C. Wu

Supernova rates from the Southern inTermediate Redshift ESO Supernova Search (STRESS)

The bulk of the cosmic infrared background resolved by ISOCAM

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

Mergers and Mass Accretion Rates in Galaxy Assembly: The Millennium Simulation Compared to Observations ofz≈ 2 Galaxies

The Chandra Deep Field–South: Optical Spectroscopy. I.

A high abundance of massive galaxies 3–6 billion years after the Big Bang

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

NUCLEAR ACTIVITY IS MORE PREVALENT IN STAR-FORMING GALAXIES

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

A Significant Population of Red, Near-Infrared-selected High-Redshift Galaxies

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

A Large Sample of Spectroscopic Redshifts in the ACS-GOODS Region of the Hubble Deep Field North

Kinematics of Galaxies in the Hubble Deep Field–South: Discovery of a Very Massive Spiral Galaxy atz= 0.6

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

Probing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts

Millimeter Observations of Obscured Spitzer 24 μm Sources

Differential Galaxy Evolution in Cluster and Field Galaxies at z=0.3

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

Differential Galaxy Evolution in Cluster and Field 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 $z\approx 0.3$ \end{document}

High‐Redshift Supernova Rates

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

Measuring the Average Evolution of Luminous Galaxies atz< 3: The Rest‐Frame Optical Luminosity Density, Spectral Energy Distribution, and Stellar Mass Density

The Canada-France Redshift Survey: The Luminosity Density and Star Formation History of the Universe to [ITAL]z[/ITAL] ∼ 1

The Dust Content and Opacity of Actively Star‐forming Galaxies

The Chandra Deep Field–South: The 1 Million Second Exposure

RELATION BETWEEN STELLAR MASS AND STAR-FORMATION ACTIVITY IN GALAXIES

Potential Measurement of the Luminosity Function of 158 Micron [Cii] at High Redshifts: A Test of Galaxy Formation Models

THE MID-INFRARED EMISSION OF NARROW-LINE ACTIVE GALACTIC NUCLEI: STAR FORMATION, NUCLEAR ACTIVITY, AND TWO POPULATIONS REVEALED BYWISE

New Results from the X‐Ray and Optical Survey of the Chandra Deep Field–South: The 300 Kilosecond Exposure. II.

The Nature of Compact Galaxies in the Hubble Deep Field. I. Global Properties

Statistical Properties of Bright Galaxies in the Sloan Digital Sky Survey Photometric System

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

The Canada-UK Deep Submillimeter Survey. IV. The Survey of the 14 Hour Field

Will Jets Identify the Progenitors of Type I[CLC]a[/CLC] Supernovae?

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

The [Cii] 158 Micron Line Deficit in Ultraluminous Infrared Galaxies Revisited

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

Ultraluminous Infrared Galaxies: QSOs in Formation?

A survey of molecular gas in luminous sub-millimetre galaxies

Properties of Millimeter Galaxies: Constraints fromK‐Band Blank Fields

Confirming a population of hot-dust dominated, star-forming, ultraluminous galaxies at high redshift

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

Spectroscopic Atlas of the Central \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 $24^{\prime \prime }\times 20^{\prime \prime }$ \end{document} of the Seyfert 2 Galaxy NGC 1068

Stellar population synthesis at the resolution of 2003

Hubble Space TelescopeImaging in the Chandra Deep Field–South. I. Multiple Active Galactic Nucleus Populations

The Photometric Performance and Calibration of theHubble Space TelescopeAdvanced Camera for Surveys

A Massive Disk Galaxy at [CLC][ITAL]z[/ITAL][/CLC] = 1.34

The UKIRT Infrared Deep Sky Survey ZY JHK photometric system: passbands and synthetic colours

A Close Look at Star Formation around Active Galactic Nuclei

AEGIS: The Color-Magnitude Relation for X-Ray-selected Active Galactic Nuclei

The heating of dust by old stellar populations in the bulge of M31

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

The [ITAL]CHANDRA[/ITAL][ITAL]Chandra[/ITAL] Deep Survey of the Hubble Deep Field North Area. IV. An Ultradeep Image of the HDF-N

A Classic Type 2 QSO

The Evolution of the Global Stellar Mass Density at 0 < z < 3

A New Photometric Technique for the Joint Selection of Star‐forming and Passive Galaxies at 1.4 ≲z≲ 2.5

Very Large Telescope–ISAAC Near-Infrared Spectroscopy of [ITAL]ISO[/ITAL]-selected Hubble Deep Field South Galaxies

HIGH-REDSHIFT STAR-FORMING GALAXIES: ANGULAR MOMENTUM AND BARYON FRACTION, TURBULENT PRESSURE EFFECTS, AND THE ORIGIN OF TURBULENCE

Multiwavelength Study of Massive Galaxies atz∼2. I. Star Formation and Galaxy Growth

THE HALO MERGER RATE IN THE MILLENNIUM SIMULATION AND IMPLICATIONS FOR OBSERVED GALAXY MERGER FRACTIONS

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

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

The farthest known supernova: Support for an accelerating universe and a glimpse of the \nepoch of deceleration

High‐Resolution Millimeter Imaging of Submillimeter Galaxies

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters

The Stellar Populations and Evolution of Lyman Break Galaxies

UV-CONTINUUM SLOPES ATz∼ 4-7 FROM THE HUDF09+ERS+CANDELS OBSERVATIONS: DISCOVERY OF A WELL-DEFINED UV COLOR-MAGNITUDE RELATIONSHIP FORz⩾ 4 STAR-FORMING GALAXIES

Evolution of the Luminosity Function, Star Formation Rate, Morphology, and Size of Star‐forming Galaxies Selected at Rest‐Frame 1500 and 2800 A

Close Pairs of Field Galaxies in the CNOC1 Redshift Survey

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

A New Catalog of Photometric Redshifts in the Hubble Deep Field

MOST SUBMILLIMETER GALAXIES ARE MAJOR MERGERS

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

Identification of the Red Supergiant Progenitor of Supernova 2005cs: Do the Progenitors of Type II‐P Supernovae Have Low Mass?

Star formation histories of early-type galaxies at z = 1.2 in cluster\nand field environments

THE RISE OF MASSIVE RED GALAXIES: THE COLOR-MAGNITUDE AND COLOR-STELLAR MASS DIAGRAMS FORz_phot≲ 2 FROM THE MULTIWAVELENGTH SURVEY BY YALE-CHILE

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

Galaxy Mergers atz ≳ 1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive Galaxies1

Hubble Space TelescopeImaging in the Chandra Deep Field–South. II. WFPC2 Observations of an X‐Ray Flux–limited Sample from the 1 Million Second Chandra Catalog

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

An interferometric CO survey of luminous submillimetre galaxies

SINFONI Integral Field Spectroscopy ofz∼ 2 UV‐selected Galaxies: Rotation Curves and Dynamical Evolution

THE GROWTH OF DARK MATTER HALOS: EVIDENCE FOR SIGNIFICANT SMOOTH ACCRETION

SHORT-LIVED STAR-FORMING GIANT CLUMPS IN COSMOLOGICAL SIMULATIONS OFz≈ 2 DISKS

TheCOBEDiffuse Infrared Background Experiment Search for the Cosmic Infrared Background. IV. Cosmological Implications

Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang

Supernovae in the Subaru Deep Field: an initial sample and Type Ia rate out to redshift 1.6

The Microjansky Radio Galaxy Population

Colors and magnitudes predicted for high redshift galaxies