Analysis of the distribution of precipitable water vapor in the Chajnantor area

Author:

Cortés Fernando1,Reeves Rodrigo1,Bustos Ricardo2

Affiliation:

1. CePIA, Departamento de Astronomía; Universidad de Concepción; Concepción Chile

2. Laboratorio de Astro-Ingeniería y Microondas; Facultad de Ingeniería, Universidad Católica de la Santísima Concepción; Concepción Chile

Funder

Fondo Gemini-Conicyt programa de astronomía/pci folio

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

Reference17 articles.

1. Bustos , R. G. Delgado L. Nyman S. Radford 2000 52 years of climatological data for the Chajnantor area http://library.nrao.edu/alma.shtml

2. Parque Astronómico de Atacama: An ideal site for millimeter, submillimeter, and mid-infrared astronomy;Bustos;Publ. Astron. Soc. Pac.,2014

3. Delgado , G. A. Otárola V. Belitsky D. Urbain 1999 The determination of precipitable water vapour at Llano de Chajnantor from observations of the 183 GHz water vapour line http://library.nrao.edu/alma.shtml

4. The optical/infrared astronomical quality of high Atacama sites: I. Preliminary results of optical seeing;Giovanelli;Publ. Astron. Soc. Pac.,2001

5. The Atacama Pathfinder Experiment (APEX)-A new submillimeter facility for southern skies;Güsten;Astron. Astrophys.,2006

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