| carrousel | stsdas.hst_calib.hrs.z_calib | carrousel |
carrousel -- Calibrate GHRS carrousel position.
carrousel dctab cctabin cctabout
Using tables of dispersion coefficients (for the same grating mode) the carrousel calibration coefficient, C, is computed by the following equation:
carpos = C - B * arcsin(m * w / A)
where:
carpos - is the carrousel position,
m - spectral order ("1" for first order gratings),
w - wavelength at the center of the
photocathode, (i.e., sample position 280),
B = 10430.378 (carrousel steps per radian),
A - constant for each grating, and
C - coefficient updated by this task.
The input dispersion coefficients are used to compute the central wavelength, w, at sample position 280.0 at each carrousel position observed by solving the following equation using Newton's iterative method;
280.0 = a0 + (a1 * m * w) + (a2 * m * m * w * w) +
(a3 * m) + (a4 * w) + (a5 * m * m * w) +
(a6 * m * w * w)
In this equation, the spectral order number, m, is set to "1" for the first order gratings. The central orders, m=42 for Echelle A and m=25 for Echelle B, are used in the two Echelle modes.
An effective carrousel position is computed for each wavelength that is computed from dispersion coefficients, using the previous calibration coefficients in the table specified by cctabin. The average of the difference between the computed and actual carrousels is used as an offset to the input value of the coefficient C.
1. Perform the carrousel calibration using dispersion coefficients in contained in the tables dcg2_1 through dcg2_8. Previous carrousel calibration coefficients will be taken from oldcctab and the updated calibration will be placed in newcctab.
hr> tmerge dcg2*.tab dcg2lib.tab append hr> carrousel dcg2lib.tab oldcctab newcctab
For assistance using this or any other tasks, please contact help@stsci.edu or call the help desk at 410-338-1082.
yfind, yfit (for computation of LIT_A, LIT_B, LIT_C and LIT_D) and wavecal (for computation of the dispersion coefficient tables).