activity
20062014
most citedThe XMM-LSS Survey: A well controlled X-ray cluster sample over the D1 CFHTLS area

64 citations · 192 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2014

Web-based tools for the analysis of TAOS data and much more

D. Ricci, P. -G. Sprimont, C. Ayala +8

We suggest a new web-based approach for browsing and visualizing data produced by a network of telescopes, such as those of the ongoing TAOS and the forthcoming TAOS II projects. W…

astro-ph.EP2014★ 1 cited

Automated differential photometry of TAOS data: preliminary analysis

D. Ricci, P. -G. Sprimont, C. Ayala +8

A preliminary data analysis of the stellar light curves obtained by the robotic telescopes of the TAOS project is presented. We selected a data run relative to one of the stellar f…

astro-ph.CO2011★ 20 cited

I. Flux and color variations of the quadruply imaged quasar HE 0435-1223

D. Ricci, J. Poels, A. Elyiv +32

aims: We present VRi photometric observations of the quadruply imaged quasar HE 0435-1223, carried out with the Danish 1.54m telescope at the La Silla Observatory. Our aim was to m…

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-ph2007★ 43 cited

The XMM large scale structure survey: optical vs. X-ray classifications of active galactic nuclei and the unified scheme

O. Garcet, P. Gandhi, E. Gosset +25

Our goal is to characterize AGN populations by comparing their X-ray and optical classifications. We present a sample of 99 spectroscopically identified X-ray point sources in the…

astro-ph2006★ 64 cited

The XMM-LSS Survey: A well controlled X-ray cluster sample over the D1 CFHTLS area

M. Pierre, F. Pacaud, P. -A. Duc +24

We present the XMM-LSS cluster catalogue corresponding to the CFHTLS D1 area. The list contains 13 spectroscopically confirmed, X-ray selected galaxy clusters over 0.8 deg2 to a re…