D. C. Leonard

The Luminous Type Ic Supernova 1992ar at z = 0.145

A catalogue of low-mass X-ray binaries

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

A test of general relativity using the LARES and LAGEOS satellites and a GRACE Earth gravity model

Late‐Time Observations of SN 2006gy: Still Going Strong

Hierarchical galaxy formation

The cosmological constant and dark energy

Cosmological Implications from Observations of Type Ia Supernovae

SNLS Spectroscopy: Testing for Evolution in 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

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION

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

Reading the Spectra of the Most Peculiar Type Ia Supernova 2002cx

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?

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

deepSIP: linking Type Ia supernova spectra to photometric quantities with deep learning

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}

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

Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests

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

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

Is There Evidence for a Hubble Bubble? The Nature of Type Ia Supernova Colors and Dust in External Galaxies

Snapshot Distances to Type Ia Supernovae: All in “One” Night's Work

Monte Carlo Simulations of Type Ia Supernova Observations in Supernova Surveys

A Light Echo from Type Ia SN 1995E?

The Lick Observatory Supernova Search with the Katzman Automatic Imaging Telescope

THE CASE FOR A POSITIVE COSMOLOGICAL Λ-TERM

Reddening, Absorption, and Decline Rate Corrections for a Complete Sample of Type Ia Supernovae Leading to a Fully Corrected Hubble Diagram tov< 30,000 km s⁻¹

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

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

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

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

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]

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

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s⁻¹ Mpc⁻¹ Uncertainty from the Hubble Space Telescope and the SH0ES Team

Cepheid Calibration of the Peak Brightness of Type Ia Supernovae. X. SN 1991T in NGC 4527

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

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

The Australia Telescope National Facility Pulsar Catalogue

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

The Subluminous Type Ia Supernova 1998de in NGC 252

Multi-color light curves of type Ia supernovae on the color-magnitude diagram: A novel step \ntoward more precise distance and extinction estimates

Weak gravitational lensing

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

Modified gravity and cosmology

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

A Black Hole in the X-Ray Nova Ophiuchi 1997

Time Dilation from Spectral Feature Age Measurements of Type IA Supernovae.

The Type I[CLC]a[/CLC] Supernova 1997[CLC]br[/CLC] in ESO 576-G40