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V. Guglielmo

Researcher at University of Padua

Publications -  11
Citations -  801

V. Guglielmo is an academic researcher from University of Padua. The author has contributed to research in topics: Galaxy & Stellar mass. The author has an hindex of 8, co-authored 9 publications receiving 703 citations. Previous affiliations of V. Guglielmo include INAF & Aix-Marseille University.

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

Marguerite Pierre, +96 more
TL;DR: The XXL-XMM survey as discussed by the authors provides constraints on the dark energy equation of state from the space-time distribution of clusters of galaxies and serves as a pathfinder for future, wide-area X-ray missions.
Journal ArticleDOI

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

TL;DR: The XXL-XMM survey as discussed by the authors provides constraints on the dark energy equation of state from the space-time distribution of clusters of galaxies and serves as a pathfinder for future, wide-area X-ray missions.
Journal ArticleDOI

The XXL Survey : XX : the 365 cluster catalogue

C. Adami, +65 more
TL;DR: In this paper, the properties of the XXL cluster catalogue are described in detail, as well as associated catalogues of more specific objects such as super-clusters and fossil groups, and the complete subset of clusters for which the selection function is well determined plus all X-ray clusters which are, to date, confirmed.
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The star formation history of galaxies: the role of galaxy mass, morphology and environment

TL;DR: In this article, the authors analyzed the star formation history (SFH) of galaxies as a function of present-day environment, galaxy stellar mass and morphology, and concluded that the variation of the SFRD with environment is not driven by different distributions of galaxy masses and morphologies in clusters and field, and must be due to an accelerated formation in high mass halos compared to low mass ones even for galaxies that will end up having the same galaxy mass today.