XMMU J100750 5+125818: a strong lensing cluster at z = 1 082

We used a large set of numerically simulated clusters for which the X-ray and the lensing properties were previously investi- gated, and compared their Einstein ring sizes

Particularly, in [5, 6, 15, 18, 19] the authors establish the asymptotic behavior of orthogonal poly- nomials with respect to nondiagonal Sobolev inner products and the authors in

Measuring the concentration–mass relation and its redshift evolution in a subsample of MUSIC-2 halos that reproduces the distribution of X-ray regularity parameters of the clusters

The density distribution of sources detected in at least one IRAC channel has been analyzed as a function of the distance from the cluster center (panel (A) of Figure 5).. The

• Analysis of long-term variability of high-energy sources in the optical and X-ray bands, using INTEGRAL observations from IBIS (the gamma-ray imager), JEM-X (the X-ray monitor)

For the optimisation of [1] + and [1-dmad] + with the PBE0 functional and various basis set systems, summary of mean unsigned errors (MUEs) with respect to their X- ray

Abstract: This paper introduces jNEP: a general, flexible, and rigorous implementation of NEPs (the basic model) and some interestenting variants; it is specifically designed to

Using a combination of optical photometry and spectroscopy we esti- mate stellar masses, ages, and foreground extinction values of the brightest part of the population