B. Milliard

NGC 6240: merger-induced star formation and gas dynamics

How do galaxies acquire their mass?

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

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

VLT narrow-band photometry in the Lyman continuum of two galaxies atz$\mathsf{\sim3}$

A luminous quasar at a redshift of z = 7.085

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

Spectroscopic confirmation of a galaxy at redshift z = 8.6

Properties of galaxies reproduced by a hydrodynamic simulation

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

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

Dust-obscured star formation and AGN fuelling in hierarchical models of galaxy evolution

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*

Ultraluminous Infrared Mergers: Elliptical Galaxies in Formation?

SPIFFI Observations of the Starburst SMM J14011+0252:Already Old, Fat, and Rich by z =2.565

COJ= 1-0 SPECTROSCOPY OF FOUR SUBMILLIMETER GALAXIES WITH THE ZPECTROMETER ON THE GREEN BANK TELESCOPE

AHubble Space TelescopeSearch for Lyman Continuum Emission from Galaxies at 1.1 <z< 1.4

The Canada–United Kingdom Deep Submillimeter Survey. II. First Identifications, Redshifts, and Implications for Galaxy Evolution

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

Millimeter Observations of Obscured Spitzer 24 μm Sources

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

Molecular gas in submillimetre-faint, star-forming ultraluminous galaxies at z > 1

High‐Redshift Supernova Rates

Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

The Dust Content and Opacity of Actively Star‐forming Galaxies

The Epochs of Early‐Type Galaxy Formation as a Function of Environment

Rotational support of giant clumps in high-z disc galaxies

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

Chemical abundances in a UV-selected sample of galaxies

Interferometric Observations of Powerful CO Emission from Three Submillimeter Galaxies at z =2.39, 2.51, and 3.35

The evolution of stellar mass and the implied star formation history

Environmental effects on satellite galaxies: the link between concentration, size and colour profile

Evolution of the atomic and molecular gas content of galaxies

The Faint Counterparts of MAMBO Millimeter Sources near the New Technology Telescope Deep Field

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

THE IMPACT OF INTERACTIONS, BARS, BULGES, AND ACTIVE GALACTIC NUCLEI ON STAR FORMATION EFFICIENCY IN LOCAL MASSIVE GALAXIES

Deep Very Large TelescopeV‐Band Imaging of the Field of az= 10 Candidate Galaxy: Below the Lyman Limit?

Ultraluminous Infrared Galaxies: QSOs in Formation?

Mission: impossible (escape from the Lyman limit)

In the beginning: the first sources of light and the reionization of the universe

On the Evolution of Star‐forming Galaxies

A survey of molecular gas in luminous sub-millimetre galaxies

Inclination- and dust-corrected galaxy parameters: bulge-to-disc ratios and size-luminosity relations

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

Properties of Millimeter Galaxies: Constraints fromK‐Band Blank Fields

A BACKWARD EVOLUTION MODEL FOR INFRARED SURVEYS: THE ROLE OF AGN– AND COLOR–L_TIRDISTRIBUTIONS

The Incidence of Highly Obscured Star‐forming Regions in SINGS Galaxies

SparsePak: A Formatted Fiber Field Unit for the WIYN Telescope Bench Spectrograph. I. Design, Construction, and Calibration

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

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

The Origin of the Mass‐Metallicity Relation: Insights from 53,000 Star‐forming Galaxies in the Sloan Digital Sky Survey

Spectrophotometry of Galaxies in the Virgo Cluster. I. The Star Formation History

A Classic Type 2 QSO

On the Determination of Star Formation Rates in Evolving Galaxy Populations

Radio Properties of Infrared‐Selected Galaxies in theIRAS2 Jy Sample

Is There a Missing Galaxy Problem at High Redshift?

