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Дата изменения: Fri Feb 23 12:58:48 1996 Дата индексирования: Tue Oct 2 18:10:19 2012 Кодировка: Поисковые слова: saturn |
The first step consists of detecting the emission lines of the comparison
spectrum to produce the line table line.tbl. It can be noted that
the command SAVE/LONG will store all keyword values as descriptors
of this table, so that a session can be saved only if the table line.tbl
is available. The commands:
Midas...> SET/LONG WLC= ccd0003 THRES=20. WIDTH=8 YWIDTH=3 YSTEP=1
Midas...> SEARCH/LONG
initialize the line searching parameters and SEARCH/LONG performs
the following operations:
The parameter can be used to improve the signal-to-noise
ratio of each row by averaging adjacent rows. The parameter
is by default equal to 1 which corresponds to the standard row-by-row
method but can be set to a larger value to accelerate the wavelength
calibration. The detections are stored in the following columns of the
table line.tbl:
Results can be checked with the command PLOT/SEARCH. For
one-dimensional spectra,
Midas...> PLOT/SEARCH
plots the central row of the spectrum as well as
the position of the detected lines. This behavior
is obtained for 2D spectra by the additional option 1D, as in:
Midas...> PLOT/SEARCH 1D
whereas typing the command without option provides a bi-dimensional
graph of the X- and Y-positions of the detected lines.