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: http://www.eso.org/~chummel/oyster/manual/node140.html
Дата изменения: Tue Apr 28 19:12:50 2015 Дата индексирования: Sun Apr 10 20:38:09 2016 Кодировка: Поисковые слова: molecular cloud |
As usual, bias correction is based in incoherent scans and is performed separately for each interferometer configuration. First, bias correction fit coefficients are computed combining all observations (for each configuration) to make sure that a basic correction is performed. Second, bias corrections are updated for each star with the measurement obtained for this star only.