

Name  Colocalization by Cross Correlation 
Software  Fiji 
Author  
Maintainer  
Status 
active 
Category 
Plugins, Colocalization 
Colocalization by Cross Correlation
This plugin attempts to determine: the average distance between nonrandomly spatially associated particles, the standard deviation of that distance (which should also reflect the width of the PSF in the image for diffraction limited images), and a statistical measure of confidence of the association. It does this by performing a crosscorrelation function (CCF) between the two images, operating in a similar manner to Van Steensel’s CCF except this plugin performs the CCF in all directions and provides additional information, such as a confidence level. It currently works on 2D/3D singlechannel images, supports timeseries analysis, and requires a mask of all possible localizations for the signal in one of the images.
Installing the Plugin:
Available on the list of ImageJ updates sites. Requires Fiji.
How to use Colocalization by Cross Correlation:
Prepare a mask for the Costes randomization
To get the best possible results, you will want to create and save a segmented mask for one of your images. This mask should contain all possible localizations for that stain/dye, or it should be a mask of localization for your null hypothesis (i.e if you hypothesize a protein is localized to the mitochondria, you would want your mask to encompass the entire cell). As an example, say you are studying correlation between two nuclear proteins, then you would want your mask to cover the nucles, which could be created easily using a DAPI or Hoechst stain (the mask itself does not need to be generated from either image your are trying to correlate). If you were studying cytoplasmic proteins, you would want your mask to cover the entire cytoplasm. The mask is very important and not using it could easily lead to undesired correlations. This is because without a mask this plugin will find correlations at any distance, and, if say you are studying nuclear proteins, can easily correlate one nuclei to the nuclei of a neighboring cell (cells are often highly repetitive and spaced relatively evenly). However, when an appropriate mask is used, these cell to cell correlations will be subtracted out during the analysis.
Prepare your data images
The two images should undergo appropriate background subtraction to lower the background pixel values to zero or near zero. Even low level background (pixel values of 10 to 20 on a 16 bit image) can lower the confidence level and result in false negatives. Additionally, the images (particularly 3D) need to be correctly scaled (Image > Properties), otherwise all axes will be assumed to have the same scale and your mean correlation distance will be in pixels.
Determine your pointspread function (PSF) dimensions
During a Costes randomization images are randomized by PSFsized chunks, rather than individual pixels. To facilitate this, the plugin needs to know the approximate size of the image PSF in pixels (rounded to the nearest whole unit). The PSF size can be calculated using the Abbe diffraction formula for fluorescence microscopy (lateral: 0.5λ/NA, axial: 2λ/NA^2), and then simply needs to be divided by the corresponding scaled pixel size (in Image > Properties).
Run the plugin
The plugin can be found in the Analyze > Colocalization menu after it has been installed. At the dialog menu, select the two images and the randomization mask to be used, and enter the PSF width and height in pixel units. Image 1 is the image that will be randomized and requires an appropriate mask. If the possible localizations for your dye/stain encompasses the entire image, you can check the no mask box. For the Costes’ randomization cycles count, you can typically input a low number (58), however if you have sparse signal within a large mask volume you will probably want to do more cycles. If the “Show intermediate images” box is checked, the plugin will open images showing the correlations (before and after subtraction of random associations), and a sample randomization image. This can be useful for understanding the function of the plugin, or for visualizing the direction of the correlation if your sample has a polarized axis. More details on the intermediate images can be found below.
Interpreting the results:
To help describe the results, we will use the simple, idealized example shown below. This example analyzes the crosscorrelation of two 2D images composed of equally sized dots (shown as a composite image). Most of these dots are paired to dots of the other channel at a set distance, however some are not at this distance or are not paired. We can see from the results that the strongly correlated dots are approximately 44 pixels apart, with a standard deviation of ~5.5 pixels (for actual microscope data, this distance would be in scaled units instead of pixels). The contribution image highlights the dots that are around this range of each other. We used correlation at a distance for this example to highlight one of the strengths of this technique, but this can be done for traditional “colocalized” images that have a mean crosscorrelation distance near zero.
Here’s a detailed description of each of the result windows:
Correlation plot
A radial profile plot will be displayed, it contains the radial profile of the original crosscorrelation image (blue line), the radial profile of the crosscorrelation after subtraction of random associations (green line), and a Gaussian curve fit to the subtracted profile (red dots). The distance between the red line and the black line is a visual indicator of the confidence value described below. The Yaxis is the average of the crosscorrelation function. While not technically arbitrary, it is most easily viewed as a measure of relative correlation. The range of the graph is set automatically to fit the Gaussian curve. If you wish to view all the data select More > Set Range to Fit all…
Gaussian fit analysis
This text window will contain (in scaled units), the mean distance for the discovered correlation, and the standard deviation of that correlation (sigma), as well as an estimation of confidence for this correlation (range 0100). The confidence is determined by taking the area under the curve (AUC) of the subtracted correlation radial profile (in range of mean ± 3×sigma) divided by the AUC of the original correlation radial profile (in same range). Values closer to 100 indicate a strong likelihood of true correlation. Values near zero indicate low to no correlation between the two images. I currently estimate that values of ~20 or greater indicate some degree of correlation (within the range specified by the Gaussian curve), though this is with very limited data. Confidence values can be affected by many things, including image noise and background, an inappropriate randomization mask, and optical abberations. Performing a simple background subtraction can improve confidence scores signficantly.
Contribution of each image to the gaussian fit
Two new images will be created that display the signal from each analyzed image that contributed to the crosscorrelation and gaussian fit result. It is important to note that this image is always generated and the data it contains will always be visible, even if you do NOT have a strong correlation between the two images. The pixel intensity values should NOT be used as an indicator of overall correlation between the images (that’s what the confidence value is for), but the relative brightness within an image can be used as an approximate indicator of how strongly that particular signal contributed to the correlation result. This relative brightness indication can be easily seen in the example data above: In our original data, all the dots are of the same size and intensity, however, in the resulting contribution images, the dots that remain are varied in their brightness based on how much they contributed to the crosscorrelation result (you’ll notice that the brightest dots are all oriented in the same direction).
Working with timeseries data:
Working with timeseries data is not that different than working with nontimeseries data. Every frame of your data is analyzed individually, in the exact same manner that nontimeseries data would be analyzed. Thus, all inputs (including the mask) must have the same number of frames. You may also The output generated from the plugin has been changed to better suit timeseries data:
The most noteable difference with timeseries data is how the data for the correlation plot is displayed. Instead of linegraphs, the plugin generates heat maps, where the xaxis is time, the yaxis is distance with 0 at the top, and the intensity is the average of the crosscorrelation function at that distance. As we cannot simultaneously show the data for the three lines that would be shown in the correlation plot when using a heat map, we instead generate a three channel image. The first channel (defaults to red), displays the gaussian curve fit to the profile of correlation after subtraction of random associations, equivalent to the red dots from the correlation plot. The second channel (defaults to green) shows the crosscorrelation function results after subtraction of random associations, equivalent to the green line from the correlation plot. And the third channel (defaults to blue) show the results of the original crosscorrelation function, equivalent to the blue line from the correlation plot.
Another change with timeseries data is that in addition to the gaussian fit analysis text window, which now displays the fit data for the frame with the highest correlation, the plugin will output a table of gaussian fit results, showing the gaussian fits and confidence for each frame. To save this table, go to File > Export > Table…, click browse and save the file as a .csv file (you must add the extension or you will get an error message).
Lastly, the contribution images will still be generated and are functionally the same as for their nontime series counterparts. However, it’s important to note that the contribution is evaluted on a per frame basis, and thus each frame shows the signal contriubtion to the gaussian fit results for that frame. Thus, if your crosscorrelation distance shifts over the course of an experiment, the contribution images will display this shifting crosscorrelation.
How it works & intermediate images description:
This plugin starts by performing an initial crosscorrelation to create a crosscorrelation image. Bright regions in the crosscorrelation image correspond to a high correlation between the images when the second image is shifted by a vector equal to the distance form the center of the crosscorrelation image to the bright region. Thus, if you see a bright spot in the crosscorrelation image that is 2 µm to the left of the image center, it means their is a positive correlation between image 1 and image2 when image2 is shited left 2 µm.
To remove the contribution from potential larger repeating structures (such as cells and nuclei), and to correct for correlation that results from high signal density, a second crosscorrelation image generated from randomized images is then subtracted from the original correlation image. This occurs through cycles of:

