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CERN Document Server Pronađeno je 5 zapisa  Pretraživanje je potrajalo 0.79 sekundi 
1.
Euclid. I. Overview of the Euclid mission / Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. [...]
arXiv:2405.13491.- 2025-04 - 94 p. - Published in : Astron. Astrophys. 697 (2025) A1 Fulltext: 2405.13491 - PDF; publication - PDF;
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2.
The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−71$_{.}^{\circ}$0 < ℓ < 67$_{.}^{\circ}$0) / Elia, Davide (INAF, Rome) ; Molinari, S. (INAF, Rome) ; Schisano, E. (INAF, Rome) ; Pestalozzi, M. (INAF, Rome) ; Pezzuto, S. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Noriega-Crespo, A. (Baltimore, Space Telescope Sci.) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Mottram, J.C. (Heidelberg, Max Planck Inst. Astron.) et al.
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the spectral energy distributions (SEDs) and heliocentric distances, based on the photometric catalogs presented in Molinari et al. [...]
arXiv:1706.01046.- 2017 - 44 p. - Published in : Mon. Not. R. Astron. Soc. 471 (2017) 100-143 Fulltext: PDF;
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3.
CLASH-VLT: The stellar mass function and stellar mass density profile of the z=0.44 cluster of galaxies MACS J1206.2-0847 / Annunziatella, M. (Trieste U. ; Trieste Observ.) ; Biviano, A. (Trieste Observ.) ; Mercurio, A. (Capodimonte Observ.) ; Nonino, M. (Trieste Observ.) ; Rosati, P. (Ferrara U.) ; Balestra, I. (Trieste Observ.) ; Presotto, V. (Trieste U. ; Trieste Observ.) ; Girardi, M. (Trieste Observ. ; Trieste U.) ; Gobat, R. (IRFU, Saclay) ; Grillo, C. (Bohr Inst.) et al.
Context. The study of the galaxy stellar mass function (SMF) in relation to the galaxy environment and the stellar mass density profile, rho(r), is a powerful tool to constrain models of galaxy evolution [...]
arXiv:1408.6356.- 2014-11-14 - 15 p. - Published in : Astron. Astrophys. 571 (2014) A80 Fulltext: PDF; External link: Preprint
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4.
Intra Cluster Light properties in the CLASH-VLT cluster MACS J1206.2-0847 / Presotto, V (Trieste U. ; Trieste Observ.) ; Girardi, M (Trieste U. ; Trieste Observ.) ; Nonino, M (Trieste Observ.) ; Mercurio, A (Capodimonte Observ.) ; Grillo, C (DARK Cosmology Ctr.) ; Rosati, P (Ferrara U.) ; Biviano, A (Trieste Observ.) ; Annunziatella, M (Trieste U. ; Trieste Observ.) ; Balestra, I (Trieste Observ. ; Capodimonte Observ.) ; Cui, W (Trieste U. ; Trieste Observ. ; Western Australia U.) et al.
We aim at constraining the assembly history of clusters by studying the intra cluster light (ICL) properties, estimating its contribution to the fraction of baryons in stars, f*, and understanding possible systematics/bias using different ICL detection techniques. We developed an automated method, GALtoICL, based on the software GALAPAGOS to obtain a refined version of typical BCG+ICL maps. [...]
arXiv:1403.4979.- 2014-05-26 - 17 p. - Published in : Astron. Astrophys. 565 (2014) A126 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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5.
CLASH-VLT: The mass, velocity-anisotropy, and pseudo-phase-space density profiles of the z=0.44 galaxy cluster MACS 1206.2-0847 / Biviano, A. ; Rosati, P. ; Balestra, I. ; Mercurio, A. ; Girardi, M. ; Nonino, M. ; Grillo, C. ; Scodeggio, M. ; Lemze, D. ; Kelson, D. et al.
We use an unprecedented data-set of about 600 redshifts for cluster members, obtained as part of a VLT/VIMOS large programme, to constrain the mass profile of the z=0.44 cluster MACS J1206.2-0847 over the radial range 0-5 Mpc (0-2.5 virial radii) using the MAMPOSSt and Caustic methods. We then add external constraints from the gravitational lensing analysis of Umetsu et al [...]
arXiv:1307.5867.- 2013 - 22 p. - Published in : Astron. Astrophys. 558 (2013) A1 Fulltext: PDF; External link: Preprint
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