We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST). By targeting massive galaxy clusters at 0.9\u3czHST field survey and a factor of three improvement in the total yield of SN detections in relatively dust-free red-sequence galaxies. In total, sixteen SNe were discovered at z\u3e0.95, nine of which were in galaxy clusters. This strategy provides a SN sample that can be used to decouple the effects of host galaxy extinction and intrinsic color in high redshift SNe, thereby reducing one of the largest systematic uncertainties in SN cosmology
Supernova (SN) rates are potentially powerful diagnostics of metal enrichment and SN physics, partic...
We present details on the observing strategy, data-processing techniques, and spectroscopic targetin...
Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Ener...
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) usi...
The See Change survey was designed to make $z>1$ cosmological measurements by efficiently discoverin...
ManuscriptWe present a new survey strategy to discover and study high redshift Type Ia supernovae (S...
We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 T...
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) usi...
The See Change survey was designed to make z > 1 cosmological measurements by efficiently discoverin...
We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 T...
The See Change survey was designed to make z > 1 cosmological measurements by efficiently discoverin...
The See Change survey was designed to make z > 1 cosmological measurements by efficiently discoverin...
We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Super...
Supernovae (SNe) are one the most energetic phenomena in the Universe and have been extensively used...
This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital S...
Supernova (SN) rates are potentially powerful diagnostics of metal enrichment and SN physics, partic...
We present details on the observing strategy, data-processing techniques, and spectroscopic targetin...
Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Ener...
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) usi...
The See Change survey was designed to make $z>1$ cosmological measurements by efficiently discoverin...
ManuscriptWe present a new survey strategy to discover and study high redshift Type Ia supernovae (S...
We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 T...
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) usi...
The See Change survey was designed to make z > 1 cosmological measurements by efficiently discoverin...
We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 T...
The See Change survey was designed to make z > 1 cosmological measurements by efficiently discoverin...
The See Change survey was designed to make z > 1 cosmological measurements by efficiently discoverin...
We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Super...
Supernovae (SNe) are one the most energetic phenomena in the Universe and have been extensively used...
This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital S...
Supernova (SN) rates are potentially powerful diagnostics of metal enrichment and SN physics, partic...
We present details on the observing strategy, data-processing techniques, and spectroscopic targetin...
Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Ener...