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Astron. Astrophys. 364, 799-815 (2000)

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4. Corrections to the photomultiplier outputs

The reduction sequence starts with the removal of instrumental effects along with the compensation for the inverse square effect of the variable distance. We refer to the output of this step as the photometric rate P. These steps will be described in García et al. (2000).

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© European Southern Observatory (ESO) 2000

Online publication: January 29, 2001
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