The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS Spectroscopic Survey of the Chandra Deep Field-South*
Cooper, M.C.; Yan, R.; Dickinson, M.; Juneau, S.; Lotz, J.M.; Newman, J.A.; Papovich, C.; Salim, S.; Walth, G.; Weiner, B.J.; Willmer, C.N.A.
Keywords:
Catalogues; Galaxies: distances and redshifts; Surveys
Date:
2012
Publisher:
The American Astronomical Society
Citation:
Cooper, M. C., Yan, R., Dickinson, M., Juneau, S., Lotz, J. M., Newman, J. A., . . . Willmer, C. N. A. (2012). The arizona CDFS environment survey (ACES): A Magellan/IMACS spectroscopic survey of the chandra deep field-south. Monthly Notices of the Royal Astronomical Society, 425(3), 2116-2127. http://dx.doi.org/10.1111/j.1365-2966.2012.21524.x
Rights:
© 2012 The Authors
Type:
Article
Abstract:
We present the Arizona CDFS Environment Survey (ACES), a recently completed spectroscopic redshift survey of the Chandra Deep Field-South (CDFS) conducted using the Inamori-Magellan Areal Camera and Spectrograph on the Magellan-Baade telescope. In total, the survey targeted 7277 unique sources down to a limiting magnitude of $R_{AB} = 24.1$, yielding 5080 secure redshifts across the $\sim30 arcmin × 30 arcmin$ extended CDFS region. The ACES data set delivers a significant increase to both the spatial coverage and the sampling density of the spectroscopic observations in the field. Combined with previously published spectroscopic redshifts, ACES now creates a highly complete survey of the galaxy population at $R < 23$, enabling the local galaxy density (or environment) on relatively small scales ($\sim 1 \text{Mpc}$) to be measured at $z < 1$ in one of the most heavily studied and data-rich fields in the sky. Here, we describe the motivation, design and implementation of the survey and present a preliminary redshift and environment catalogue. In addition, we utilize the ACES spectroscopic redshift catalogue to assess the quality of photometric redshifts from both the COMBO-17 and Multiwavelength Survey by Yale-Chile imaging surveys of the CDFS.
Description:
*This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.
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