We present the catalogue of a wide-field CFHT/WHT spectroscopic survey of the lensing cluster Cl0024+1654 at z=0.395. This catalogue contains 618 new spectra, of which 581 have identified redshifts. Adding redshifts available from the literature, the final

Astronomy&Astrophysicsmanuscriptno.(willbeinsertedbyhandlater)

Awide- eldspectroscopicsurveyoftheclusterofgalaxies

Cl0024+1654

arXiv:astro-ph/0103123v1 7 Mar 2001

I.Thecatalogue

OliverCzoske1,Jean-PaulKneib1,Genevi`eveSoucail1,TerryJ.Bridges2

Jean-CharlesCuillandre4,5

12345

,YannickMellier3,5,and

ObservatoireMidi-Pyr´en´ees,UMR5572,14Av.EdouardBelin,31400Toulouse,FranceInstituteofAstronomy,MadingleyRoad,Cambridge,CB30HA,UKInstitutd’AstrophysiquedeParis,98bisBd.Arago,75014Paris,FranceCFHTCorporation,P.O.Box1597,Kamuela,Hawaii96743,USA

ObservatoiredeParis,DEMIRM,61Av.del’Observatoire,75014Paris,France

Receivedtoolate,Acceptedevenlater

Abstract.Wepresentthecatalogueofawide- eldCFHT/WHTspectroscopicsurveyofthelensingclusterCl0024+1654atz=0.395.Thiscataloguecontains618newspectra,ofwhich581haveidenti edredshifts.Addingredshiftsavailablefromtheliterature,the nalcataloguecontainsdatafor687objectswithredshiftsidenti edfor650ofthem.295galaxieshaveredshiftsintherange0.37<z<0.41,i.e.areclustermembersorlieintheimmediateneighbourhoodofthecluster.Theareacoveredbythesurveyis21×25arcmin2insize,correspondingto4×4.8h 2Mpc2attheclusterredshift.Thesurveyis45%completedowntoV=22overthewhole eldcovered;within3arcminoftheclustercentrethecompletenessexceeds80%atthesamemagnitude.Adetailedcompletenessanalysisispresented.Thecataloguegivesastrometricposition,redshift,VmagnitudeandV Icolour,aswellastheequivalentwidthsforanumberoflines.ApartfromtheclusterCl0024+1654itself,threeotherstructuresareidenti edinredshiftspace:agroupofgalaxiesatz=0.38,justinfrontofCl0024+1654andprobablyinteractingwithit,aclosepairofgroupsofgalaxiesatz～0.495andanoverdensityofgalaxiesatz～0.18withnoobviouscentre.Thespectroscopiccataloguewillbeusedtotracethethree-dimensionalstruc-tureoftheclusterCl0024+1654aswellasstudythephysicalpropertiesofthegalaxiesintheclusterandinitsenvironment.

Keywords.galaxies:clusters:Cl0024+1654–cosmology:observations–cosmology:large-scalestructureoftheUniverse

1.Introduction

Clustersofgalaxiesareincreasinglyviewednotassimpleisolatedandrelaxedsystemsbutasembeddedinandcon-nectedtothegenerallarge-scalestructureintheUniverse.Thisviewofclustersinalargercontexthasconsequencesfortheinterpretationofclustergalaxypopulations,clusterdynamicsandmassestimates.

Clustersofgalaxiesgrowbycontinuouslyaccretinggalaxiesandgroupsofgalaxiesfromthesurrounding eld,mostlyalong lamentarystructures.Intheprocess,galax-