The Evolution of Dust Opacity in Galaxies

Modelling feedback from stars and black holes in galaxy mergers

The Luminosity Function of Morphologically Classified Galaxies in the Sloan Digital Sky Survey

An analytical model for the history of cosmic star formation

The Sloan Digital Sky Survey: The Cosmic Spectrum and Star Formation History

Galaxy number counts -- V. Ultradeep counts: the Herschel and Hubble Deep Fields

Ultraviolet through Infrared Spectral Energy Distributions from 1000 SDSS Galaxies: Dust Attenuation

Infrared Luminosity Functions from the Chandra Deep Field–South: TheSpitzerView on the History of Dusty Star Formation at 0 ≲z≲ 1

Caltech Faint Galaxy Redshift Survey. XVI. The Luminosity Function for Galaxies in the Region of the Hubble Deep Field–North toz = 1.5

The nature of faint submillimetre-selected galaxies

Intense Star Formation and Feedback at High Redshift: Spatially Resolved Properties of thez= 2.6 Submillimeter Galaxy SMM J14011+0252

Lyman Break Galaxies at z>4 and the Evolution of the UV Luminosity Density at High Redshift

Submillimeter Galaxies atz∼ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO‐H₂Conversion Factor

The history of star formation in a   cold dark matter universe

The ExtendedHSTSupernova Survey: The Rate of SNe Ia atz> 1.4 Remains Low

Ultraviolet dust attenuation in star-forming galaxies – II. Calibrating the A(UV) versus L_TIR/L_UVrelation

High‐Redshift Supernovae in the Hubble Deep Field

High‐Resolution Millimeter Imaging of Submillimeter Galaxies

The nature of high-redshift galaxies

How many supernovae are we missing at high redshift?

The Shortest-Known–Period Star Orbiting Our Galaxy’s Supermassive Black Hole

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

Interferometric CO Observations of Submillimeter‐faint, Radio‐selected Starburst Galaxies atz∼ 2

MOST SUBMILLIMETER GALAXIES ARE MAJOR MERGERS

Lyman‐Break 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 $z\gtrsim 4$ \end{document} and the Evolution of the Ultraviolet Luminosity Density at High Redshift

SpitzerView on the Evolution of Star‐forming Galaxies fromz= 0 toz∼ 3

Toward a Resolution of the Discrepancy between Different Estimators of Star Formation Rate

The Magnification of SN 1997[CLC]ff[/CLC], the Farthest Known Supernova

A Comparison of Independent Star Formation Diagnostics for an Ultraviolet‐selected Sample of Nearby Galaxies

Global Star Formation History: A Local Group Perspective

1.65 Micron ([ITAL]H[/ITAL] Band) Surface Photometry of Galaxies. VI. The History of Star Formation in Normal Late-Type Galaxies

Spatially Resolved Millimeter Interferometry of SMM J02399−0136: AVery Massive Galaxy atz= 2.8

Measurement of the star formation rate from Ha in field galaxies at z=1

A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS★

Mapping the Evolution of High-Redshift Dusty Galaxies with Submillimeter Observations of a Radio-selected Sample

An interferometric CO survey of luminous submillimetre galaxies

The history of star formation in dusty galaxies

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

Cosmological smoothed particle hydrodynamics simulations: a hybrid multiphase model for star formation

The Universe Was Reionized Twice

Numerical simulations of the cosmic star formation history

Star Formation in the Milky Way and Nearby Galaxies

Constraints on the Lyman continuum radiation from galaxies: First results with FUSE on Mrk 54

The ESO UVES advanced data products quasar sample

An ultraviolet-selected galaxy redshift survey: new estimates of the local star formation rate

A 40-cm UV (2000 Å) balloon-borne imaging telescope: Results and current work

Two‐dimensional Analytical Modeling of Distortion and Sky Background in Multifiber Spectrographs: The Case of the Norris Spectrograph at Palomar Mountain

Far infrared and Ultraviolet emissions of individual galaxies at z=0: selection effects on the estimate of the dust extinction

The radial extinction profiles of late-type galaxies