H. E. Jørgensen

The Luminous Type Ic Supernova 1992ar at z = 0.145

On the relation of optical obscuration and X-ray absorption in Seyfert galaxies

Doppler follow-up of OGLE transiting companions in the Galactic bulge

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

Phantom Energy: Dark Energy withw<−1Causes a Cosmic Doomsday

f(T) teleparallel gravity and cosmology

The Cosmological Constant

Supernovae in the nuclear regions of starburst galaxies

Hierarchical galaxy formation

The cosmological constant and dark energy

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

Cosmological Implications from Observations of Type Ia Supernovae

DYNAMICS OF DARK ENERGY

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

Results from the High-z Supernova Search Team

Hubble Space TelescopeImaging of the Circumnuclear Environments of the CfA Seyfert Galaxies: Nuclear Spirals and Fueling

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

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION

High‐Redshift Supernova Rates

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

Microwave cavity searches for dark-matter axions

Supernova Rates: A Cosmic History

Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys

The evolution of stellar mass and the implied star formation history

Testing the DGP model with ESSENCE

f(R)theories of gravity

THE MEAN TYPE IA SUPERNOVA SPECTRUM OVER THE PAST NINE GIGAYEARS

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

The Luminous Type Ic Supernova 1992ar 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 $z=0.145$ \end{document}

The origin and abundances of the chemical elements

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

The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey

Monte Carlo Simulations of Type Ia Supernova Observations in Supernova Surveys

Cross section measurements and thermonuclear reaction rates for 48Ca(p, γ)49Sc and 48Ca(p, n)48Sc

Type Ia Supernovae: Influence of the Initial Composition on the Nucleosynthesis, Light Curves, and Spectra and Consequences for the Determination of Ω_Mand Λ

Modelling feedback from stars and black holes in galaxy mergers

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

An analytical model for the history of cosmic star formation

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

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

The Rise Time of Nearby Type I[CLC]a[/CLC] Supernovae

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

Solar-system abundances of the elements

Time Dilation in the Light Curve of the Distant Type Ia Supernova SN 1995K

A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex

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

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

How many supernovae are we missing at high redshift?

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

Optical and Infrared Photometry of the Type I[CLC]a[/CLC] Supernovae 1999[CLC]da[/CLC], 1999[CLC]dk[/CLC], 1999[CLC]gp[/CLC], 2000[CLC]bk[/CLC], and 2000[CLC]ce[/CLC]

Cosmic shear analysis of archival HST/ACS data: I. Comparison of early ACS pure parallel data to the HST/GEMS Survey

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

The evolution and explosion of massive stars

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

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

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

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

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

The Visual Orbit and Evolutionary State of 12 Bootis

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

Weak gravitational lensing

The history of star formation in dusty galaxies

Accurate masses and radii of normal stars

Hubble's diagram and cosmic expansion

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

Central Masses and Broad‐Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation‐Mapping Database

Modified gravity and cosmology

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

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

Multi-object spectroscopy of low redshift EIS clusters. I.

ESO imaging survey: infrared deep public survey

The discovery of a type Ia supernova at a redshift of 0.31

Evolution of Supernova Explosion Rates in the Universe

Dust in elliptical galaxies

The Helium Abundance in Population i Stars