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APEX-MPI-IFD-0002 Atacama Pathfinder Experiment Interface Description Revision: 1.57 Release: December 6, 2005, Category: 4 Author: Dirk Murders Multi-Beam FITS Raw Data Format Dirk Murders, Edward

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What is multi-beam fits raw data?

Multi-beam fits raw data refers to the digital information collected from multiple radio beams in astronomy, which is stored in Flexible Image Transport System (FITS) format without any processing or calibration applied.

Who is required to file multi-beam fits raw data?

The astronomers or research institutions conducting observations using multi-beam instruments are required to file the multi-beam fits raw data.

How to fill out multi-beam fits raw data?

Multi-beam fits raw data is filled out by capturing the raw digital signals from multiple radio beams using multi-beam instruments and saving them in the FITS format without any processing or calibration.

What is the purpose of multi-beam fits raw data?

The purpose of multi-beam fits raw data is to preserve the unprocessed observations collected from multiple radio beams in astronomy. It allows for future analysis, calibration, and study of astronomical phenomena.

What information must be reported on multi-beam fits raw data?

The multi-beam fits raw data must include information such as the date and time of the observation, the antenna configuration, the instrument used, the observing parameters, and any relevant metadata.

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