STAGES: the Space Telescope A901/2 Galaxy Evolution Survey
arXiv:0811.3890 · doi:10.1111/j.1365-2966.2008.14259.x
Abstract
We present an overview of the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). STAGES is a multiwavelength project designed to probe physical drivers of galaxy evolution across a wide range of environments and luminosity. A complex multi-cluster system at z~0.165 has been the subject of an 80-orbit F606W HST/ACS mosaic covering the full 0.5x0.5 (~5x5 Mpc^2) span of the supercluster. Extensive multiwavelength observations with XMM-Newton, GALEX, Spitzer, 2dF, GMRT, and the 17-band COMBO-17 photometric redshift survey complement the HST imaging. Our survey goals include simultaneously linking galaxy morphology with other observables such as age, star-formation rate, nuclear activity, and stellar mass. In addition, with the multiwavelength dataset and new high resolution mass maps from gravitational lensing, we are able to disentangle the large-scale structure of the system. By examining all aspects of environment we will be able to evaluate the relative importance of the dark matter halos, the local galaxy density, and the hot X-ray gas in driving galaxy transformation. This paper describes the HST imaging, data reduction, and creation of a master catalogue. We perform Sersic fitting on the HST images and conduct associated simulations to quantify completeness. In addition, we present the COMBO-17 photometric redshift catalogue and estimates of stellar masses and star-formation rates for this field. We define galaxy and cluster sample selection criteria which will be the basis for forthcoming science analyses, and present a compilation of notable objects in the field. Finally, we describe the further multiwavelength observations and announce public access to the data and catalogues.
29 pages, 22 figures; accepted to MNRAS. Full data release available at http://www.nottingham.ac.uk/astronomy/stages
References in corpus (17)
- Star Formation and the Growth of Stellar Mass
- The DEEP2 Galaxy Redshift Survey: Evolution of the Color-Density Relation at 0.4 < z < 1.35
- A Wide-field Survey of Two Z~0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s
- The Stability of the Point Spread Function of the Advanced Camera for Surveys on the Hubble Space Telescope and Implications for Weak Gravitational Lensing
- The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey
- A Panoramic Mid-infrared Survey of Two Distant Clusters
- The dark matter environment of the Abell 901/902 supercluster: a weak lensing analysis of the HST STAGES survey
- The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
- The Cosmic Evolution Survey (COSMOS): a large-scale structure at z=0.73 and the relation of galaxy morphologies to local environment
- The Different Environmental Dependencies of Star-formation for Giant and Dwarf Galaxies
- A blind test of photometric redshifts on ground-based data
- Environmental dependence of AGN activity in the supercluster A901/2
- A wide angle tail radio galaxy in the COSMOS field: evidence for cluster formation
- Deep 610-MHz GMRT observations of the Spitzer extragalactic First Look Survey field - I. Observations, data analysis and source catalogue
- Infrared Spectral Energy Distributions of z~0.7 Star-Forming Galaxies
- Galaxy morphologies and environment in the Abell 901/902 supercluster from COMBO-17
- Morphology-dependent trends of galaxy age with environment in Abell 901/902 seen with COMBO-17