most citedXMM-Newton study of the lensing cluster of galaxies CL0024+17

47 citations

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astro-ph200537 cited

Discovery of a high-redshift Einstein ring

R. A. Cabanac, D. Valls-Gabaud, A. O. Jaunsen +2

We report the discovery of a partial Einstein ring of radius 1.48arcsec produced by a massive (and seemingly isolated) elliptical galaxy. The spectroscopic follow-up at the VLT rev…

astro-ph20051 cited

Cosmological Interpretation from High Redshift Clusters Observed Within the XMM-Newton -Project

Alain Blanchard

During the last ten years astrophysical cosmology has brought three remarkable results of deep impact for fundamental physics: the existence of non-baryonic dark matter, the (nearl…

astro-ph2004

Ionising stellar populations in circumnuclear star forming regions

Enrique Perez-Montero, Angeles I. Diaz, Marcelo Castellanos

We present a study of the stellar populations and gas physical conditions in Circumnuclear Star Forming Regions (CNSFRs) based on spectrophotometric data, including the 7000 angstr…

astro-ph200447 cited

XMM-Newton study of the lensing cluster of galaxies CL0024+17

Y. -Y. Zhang, H. Boehringer, Y. Mellier +2

We present a detailed gravitational mass measurement based on the XMM-Newton imaging spectroscopy analysis of the lensing cluster of galaxies CL0024+17 at z=0.395. The emission app…

astro-ph200429 cited

An ISOCAM survey through gravitationally lensing galaxy clusters. II. The properties of infrared galaxies in the A2218 field

A. Biviano, L. Metcalfe, B. McBreen +10

We observed the cluster Abell 2218 (z=0.175), with ISOCAM on board the Infrared Space Observatory, using two filters with reference wavelengths of 6.7 and 14.3 microns. We detected…

astro-ph200410 cited

Detecting compact dark matter in galaxy clusters via gravitational microlensing: A2218 & A370

Artem Tuntsov, Geraint Lewis, Rodrigo Ibata +1

After decades of searching, the true nature of dark matter still eludes us. One potential probe of the form of dark matter in galaxy clusters is to search for microlensing variabil…