Abstract
The Cosmic Evolution Survey (COSMOS) was initiated with an extensive allocation (590 orbits in Cycles 12-13) using the Hubble Space Telescope (HST) for high-resolution imaging. Here we review the characteristics of the HST imaging with the Advanced Camera for Surveys (ACS) and parallel observations with NICMOS and WFPC2. A square field (1.8 deg 2) has been imaged with single-orbit ACS I-band F814W exposures with 50% completeness for sources 0.5″ in diameter at I AB = 26.0 mag. The ACS is a key part of the COSMOS survey, providing very high sensitivity and high-resolution (0.09″ FWHM and 0.05″ pixels) imaging and detecting a million objects. These images yield resolved morphologies for several hundred thousand galaxies. The small HST PSF also provides greatly enhanced sensitivity for weak-lensing investigations of the dark matter distribution.
Original language | English (US) |
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Pages (from-to) | 38-45 |
Number of pages | 8 |
Journal | Astrophysical Journal, Supplement Series |
Volume | 172 |
Issue number | 1 |
DOIs | |
State | Published - 2007 |
Keywords
- Cosmology: observations
- Dark matter
- Galaxies: evolution
- Galaxies: formation large-scale structure of universe
- Surveys
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science