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

dc.contributor.authorJarvis, M. J.
dc.contributor.authorMuxlow, T. W. B.
dc.contributor.authorThomson, A. P.
dc.date.accessioned2021-02-08T12:10:00Z
dc.date.available2021-02-08T12:10:00Z
dc.date.issued2020
dc.description.abstractWe 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.en_US
dc.identifier.citationJarvis, M. J. et al. (2020). The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): Overview and survey description. Monthly Notices of the Royal Astronomical Society,495(1), 1188–1208en_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/staa1279
dc.identifier.urihttp://hdl.handle.net/10566/5861
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectGalaxies: evolutionen_US
dc.subjectGalaxies: high-redshiften_US
dc.subjectRadio continuum: galaxiesen_US
dc.subjecte-MERGE surveyen_US
dc.titleThe e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): Overview and survey descriptionen_US
dc.typeArticleen_US

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