| 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,...}} |