A "slipping" method of observations at RATAN-600 allowing to increase the integration time is described. Within a tolerable range of aberration a source can be tracked by simple shift of the feed horns along the focal line of the secondary reflector. The results of effectiveness evaluation are given.
Astrofizicheskie Issledovaniia Izvestiya Spetsial'noj Astrofizicheskoj Observatorii
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