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- National Institute for AstrophysicsIT100 papers
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10 papers · 1 filter
MOSE: a feasibility study for optical turbulence forecasts with the Meso-Nh mesoscale model to support AO facilities at ESO sites (Paranal and Armazones)
E. Masciadri, F. Lascaux
We present very encouraging preliminary results obtained in the context of the MOSE project, an on-going study aiming at investigating the feasibility of the forecast of the optica…
MOSE: zooming on the Meso-NH mesoscale model performances at the surface layer at ESO sites (Paranal and Armazones)
Franck Lascaux, Elena Masciadri, INAF / Osservatorio Astrofisico di Arcetri
In the context of the MOSE project, in this contribution we present a detailed analysis of the Meso-NH mesoscale model performances and their dependency on the model and orography…
Shape Evolution of Massive Early-Type Galaxies: Confirmation of Increased Disk Prevalence at z>1
Yu-Yen Chang, Arjen van der Wel, Hans-Walter Rix +4
We use high-resolution K-band VLT/HAWK-I imaging over 0.25 square degrees to study the structural evolution of massive early-type galaxies since z~1. Mass-selected samples, complet…
Analysis of Spitzer-IRS spectra of hyperluminous infrared galaxies
A. Ruiz, G. Risaliti, E. Nardini +2
Hyperluminous infrared galaxies (HLIRG) are the most luminous persistent objects in the Universe. They exhibit extremely high star formation rates, and most of them seem to harbour…
Can habitable planets form in clustered environments?
M. de Juan Ovelar, J. M. D. Kruijssen, E. Bressert +3
We present observational evidence of environmental effects on the formation and evolution of planetary systems. We combine catalogues of resolved protoplanetary discs (PPDs) and yo…
CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release
CALIFA collaboration, B. Husemann, K. Jahnke +74
We present the first public data release of the CALIFA survey. It consists of science-grade optical datacubes for the first 100 of eventually 600 nearby (0.005<z<0.03) galaxies, ob…