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Tableau de de Vassily Kandinsky qui apparait comme un visionnaire: - le cercle représente le champ de vue d'XMM - le grand X, représente "rayons X" et symbolise les digrammes cosmologiques - les cercles de différentes couleurs: les amas de galaxies vus en rayons X avec des temperatures différentes - les petits points: les noyaux actifs de galaxies vus en rayons X - les grands traits noirs fins: les grandes structure de l'univers |
The XXL survey has mapped two extragalactic regions of 25 deg2, using 10 ks XMM observations down to a point-source sensitivity of ~ 5 10-15 erg/s/cm2 in the [0.5-2] keV band.
It is the largest XMM project approved to date (3Ms in December 2010, >6Ms in total).
As of December 2015, some 450 new galaxy clusters are detected out to z~1.5-2 as well as more than 22,000 active galactic nuclei (AGNs) out to z~4.
The main goal of the project is to constrain the Dark Energy equation of state using clusters of galaxies. This survey will also have lasting legacy value for cluster scaling laws and studies of AGNs and X-ray background.
This project builds on the experience acquired during the ten years XMM-LSS pilot survey. It is open to any scientist belonging to the international astronomical community, and interested in actively contributing to the general legacy effort.
The two surveyed regions are:
CFHTLS W1 centre: 2h23min -4deg30' (J2000), 25 deg2
BCS centre: 23h30min -55deg00' (J2000), 25 deg2
Observations were completed in 2013
The XXL exposure ans sensitivity maps are available here
(Download a synthetic overview of the XXL project xxl-overview.pdf)
M. Pierre (CEA Saclay, principal investigator)
M. Birkinshaw (Univ. Bristol)
A. Evrard (Univ. Michigan)
C. Horellou (Chalmers Univ. of Technology)
A. Iovino (INAF-OAB, Brera)
C. Lidman (AAO, Epping)
S. Maurogordato (Obs. Nice)
S. Paltani (Univ. Geneva)
M. Plionis (Univ. Thessaloniki)
V. Smolcic (Univ. Zagreb)
J. Surdej (Univ. Liege)
C. Vignali (Univ. Bologna)
J. Willis (Univ. Victoria)
The work is organised in working groups, with the following coodinators
DATA
X-ray processing : F. Pacaud
X-ray background : S. Snowden
General catalogue : L. Chiappetti, S. Maurogordato
Catalogue information : A. Elyiv, O. Melnyk, E. Pompei
Photometric redshifts : S. Paltani
Spectroscopic follow-up : C. Lidman, S. Murray, J. Willis
Redshift archival : C. Adami, L. Guennou
Radio follow-up : M. Birkinshaw, C. Horellou, V. Smolcic
SCIENCE
Theory and simulations : A. Evrard
Clusters of galaxies (general) : M. Pierre
Cosmology : F. Pacaud, D.Rappetti
Mass measurements : G. Smith, F. Menanteau
z>>1 clusters: M. Bremer, J. Santos
The z~0.3-0.5 groups: B. Poggianti, F. Gastaldello
AGNs (general) : M. Plionis
Environmental studies : S. Raychaudhury, O. Melnyk
Large scale structure : N. Cappelluti, A. Elyiv
Evolution : I. Georgantopoulos, R. Hickox
Miscellaneous : A. Comastri
Cosmology: S. Basilakos, A. Goobar
NUMERICAL SIMULATIONS
Birmigham group (I. McCarthy et al)
Michigan group (A. Evrard et al)
Oxford group (J. Devriendt et al)
Princeton group (D. Spergel et al)
Meudon group (P.S. Corasaniti et al)
Previous papers
(with on-line presentation links if available)
Pacaud et al., 2014: Cluster Cosmology with XXL, Madrid, November, 4-7 2014
Faccioli et al., 2014: Real-size XXL simulations of the X-ray sky, Madrid, November, 4-7 2014
Husband et al., 2014: The High Redshift (z > 0.8) XXL Cluster Sample, Madrid, November, 4-7 2014
Maughan et al., 2014: Scaling-laws in XXL, Madrid, November, 4-7 2014
Lieu et al., 2014: XXL Bright Sample: Weak Lensing MT scaling relation of groups and clusters, Madrid, November, 4-7 2014
Willis et al., 2014: Bias in galaxy cluster samples: SpARCS versus XMM-LSS, Madrid, November, 4-7 2014
Pierre 2014: The ultimate XMM extragalactic survey, X-ray universe 2014, Dublin, June, 16-19 2014
Giles 2014: The Luminosity-Temperature Relation of Clusters Detected in the XXL Survey, X-ray universe 2014, Dublin, June, 16-19 2014
Democles 2014: The 100 brightest XXL clusters: morphological study, X-ray universe 2014, Dublin, June, 16-19 2014
