An Advanced Atmospheric Model for ESO Observing Sites

Author(s)
W. Kausch, M. Kondrak, S. Noll, M. Lakićević, S. Kimeswenger, N. Przybilla, S. Unterguggenberger, K. Leschinski, O. Czoske, W. Zeilinger
Abstract

Any observation taken with a ground-based telescope is affected by absorption, emission and scattering of light arising within the Earth's atmosphere. The size of the effect depends on its composition and the physical state of the involved molecular species, and is usually highly variable on time scales from seconds to decades rendering the prediction of exposure times and the removal of this influence from observations a challenging matter. Here we present a progress report on our work on an improved new model of the Earth's atmosphere based on theoretical calculations and newly available measurements and data from ground- and space-based Earth science facilities.

Organisation(s)
Department of Astrophysics
Volume
512
Publication date
12-2017
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
ASJC Scopus subject areas
Astronomy and Astrophysics, Computer Science Applications
Portal url
https://ucrisportal.univie.ac.at/en/publications/6b4b6213-c53c-4395-a1a4-bac98ca0745e