Re-calibrated Generalized-Scidar measurements at Cerro Paranal (VLT's site)
E. Masciadri (1), F. Lascaux (1), J. J. Fuensalida (2),(3), G., Lombardi (4), H. Vazquez-Ramio (3) ((1) INAF - Osservatorio Astrofisico di, Arcetri, Florence, Italy (2) Dep. Astrofisica, Universidad La Laguna,, Astrofisico Francisco Sanchez, Tenerife

TL;DR
This study re-calibrates Generalized Scidar measurements at Cerro Paranal to correct biases, providing more accurate turbulence profiles and error estimates crucial for astronomical site assessment.
Contribution
It introduces a re-calibration method for GS data that corrects biases and improves turbulence profile accuracy at Cerro Paranal.
Findings
Relative errors of CN2 profiles can reach 60% in some cases.
Total seeing errors are up to 12%, with median errors around 0.05-0.06 arcsec.
Absolute error of the median isoplanatic angle is 0.13 arcsec.
Abstract
Generalized Scidar (GS) measurements taken at the Paranal Observatory in November/December 2007 in the context of a site qualification for the future European Extremely Large Telescope E-ELT are re-calibrated to overcome the bias induced on the CN2 profiles by a not correct normalization of the autocorrelation of the scintillation maps that has been recently identified in the GS technique. A complete analysis of the GS corrected measurements as well as of the corrected errors is performed statistically as well as on individual nights and for each time during all nights. The relative errors of the CN2 profiles can reach up to 60% in some narrow temporal windows and some vertical slabs, the total seeing up to 12% and the total integrated turbulence J up to 21%. However, the statistic analysis tells us that the absolute errors of the median values of the total seeing is 0.06 arcsec…
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