Ranalli 2014: The 2-10 keV luminosity function of AGN in the XMM-LSS and XMM-CDFS surveys, X-ray universe 2014, Dublin, June, 16-19 2014
Lavoie 2014: Passive galaxies and new perspectives on cluster galaxy evolution (SITELLE and the possibility to use wide-field optical imaging Fourier Transform), CASCA annual meeting, Quebec June, June 8-11, 2014
Pacaud 2013, XXL: the detection of galaxy clusters & the determination of their physical properties. The Mass profiles of galaxy clusters from the core to the outskirts, Madonna di Campiglio, Italy - March 2103
Pierre 2012, XXL – The utlimate XMM extragalctic survey, Science from the next generation Imaging and Spectroscopic surveys, ESO-Munich, Germany, October 2012
Pierre 2012, Large area cluster surveys with XMM. Half a century of X-ray astronomy, Mykonos, Greece – september 2012
Pacaud 2012, The XMM-LSS and XXL surveys. In Growing-up at high redshift: from proto-clusters to galaxy clusters, Madrid, Spain - September 2012
Willis 2012, Distant clusters in the XMM LSS survey. In Growing-up at high redshift: from proto-clusters to galaxy clusters, Madrid, Spain - September 2012
Pierre 2011, XXL or the Dark Energy, now, The X-ray Universe 2011 Symposium, Berlin, Germany – June 2012
R. Adam (Observatoire de la Cote d'Azur, Nice, FR)
C. Adami (Laboratoire d'Astrophysique, Marseille, FR)
S. Alis (Faculty of Science, Istanbul University, TR)
B. Altieri (European Space Astronomy Center, Madrid, ES)
C. Baguley (University of Bristol, UK)
N. Baran (University of Zagreb, HR)
C. Benoist (Observatoire de la Cote d'Azur, Nice, FR) S. Bhargava (Département d'Astrophysique CEA, Saclay, FR)
M. Birkishaw (University of Bristol, UK)
W. Black (University of Michigan, Ann Arbor, US) A. Bongiorno (Rome Observatory, Italy)
M. Bremer (University of Bristol, UK)
A. Cappi (INAF-OABO, Bologna, IT)
C. Caretta (Laboratoire d'Astrophysique, Marseille, FR)
N. Cerardi (Département d'Astrophysique CEA, Saclay, FR)
L. Chiappetti (INAF-IASF, Milano, IT)
P. Ciliegi (INAF-OABO, Bologna, IT)
N. Clerc (MPE, Garching, DE)
P. S. Corasaniti (Observatoire de Paris, FR)
J. Crossett (Leiden University, NL)
J. Coupon (ISCD, Geneva Observatory, CH)
J. Delhaize (University of Zagreb, HR)
I. Delvecchio (University of Zagreb, HR)
Sh. Desai (University of Illinois, US)
J. Devriendt (University of Oxford, UK)
Y. Dubois (University of Oxford, UK)
D. Eckert (ISCD, Geneva Observatory, CH)
S. Ettori (Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, IT)
A. E. Evrard (University of Michigan, Ann Arbor, US)
A. Farahi (Carnegie Mellon University, US)
C. Ferrari (Observatoire de la Cote d'Azur, FR)
S. Fotopoulou (ISCD, Geneva Observatory, CH)
C. Garrel (Département d'Astrophysique CEA, Saclay, FR)
F. Gastadello (INAF-IASF, Milan, IT)
I. Georgantopoulos (Observatory of Athens, GR)
P. Giles (University of Bristol, UK)
C. Horellou (Chalmers University of Technology, Onsala, SE)
M. Huynh (University of Western Austalia, AU)
A. Iovino (INAF-OAB, Brera, IT)
N. Jerlin (University of Zagreb, HR)
A. Le Brun (Département d'Astrophysique CEA, Saclay, FR)
J.-P. Le Fevre (Département d'Informatique CEA, Saclay, FR)
M. Lieu (European Space Astronomy Center, Madrid, ES)
G. Lingsong (ISCD, Geneva Observatory, CH)
C. Logan (University of Bristol, UK)
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M. Kilbinger (Département d'Astrophysique CEA, Saclay, FR)
K. Kolokythas (IUCAA, Pune, IN)
E. Koulouridis (National Observatory of Athens, GR)
Ch. Lidman (Australian Astronomical Observatory, Epping, AU)
F. Marulli (University of Bologna, IT)
B. Maughan (University of Bristol, UK)
A. Mantz (Stanford University, US)
V. Masoura (Observatory of Athens, GR)
S. Maurogordato (Observatoire de la Cote d'Azur, Nice, FR)
I. McCarthy (University of Liverpool, UK)
S. McGee (University of Birmingham, UK)
J.-B. Melin (Département de Physique des Particules CEA, Saclay, FR)
O. Melnyk (University of Zagreb, HR)
L. Moscardini (University of Bologna, IT)
M. Novak (University of Zagreb, HR)
F. Pacaud (Argelander-Institut fur Astronomie, Bonn, DE)
S. Paltani (ISCD, Geneva Observatory, CH)
E. Piconcelli (INAF-OAR, Roma, IT) M. Pierre (Département d'Astrophysique CEA, Saclay, FR)
