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The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description

Muxlow, T. W. B. (author)
University of Manchester
Thomson, A. P. (author)
University of Southampton,University of Manchester
Radcliffe, J. F. (author)
Universiteit van Pretoria,University of Pretoria,University of Manchester
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Wrigley, N. H. (author)
University of Manchester
Beswick, R. J. (author)
University of Manchester
Smail, Ian (author)
Durham University
McHardy, I. M. (author)
University of Southampton
Garrington, S. T. (author)
University of Manchester
Ivison, R. J. (author)
University of Edinburgh,European Southern Observatory Santiago
Jarvis, M. J. (author)
University Of Oxford,University of the Western Cape
Prandoni, I. (author)
Istituto nazionale di astrofisica (INAF)
Bondi, M. (author)
Istituto nazionale di astrofisica (INAF)
Guidetti, D. (author)
Istituto nazionale di astrofisica (INAF)
Argo, M. K. (author)
University of Central Lancashire
Bacon, David (author)
University of Portsmouth
Best, P. N. (author)
University of Edinburgh
Biggs, A. D. (author)
European Southern Observatory Santiago
Chapman, S. C. (author)
Dalhousie University
Coppin, K. (author)
University of Hertfordshire
Chen, H. (author)
University of Manchester,Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences,Chinese Academy of Sciences
Garratt, T. K. (author)
University of Hertfordshire
Garrett, M. A. (author)
Universiteit Leiden (UL),Leiden University (UL),University of Manchester
Ibar, E. (author)
Universidad de Valparaíso,University of Valparaíso
Kneib, Jean-Paul (author)
Aix-Marseille Université,Aix Marseille University,Ecole Polytechnique Federale de Lausanne (EPFL),Swiss Federal Institute of Technology in Lausanne (EPFL)
Knudsen, Kirsten Kraiberg, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Koopmans, L. V. E. (author)
Rijksuniversiteit Groningen,University of Groningen
Morabito, L. K. (author)
Durham University
Murphy, E. J. (author)
National Radio Astronomy Observatory
Njeri, A. (author)
University of Manchester
Pearson, Chris (author)
STFC Rutherford Appleton Laboratory
Perez-Torres, M. A. (author)
Agencia Estatal Consejo Superior de Investigaciones Científicas,Spanish National Research Council
Richards, A. M. S. (author)
University of Manchester
Rottgering, H. J. A. (author)
Universiteit Leiden (UL),Leiden University (UL)
Sargent, M. T. (author)
University of Sussex
Serjeant, Stephen (author)
Open University
Simpson, C. (author)
Gemini Observatory North
Simpson, J. M. (author)
Academia Sinica Taiwan
Swinbank, A. M. (author)
Durham University
Varenius, Eskil, 1986 (author)
University of Manchester,Chalmers tekniska högskola,Chalmers University of Technology
Venturi, T. (author)
Istituto nazionale di astrofisica (INAF)
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 (creator_code:org_t)
2020-05-08
2020
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 495:1, s. 1188-1208
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We present an overview and description of the e-MERGE Survey (e-MERLIN Galaxy Evolution Survey) Data Release 1 (DR1), a large program of high-resolution 1.5-GHz radio observations of the GOODS-N field comprising similar to 140 h of observations with enhanced-Multi-Element Remotely Linked Interferometer Network (e-MERLIN) and similar to 40 h with the Very Large Array (VLA). We combine the long baselines of e-MERLIN (providing high angular resolution) with the relatively closely packed antennas of the VLA (providing excellent surface brightness sensitivity) to produce a deep 1.5-GHz radio survey with the sensitivity (similar to 1.5 mu Jy beam(-1)), angular resolution (0.2-0.7 arcsec) and field-of-view (similar to 15x15 arcmin(2)) to detect and spatially resolve star-forming galaxies and active galactic nucleus (AGN) at z greater than or similar to 1. The goal of e-MERGE is to provide new constraints on the deep, sub-arcsecond radio sky which will be surveyed by SKA1-mid. In this initial publication, we discuss our data analysis techniques, including steps taken to model in-beam source variability over an similar to 20-yr baseline and the development of newpoint spread function/primary beam models to seamlessly merge e-MERLIN and VLA data in the uv plane. We present early science results, including measurements of the luminosities and/or linear sizes of similar to 500 galaxies selected at 1.5 GHz. In combination with deep Hubble Space Telescope observations, we measure a mean radio-to-optical size ratio of r(e-MERGE)/r(HST) similar to 1.02 +/- 0.03, suggesting that in most high-redshift galaxies, the similar to GHz continuum emission traces the stellar light seen in optical imaging. This is the first in a series of papers that will explore the similar to kpc-scale radio properties of star-forming galaxies and AGN in the GOODS-N field observed by e-MERGE DR1.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Annan fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Other Physics Topics (hsv//eng)

Keyword

radio continuum: galaxies
Galaxies: high-redshift
Galaxies: evolution

Publication and Content Type

art (subject category)
ref (subject category)

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