The HST eXtreme Deep Field XDF: Combining all ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever
G. D. Illingworth (UCSC), D. Magee (UCSC), P. A. Oesch (UCSC), R. J., Bouwens (Leiden), I. Labbe (Leiden), M. Stiavelli (STScI), P. G. van Dokkum, (Yale), M. Franx (Leiden), M. Trenti (Cambridge), C. M. Carollo (ETH), V., Gonzalez (UCR)

TL;DR
The XDF combines a decade of HST data into the deepest optical/near-IR image, revealing over 14,000 sources and reaching unprecedented faintness levels, significantly surpassing previous deep field images.
Contribution
This work creates the deepest combined optical and near-IR image of the sky by integrating all relevant HST data and applying improved processing techniques.
Findings
Deepest optical/near-IR image ever created
Detected over 14,000 sources in the full field
Reaches 31.2 AB mag at 5sigma in a 0.35" aperture
Abstract
The eXtreme Deep Field (XDF) combines data from ten years of observations with the HST Advanced Camera for Surveys (ACS) and the Wide-Field Camera 3 Infra-Red (WFC3/IR) into the deepest image of the sky ever in the optical/near-IR. Since the initial observations on the Hubble Ultra-Deep Field (HUDF) in 2003, numerous surveys and programs, including supernova followup, HUDF09, CANDELS, and HUDF12 have contributed additional imaging data across the HUDF region. Yet these have never been combined and made available as one complete ultra-deep optical and near-infrared image dataset. We do so now for the eXtreme Deep Field (XDF) program. Our new and improved processing techniques provide higher quality reductions of the total dataset. All WFC3 near-IR and optical ACS data sets have been fully combined and accurately matched, resulting in the deepest imaging ever taken at these wavelengths…
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