M. Plionis (Aristotle University of Thessaloniki, Department of Physics, GR)
B. Poggianti (Observatory of Padova, IT)
D. Pomarede (Département d'Informatique CEA, Saclay, FR)
E. Pompei (European Southern Observatory, Garching, DE)
T. Ponman (University of Birmingham, UK)
E. Pouliasis (National Observatory of Athens, GR) M. E. Ramos Ceja (Argelander-Institut fur Astronomie, Bonn, DE)
P. Ranalli (University of Lund, SE)
D. Rapetti (Copenhagen University, DK)
S. Raychaudhury (University of Birmingham, UK)
T. Reiprich (Argelander-Institut fur Astronomie, Bonn, DE)
M. Ricci (Observatoire de la Cote d'Azur, Nice, FR)
D. Rosario (Durham University, UK)
H. Rottgering (Leiden Observatory, NL)
T. Sadibekova (Département d'Astrophysique CEA, Saclay, FR)
J.-L. Sauvageot (Département d'Astrophysique CEA, Saclay, FR)
C. Schimd (Laboratoire d'Astrophysique, Marseille, FR)
M. Sereno (University of Bologna, IT)
G.P. Smith (University of Birmingham, UK)
B. Slaus (University of Zagreb, HR)
V. Smolcic (University of Zagreb, HR)
J. Surdej (University of Liege, BE)
A. Trudeau (University of Victoria, CA)
K. Umetsu (ASIAA, Taipei, TW)
P. Valageas (Institut de Physique Theorique du CEA, Saclay, FR)
I. Valtchanov (European Space Astronomy Center, Madrid, ES)
A. Veropalumbo (University of Bologna, IT)
C. Vignali (University of Bologna, IT)
J. Willis (University of Victoria, CA)
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ESA Space science image of the week (Oct. 8th, 2018)
A survey of the Universe, XXL size
- What are the XXL clusters (2012)?
- A century of X-ray cluster astronomy (1913-2013)
"Interactive Visualization of 3D Redshift Surveys with SDvision"
by D. Pomarède and M. Pierre
Published in the Proceedings of the IAU Symposium 277 Tracing the Ancestry of Galaxies
(on the land of our ancestors), 2010,Vol.6, Symposium S277, p.154,
Cambridge Journals, ed. C. Carignan, F. Combes, K.C. Freeman.
Visual comparison of the XMM-LSS and CFHTLS Surveys.
Click this picture to download the video (20.8Mb)
The three-dimensional visualization of redshift surveys is a key player in the comprehension of the structuration of the cosmic web. The SDvision software package, intended primarily for the visualization of massive cosmological simulations, has been extended to provide an interactive visual representation of different classes of redshift surveys, with the objective to enable direct comparisons between the rare highest-density peaks traced by the clusters of galaxies found in the XMM-LSS Survey and the densely populated catalogues of galaxy photometric redshifts. We present the various possibilities offered by this tool in terms of filtering of the data, reconstruction of density fields, interactivity and visual rendering, including various techniques such as ray-casting, isosurfaces, slicing and texturing. This is illustrated using the C1 and C2 samples of the XMM-LSS Survey, and the publicly released COSMOS and CFHTLS photometric redshift Catalogs. Comparisons with published results are presented and discussed. (download pdf)
Any scientist is welcome to enter the consortium in order to participate in the data analysis and science activities. Privileged access to the entire XXL data set will be granted to all consortium members.
For further information, contact the PI.
Acknowledgement
XXL is an international project based around an XMM Very Large Programme surveying two 25 deg2 extragalactic fields at a depth of ~6 x 10-15 erg cm-2 s-1 in the [0.5-2] keV band for point-like sources. The XXL website is http://irfu.cea.fr/xxl. Multi-band information and spectroscopic follow-up of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/.
*** Append here any specific observatory acknowledgements (XMM, ESO, CFHT, etc.) pertaining to the data used in the paper in question, as well as acknowledgements to the relevant funding agencies. ***
• Thèmes de recherche du Service d'astrophysique › Data-SAp Structure et évolution de l'Univers
• Le Département d'Astrophysique (DAp) // UMR AIM • Department of Astrophysics (DAp) // UMR AIM
• Cosmologie et Evolution des Galaxies • Cosmology and Galaxy Evolution