Lyα Systems: A Hidden Metal Reservoir

Molecular hydrogen atz_abs=1.973 toward Q 0013−004: dust depletion pattern in damped Lymanαsystems

The UVES Paranal Observatory Project: A Library of High- Resolution Spectra of Stars across the Hertzsprung-Russell Diagram

Mass–metallicity relation from z = 5 to the present: evidence for a transition in the mode of galaxy growth at z = 2.6 due to the end of sustained primordial gas infall

Dust-to-metal ratios in damped Lyman-α absorbers Fresh clues to the origins of dust and optical extinction towards γ-ray bursts

The VLT-UVES survey for molecular hydrogen in high-redshift damped Lyman α systems: physical conditions in the neutral gas

The Very Large Telescope Ultraviolet and Visible Echelle Spectrograph survey for molecular hydrogen in high-redshift damped Lyman   systems

C IV absorption in damped and sub-damped Lyman-alpha systems: correlations with metallicity and implications for galactic winds at z~2-3

HD molecules at high redshift: the absorption system atz = 2.3377towards Q 1232 + 082

Galaxy counterparts of metal-rich damped Lyα absorbers - I. The case of the z= 2.35 DLA towards Q 2222−0946★

A new constraint on the time dependence of the proton-to-electron mass ratio

DUST EXTINCTION IN HIGH-zGALAXIES WITH GAMMA-RAY BURST AFTERGLOW SPECTROSCOPY: THE 2175 Å FEATURE ATz= 2.45