activity
20092021
most citedThe XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

272 citations · 1.2k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2021

Discovery of a shock front in the merging cluster of galaxies A2163

Nceba Mhlahlo, Loic Guennou, Luigina Feretti

ACO2163 is one of the hottest (mean keV) and extremely X-ray overluminous merging galaxy clusters which is located at . The cluster hosts one of the largest g…

astro-ph.GA2018★ 11 cited

The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations

V. Guglielmo, B. M. Poggianti, B. Vulcani +34

Superclusters form from the largest enhancements in the primordial density perturbation field and extend for tens of Mpc, tracing the large-scale structure of the Universe. We char…

astro-ph.CO2017★ 19 cited

The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy

A. Farahi, V. Guglielmo, A. E. Evrard +34

An X-ray survey with the XMM-Newton telescope, XMM-XXL, has identified hundreds of galaxy groups and clusters in two 25 deg fields. Combining spectroscopic and X-ray observatio…

astro-ph.GA2017★ 15 cited

The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters

V. Guglielmo, B. M. Poggianti, B. Vulcani +42

The fraction of galaxies bound in groups in the nearby Universe is high (50% at z~0). Systematic studies of galaxy properties in groups are important in order to improve our unders…

astro-ph.GA2016★ 38 cited

The XXL survey XV: Evidence for dry merger driven BCG growth in XXL-100-GC X-ray clusters

S. Lavoie, J. P. Willis, J. Democles +33

The growth of brightest cluster galaxies is closely related to the properties of their host cluster. We present evidence for dry mergers as the dominant source of BCG mass growth a…

astro-ph.CO2016★ 32 cited

Weak lensing study of 16 DAFT/FADA clusters: substructures and filaments

Nicolas Martinet, Douglas Clowe, Florence Durret +7

While our current cosmological model places galaxy clusters at the nodes of a filament network (the cosmic web), we still struggle to detect these filaments at high redshifts. We p…

astro-ph.GA2016★ 43 cited

The XXL Survey: VI. The 1000 brightest X-ray point sources

S. Fotopoulou, F. Pacaud, S. Paltani +36

X-ray extragalactic surveys are ideal laboratories for the study of the evolution and clustering of active galactic nuclei (AGN). The XXL Survey spans two fields of a combined 50 $…

astro-ph.GA2016★ 23 cited

The XXL Survey VIII: MUSE characterisation of intracluster light in a z0.53 cluster of galaxies

C. Adami, E. Pompei, T. Sadibekova +11

Within a cluster, gravitational effects can lead to the removal of stars from their parent galaxies. Gas hydrodynamical effects can additionally strip gas and dust from galaxies. T…

astro-ph.CO2015★ 272 cited

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

M. Pierre, F. Pacaud, C. Adami +89

We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extrag…

astro-ph.CO2015★ 143 cited

The XXL Survey. II. The bright cluster sample: catalogue and luminosity function

F. Pacaud, N. Clerc, P. A. Giles +40

Context. The XXL Survey is the largest survey carried out by the XMM-Newton satellite and covers a total area of 50 square degrees distributed over two fields. It primarily aims at…

astro-ph.GA2015★ 92 cited

The VIMOS Public Extragalactic Redshift Survey (VIPERS). Environmental effects shaping the galaxy stellar mass function

I. Davidzon, O. Cucciati, M. Bolzonella +38

We exploit the first public data release of VIPERS to investigate environmental effects in galaxy evolution between and . The large number of spectroscopic redshift…

astro-ph.GA2014★ 25 cited

The evolution of the cluster optical galaxy luminosity function between z=0.4 and 0.9 in the DAFT/FADA survey

