Daniel D. Kelson

Weak lensing by high-redshift clusters of galaxies

Results of the Mount Stromlo Abell cluster supernova search

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

THE RADIAL DISTRIBUTION OF STAR FORMATION IN GALAXIES AT z ∼ 1 FROM THE 3D-HST SURVEY

Energy input from quasars regulates the growth and activity of black holes and their host galaxies

Optical and Near‐Infrared Photometry of the Type Ia Supernova 2000E in NGC 6951

Simulations of the formation, evolution and clustering of galaxies and quasars

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

Properties of galaxies reproduced by a hydrodynamic simulation

A Direct Measurement of Major Galaxy Mergers atz3

THE INITIAL-FINAL MASS RELATION AMONG WHITE DWARFS IN WIDE BINARIES

Host Dynamics and Origin of Palomar‐Green QSOs

Red mergers and the assembly of massive elliptical galaxies: the fundamental plane and its projections

Metallicity Effects on Dust Properties in Starbursting Galaxies

The Galactic Center massive black hole and nuclear star cluster

NUCLEAR ACTIVITY IS MORE PREVALENT IN STAR-FORMING GALAXIES

Luminosity Function Constraints on the Evolution of Massive Red Galaxies sincez∼ 0.9

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

Do Type Ia supernovae prove Λ>0?

Hubble Space TelescopeWeak‐Lensing Study of thez=0.83 Cluster MS 1054−03

Cosmological Implications from Observations of Type Ia Supernovae

Cepheid Distances to SNe Ia Host Galaxies Based on a Revised Photometric Zero Point of theHSTWFPC2 and New PL Relations and Metallicity Corrections

The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter

Cepheid Calibrations from theHubble Space Telescopeof the Luminosity of Two Recent Type Ia Supernovae and a Redetermination of the Hubble Constant

A DeepHubble Space Telescope H‐Band Imaging Survey of Massive Gas‐rich Mergers

Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation

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

PACS Evolutionary Probe (PEP) - A Herschel key program

Galaxy merging, the fundamental plane of elliptical galaxies and the MBH --  0 relation

Weak Lensing Analysis of Cl 1358+62 UsingHubble Space TelescopeObservations

The Redshift Evolution of Wet, Dry, and Mixed Galaxy Mergers from Close Galaxy Pairs in the DEEP2 Galaxy Redshift Survey

The age-metallicity dependence for white dwarf stars

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 Distance to SN 1999em in NGC 1637 from the Expanding Photosphere Method

Stellar Orbits around the Galactic Center Black Hole

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

The distance to Supernova 1998aq in NGC 3982

Cepheid Calibration of the Peak Brightness of Type Ia Supernovae. XI. SN 1998aq in NGC 3982

Evidence for a Long‐standing Top‐heavy Initial Mass Function in the Central Parsec of the Galaxy

Galaxy Environments over Cosmic Time: The Non-evolving Radial Galaxy Distributions around Massive Galaxies since <i>z</i> = 1.6

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

Dynamical Family Properties and Dark Halo Scaling Relations of Giant Elliptical Galaxies

EQUAL- AND UNEQUAL-MASS MERGERS OF DISK AND ELLIPTICAL GALAXIES WITH BLACK HOLES

Spectral models for solar-scaled and α-enhanced stellar populations

The Cepheid Distance to NGC 1637: A Direct Test of the Expanding Photosphere Method Distance to SN 1999em

The Star‐forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC 3227

The Cepheid Distance to NGC 5236 (M83) with the ESO Very Large Telescope

REVISITING THE ABUNDANCE GRADIENT IN THE MASER HOST GALAXY NGC 4258

Hot stars in old stellar populations: a continuing need for intermediate ages

A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies

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

Redshift Evolution of the Merger Fraction of Galaxies in Cold Dark Matter Cosmologies

The initialfinal mass relationship of white dwarfs revisited: effect on the luminosity function and mass distribution

Ultraluminous Infrared Galaxies: QSOs in Formation?

