European Extremely Large Telescope Site Characterization II: High angular resolution parameters
H\'ector V\'azquez Rami\'o, Jean Vernin, Casiana Mu\~noz-Tu\~n\'on,, Marc Sarazin, Antonia M. Varela, Herv\'e Trinquet, Jos\'e Miguel Delgado,, Jes\'us J. Fuensalida, Marcos Reyes, Abdelmajid Benhida, Zouhair Benkhaldoun,, Diego Garc\'ia Lambas, Youssef Hach, M. Lazrek

TL;DR
This study characterizes high angular resolution observational parameters at four potential E-ELT sites using consistent measurement techniques, providing detailed turbulence and atmospheric stability data crucial for telescope performance optimization.
Contribution
It offers a comprehensive comparison of turbulence parameters across four candidate sites using standardized instruments and methods during the E-ELT design phase.
Findings
Quantified seeing conditions and isoplanatic angles for each site.
Analyzed seasonal and nightly variations of turbulence parameters.
Estimated coherence time and 'coherence étendue' from wind profile data.
Abstract
This is the second article of a series devoted to European Extremely Large Telescope (E-ELT) site characterization. In this article we present the main properties of the parameters involved in high angular resolution observations from the data collected in the site testing campaign of the E-ELT during the Design Study (DS) phase. Observations were made in 2008 and 2009, in the four sites selected to shelter the future E-ELT (characterized under the ELT-DS contract): Aklim mountain in Morocco, Observatorio del Roque de los Muchachos (ORM) in Spain, Mac\'on range in Argentina, and Cerro Ventarrones in Chile. The same techniques, instruments and acquisition procedures were taken on each site. A Multiple Aperture Scintillation Sensor (MASS) and a Differential Image Motion Monitor (DIMM) were installed at each site. Global statistics of the integrated seeing, the free atmosphere seeing, the…
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