Volume 455, Number 1, August III 2006
|Page(s)||385 - 393|
|Section||Instruments, observational techniques, and data processing|
|Published online||31 July 2006|
UBVRI twilight sky brightness at ESO-Paranal
European Southern Observatory (ESO), K. Schwarzschildstr. 2, 85748, Garching b. München, Germany e-mail: firstname.lastname@example.org
2 Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul., 84/32, Moscow, 117997 Russia e-mail: email@example.com
3 A.M.Obukhov's Institute of Atmospheric Physics, Russian Academy of Sciences, Pyzhevsky per., 3, Moscow, 119017 Russia e-mail: firstname.lastname@example.org
Accepted: 10 April 2006
Context.Twilight studies have proved to be important tools for analyzing the atmospheric structure with interesting consequences on the characterization of astronomical sites. Active discussions of this topic have started again recently in connection with the evaluation of Dome C, Antarctica, as a potential astronomical site and several site-testing experiments, including twilight brightness measurements, are being prepared.
Aims.The present work provides the first absolute photometric measurements of twilight sky brightness for ESO-Paranal (Chile). They are meant both as a contribution to the site monitoring and as reference values in the analysis of other sites, including Dome C.
Methods.The twilight sky brightness was estimated on more than 2000 FORS1 archival images, which include both flats and standard star observations taken in twilight and covering a Sun zenith distance range 94°–112°.
Results.The comparison with a low-altitude site shows that Paranal V twilight sky brightness is about 30% lower, implying that some fraction of multiple scattering has to take place at an altitude of a few km above sea level.
Key words: atmospheric effects / site testing / techniques: photometric
© ESO, 2006
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