# Resampling and k-coefficients¶

With the `doResampling`

option in the `param.dat`

file, the
per bin sorted opacity function can be resampled with a Chebyshev
polynomial. The number of Chebyshev can also be set in the `param.dat`

file with the `nC`

option. By using the resampling method,
a lot of storage space can be saved. However, the exact location of
individual transition lines is not contained in the resampled data.
The Chebyshev coefficients are reported the `Out<name>_cbin.dat`

files.

An example of a resampled bin is shown in Fig. 8.

doResampling = 1

nC = 20

doStoreSK = 2

nbins = 1

## Bins with empty parts¶

Some bins can contain an empty parts, where the opacity function have no transition lines. This empty parts causes the sorted opacity parts to have a sharp edge between the empty parts and the rest, as shown in Fig. 9. Using the Chebyshev polynomial to resample over these sharp edge would introduce oscillations into the resampled opacity functions. In order to avoid these oscillations, we resample only the part of the sorted opacity function, which is not 0 or kmin. That leads to better results, but when reconstructing the polynomial from the Chebyshev coefficients, then the empty parts must be added again. How this can be done is shown next.

## Using the Chebyshev coefficients¶

The resampled opacity function can be reconstruced with the following code:

```
import numpy as np
from numpy.polynomial.chebyshev import chebval
#change here the name of the file
data_c = np.loadtxt('Out_name_cbin.dat')
#change here the bin index and the bin size:
binIndex = 0
binSize = 300
#extract Chebyshev coefficients
c = data_c[binIndex,2:]
#extract starting point in x of opacity function
xs = data_c[binIndex,1]
#rescale x to the standard Chebychev polynomial range [-1:1]
x1 = x * 2.0 - 1.0
k_res = chebval(x1,c,tensor=False)
x2 = x * (1.0 - xs) + xs
#result is in k_res for x values in x2
k_res = np.exp(k_res)
```