Contribution of the CSO to our Knowledge of the Atmospheric Opacity and Phase Delay at Submillimeter Wavelengths. Application to the ALMA Project

Details Contribution of the CSO to our Knowledge of the Atmospheric Opacity and Phase Delay at Submillimeter Wavelengths. Application to the ALMA Project Contribution of the CSO to our Knowledge of the Atmospheric Opacity and Phase Delay at Submillimeter Wavelengths. Application to the ALMA Project

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..417..125p&link_type=abstract

Submillimeter Astrophysics and Technology: a Symposium Honoring Thomas G. Phillips ASP Conference Series, Vol. 417, proceedings

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The aim of the poster shown at the meeting was to summarize the work performed with the Fourier Transform Spectrometer mounted on the Caltech Submillimeter Observatory in the mid-1990s to understand the atmospheric spectrum at submillimeter wavelengths. The long-term goal was to provide an atmospheric model for ALMA and other submillimeter observatories as accurate as possible.

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