Abstract
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 < z < 1.5, we obtain a twofold improvement in the efficiency of finding SNe compared to an HST field survey and a factor of 3 improvement in the total yield of SN detections in relatively dust-free red-sequence galaxies. In total, sixteen SNe were discovered at z>0.95, nine of which were in galaxy clusters. This strategy provides an 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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1271-1283 |
| Number of pages | 13 |
| Journal | Astronomical Journal |
| Volume | 138 |
| Issue number | 5 |
| DOIs | |
| State | Published - 2009 |
| Externally published | Yes |
Keywords
- Cosmology
- General
- Observations supernovae
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science