PI: Keith Bechtol, U. of Wisconsin, Madison, firstname.lastname@example.org
Address: Physics Department, 1150 University Avenue, Madison, WI 53706-1390 USA
CoI: Sahar Allam, FNAL
CoI: Alex Amon, Stanford U.
CoI: Manda Banerji, University of Cambridge
CoI: Franz Bauer, PUC-Chile
CoI: Gary Bernstein, U. of Pennsylvania
CoI: Ami Choi, CCAPP/The Ohio State University
CoI: Andrew Connolly, U. of Washington
CoI: Ian Dell'Antonio, Brown U.
CoI: Alex Drlica-Wagner, Fermilab/UChicago
CoI: Eric Gawiser, Rutgers U.
CoI: Daniel Gruen, SLAC
CoI: Robert Gruendl, NCSA/University of Illinois
CoI: Will Hartley, University College London
CoI: Sebastian Hoenig, Southampton
CoI: Lynne Jones, U. of Washington
CoI: Jason Rhodes, CalTech-JPL
CoI: Claudia Scarlata, U. of Minnesota
CoI: Samuel Schmidt, UC Davis
CoI: Douglas Tucker, FNAL
CoI: Christopher Walter, Duke U.
CoI: Brian Yanny, FNAL
Title: A new DECam deep field covering the full Euclid Deep Field South
Abstract: Deep fields are an essential component of many astronomical surveys, enabling the study of galaxies at higher redshifts and lower luminosities, and providing high signal-to-noise measurements that are used to calibrate wide-area survey components (e.g., detection efficiency and blending effects, object classification, photometric redshifts, and weak lensing shear). The impact of deep fields in survey science is amplified through overlaps with external datasets: multiwavelength imaging, space-based imaging, and spectroscopy. In June 2019, the Euclid Consortium announced the selection of three deep fields for space-based optical and near-IR imaging and spectroscopy, including the Euclid Deep Field South (EDFS; 23~deg$^2$) centered at (RA, Dec) = (61.24, -48.42). EDFS is a candidate Deep Drilling Field (DDF) for the Vera Rubin Observatory Legacy Survey of Space and Time (LSST). Deep multiband imaging of the entire EDFS using the Dark Energy Camera (DECam) extending 1.25 mag deeper than the Dark Energy Survey (DES) would accelerate characterization of this field, enhance the accuracy of photometric redshifts for DES, inform the LSST survey strategy and commissioning efforts, and begin the assembly of a legacy multiwavelength dataset of broad utility to the international astronomical community.
Program Type: Standard/Extragalactic
Run 1 (2020B): CT-4m/DECam -- 3n on Oct 12 - Oct 17 2020
Run 2 (2020B): CT-4m/DECam -- 5n on Oct 29 - Nov 02 2020
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360