Randomizing Image1 using the Costes randomization method and the mask of all theoretically possible localizations for the signal in Image1 (i.e. a mask of the cells, or the nuclei), which is provided by the user.

Calculating the crosscorrelation of the randomized image with Image2, then averaging this over successive cycles.
After the subtraction process, we generate a radial profile of the subtracted data, showing the correlation between the images at different offsets, then fit a gaussian curve to it. We also generate a radial profile for the original correlation data before subtraction, as this is needed to establish a measure of confidence. The confidence is calculated as the area under the curve (AUC) of the subtracted correlation radial profile (in the range of mean ± 3×sigma) divided by the AUC of the original correlation radial profile (in same range) as a percentage. The confidence value, along with the mean and sigma of the gaussian fit are displayed in a log window. Higher values of confidence, closer to 100, indicate that two images likely have a true spatial correlation at the indicated distance.
To generate the contribution images, we further modify the subtracted crosscorrelation image, by effectively multiplying it with the gaussian fit in order to create a crosscorrelation image that only retains the data within our gaussian curve range. This gaussianmodified crosscorrelation image is then used to backcalculate the contribution images. Image1Contribution = (image2 ∗ gaussModifiedCorr) × image1. Image2Contribution = (image1 ★ gaussModifiedCorr) × image2. Key: ∗ > convolve, ★ > correlate.