Berger, A.A.Berger0000-0001-9680-7092Adebahr, B.B.AdebahrHerrera Ruiz, N.N.Herrera RuizWright, A. H.A. H.WrightPRANDONI, ISABELLAISABELLAPRANDONIDettmar, R. -J.R. -J.Dettmar2022-06-102022-06-102021http://hdl.handle.net/20.500.12386/32278This study is based on the WSRT observations of the Lockman Hole field at 1.4GHz (Prandoni et al., 2018MNRAS.481.4548P). The data consist of 16 individual pointings, each observed for a full synthesis of 12-hrs between December 2006 and January 2007. The centre of the mosaic was chosen to be at RA=10:53:16.6; DE=+58:01:15 (J2000). <P />We present a new deep-field analysis of polarised sources in the Lockman Hole at 1.4GHz, using a bespoke polarised mosaic with a central RMS of 7uJy/beam. We find 150 polarised sources in an area of 6.5deg<SUP>2</SUP> out of 1708 total-intensity sources in this field (8.8%). This equates to a polarised source density of 23deg<SUP>-2</SUP>. <P />(3 data files).en10.26093/cds/vizier.36530155https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/653/A1552021yCat..36530155BFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation