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HDUV: The Hubble Deep UV Legacy Survey

Oesch, P. A. and Montes, M. and Reddy, N. and Bouwens, R. J. and Illingworth, G. D. and Magee, D. and Atek, H. and Carollo, C. M. and Cibinel, A. and Franx, M. and Holden, B. and Labbé, I. and Nelson, E. J. and Steidel, C. C. and van Dokkum, P. G. and Morselli, L. and Naidu, R. P. and Wilkins, S. (2018) HDUV: The Hubble Deep UV Legacy Survey. Astrophysical Journal Supplement Series, 237 (1). Art. No. 12. ISSN 0067-0049. https://resolver.caltech.edu/CaltechAUTHORS:20180801-164036045

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Abstract

We present the Hubble Deep UV Legacy Survey (HDUV), a 132-orbit imaging program with the WFC3/UVIS camera on board the Hubble Space Telescope (HST). The HDUV extends and builds on the few previous UV imaging surveys in the two GOODS/CANDELS-Deep fields to provide deep images over a total area of ~100 arcmin2 in the two filters F275W and F336W. Our release also includes all the F275W imaging data taken by the CANDELS survey, which were aligned using a novel approach and combined with the HDUV survey data. By reaching depths of 27.5–28.0 mag (5σ in 0farcs4 apertures), these are the deepest high-resolution UV data over such a large area taken to date. Such unique UV imaging enables a wide range of science by the community. A few of the main goals of the HDUV survey are as follows: (1) to provide a complete sample of faint star-forming galaxies at z ~ 1–3; (2) to constrain the ionizing photon escape fraction from galaxies at z ~ 2–3; and (3) to track the build-up of bulges and the disappearance of clumpy disk galaxies through reliable internal stellar population properties at sub-kiloparsec resolution out to z ~ 3. The addition of the HDUV data further enhances the legacy value of the two GOODS/CANDELS-Deep fields, which now include deep 11-band HST imaging, as well as very deep ancillary data from X-ray to radio, enabling unique multi-wavelength studies. Here, we provide an overview of the survey design, describe the data reduction, and highlight a few basic analyses of the images that are available to the community as high-level science products, via the Mikulski Archive for Space Telescopes.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4365/aacb30DOIArticle
https://arxiv.org/abs/1806.01853arXivDiscussion Paper
ORCID:
AuthorORCID
Oesch, P. A.0000-0001-5851-6649
Montes, M.0000-0001-7847-0393
Reddy, N.0000-0001-9687-4973
Bouwens, R. J.0000-0002-4989-2471
Illingworth, G. D.0000-0002-8096-2837
Atek, H.0000-0002-7570-0824
Carollo, C. M.0000-0003-1624-7609
Cibinel, A.0000-0003-4578-514X
Holden, B.0000-0002-6153-3076
Labbé, I.0000-0002-2057-5376
Nelson, E. J.0000-0002-7524-374X
Steidel, C. C.0000-0002-4834-7260
van Dokkum, P. G.0000-0002-8282-9888
Naidu, R. P.0000-0003-3997-5705
Additional Information:© 2018. The American Astronomical Society. Received 2016 September 1; revised 2018 May 17; accepted 2018 June 5; published 2018 July 13. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Science Institute (STScI). STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. The data are available from the Mikulski Archive for Space Telescopes (MAST) at doi:10.17909/T90T2N. The authors thank the anonymous referee who helped improve this manuscript and encouraged the release of the initial catalogs. The authors thank Marc Rafelski, Brian Siana, and Harry Teplitz for several very helpful discussions regarding the WFC3/UVIS data acquisition and reduction. The authors also thank Tomer Tal for help during the proposal stage, and Ros Skelton for help with the 3D-HST detection images and SExtractor settings. Support for this work was provided by NASA through grant HST-GO-13872 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. P.O. further acknowledges support by the Swiss National Science Foundation. The data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). Facility: HST(ACS/WFC3). -
Funders:
Funding AgencyGrant Number
NASAHST-GO-13872
NASANAS 5-26555
Swiss National Science Foundation (SNSF)UNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Subject Keywords:cosmology: observations; galaxies: abundances; galaxies: evolution; techniques: image processing
Issue or Number:1
Record Number:CaltechAUTHORS:20180801-164036045
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180801-164036045
Official Citation:P. A. Oesch et al 2018 ApJS 237 12
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:88485
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:02 Aug 2018 14:23
Last Modified:03 Oct 2019 20:07

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