Cepheid Calibration of the Peak Brightness of Type Ia Supernovae. VIII. SN 1990N in NGC 4639

NICMOS observations of extragalactic Cepheids. I. Photometry database and a test of the standard extinction law

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

Dynamical Properties of Ultraluminous Infrared Galaxies. I. Mass Ratio Conditions for ULIRG Activity in Interacting Pairs

The Hubble Constant: A Summary of theHubble Space TelescopeProgram for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids

The Evolving Luminosity Function of Red Galaxies

The Evolution of Field Early-Type Galaxies to [CLC][ITAL]z[/ITAL][/CLC] ∼ 0.7

Distances to Galaxies from the Correlation between Luminosities and Line Widths. III. Cluster Template and Global Measurement ofH₀

Star Formation Thresholds in Galactic Disks

Mass limits for the progenitor star of supernova 2001du and other Type II-P supernovae

Photometric Stellar Variability in the Galactic Center

THE MASSES OF POPULATION II WHITE DWARFS

The Nature of the Variable Galactic Center Source IRS 16SW

The Discovery of Cepheids and a Distance to NGC 5128

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

Supernovae in deep Hubble Space Telescope galaxy cluster fields: cluster rates and field counts

Chemistry and Star Formation in the Host Galaxies of Type Ia Supernovae

Uniformity of (V−Near‐Infrared) Color Evolution of Type Ia Supernovae and Implications for Host Galaxy Extinction Determination

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

A unified model for AGN feedback in cosmological simulations of structure formation

The Munich Near‐Infrared Cluster Survey (MUNICS). VI. The Stellar Masses ofK‐Band–selected Field Galaxies toz ∼ 1.2

A REDETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEFROM A DIFFERENTIAL DISTANCE LADDER

Detection of weak gravitational lensing distortions of distant galaxies by cosmic dark matter at large scales

TheIRASRevised Bright Galaxy Sample

Planetary Nebulae as Standard Candles. XI. Application to Spiral Galaxies

The Mass Assembly History of Field Galaxies: Detection of an Evolving Mass Limit for Star‐Forming Galaxies

THE RISE AND FALL OF TYPE Ia SUPERNOVA LIGHT CURVES IN THE SDSS-II SUPERNOVA SURVEY

A DEEPHUBBLE SPACE TELESCOPEH-BAND IMAGING SURVEY OF MASSIVE GAS-RICH MERGERS. II. THE QUEST QSOs

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

Dry Mergers in GEMS: The Dynamical Evolution of Massive Early‐Type Galaxies

Nearly 5000 Distant Early‐Type Galaxies in COMBO‐17: A Red Sequence and Its Evolution sincez ∼ 1

GCIRS 16SW: A Massive Eclipsing Binary in the Galactic Center

The Adequacy of Stellar Evolution Models for the Interpretation of the Color-Magnitude Diagrams of Resolved Stellar Populations

MOST SUBMILLIMETER GALAXIES ARE MAJOR MERGERS

CEPHEID CALIBRATIONS OF MODERN TYPE Ia SUPERNOVAE: IMPLICATIONS FOR THE HUBBLE CONSTANT

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

Comparison of Distances from RR Lyrae Stars, the Tip of the Red Giant Branch, and Classical Cepheids

The Relationship between Gas Content and Star Formation in Molecule‐rich Spiral Galaxies

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

A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEAND WIDE FIELD CAMERA 3

The Evolution of Early‐Type Red Galaxies with the GEMS Survey: Luminosity‐Size and Stellar Mass–Size Relations Sincez = 1

DISSECTING THE RED SEQUENCE. I. STAR-FORMATION HISTORIES OF QUIESCENT GALAXIES: THE COLOR-MAGNITUDE VERSUS THE COLOR-σ RELATION

Improved Distances to Type Ia Supernovae with Multicolor Light‐Curve Shapes: MLCS2k2

Stellar Populations and Kinematics of Red Galaxies atz> 2: Implications for the Formation of Massive Galaxies

First results from the IllustrisTNG simulations: the galaxy colour bimodality

MeanJHKMagnitudes of Fundamental‐Mode Cepheids from Single‐Epoch Observations

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

THE GALAXY CONTENT OF SDSS CLUSTERS AND GROUPS

Weak gravitational lensing

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

Population Synthesis in the Blue. IV. Accurate Model Predictions for Lick Indices and UBV Colors in Single Stellar Populations

