D. Balam

Implications of Two Type Ia Supernova Populations for Cosmological Measurements

SECONDARY PARAMETERS OF TYPE Ia SUPERNOVA LIGHT CURVES

IMPROVED DARK ENERGY CONSTRAINTS FROM ∼100 NEW CfA SUPERNOVA TYPE Ia LIGHT CURVES

Type Ia Supernovae Are Excellent Standard Candles in the Near-infrared

Observational probes of cosmic acceleration

Luminosity Indicators in the Ultraviolet Spectra of Type Ia Supernovae

The Effect Of Progenitor Age And Metallicity On Luminosity And Ni-56 Yield In Type Ia Supernovae

THE MEAN TYPE IA SUPERNOVA SPECTRUM OVER THE PAST NINE GIGAYEARS

THE CARNEGIE SUPERNOVA PROJECT: LIGHT-CURVE FITTING WITH SNooPy

f(R,T)gravity

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

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

Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

SNLS Spectroscopy: Testing for Evolution in Type Ia Supernovae

SiFTO: An Empirical Method for Fitting SN Ia Light Curves

Verifying the Cosmological Utility of Type Ia Supernovae: Implications of a Dispersion in the Ultraviolet Spectra