Name |
# |
Type |
Description |
Channel # of YFP |
1 |
integer |
The first linked image window with matching channel number will be invoked. |
Channel # of CFP |
2 |
integer |
The first linked image window with matching channel number will be invoked. |
Channel # of CFP-YFP FRET |
3 |
integer |
The first linked image window with matching channel number will be invoked. |
Channel # of Fura 340nm |
4 |
integer |
The first linked image window with matching channel number will be invoked. |
Channel # of Fura 380nm |
5 |
integer |
The first linked image window with matching channel number will be invoked. |
Background Level (percentile) |
6 |
real |
Background is calculated as frame-by-frame mean of those pixels that are the darker than this percentile of image histogram for the duration of the entire recording. |
Spectral Unmixing Coefficient Matrix |
7 |
string |
To determine spectral crossbleed coefficients use the Tools/Calculate Crossbleed Correction Factor main menu point, or the Math/Blind Spectral Unmix with NMF function. See more on the layout of the Spectral Unmix Coefficient Matrix in the description of Math/Spectral Unmix. |
Correct exposure time |
8 |
boolean |
Set this True to normalize the cross-talk matrix with the exposure times |
Exposure correction for Coefficient Matrix |
9 |
string |
A column or row vector can be defined as Convolution kernels in the Preferences dialog, or define it here as ={{a,b,c,...}} |
Exposure correction for Image data |
10 |
string |
A column or row vector can be defined as Convolution kernels in the Preferences dialog, or define it here as ={{a,b,c,...}} |