Atacama Pathfinder EXperiment
APEX
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Observing with APEX allows us to study cold dust and gas in our own Milky Way and in distant galaxies. Tracing the thermal continuum emission and analyzing high frequency spectral lines improve our understanding of the structure and chemistry of planetary atmospheres, dying stars, regions of star formation as well as distant starburst galaxies. We can address issues from the vast scales of the structure of the Universe down to the physics and chemistry of comets.
Observations |
Site Information and Logistics |
The telescope | About Sequitor base |
Atmosphere | About Chajnantor site |
Instrumentation | APEX telephone list |
Observing with APEX |
Safety |
Preparing an observing run | Emergency procedures |
APEX data archiving | Safety documents and links |
The APEX project |
Miscellaneous Information |
The APEX staff and news | Picture gallery |
TWiki | Chajnantor camera image (Refresh each five minutes) |
eGroupware | Weather monitor Weather monitor --> |
APEX Documents Management System | |
APEX Intranet (Password protected) |
Last update: June 7th, 2011 |
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