Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

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

Venturi, T. and Varenius, E. and Swinbank, A.M. and Simpson, J.M. and Simpson, C. and Serjeant, S. and Sargent, M.T. and Röttgering, H.J.A. and Richards, A.M.S. and Pérez-Torres, M.A. and Pearson, C. and Njeri, A. and Murphy, E.J. and Morabito, L.K. and Koopmans, L.V.E. and Knudsen, K.K. and Kneib, J-P. and Ibar, E. and Garrett, M.A. and Garratt, T.K. and Chen, H. and Coppin, K. and Chapman, S.C. and Biggs, A.D. and Best, P.N. and Bacon, D. and Argo, M.K. and Guidetti, D. and Bondi, M. and Prandoni, I. and Jarvis, M.J. and Ivison, R.J. and Garrington, S.T. and McHardy, I.M. and Smail, I. and Beswick, R.J. and Wrigley, N.H. and Radcliffe, J.F. and Thomson, A.P. and Muxlow, T.W.B. (2020) 'The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey) : overview and survey description.', Monthly notices of the Royal Astronomical Society., 495 (1). pp. 1188-1208.

Abstract

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 ∼140 h of observations with enhanced-Multi-Element Remotely Linked Interferometer Network (e-MERLIN) and ∼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 (⁠∼1.5μ Jy beam−1), angular resolution (0.2–0.7 arcsec) and field-of-view (∼15 × 15 arcmin2) to detect and spatially resolve star-forming galaxies and active galactic nucleus (AGN) at z ≳ 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 ∼20-yr baseline and the development of new point 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 ∼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 re-MERGE/rHST ∼ 1.02 ± 0.03, suggesting that in most high-redshift galaxies, the ∼GHz continuum emission traces the stellar light seen in optical imaging. This is the first in a series of papers that will explore the ∼kpc-scale radio properties of star-forming galaxies and AGN in the GOODS-N field observed by e-MERGE DR1.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
(8682Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnras/staa1279
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:05 May 2020
Date deposited:24 June 2020
Date of first online publication:08 May 2020
Date first made open access:24 June 2020

Save or Share this output

Export:
Export
Look up in GoogleScholar