The Cepheid Period‐Luminosity Relation in the Large Magellanic Cloud

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

The Growth of Luminous Red Galaxies by Merging

Reconciliation of the Surface Brightness Fluctuation and Type Ia Supernova Distance Scales

Probing The Lower Mass Limit For Supernova Progenitors And The High-Mass End Of The Initial-Final Mass Relation From White Dwarfs In The Open Cluster M35 (NGC 2168)

The Fundamental Planes of E+A galaxies and GALEX UV-excess early-type galaxies: revealing their intimate connection

Supernova Type Ia Luminosities, Their Dependence on Second Parameters, and the Value ofH₀

Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Spectroscopic Confirmation of Multiple Red Galaxy-Galaxy Mergers in MS 1054-03 ( z = 0.83)

The Velocity Dispersion of MS 1054−03: A Massive Galaxy Cluster at High Redshift

Line Strengths in Early‐Type Cluster Galaxies atz= 0.33: Implications for α/Fe, Nitrogen, and the Histories of E/S0s

Field E+A Galaxies at Intermediate Redshifts (0.3 <z< 1)

TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XXVI. The Calibration of Population II Secondary Distance Indicators and the Value of the Hubble Constant

The Extragalactic Distance Scale Key Project. III. The Discovery of Cepheids and a New Distance to M101 Using the Hubble Space Telescope

The Evolution of Early‐Type Galaxies in Distant Clusters. III. \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 $M/ L_{V}$ \end{document} Ratios in the \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 $z=0.33$ \end{document} Cluster Cl 1358+62

THE STAR-FORMATION-RATE-DENSITY RELATION AT 0.6 <z< 0.9 AND THE ROLE OF STAR-FORMING GALAXIES $^,$ $^,$ $^,$ $^,$

Stellar Evolution in NGC 6791: Mass Loss on the Red Giant Branch and the Formation of Low‐Mass White Dwarfs

The Detailed Fundamental Plane of Two High‐Redshift Clusters: MS 2053−04 atz = 0.58 and MS 1054−03 atz = 0.83

The Color‐Magnitude Relation in CL 1358+62 atz= 0.33: Evidence for Significant Evolution in the S0 Population

A Database of Cepheid Distance Moduli and Tip of the Red Giant Branch, Globular Cluster Luminosity Function, Planetary Nebula Luminosity Function, and Surface Brightness Fluctuation Data Useful for Distance Determinations

Spectroscopic Confirmation of a Large Population of Active Galactic Nuclei in Clusters of Galaxies

The Evolution of Early‐Type Galaxies in Distant Clusters. II. Internal Kinematics of 55 Galaxies in the \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 $z=0.33$ \end{document} Cluster Cl 1358+62

TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XXV. A Recalibration of Cepheid Distances to Type Ia Supernovae and the Value of the Hubble Constant

Determination of the Dark Matter Profile of A2199 from Integrated Starlight

The Evolution of Early‐Type Galaxies in Distant Clusters. I. Surface Photometry and Structural Parameters for 53 Galaxies in the \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 $z=0.33$ \end{document} Cluster Cl 1358+62

Errata: TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XXVIII. Combining the Constraints on the Hubble Constant

TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XXII. The Discovery of Cepheids in NGC 1326A

The Evolution of the Field and Cluster Morphology‐Density Relation for Mass‐Selected Samples of Galaxies

A High Merger Fraction in the Rich Cluster MS 1054−03 at [CLC][ITAL]z[/ITAL][/CLC] = 0.83: Direct Evidence for Hierarchical Formation of Massive Galaxies

TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XIX. The Discovery of Cepheids in and a New Distance to NGC 3198

Hubble Space TelescopePhotometry and Keck Spectroscopy of the Rich Cluster MS 1054−03: Morphologies, Butcher‐Oemler Effect, and the Color‐Magnitude Relation atz= 0.83

Mass Selection and the Evolution of the Morphology‐Density Relation fromz= 0.8 to 0