Dome A, the highest plateau in Antarctica, is being developed as a site for an astronomical observatory. The planned telescopes and instrumentation and the unique site characteristics are conducive toward Type Ia supernova surveys for cosmology. A self-contained search and survey over five years can yield a spectro-photometric time series of ∼1000 z \u3c 0.08 supernovae. These can serve to anchor the Hubble diagram and quantify the relationship between luminosities and heterogeneities within the Type Ia supernova class, reducing systematics. Larger aperture (\u3e4-m) telescopes are capable of discovering supernovae shortly after explosion out to z ∼ 3. These can be fed to space telescopes, and can isolate systematics and extend the redshift...
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 discove...
We present a measurement of the distant Type Ia supernova (SN Ia) rate derived from the first 2 yr o...
Dome A, the highest plateau in Antarctica, is being developed as a site for an astronomical observat...
Dome A, the highest plateau in Antarctica, is being developed as a site for an astronomical observat...
Type Ia Supernovae (SNe Ia) are the thermonuclear explosion of a carbon-oxygen white dwarf (WD) and ...
20International audiencePreliminary site testing datasets suggest that Dome C in Antarctica is one o...
Galaxies, and clusters of galaxies, can act as gravitational lenses and magnify the light of objects...
Aims. We present multi-band light curves and distances for five type Ia supernovae at intermediate r...
In 2008 January the twenty-fourth Chinese expedition team successfully deployed the Chinese Small Te...
We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 T...
International audienceThe See Change survey was designed to make z > 1 cosmological measurements by ...
We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) usi...
The remarkable uniformity of Type Ia supernovae has allowed astronomers to use them as distance indi...
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 discove...
We present a measurement of the distant Type Ia supernova (SN Ia) rate derived from the first 2 yr o...
Dome A, the highest plateau in Antarctica, is being developed as a site for an astronomical observat...
Dome A, the highest plateau in Antarctica, is being developed as a site for an astronomical observat...
Type Ia Supernovae (SNe Ia) are the thermonuclear explosion of a carbon-oxygen white dwarf (WD) and ...
20International audiencePreliminary site testing datasets suggest that Dome C in Antarctica is one o...
Galaxies, and clusters of galaxies, can act as gravitational lenses and magnify the light of objects...
Aims. We present multi-band light curves and distances for five type Ia supernovae at intermediate r...
In 2008 January the twenty-fourth Chinese expedition team successfully deployed the Chinese Small Te...
We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 T...
International audienceThe See Change survey was designed to make z > 1 cosmological measurements by ...
We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) usi...
The remarkable uniformity of Type Ia supernovae has allowed astronomers to use them as distance indi...
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 discove...
We present a measurement of the distant Type Ia supernova (SN Ia) rate derived from the first 2 yr o...