Determining an accurate position for a submm galaxy (SMG) is the crucial step that enables us to move from the basic properties of an SMG sample - source counts and 2-D clustering - to an assessment of their detailed, multi-wavelength properties, their con
Identi cationofsubmillimetregalaxiesintheSHADESSourceCatalogue
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FigureA1.25×25-arcsecpostagestampimagesofeachSMGintheLHSHADESSourceCatalogue.GreyscaleR-bandand24-µmdataareshownintheleft-andright-handpanels,respectively,superimposedwithradiocontours.Circlesindicate2σpositionaluncertainties.Solidboxesindicaterobustidenti cations,whereP 0.05basedontheradioor24-µmcounts,oracombinationofthetwo.Dashedboxesindicatetentativeassociations.c0000RAS,MNRAS000,000–000
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