The <scp>XXL</scp> survey: First results and future
M. PierreService d'Astrophysique du CEA Saclay FranceC. AdamiLaboratoire d'Astrophysique Marseille FranceM. BirkinshawUniversity of Bristol Bristol UKL. ChiappettiINAF‐IASF Milano ItalyS. EttoriINAF‐OABO Bologna ItalyA. E. EvrardUniversity of Michigan Ann Arbor MichiganL. FaccioliService d'Astrophysique du CEA Saclay FranceF. GastaldelloINAF‐IASF Milano ItalyPaul GilesUniversity of Bristol Bristol UKC. HorellouChalmers University of Technology Onsala SwedenA. IovinoINAF‐OAB Brera ItalyE. KoulouridisService d'Astrophysique du CEA Saclay FranceC. LidmanAustralian Astronomical Observatory Epping AustraliaA. M. C. Le BrunService d'Astrophysique du CEA Saclay FranceB. J. MaughanUniversity of Bristol Bristol UKS. MaurogordatoObservatoire de la Cote d'Azur Nice FranceIan G. McCarthyUniversity of Liverpool Liverpool UKSatoshi MiyazakiNAOJ Tokyo JapanF. PacaudArgelander‐Institut fur Astronomie Bonn GermanyS. PaltaniISDC, Geneva Observatory SwitzerlandM. PlionisAristotle University Thessaloniki GreeceT. H. ReiprichArgelander‐Institut fur Astronomie Bonn GermanyT. SadibekovaService d'Astrophysique du CEA Saclay FranceV. SmolčićUniversity of Zagreb CroatiaS. L. SnowdenNASA, GSFC Greenbelt MarylandJean SurdejUniversity of Liège BelgiumM. TsirouService d'Astrophysique du CEA Saclay FranceC. VignaliUniversity of Bologna Bologna ItalyJ. P. WillisUniversity of Victoria CanadaSinan AlişIstanbul University Istanbul TurkeyB. AltieriEuropean Space Astronomy Center Madrid SpainN. BaranUniversity of Zagreb CroatiaC. BenoistObservatoire de la Cote d'Azur Nice FranceA. BongiornoINAF‐OAR Roma ItalyL. PozzettiUniversity of Bristol Bristol UKA. ButlerUniversity of Western Australia AustraliaA. CappiINAF‐OABO Bologna ItalyC. A. CarettaLaboratoire d'Astrophysique Marseille FranceP. CiliegiINAF‐OABO Bologna ItalyN. ClercMPI for Extraterrestrial Physics Garching GermanyPier-Stefano CorasanitiObservatoire de Paris FranceJ. CouponISDC, Geneva Observatory SwitzerlandJ. DelhaizeUniversity of Zagreb CroatiaI. DelvecchioUniversity of Zagreb CroatiaJ. DémoclèsHSCenter for Astrophysics Cambridge MassachusettsS. DesaiIIT Hyderabad IndiaJulien DevriendtUniversity of Oxford UKYohan DuboisUniversity of Oxford UKD. EckertISDC, Geneva Observatory SwitzerlandA. ElyivUniversity of Liège BelgiumArya FarahiUppsala University SwedenC. FerrariObservatoire de la Cote d'Azur Nice FranceS. FotopoulouISDC, Geneva Observatory SwitzerlandW. FormanHSCenter for Astrophysics Cambridge MassachusettsI. GeorgantopoulosObservatory of Athens GreeceV. GuglielmoINAF‐OAP Padova ItalyMinh HuynhUniversity of Western Australia AustraliaN. JerlinUniversity of Zagreb CroatiaC. JonesHSCenter for Astrophysics Cambridge MassachusettsS. LavoieUniversity of Victoria CanadaJ. P. Le FèvreService d'Informatique du CEA Saclay FranceMaggie LieuEuropean Space Astronomy Center Madrid SpainM. KilbingerService d'Astrophysique du CEA Saclay FranceF. MaruIliUniversity of Bologna Bologna ItalyA. MantzUniversity of Chicago Chicago IllinoisSean McGeeUniversity of Birmingham Birmingham UKJ.‐B. MelinService de Physique des Particules du CEA Saclay FranceО. MelnykUniversity of Zagreb CroatiaL. MoscardiniUniversity of Bologna Bologna ItalyMladen NovakUniversity of Zagreb CroatiaE. PiconcelliINAF‐OAR Roma ItalyBianca M. PoggiantiINAF‐OAP Padova ItalyD. M. PomaredeService d'Informatique du CEA Saclay FranceE. PompeiEuropean Southern Observatory Garching GermanyT. J. PonmanUniversity of Birmingham Birmingham UKM. E. Ramos-CejaArgelander‐Institut fur Astronomie Bonn GermanyParul RanaUniversity of Lund Lund SwedenDavid RapettiUniversity of Colorado Boulder ColoradoSomak RaychaudhuryUniversity of Birmingham Birmingham UKM. RicciObservatoire de la Cote d'Azur Nice FranceH. RöttgeringLeiden University Leiden The NetherlandsM SahlénUppsala University SwedenJ.‐L. SauvageotService d'Astrophysique du CEA Saclay FranceC. SchimdLaboratoire d'Astrophysique Marseille FranceM. SerenoINAF‐OABO Bologna ItalyG. P. SmithUniversity of Birmingham Birmingham UKKeiichi UmetsuASIAA Taipei TaiwanPatrick ValageasInstitut de Physique Theorique du CEA Saclay FranceA. ValottiService d'Astrophysique du CEA Saclay FranceI. ValtchanovEuropean Space Astronomy Center Madrid SpainA. VeropalumboINAF‐OABO Bologna ItalyB. AscasoUniversity Paris‐Diderot Paris FranceDavid J BarnesJodrell Bank Manchester UKM. De PetrisUniversity La Sapienza Rome ItalyF. DurretInstitut d'Astrophysique de Paris Paris FranceMegan DonahueUniversity of Michigan Ann Arbor MichiganM. IthanaYamagata University JapanM. J. JarvisUniversity of Oxford UKM. Johnston‐HollittVictoria University Wellington New ZealandE. KalfountzouEuropean Space Astronomy Center Madrid Spain
ABI
Аннотация
The XXL survey currently covers two 25 deg 2 patches with XMM observations of ∼10 ks. We summarize the scientific results associated with the first release of the XXL dataset, which occurred in mid‐2016. We review several arguments for increasing the survey depth to 40 ks during the next decade of XMM operations. X‐ray ( z < 2) cluster, ( z < 4) active galactic nuclei ( AGN ), and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi‐ λ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN , clusters, and the X‐ray background. In particular, it will offer a unique opportunity to pinpoint the z > 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.
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