Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1771380 | Astroparticle Physics | 2010 | 7 Pages |
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 5 years can yield a spectro-photometric time series of ∼1000z<0.08∼1000z<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 (≳4-m)(≳4-m) telescopes are capable of discovering supernovae shortly after explosion out to z∼3z∼3. These can be fed to space telescopes, and can isolate systematics and extend the redshift range over which we measure the expansion history of the universe.