Add to ORKGManuscriptWe 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 0.95, 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
International audienceSupernova (SN) rates are potentially powerful diagnostics of metal enrichment ...
We describe our ongoing program designed to measure the SN-Ia rate in a sample of massive z=0.5-0.9 ...
This thesis presents Type Ia supernova (SN Ia) rates from the Hubble Space Telescope (HST) Cluster S...
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) usi...
We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) usi...
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...
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 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...
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...
Supernova (SN) rates are potentially powerful diagnostics of metal enrichment and SN physics, partic...
International audienceSupernova (SN) rates are potentially powerful diagnostics of metal enrichment ...
We describe our ongoing program designed to measure the SN-Ia rate in a sample of massive z=0.5-0.9 ...
This thesis presents Type Ia supernova (SN Ia) rates from the Hubble Space Telescope (HST) Cluster S...
We present a new survey strategy to discover and study high-redshift Type Ia supernovae (SNe Ia) usi...
We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) usi...
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...
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 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...
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...
Supernova (SN) rates are potentially powerful diagnostics of metal enrichment and SN physics, partic...
International audienceSupernova (SN) rates are potentially powerful diagnostics of metal enrichment ...
We describe our ongoing program designed to measure the SN-Ia rate in a sample of massive z=0.5-0.9 ...
This thesis presents Type Ia supernova (SN Ia) rates from the Hubble Space Telescope (HST) Cluster S...