Nicolas Martinet, Florence Durret, Loic Guennou +8

We compute optical galaxy luminosity functions (GLFs) in the B, V, R, and I rest-frame bands for one of the largest medium-to-high-redshift (0.4 < z < 0.9) cluster samples to date…

astro-ph.CO2014★ 16 cited

The mass profile and dynamical status of the z~0.8 galaxy cluster LCDCS 0504

L. Guennou, A. Biviano, C. Adami +34

Constraints on the mass distribution in high-redshift clusters of galaxies are not currently very strong. We aim to constrain the mass profile, M(r), and dynamical status of the $z…

astro-ph.CO2013★ 36 cited

Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range

L. Guennou, C. Adami, F. Durret +29

We analyse the structures of all the clusters in the DAFT/FADA survey for which XMM-Newton and/or a sufficient number of galaxy redshifts in the cluster range is available, with th…

astro-ph.HE2013★ 67 cited

A Tidal Flare Candidate in Abell 1795

W. P. Maksym, M. P. Ulmer, M. C. Eracleous +2

As part of our ongoing archival X-ray survey of galaxy clusters for tidal flares, we present evidence of an X-ray transient source within 1 arcmin of the core of Abell 1795. The ex…

astro-ph.CO2013★ 9 cited

VIPERS: An Unprecedented View of Galaxies and Large-Scale Structure Halfway Back in the Life of the Universe

L. Guzzo, U. Abbas, C. Adami +48

The VIMOS Public Extragalactic Redshift Survey (VIPERS) is an ongoing ESO Large Programme to map in detail the large-scale distribution of galaxies at 0.5 < z <1.2. With a combinat…

astro-ph.CO2012★ 39 cited

Diffuse light in the young cluster of galaxies CL J1449+0856 at z=2.07

C. Adami, F. Durret, L. Guennou +1

Cluster properties do not seem to be changing significantly during their mature evolution phase, for example they do not seem to show strong dynamical evolution at least up to z~0.…

astro-ph.CO2012★ 31 cited

The VIMOS Public Extragalactic Redshift Survey (VIPERS): spectral classification through Principal Component Analysis

A. Marchetti, B. R. Granett, L. Guzzo +51

We develop a Principal Component Analysis aimed at classifying a sub-set of 27,350 spectra of galaxies in the range 0.4 < z < 1.0 collected by the VIMOS Public Extragalactic Redshi…

astro-ph.CO2012★ 22 cited

Comparison of the properties of two fossil groups of galaxies with the normal group NGC 6034 based on multiband imaging and optical spectroscopy

C. Adami, S. Jouvel, L. Guennou +9

We collected multiband imaging and spectroscopy for two fossil groups (RX J1119.7+2126 and 1RXS J235814.4+150524) and one normal group (NGC 6034). We computed photometric redshifts…

astro-ph.CO2011★ 41 cited

Intracluster light in clusters of galaxies at redshifts 0.4<z<0.8

L. Guennou, C. Adami, C. Da Rocha +27

The study of intracluster light can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical pro…

astro-ph.CO2011★ 49 cited

Galaxy cluster searches based on photometric redshifts in the four CFHTLS Wide fields

F. Durret, C. Adami, A. Cappi +19

We have developed a method for detecting clusters in large imaging surveys, based on the detection of structures in galaxy density maps made in slices of photometric redshifts. Thi…

astro-ph.CO2011★ 4 cited

A search for faint low surface brightness galaxies in the relaxed cluster Abell 496

Melville P. Ulmer, Christophe Adami, Florence Durret +2

Cluster faint low surface brightness galaxies (fLSBs) are difficult to observe. Consequently, their origin, physical properties and number density are not well known. After a first…

astro-ph.CO2010★ 64 cited

The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes

C. Adami, A. Mazure, M. Pierre +29

XMM and Chandra opened a new area for the study of clusters of galaxies. Not only for cluster physics but also, for the detection of faint and distant clusters that were inaccessib…

astro-ph.CO2010★ 26 cited

The DAFT/FADA survey. I.Photometric redshifts along lines of sight to clusters in the z=[0.4,0.9] interval

L. Guennou, C. Adami, M. P. Ulmer +20

As a contribution to the understanding of the dark energy concept, the Dark energy American French Team (DAFT, in French FADA) has started a large project to characterize statistic…